HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere

Abstract

HEALPix -- the Hierarchical Equal Area iso-Latitude Pixelization -- is a versatile data structure with an associated library of computational algorithms and visualization software that supports fast scientific applications executable directly on very large volumes of astronomical data and large area surveys in the form of discretized spherical maps. Originally developed to address the data processing and analysis needs of the present generation of cosmic microwave background (CMB) experiments (e.g. BOOMERanG, WMAP), HEALPix can be expanded to meet many of the profound challenges that will arise in confrontation with the observational output of future missions and experiments, including e.g. Planck, Herschel, SAFIR, and the Beyond Einstein CMB polarization probe. In this paper we consider the requirements and constraints to be met in order to implement a sufficient framework for the efficient discretization and fast analysis/synthesis of functions defined on the sphere, and summarise how they are satisfied by HEALPix.

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• Limits on f_NL parameters from WMAP 3yr data
• Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations
• Probabilistic Cross-Identification of Astronomical Sources
• A simplified, lossless re-analysis of PAPER-64
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization
• Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect--cosmic infrared background correlation
• A Measurement of the Cosmic Microwave Background Gravitational Lensing Potential from 100 Square Degrees of SPTpol Data
• Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
• No large-angle correlations on the non-Galactic microwave sky
• Stellar Inventory of the Solar Neighborhood using Gaia DR1
• The effect of peculiar velocities on supernova cosmology
• A Search for Warm/Hot Gas Filaments Between Pairs of SDSS Luminous Red Galaxies
• Observation of Anisotropy in the Arrival Directions of Galactic Cosmic Rays at Multiple Angular Scales with IceCube
• Detecting a Stochastic Gravitational Wave Background in the presence of a Galactic Foreground and Instrument Noise
• Planck 2013 results. VI. High Frequency Instrument data processing
• Bayesian analysis of sparse anisotropic universe models and application to the 5-yr WMAP data
• A sharper view of Pal 5's tails: Discovery of stream perturbations with a novel non-parametric technique
• BIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal
• Through Thick and Thin - HI Absorption in Cosmological Simulations
• Mapping gravitational-wave backgrounds using methods from CMB analysis: Application to pulsar timing arrays
• Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance
• Galaxy Zoo: The large-scale spin statistics of spiral galaxies in the Sloan Digital Sky Survey
• Magnetohydronamic Evolution of HII Regions in Molecular Clouds: Simulation Methodology, Tests, and Uniform Media
• Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of the Cosmic Microwave Background and Large-scale Structure
• Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
• Clustering of luminous red galaxies I: large scale redshift space distortions
• A non-ideal MHD Gadget: Simulating massive galaxy clusters
• Full-Sky Weak Lensing Simulation with 70 Billion Particles
• A novel scheme for rapid parallel parameter estimation of gravitational waves from compact binary coalescences
• Planck 2013 results. XXVI. Background geometry and topology of the Universe
• The nature of the Diffuse Gamma-Ray Background
• Kinematic modelling of the Milky Way using the RAVE and GCS stellar surveys
• How long does it take to form a molecular cloud?
• Radiation driven implosion and triggered star formation
• The Science Case for LIGO-India
• Improved Constraints on Cosmic Birefringence from the WMAP and Planck Cosmic Microwave Background Polarization Data
• CMB component separation by parameter estimation
• Modelling the Galactic Magnetic Field on the Plane in 2D
• Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry
• WISE x SuperCOSMOS photometric redshift catalog: 20 million galaxies over 3pi steradians
• Limits on anisotropic inflation from the Planck data
• Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect
• Planck 2013 results. XIV. Zodiacal emission
• Submillimetre point sources from the Archeops experiment: Very Cold Clumps in the Galactic Plane
• Cosmic-ray induced destruction of CO in star-forming galaxies
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• Cross-correlation of the CMB and radio galaxies in real, harmonic and wavelet spaces: detection of the integrated Sachs-Wolfe effect and dark energy constraints
• A Measurement of the Cosmic Microwave Background $B$-Mode Polarization Power Spectrum at Sub-Degree Scales from 2 years of POLARBEAR Data
• Observation of Cosmic Ray Anisotropy with the IceTop Air Shower Array
• DustPedia: Multiwavelength Photometry and Imagery of 875 Nearby Galaxies in 42 Ultraviolet--Microwave Bands
• High redshift radio galaxies and divergence from the CMB dipole
• Stellar GADGET: A smooth particle hydrodynamics code for stellar astrophysics and its application to Type Ia supernovae from white dwarf mergers
• Quantifying the impact of the Large Magellanic Cloud on the structure of the Milky Way's dark matter halo using Basis Function Expansions
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Bayesian Estimation of CMB Polarization Maps
• Probing the Cosmological Principle in the counts of radio galaxies at different frequencies
• Constraints on the Galactic Population of TEV Pulsar Wind Nebulae Using Fermi Large Area Telescope Observations
• Improving the open cluster census. I. Comparison of clustering algorithms applied to Gaia DR2 data
• Extragalactic Foreground Contamination in Temperature-based CMB Lens Reconstruction
• Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• Exploring Cosmic Origins with CORE: Survey requirements and mission design
• Likelihood-free inference with neural compression of DES SV weak lensing map statistics
• A deep search for decaying dark matter with XMM-Newton blank-sky observations
• Metrics for next-generation gravitational-wave detectors
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• Is molecular gas necessary for star formation?
• 3D-PDR: A new three-dimensional astrochemistry code for treating Photodissociation Regions
• Empirical Covariance Modeling for 21 cm Power Spectrum Estimation: A Method Demonstration and New Limits from Early Murchison Widefield Array 128-Tile Data
• A radio spectral index map and catalogue at 147-1400 MHz covering 80 per cent of the sky
• Second and third season QUaD CMB temperature and polarization power spectra
• Density split statistics: Cosmological constraints from counts and lensing in cells in DES Y1 and SDSS data
• Revisiting the NVSS number count dipole
• CMB Polarization Systematics Due to Beam Asymmetry: Impact on Inflationary Science
• Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift
• First AGILE Catalog of High Confidence Gamma-Ray Sources
• Constraints on primordial non-Gaussianity from 800,000 photometric quasars
• Probing the isotropy of cosmic acceleration traced by Type Ia supernovae
• CMB lensing tomography with the DES Science Verification galaxies
• The DECam Local Volume Exploration Survey: Overview and First Data Release
• Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
• Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature Anisotropies
• All-Sky Dynamical Response of the Galactic Halo to the Large Magellanic Cloud
• Fast Estimator of Primordial Non-Gaussianity from Temperature and Polarization Anisotropies in the Cosmic Microwave Background
• SOMz: photometric redshift PDFs with self organizing maps and random atlas
• Planck pre-launch status: the Planck-LFI programme
• Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles
• High-Energy Gamma Rays from the Milky Way: Three-Dimensional Spatial Models for the Cosmic-Ray and Radiation Field Densities in the Interstellar Medium
• Planck early results: Cluster Sunyaev-Zeldovich optical scaling relations
• Detection of Ocean Glint and Ozone Absorption Using LCROSS Earth Observations
• Search for gamma-ray emission from the Coma Cluster with six years of Fermi-LAT data
• Simulating polarized Galactic synchrotron emission at all frequencies, the Hammurabi code
• Cosmic Voids and Void Lensing in the Dark Energy Survey Science Verification Data
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• The Galactic Center GeV Excess from a Series of Leptonic Cosmic-Ray Outbursts
• Anisotropy in Cosmic-Ray Arrival Directions in the Southern Hemisphere with Six Years of Data from the IceCube Detector
• Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
• Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge
• A classifier for spurious astrometric solutions in Gaia EDR3
• Dark Matter Strikes Back at the Galactic Center
• Probing the anisotropies of a stochastic gravitational-wave background using a network of ground-based laser interferometers
• Black hole formation and fallback during the supernova explosion of a $40{\mathrm{M}}_{\odot }$ star
• Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing
• Understanding the escape of LyC and Ly$\alpha$ photons from turbulent clouds
• Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window Functions
• Zooming in on accretion - I. The structure of halo gas
• Planck pre-launch status: High Frequency Instrument polarization calibration
• Gaia Data Release 1, Pre-processing and source list creation
• Planck Early Results: The submillimetre properties of a sample of Galactic cold clumps
• Cosmic Reionization On Computers II. Reionization History and Its Back Reaction on Early Galaxies
• Balloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion
• Anisotropies in the diffuse gamma-ray background measured by the Fermi LAT
• The Websky Extragalactic CMB Simulations
• High angular resolution Sunyaev-Zel'dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis
• Shadows in the Dark: Low-Surface-Brightness Galaxies Discovered in the Dark Energy Survey
• Reconstructing Patchy Reionization from the Cosmic Microwave Background
• The modelling of feedback in star formation simulations
• Maximum Likelihood algorithm for parametric component separation in CMB experiments
• SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
• Asymmetric Beams and CMB Statistical Anisotropy
• The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies
• SIXTE -- The Generic X-ray Instrument Simulation Toolkit
• Planck intermediate results. XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps
• Planck 2013 results. VII. HFI time response and beams
• Fermi LAT Observation of Diffuse Gamma-Rays Produced Through Interactions between Local Interstellar Matter and High Energy Cosmic Rays
• The relative impact of photoionizing radiation and stellar winds on different environments
• The Atacama Cosmology Telescope: DR5 maps of 18,000 square degrees of the microwave sky from ACT 2008-2018 data
• Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835
• Distributing many points on spheres: minimal energy and designs
• Exact reconstruction with directional wavelets on the sphere
• Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
• Searching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)
• Fink, a new generation of broker for the LSST community
• Asymptotics for spherical needlets
• A Catalog of Cool Dwarf Targets for the Transiting Exoplanet Survey Satellite
• PLATO as it is: a legacy mission for Galactic archaeology
• Measuring Distances and Reddenings for a Billion Stars: Towards A 3D Dust Map from Pan-STARRS 1
• Cosmological parameters from WMAP 5-year temperature maps
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys III: Measurement Biases and Cosmological Evolution of Gas and Stellar Mass Fractions
• On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• The Collision Between The Milky Way And Andromeda
• Constraints on cosmic hemispherical power anomalies from quasars
• The Cosmic Radio Dipole: Estimators and Frequency Dependence
• Confined Population III Enrichment and the Prospects for Prompt Second-Generation Star Formation
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• Mapping the Magnetic Interstellar Medium in Three Dimensions Over the Full Sky with Neutral Hydrogen
• A needlet ILC analysis of WMAP 7-year data: estimation of CMB temperature map and power spectrum
• The significance of the integrated Sachs-Wolfe effect revisited
• Cosmic Shear Measurements with DES Science Verification Data
• No Sun-like dynamo on the active star $\zeta$ Andromedae from starspot asymmetry
• BICEP2 / Keck Array V: Measurements of B-mode Polarization at Degree Angular Scales and 150 GHz by the Keck Array
• Mapping Earth Analogs from Photometric Variability: Spin-Orbit Tomography for Planets in Inclined Orbits
• Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds
• Maximum a posteriori CMB lensing reconstruction
• The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect
• A 189 MHz, 2400 square degree polarization survey with the Murchison Widefield Array 32-element prototype
• Bayesian analysis of an anisotropic universe model: systematics and polarization
• Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis
• Imprints of Cosmic Rays in Multifrequency Observations of the Interstellar Emission
• Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible
• Gravitationally lensed quasars in Gaia: III. 22 new lensed quasars from Gaia Data Release 2
• The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
• Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects
• Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
• A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg${}^2$ of SPTpol Temperature and Polarization Data
• Dust models compatible with Planck intensity and polarization data in translucent lines of sight
• Thermal SZ fluctuations in the ICM: probing turbulence and thermodynamics in Coma cluster with $Planck$
• StarBench: The D-type expansion of an HII region
• Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit
• Multi-resolution internal template cleaning: An application to the Wilkinson Microwave Anisotropy Probe 7-yr polarization data
• Anisotropies in the stochastic gravitational-wave background: Formalism and the cosmic string case
• Planck 2018 results. II. Low Frequency Instrument data processing
• Lensing Measurements of the Mass Distribution in SDSS Voids
• The S-PASS view of polarized Galactic Synchrotron at 2.3 GHz as a contaminant to CMB observations
• Cosmic Ray Electrons, Positrons and the Synchrotron emission of the Galaxy: consistent analysis and implications
• Planck 2015 results. IV. Low Frequency Instrument beams and window functions
• First Season QUIET Observations: Measurements of CMB Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
• Reconstruction of Gaussian and log-normal fields with spectral smoothness
• The Palermo Swift-BAT Hard X-ray Catalogue. II- Results after 39 months of sky survey
• Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies
• Diffuse emission measurement with INTEGRAL/SPI as indirect probe of cosmic-ray electrons and positrons
• Second Season QUIET Observations: Measurements of the CMB Polarization Power Spectrum at 95 GHz
• Planck 2015 results. III. LFI systematic uncertainties
• Gammapy: A Python package for gamma-ray astronomy
• The LWA1 Low Frequency Sky Survey
• Density split statistics: joint model of counts and lensing in cells
• Planck 2013 results. II. Low Frequency Instrument data processing
• Survey geometry and the internal consistency of recent cosmic shear measurements
• Gaia Data Release 3: The extragalactic content
• Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map
• No galaxy left behind: accurate measurements with the faintest objects in the Dark Energy Survey
• Kinematics of Antlia 2 and Crater 2 from The Southern Stellar Stream Spectroscopic Survey (S5)
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• MAGIC gamma-ray and multifrequency observations of flat spectrum radio quasar PKS 1510-089 in early 2012
• Detection of the ISW effect and corresponding dark energy constraints
• The CMB cold spot: texture, cluster or void?
• Detection of the ISW effect and corresponding dark energy constraints made with directional spherical wavelets
• The influence of streaming velocities and Lyman-Werner radiation on the formation of the first stars
• Statistical properties of dust far-infrared emission
• All-purpose, all-sky photometric redshifts for the Legacy Imaging Surveys Data Release 8
• Gamma ray tests of Minimal Dark Matter
• Cosmic Microwave Background, Accelerating Universe and Inhomogeneous Cosmology
• Modelling [CI] emission from turbulent molecular clouds
• Planck 2015 results. V. LFI calibration
• Analytic Minkowski Functionals of the Cosmic Microwave Background: Second-order Non-Gaussianity with Bispectrum and Trispectrum
• MITEoR: A Scalable Interferometer for Precision 21 cm Cosmology
• Two Ultra-Faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey
• The Link between Galactic Satellite Orbits and Subhalo Accretion
• Spectral estimation on a sphere in geophysics and cosmology
• Powering galactic super-winds with small-scale AGN winds
• Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction
• Star catalog position and proper motion corrections in asteroid astrometry
• Non-Gaussian statistics of critical sets in 2 and 3D: Peaks, voids, saddles, genus and skeleton
• Dipole anisotropy in sky brightness and source count distribution in radio NVSS data
• Improved constraints on cosmic microwave background secondary anisotropies from the complete 2008 South Pole Telescope data
• Reionization optical depth determination from Planck HFI data with ten percent accuracy
• A Possible Cold Imprint of Voids on the Microwave Background Radiation
• From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays
• Lack of large-angle TT correlations persists in WMAP and Planck
• Galaxy clustering, photometric redshifts and diagnosis of systematics in the DES Science Verification data
• The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations
• Splashback Shells of Cold Dark Matter Halos
• SPIDER: Probing the Early Universe with a Suborbital Polarimeter
• Large-scale alignments from WMAP and Planck
• Measuring the spectrum of primordial gravitational waves with CMB, PTA and Laser Interferometers
• Modeling Thermal Dust Emission with Two Components: Application to the Planck HFI Maps
• Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• A data science platform to enable time-domain astronomy
• Polarised radio filaments outside the Galactic plane
• Smoothed Particle Hydrodynamics simulations of expanding HII regions. I. Numerical methods and tests
• Exploring the diffuse interstellar bands with the Sloan Digital Sky Survey
• Sensitivity and foreground modelling for large-scale CMB B-mode polarization satellite missions
• Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
• Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach
• Gravitational wave radiometry: Mapping a stochastic gravitational wave background
• Detection of a Supervoid Aligned with the Cold Spot of the Cosmic Microwave Background
• Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis
• Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey
• Detecting and Constraining N${}_2$ Abundances in Planetary Atmospheres Using Collisional Pairs
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• Detecting the integrated Sachs-Wolfe effect with stacked voids
• Modeling the magnetized Local Bubble from dust data
• Planck Early Results. V. The Low Frequency Instrument data processing
• Searches for Cosmic-Ray Electron Anisotropies with the Fermi Large Area Telescope
• GammaLib and ctools: A software framework for the analysis of astronomical gamma-ray data
• The Kinematic Sunyaev-Zel'dovich Effect with Projected Fields II: prospects, challenges, and comparison with simulations
• Diffuse cosmic rays shining in the Galactic center: A novel interpretation of H.E.S.S. and Fermi-LAT gamma-ray data
• Anisotropies in the astrophysical gravitational-wave background: Predictions for the detection of compact binaries by LIGO and Virgo
• Discovery of Magnetic Fields Along Stacked Cosmic Filaments as Revealed by Radio and X-Ray Emission
• The Radio Sky at Meter Wavelengths: m-Mode Analysis Imaging with the Owens Valley Long Wavelength Array
• Constraints on the diffuse high-energy neutrino flux from the third flight of ANITA
• Fast-transient Searches in Real Time with ZTFReST: Identification of Three Optically-discovered Gamma-ray Burst Afterglows and New Constraints on the Kilonova Rate
• The Direct Collapse of a Massive Black Hole Seed Under the Influence of an Anisotropic Lyman-Werner Source
• Constraints on CPT violation from WMAP three year polarization data: a wavelet analysis
• Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal
• Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory
• Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT
• The LSST DESC DC2 Simulated Sky Survey
• A robust public catalogue of voids and superclusters in the SDSS Data Release 7 galaxy surveys
• Estimating the large-scale angular power spectrum in the presence of systematics: a case study of Sloan Digital Sky Survey quasars
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach
• Nonphotosynthetic Pigments as Potential Biosignatures
• Statistics of gamma-ray point sources below the Fermi detection limit
• Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
• The Atacama Cosmology Telescope: Constraints on Cosmic Birefringence
• Bianchi Type VII_h Models and the WMAP 3-year Data
• Dark Sky Simulations: Early Data Release
• NIFTY - Numerical Information Field Theory - a versatile Python library for signal inference
• Double detonations of sub-Chandrasekhar mass CO white dwarfs: Can different core and He shell masses explain variations of Type Ia supernovae?
• A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation
• Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
• Chemical gradients in the Milky Way from the RAVE data. I. Dwarf stars
• Gaia DR3: Apsis III -- Non-stellar content and source classification
• ARCADE 2 Observations of Galactic Radio Emission
• First Observational Tests of Eternal Inflation
• Testable polarization predictions for models of CMB isotropy anomalies
• Fingerprints of Galactic Loop I on the Cosmic Microwave Background
• Gaia Early Data Release 3. Building the Gaia DR3 source list -- Cross-match of Gaia observations
• A measurement of large-scale peculiar velocities of clusters of galaxies: technical details
• Homogeneity and isotropy in the 2MASS Photometric Redshift catalogue
• Frequency-Dependent Constraints on Cosmic Birefringence from the LFI and HFI Planck Data Release 4
• Cosmological constraints from noisy convergence maps through deep learning
• Tree-based solvers for adaptive mesh refinement code FLASH - I: gravity and optical depths
• S-band Polarization All Sky Survey (S-PASS): survey description and maps
• Cross-correlations as a cosmological carbon monoxide detector
• Missing Thermal Energy of the Intracluster Medium
• Optically thick HI dominant in the local interstellar medium; an alternative interpretation to "dark gas"
• Atmospheric circulation of brown dwarfs and directly imaged exoplanets driven by cloud radiative feedback: effects of rotation
• The slight spin of the old stellar halo
• DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics
• Cold Milky Way Hi gas in filaments
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• An empirical model of the Gaia DR3 selection function
• A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets
• The Coherent Magnetic Field of the Milky Way
• Planck 2013 results. XXXI. Consistency of the Planck data
• Directional detection as a strategy to discover Galactic Dark Matter
• Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample
• A Full-sky, High-resolution Atlas of Galactic 12 micron Dust Emission with WISE
• Planck intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane
• HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• Channeling in direct dark matter detection I: channeling fraction in NaI (Tl) crystals
• Search for Dark Matter Annihilation in the Galactic Center with IceCube-79
• Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data
• Global universe anisotropy probed by the alignment of structures in the cosmic microwave background
• Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science
• Characterization of the BICEP Telescope for High-Precision Cosmic Microwave Background Polarimetry
• VISION - Vienna survey in Orion I. VISTA Orion A Survey
• Foreground Mismodeling and the Point Source Explanation of the Fermi Galactic Center Excess
• An Alternative Accurate Tracer of Molecular Clouds: The "$X_{\mathrm{CI}}$-Factor"
• Dust-Gas Scaling Relations and OH Abundance in the Galactic ISM
• Properties of Galactic cirrus clouds observed by BOOMERanG
• An Estimate of the Primordial Non-Gaussianity Parameter f_NL Using the Needlet Bispectrum from WMAP
• New Measurements of Fine-Scale CMB Polarization Power Spectra from CAPMAP at Both 40 and 90 GHz
• Planck 2013 results. V. LFI calibration
• Mitigating Internal Instrument Coupling for 21 cm Cosmology I: Temporal and Spectral Modeling in Simulations
• Non Gaussianity and Minkowski Functionals: forecasts for Planck
• A re-analysis of the three-year WMAP temperature power spectrum and likelihood
• unWISE tomography of Planck CMB lensing
• First detection of stacked X-ray emission from cosmic web filaments
• The DECam Local Volume Exploration Survey Data Release 2
• Full-sky map of the ISW and Rees-Sciama effect from Gpc simulations
• Integral constraints in spectroscopic surveys
• MADmap: A Massively Parallel Maximum-Likelihood Cosmic Microwave Background Map-Maker
• New constraints on Parity Symmetry from a re-analysis of the WMAP-7 low resolution power spectra
• Detecting Ocean Glint on Exoplanets Using Multiphase Mapping
• A Search for Point Sources of EeV Neutrons
• The all-sky PLATO input catalogue
• Observation of Small-scale Anisotropy in the Arrival Direction Distribution of TeV Cosmic Rays with HAWC
• Broken Isotropy from a Linear Modulation of the Primordial Perturbations
• Comparison of filters for the detection of point sources in Planck simulations
• Constraining Gravity at the Largest Scales through CMB Lensing and Galaxy Velocities
• Characterising Open Clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution
• The second data release from the European Pulsar Timing Array V. Search for continuous gravitational wave signals
• Cosmic Cartography of the Large-Scale Structure with Sloan Digital Sky Survey Data Release 6
• The optical depth of the Universe to ultrahigh energy cosmic ray scattering in the magnetized large scale structure
• Measurements of the Intensity and Polarization of the Anomalous Microwave Emission in the Perseus molecular complex with QUIJOTE
• DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos
• Error analysis of quadratic power spectrum estimates for CMB polarization: sampling covariance
• Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?
• The Denoised, Deconvolved, and Decomposed Fermi $\gamma$-ray sky - An application of the D${}^3$PO algorithm
• Exploring Cosmic Origins with CORE: B-mode Component Separation
• Revealing dark matter substructure with anisotropies in the diffuse gamma-ray background
• Metal Transport and Chemical Heterogeneity in Early Star Forming Systems
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• Survey of Surveys I: The largest catalogue of radial velocities for the Galaxy
• Fast simulations for intensity mapping experiments
• Improved simulation of non-Gaussian temperature and polarization CMB maps
• Estimation of Polarized Power Spectra by Gibbs sampling
• Voids in the SDSS DR9: observations, simulations, and the impact of the survey mask
• The ${}^{12}$CO/${}^{13}$CO ratio in turbulent molecular clouds
• Diffuse gamma-ray emission from galactic pulsars
• Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples
• Planck 2015 results. VII. HFI TOI and beam processing
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• On the Viability of Bianchi Type VIIh Models with Dark Energy
• Looking at cosmic near-infrared background radiation anisotropies
• SNe Ia from double detonations: Impact of core-shell mixing on the carbon ignition mechanism
• Simulations for single-dish intensity mapping experiments
• A simulation pipeline for the Planck mission
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
• Redundant Array Configurations for 21 cm Cosmology
• Planck's view on the spectrum of the Sunyaev-Zeldovich effect
• Heating of the Intergalactic Medium by Hydrogen Reionization
• Two- and three-dimensional wide-field weak lensing mass maps from the Hyper Suprime-Cam Subaru Strategic Program S16A data
• Peeling off foregrounds with the constrained moment ILC method to unveil primordial CMB $B$-modes
• Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data
• CLUMPY: Jeans analysis, $\gamma$-ray and neutrino fluxes from dark matter (sub-)structures
• Mapping the large-scale anisotropy in the WMAP data
• Optimizing searches for electromagnetic counterparts of gravitational wave triggers
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• A Measurement of the Degree Scale CMB B-mode Angular Power Spectrum with POLARBEAR
• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
• The Three-Dimensional Spatial Distribution of Interstellar Gas in the Milky Way: Implications for Cosmic Rays and High-Energy Gamma-Ray Emissions
• Quaia, the Gaia-unWISE Quasar Catalog: An All-Sky Spectroscopic Quasar Sample
• New constraints on modelling the random magnetic field of the MW
• The meaning of WISE colours - I. The Galaxy and its satellites
• Hubble flow variance and the cosmic rest frame
• The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology
• Supernova-blast waves in wind-blown bubbles, turbulent, and power-law ambient media
• The parallax zero point offset from Gaia EDR3 data
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• The multiplicity and anisotropy of galactic satellite accretion
• Shear Power Spectrum Reconstruction using Pseudo-Spectrum Method
• Simple foreground cleaning algorithm for detecting primordial B-mode polarization of the cosmic microwave background
• Data Release 3: the Solar System survey
• Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps
• A 14 $h^{-3}$ Gpc${}^3$ study of cosmic homogeneity using BOSS DR12 quasar sample
• Measurement of the $T_{\mathrm{CMB}}$ evolution from the Sunyaev-Zel'dovich effect
• Fast directional continuous spherical wavelet transform algorithms
• Gaia Data Release 2: Summary of the variability processing & analysis results
• A new model to predict weak-lensing peak counts I. Comparison with $N$-body Simulations
• Fast optimal CMB power spectrum estimation with Hamiltonian sampling
• Accurate cosmic shear errors: do we need ensembles of simulations?
• A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data
• Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol
• The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence
• Planck Intermediate Results. IX. Detection of the Galactic haze with Planck
• The fully connected N-dimensional skeleton: probing the evolution of the cosmic web
• Identification of a Local Sample of Gamma-Ray Bursts Consistent with a Magnetar Giant Flare Origin
• Gamma-ray background anisotropy from galactic dark matter substructure
• Star/galaxy separation at faint magnitudes: Application to a simulated Dark Energy Survey
• Gaia 1 and 2. A pair of new Galactic star clusters
• Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog
• Constraining models of the large scale Galactic magnetic field with WMAP5 polarization data and extragalactic Rotation Measure sources
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• Neutron Star Mergers and How to Study Them
• unWISE Coadds: The Five-year Data Set
• Non-blind catalogue of extragalactic point sources from the Wilkinson Microwave Anisotropy Probe (WMAP) first 3--year survey data
• Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
• A WISE measurement of the ISW effect
• IceCat-1: the IceCube Event Catalog of Alert Tracks
• Planck intermediate results. X. Physics of the hot gas in the Coma cluster
• Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
• First season QUaD CMB temperature and polarization power spectra
• Complete super-sample lensing covariance in the response approach
• Fermi-LAT Observations of the LIGO event GW150914
• Fast Estimator of Primordial Non-Gaussianity from Temperature and Polarization Anisotropies in the Cosmic Microwave Background II: Partial Sky Coverage and Inhomogeneous Noise
• Supplement: Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
• On the CMB large-scales angular correlations
• Spatial variations in the spectral index of polarized synchrotron emission in the 9 yr WMAP sky maps
• Directional Lya equivalent boosting I. Spherically symmetric distributions of clumps
• Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust
• Chemical gradients in the Milky Way from the RAVE data. II. Giant stars
• A Framework for Telescope Schedulers: With Applications to the Large Synoptic Survey Telescope
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Needlet Detection of Features in WMAP CMB Sky and the Impact on Anisotropies and Hemispherical Asymmetries
• SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps
• Cross-correlation of Planck CMB Lensing and CFHTLenS Galaxy Weak Lensing Maps
• Extracting HI cosmological signal with Generalized Needlet Internal Linear Combination
• Excess Clustering on Large Scales in the MegaZ DR7 Photometric Redshift Survey
• A Pixelated Approach to Galaxy Catalogue Incompleteness: Improving the Dark Siren Measurement of the Hubble Constant
• The PLATO field selection process I. Identification and content of the long-pointing fields
• Joint Planck and WMAP CMB Map Reconstruction
• Demonstration of cosmic microwave background delensing using the cosmic infrared background
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• Results from the Wilkinson Microwave Anisotropy Probe
• Primordial Non-Gaussianity and the NRAO VLA Sky Survey
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
• Disks in the sky: A reassessment of the WMAP "cold spot"
• A Sino-German 6 cm polarization survey of the Galactic plane III. The region from 10 degree to 60 degree longitude
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• Alignment tests for low CMB multipoles
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps -- validation on simulations
• A catalogue of cataclysmic variables from 20 years of the Sloan Digital Sky Survey with new classifications, periods, trends and oddities
• Scale Dependent Galaxy Bias in the SDSS as a function of Luminosity and Colour
• First Observational Tests of Eternal Inflation: Analysis Methods and WMAP 7-Year Results
• On the joint analysis of CMB temperature and lensing-reconstruction power spectra
• Common-envelope evolution with an asymptotic giant branch star
• Constructing stable 3D hydrodynamical models of giant stars
• CHIME/FRB Catalog 1 results: statistical cross-correlations with large-scale structure
• QUIJOTE Scientific Results. II. Polarisation Measurements of the Microwave Emission in the Galactic molecular complexes W43 and W47 and supernova remnant W44
• HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron
• ROMA: a map-making algorithm for polarised CMB data sets
• Gaia Data Release 3: Chemical cartography of the Milky Way
• QUBIC: The QU Bolometric Interferometer for Cosmology
• Deep learning dark matter map reconstructions from DES SV weak lensing data
• Searches for Neutrinos from Gamma-Ray Bursts using the IceCube Neutrino Observatory
• Cosmological Forecast for non-Gaussian Statistics in large-scale weak Lensing Surveys
• A high-significance detection of non-Gaussianity in the WMAP 3-year data using directional spherical wavelets
• CMB/kSZ and Compton-$y$ Maps from 2500 square degrees of SPT-SZ and Planck Survey Data
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Non-Gaussian structure of the lensed CMB power spectra covariance matrix
• Combining power spectrum and bispectrum measurements to detect oscillatory features
• Tomography of the Fermi-LAT gamma-ray diffuse extragalactic signal via cross-correlations with galaxy catalogs
• Solution to the cosmic ray anisotropy problem
• Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
• The Hydrogen Epoch of Reionization Array Dish I: Beam Pattern Measurements and Science Implications
• Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB $B$-mode analysis
• The Center of Light: Spectroastrometric Detection of Exomoons
• Mapping and simulating systematics due to spatially-varying observing conditions in DES Science Verification data
• Cosmic-Ray Propagation in Light of Recent Observation of Geminga
• Probing Cosmological Isotropy With Type IA Supernovae
• Fast Pixel Space Convolution for CMB Surveys with Asymmetric Beams and Complex Scan Strategies: FEBeCoP
• Discovery and redshift of an optical afterglow in 71 square degrees: iPTF13bxl and GRB 130702A
• Planck 2013 results. III. LFI systematic uncertainties
• A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
• Measuring the dark flow with public X-ray cluster data
• A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data
• The stacked ISW signal of rare superstructures in ΛCDM
• Compressed sensing for wide-field radio interferometric imaging
• Making sky maps from Planck data
• Properties of cold and warm HI gas phases derived from a Gaussian decomposition of HI4PI data
• Cosmological Measurements from Angular Power Spectra Analysis of BOSS DR12 Tomography
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• Mapping Clouds and Terrain of Earth-like Planets from Photometric Variability: Demonstration with Planets in Face-on Orbits
• Connecting Synchrotron, Cosmic Rays, and Magnetic Fields in the Plane of the Galaxy
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Is there an unaccounted excess Extragalactic Cosmic Radio Background?
• Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data
• Recovery of 21 cm intensity maps with sparse component separation
• Results from EDGES High-Band: III. New Constraints on Parameters of the Early Universe
• A Case Against Spinning PAHs as the Source of the Anomalous Microwave Emission
• An estimate of the local ISW signal, and its impact on CMB anomalies
• Faraday rotation, stochastic magnetic fields and CMB maps
• Can a supervoid explain the Cold Spot?
• Exploring cosmic origins with CORE: gravitational lensing of the CMB
• Measuring the Integrated Sachs-Wolfe Effect
• deep21: a Deep Learning Method for 21cm Foreground Removal
• A low CMB variance in the WMAP data
• The XMM Cluster Outskirts Project (X-COP): Physical conditions to the virial radius of Abell 2142
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• Mapping gravitational-wave backgrounds in modified theories of gravity using pulsar timing arrays
• A Search for Dark Matter Annihilation in Galaxy Groups
• Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise
• Blind and non-blind source detection in WMAP 5-year maps
• CMB data analysis and sparsity
• The Spectroscopy of Plasma Evolution from Astrophysical Radiation Mission
• The angular power spectrum of the diffuse gamma-ray emission as measured by the Fermi Large Area Telescope and constraints on its Dark Matter interpretation
• Madam - a map-making method for CMB experiments
• Magnetic field strength in cosmic web filaments
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Planck 2015 results. II. Low Frequency Instrument data processing
• Towards a realistic astrophysical interpretation of the gamma-ray Galactic center excess
• The Rapid ASKAP Continuum Survey IV: continuum imaging at 1367.5 MHz and the first data release of RACS-mid
• Six More Ultra-Faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
• The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
• The BAyesian STellar Algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology
• The Local Bubble: a magnetic veil to our Galaxy
• PS1-STRM: Neural network source classification and photometric redshift catalogue for PS1 $3\pi$ DR1
• Characterization of Dark-Matter-induced anisotropies in the diffuse gamma-ray background
• Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
• Exploiting the full potential of photometric quasar surveys: Optimal power spectra through blind mitigation of systematics
• Deciphering Contributions to the Extragalactic Gamma-Ray Background from 2 GeV to 2 TeV
• A search for cyclical sources of gamma-ray emission on the period range from days to years in the Fermi-LAT sky
• The first multi-dimensional view of mass loss from externally FUV irradiated protoplanetary discs
• Cosmic shear power spectra in practice
• Limiting Magnetic Fields in the Cosmic Web with Diffuse Radio Emission
• Efficient Wiener filtering without preconditioning
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• Bifurcation in the history of Uranus and Neptune: the role of giant impacts
• Disconnected pseudo-$C_{\ell }$ covariances for projected large-scale structure data
• The observational signature of the first H II regions
• Planck intermediate results. XIII. Constraints on peculiar velocities
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• Gaia data release 1, the photometric data
• Planck 2013 results. IV. Low Frequency Instrument beams and window functions
• Using correlations between CMB lensing and large-scale structure to measure primordial non-Gaussianity
• The needlets bispectrum
• Star-galaxy separation strategies for WISE-2MASS all-sky infrared galaxy catalogs
• The Galactic ${}^{26}$Al emission map as revealed by INTEGRAL/SPI
• Exhausting the Information: Novel Bayesian Combination of Photometric Redshift PDFs
• Measuring the Galaxy Cluster Bulk Flow from WMAP data
• CMB power spectrum estimation using wavelets
• Hydrogen Reionization in the Illustris universe
• CMB spectral distortions revisited: a new take on $\mu$ distortions and primordial non-Gaussianities from FIRAS data
• Polarized galactic synchrotron and dust emission and their correlation
• Characterization of foreground emission at degree angular scale for CMB B-modes observations. Thermal Dust and Synchrotron signal from Planck and WMAP data
• Do we Live in a "Small Universe"?
• A Map of the Integrated Sachs-Wolfe Signal from Luminous Red Galaxies
• Joint Measurement of Lensing-Galaxy Correlations Using SPT and DES SV Data
• Making CMB temperature and polarization maps with Madam
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• Modeling the Infrared Spectrum of the Earth-Moon System: Implications for the Detection and Characterization of Earthlike Extrasolar Planets and their Moonlike Companions
• Search for Cosmic-Ray Electron and Positron Anisotropies with Seven Years of Fermi Large Area Telescope Data
• Temperature and Polarization CMB Maps from Primordial non-Gaussianities of the Local Type
• Improved Limits on Sterile Neutrino Dark Matter using Full-Sky Fermi Gamma-Ray Burst Monitor Data
• On the significance of power asymmetries in Planck CMB data at all scales
• All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field
• A model-independent analysis of the Fermi Large Area Telescope gamma-ray data from the Milky Way dwarf galaxies and halo to constrain dark matter scenarios
• Daily monitoring of TeV gamma-ray emission from Mrk 421, Mrk 501, and the Crab Nebula with HAWC
• Testing cosmology with a catalogue of voids in the BOSS galaxy surveys
• Interstellar neutral helium in the heliosphere from IBEX observations. II. The Warsaw Test Particle Model (WTPM)
• CMB Maximum Temperature Asymmetry Axis: Alignment with Other Cosmic Asymmetries
• Radio data and synchrotron emission in consistent cosmic ray models
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• Detecting Bispectral Acoustic Oscillations from Inflation Using a New Flexible Estimator
• WMAP 3yr data with the CCA: anomalous emission and impact of component separation on the CMB power spectrum
• Dipole Anisotropy in Integrated Linearly Polarized Flux Density in NVSS Data
• Hierarchical progressive surveys. Multi-resolution HEALPix data structures for astronomical images, catalogues, and 3-dimensional data cubes
• The SDSS Galaxy Angular Two-Point Correlation Function
• Cross-correlation of gravitational lensing from DES Science Verification data with SPT and Planck lensing
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• Dust properties inside molecular clouds from coreshine modeling and observations
• On the detection of spectral ripples from the Recombination Epoch
• Low Variance at large scales of WMAP 9 year data
• The High Redshift Integrated Sachs-Wolfe Effect
• Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
• A DECam Search for an Optical Counterpart to the LIGO Gravitational Wave Event GW151226
• Anisotropic dark energy and CMB anomalies
• Modeling UV Radiation Feedback from Massive Stars: I. Implementation of Adaptive Ray Tracing Method and Tests
• The JCMT Gould Belt Survey: A Quantitative Comparison Between SCUBA-2 Data Reduction Methods
• Large-Angle Correlations in the Cosmic Microwave Background
• Fervent: Chemistry-coupled, ionising and non-ionising radiative feedback in magnetohydrodynamical simulations
• HI, CO, and Planck/IRAS dust properties in the high-latitude-cloud complex, MBM 53, 54, 55 and HLCG 92-35; Possible evidence for an optically thick HI envelope around the CO clouds
• Density and temperature of cosmic-web filaments on scales of tens of megaparsecs
• The $N_{\ell }$ of gravitational wave background experiments
• Star cluster formation and cloud dispersal by radiative feedback: dependence on metallicity and compactness
• Observation of the Far-ultraviolet Continuum Background with SPEAR/FIMS
• Ultra-High-Energy Cosmic Rays from Radio Galaxies
• Extragalactic Imprints in Galactic Dust Maps
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
• A Gaia DR2 Mock Stellar Catalog
• Inference of the optical depth to reionization from low multipole temperature and polarisation Planck data
• SILCC-ZOOM: The early impact of ionizing radiation on forming molecular clouds
• Extragalactic gamma-ray background radiation from dark matter annihilation
• Measuring the tensor to scalar ratio from CMB B-modes in presence of foregrounds
• Foreground Subtraction of Cosmic Microwave Background Maps using WI-FIT (Wavelet based hIgh resolution Fitting of Internal Templates)
• Shot noise in the astrophysical gravitational-wave background
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• Fitting the nonlinear matter bispectrum by the Halofit approach
• The Gaia DR2 parallax zero point: Hierarchical modeling of red clump stars
• The Lyman Continuum Escape Survey: Connecting Time-Dependent [OIII] and [OII] Line Emission with Lyman Continuum Escape Fraction in Simulations of Galaxy Formation
• Radio constraints on dark matter annihilation in the galactic halo and its substructures
• Non-detection of a statistically anisotropic power spectrum in large-scale structure
• Impact of Foregrounds on HI Intensity Mapping Cross-Correlations with Optical Surveys
• Bias to CMB Lensing Reconstruction from Temperature Anisotropies due to Large-Scale Galaxy Motions
• Measuring Phased-Array Antenna Beampatterns with High Dynamic Range for the Murchison Widefield Array using 137 MHz ORBCOMM Satellites
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• Chemistry and radiative shielding in star forming galactic disks
• SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
• The Needle in the 100 deg2 Haystack: Uncovering Afterglows of Fermi GRBs with the Palomar Transient Factory
• Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
• Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA
• Supernova feedback and the energy deposition in molecular clouds
• Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914
• Mock galaxy shape catalogs in the Subaru Hyper Suprime-Cam Survey
• Bias and scatter in the Hubble diagram from cosmological large-scale structure
• Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich Effect
• Planck 2015 results. VI. LFI mapmaking
• A new way to test the Cosmological Principle: measuring our peculiar velocity and the large scale anisotropy independently
• iPTF Search for an Optical Counterpart to Gravitational Wave Trigger GW150914
• The Hydrodynamic Feedback of Cosmic Reionization on Small-Scale Structures and Its Impact on Photon Consumption during the Epoch of Reionization
• Testing the Strong Equivalence Principle. II. Relating the External Field Effect in Galaxy Rotation Curves to the Large-Scale Structure of the Universe
• Unveiling the Gamma-ray Source Count Distribution Below the Fermi Detection Limit with Photon Statistics
• Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
• Measurement of the electron-pressure profile of galaxy clusters in Wilkinson Microwave Anisotropy Probe (WMAP) 3-year data
• The Heraklion Extragalactic Catalogue (HECATE): a value-added galaxy catalogue for multi-messenger astrophysics
• Inferring the Redshift Distribution of the Cosmic Infrared Background
• Compact Groups of Galaxies selected by stellar mass: The 2MASS Compact Group Catalogue
• QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
• Polyspectra searches for sharp oscillatory features in cosmic microwave sky data
• Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground
• An Optimal-Dimensionality Sampling Scheme on the Sphere with Fast Spherical Harmonic Transforms
• A comprehensive overview of the Cold Spot
• Clustering of Luminous Red Galaxies III: Detection of the Baryon Acoustic Peak in the 3-point Correlation Function
• Reducing Noise in Cosmological N-body Simulations with Neutrinos
• Full-sky CMB lensing reconstruction in presence of sky-cuts
• Methods for Bayesian power spectrum inference with galaxy surveys
• Forecasting performance of CMB experiments in the presence of complex foreground contaminations
• Testing Isotropy of Cosmic Microwave Background Radiation
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• A cross-correlation study of the Fermi-LAT $\gamma$-ray diffuse extragalactic signal
• Modelling of the Spectral Energy Distribution of Fornax A: Leptonic and Hadronic Production of High Energy Emission from the Radio Lobes
• Limits on Defects Formation and Hybrid Inflationary Models with Three-Year WMAP Observations
• Evidence for Line-of-Sight Frequency Decorrelation of Polarized Dust Emission in $Planck$ Data
• Imprint of DES super-structures on the Cosmic Microwave Background
• Characterizing the Nature of the Unresolved Point Sources in the Galactic Center
• The large scale polarization explorer (LSPE) for CMB measurements: performance forecast
• Deciphering Lyman-$\alpha$ Emission Deep into the Epoch of Reionisation
• Distinguishing Dark Matter from Unresolved Point Sources in the Inner Galaxy with Photon Statistics
• Magnetic field morphology in nearby molecular clouds as revealed by starlight and submillimetre polarization
• Improving Galaxy Clustering Measurements with Deep Learning: analysis of the DECaLS DR7 data
• The Splashback Radius of Planck-SZ clusters
• How an improved implementation of H2 self-shielding influences the formation of massive stars and black holes
• Numerical aspects of Giant Impact simulations
• AGN-driven outflows and the formation of Ly$\alpha$ nebulae around high-z quasars
• To beta or not to beta: can higher-order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
• Alignment and signed-intensity anomalies in WMAP data
• Large-scale Maps of the Cosmic Infrared Background from Planck
• Results from the Atacama B-mode Search (ABS) Experiment
• Null Signal for the Cosmic Anisotropy in the Pantheon Supernovae Data
• S2LET: A code to perform fast wavelet analysis on the sphere
• Forecasting pulsar timing array sensitivity to anisotropy in the stochastic gravitational wave background
• Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE
• TRIS I: Absolute Measurements of the Sky Brightness Temperature at 0.6, 0.82 and 2.5 GHz
• Systematic effects in large-scale angular power spectra of photometric quasars and implications for constraining primordial nongaussianity
• Modelling of the Effects of Stellar Feedback during Star Cluster Formation Using a Hybrid Gas and N-Body Method
• Full-sky maps for gravitational lensing of the CMB
• A Full $w$CDM Analysis of KiDS-1000 Weak Lensing Maps using Deep Learning
• Modeling UV Radiation Feedback from Massive Stars: III. Escape of Radiation from Star-forming Giant Molecular Clouds
• Planck intermediate results. VIII. Filaments between interacting clusters
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• Swiss Cheese and a Cheesy CMB
• Maximum likelihood map-making with the Laser Interferometer Space Antenna
• A Relationship Between Stellar Age and Spot Coverage
• Planck intermediate results. XXIV. Constraints on variation of fundamental constants
• Parity Asymmetry in the CMBR Temperature Power Spectrum
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• A Large Sky Simulation of the Gravitational Lensing of the Cosmic Microwave Background
• Magnetic field evolution in cosmic filaments with LOFAR data
• Simulating the diversity of shapes of the Lyman-$\alpha$ line
• Unveiling the Dynamics of the Universe
• Cleaned Three-Year WMAP CMB Map: Magnitude of the Quadrupole and Alignment of Large Scale Modes
• Lensing Reconstruction in Post-Born Cosmic Microwave Background Weak Lensing
• Multiwavelength follow-up of a rare IceCube neutrino multiplet
• Joint 3D modelling of the polarized Galactic synchrotron and thermal dust foreground diffuse emission
• Comparing Polarised Synchrotron and Thermal Dust Emission in the Galactic Plane
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• Structure and dynamics of the Shapley Supercluster
• The LMC geometry and outer stellar populations from early DES data
• Improving Weak Lensing Mass Map Reconstructions using Gaussian and Sparsity Priors: Application to DES SV
• What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations
• Grand challenges in protoplanetary disc modelling
• Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
• YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-Loop
• Lunar Crater Identification in Digital Images
• The impact of Galactic synchrotron emission on CMB anisotropy measurements. I. Angular power spectrum analysis of total intensity all-sky surveys
• Directional Variations of Cosmological Parameters from the Planck CMB Data
• Anomalies in the low CMB multipoles and extended foregrounds
• Galactic foreground contributions to the WMAP5 maps
• Robust covariance estimation of galaxy-galaxy weak lensing: validation and limitation of jackknife covariance
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• Sparse component separation for accurate CMB map estimation
• The GCE in a New Light: Disentangling the $\gamma$-ray Sky with Bayesian Graph Convolutional Neural Networks
• Three-Dimensional Distribution of the Interstellar Dust in the Milky Way
• First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
• Swift follow-up of the Gravitational Wave source GW150914
• Like a spider in its web: a study of the Large Scale Structure around the Coma cluster
• Future virialized structures: An analysis of superstructures in SDSS-DR7
• The FHD/$\mathbf{\epsilon }$ppsilon Epoch of Reionization Power Spectrum Pipeline
• Measurement of CIB power spectra over large sky areas from Planck HFI maps
• Supervoids in the WISE-2MASS catalogue imprinting Cold Spots in the Cosmic Microwave Background
• Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data
• Milky Way Tomography with the SkyMapper Southern Survey. II. Photometric Re-calibration of SMSS DR2
• Fast spin +-2 spherical harmonics transforms and application in cosmology
• Ab initio Simulations of a Supernova Driven Galactic Dynamo in an Isolated Disk Galaxy
• From the supernova to the supernova remnant: the three-dimensional imprint of a thermonuclear explosion
• The Imprint of Large Scale Structure on the Ultra-High-Energy Cosmic Ray Sky
• Simulated SKA maps from Galactic 3D-emission models
• A Hybrid Ensemble Learning Approach to Star-Galaxy Classification
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• INTEGRAL/IBIS 17-yr hard X-ray all-sky survey
• Galactic diffuse gamma rays meet the PeV frontier
• LIGER: mock relativistic light-cones from Newtonian simulations
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Star catalog position and proper motion corrections in asteroid astrometry II: The Gaia era
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Fast directional correlation on the sphere with steerable filters
• Results from EDGES High-Band: II. Constraints on Parameters of Early Galaxies
• Full-sky Cosmic Microwave Background Foreground Cleaning Using Machine Learning
• Anisotropy of Cosmic Acceleration
• Cross-correlating Astrophysical and Cosmological Gravitational Wave Backgrounds with the Cosmic Microwave Background
• Second Data Release of the All-sky NOIRLab Source Catalog
• Dipolar modulation in number counts of WISE-2MASS sources
• Cosmic Structure and Dynamics of the Local Universe
• CO-dark gas and molecular filaments in Milky Way-type galaxies - II: The temperature distribution of the gas
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• Gaia Data Release 1. Cross-match with external catalogues - Algorithm and results
• Mitigating contamination in LSS surveys: a comparison of methods
• Observed parity-odd CMB temperature bispectrum
• Probing the Dark Flow signal in WMAP 9 yr and PLANCK cosmic microwave background maps
• Microwave Background Correlations from Dipole Anisotropy Modulation
• Estimating the spectral indices of correlated astrophysical foregrounds by a second-order statistical approach
• Swift follow-up of gravitational wave triggers: results from the first aLIGO run and optimisation for the future
• Mapmaking for Precision 21 cm Cosmology
• Cosmological constraints from Subaru weak lensing cluster counts
• Gaia-like astrometry and gravitational waves
• Constraints on Primordial Non-Gaussianity from a Needlet Analysis of the WMAP-5 Data
• Anomalous CMB north-south asymmetry
• Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-Faint Dwarf Galaxy in the Constellation Pegasus
• Directional Sensitivity In Light-Mass Dark Matter Searches With Single-Electron Resolution Ionization Detectors
• Non-Gaussianity and large-scale structure in a two-field inflationary model
• 3D template-based $Fermi$-LAT constraints on the diffuse supernova axion-like particle background
• Optimising gravitational waves follow-up using galaxies stellar mass
• The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory
• The significance of anisotropic signals hiding in the type Ia supernovae
• Trapping of HII regions in Population III star formation
• On the signature of $z\sim 0.6$ superclusters and voids in the Integrated Sachs-Wolfe effect
• Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
• The axis of evil - a polarization perspective
• Mapping Incoherent Gravitational Wave Backgrounds
• A 3-D model of polarised dust emission in the Milky Way
• Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation
• Diffuse Emission of Galactic High-Energy Neutrinos from a Global Fit of Cosmic Rays
• Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA
• DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power Spectra
• New constraints on the Polarization of Anomalous Microwave Emission in nearby molecular clouds
• A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• Discovery of an Ultra-Faint Stellar System near the Magellanic Clouds with the DECam Local Volume Exploration (DELVE) Survey
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• Small-Scale Anisotropies of Cosmic Rays from Relative Diffusion
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Non-parametric modeling of the intra-cluster gas using APEX-SZ bolometer imaging data
• Fermi-LAT Observations of High- and Intermediate-Velocity Clouds: Tracing Cosmic Rays in the Halo of the Milky Way
• Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z=2.16 in the Cosmos field
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Cross-correlating the gamma-ray sky with catalogs of galaxy clusters
• The cosmic web of the Local Universe: cosmic variance, matter content and its relation to galaxy morphology
• Localisation of directional scale-discretised wavelets on the sphere
• Convolutional Neural Networks on the HEALPix sphere: a pixel-based algorithm and its application to CMB data analysis
• A Gaia early DR3 mock stellar catalog: Galactic prior and selection function
• Calcium H & K and sodium D absorption induced by the interstellar and circumgalactic media of the Milky Way
• The formation of secondary stellar generations in massive young star clusters from rapidly cooling shocked stellar winds
• The Connection between Supernova Remnants and the Galactic Magnetic Field: A Global Radio Study of the Axisymmetric Sample
• SWIPE: a bolometric polarimeter for the Large-Scale Polarization Explorer
• Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck
• Mapping UHECRs deflections through the turbulent galactic magnetic field with the latest RM data
• Improved Cosmic-Ray Injection Models and the Galactic Center Gamma-Ray Excess
• Constraining f(R) gravity with PLANCK data on galaxy cluster profiles
• Black hole obscuration and duty cycles mediated by AGN feedback in high redshift galaxies
• Evaluation of Automated Fermi GBM Localizations of Gamma-ray Bursts
• Machine-learning identification of galaxies in the WISExSuperCOSMOS all-sky catalogue
• Rapid Identification of Strongly Lensed Gravitational-Wave Events with Machine Learning
• IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
• The Gravitational Wave Treasure Map: A Tool to Coordinate, Visualize, and Assess the Electromagnetic Follow-Up of Gravitational Wave Events
• Joint analysis of the thermal Sunyaev-Zeldovich effect and 2MASS galaxies: Probing gas physics in the local Universe and beyond
• Anisotropies in the gamma-ray sky from millisecond pulsars
• Constraining Spinning Dust Parameters with the WMAP Five-Year Data
• Planck CMB Anomalies: Astrophysical and Cosmological Secondary Effects and the Curse of Masking
• The magnetic environment of the Orion-Eridanus superbubble as revealed by Planck
• Via Machinae: Searching for Stellar Streams using Unsupervised Machine Learning
• Observation of Anisotropy of TeV Cosmic Rays with Two Years of HAWC
• Is the CMB asymmetry due to the kinematic dipole?
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• The effect of aberration on partial-sky measurements of the cosmic microwave background temperature power spectrum
• The characteristic halo masses of half-a-million WISE-selected quasars
• Probing dark energy with steerable wavelets through correlation of WMAP and NVSS local morphological measures
• Creating mock catalogues of stellar haloes from cosmological simulations
• Statistical Measurement of the Gamma-ray Source-count Distribution as a Function of Energy
• Cosmic troublemakers: the Cold Spot, the Eridanus Supervoid, and the Great Walls
• A Search for Dark Matter Annihilation in the Milky Way Halo
• Secondary radiation from the Pamela/ATIC excess and relevance for Fermi
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies
• Cosmological constraints from the convergence 1-point probability distribution
• New estimates of the CMB angular power spectra from the WMAP 5 yrs low resolution data
• Constraints on the Polarization of the Anomalous Microwave Emission in the Perseus Molecular Complex from 7-year WMAP data
• A systematic study of the escape of LyC and Ly$\alpha$ photons from star-forming, magnetized turbulent clouds
• First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
• Redshift inference from the combination of galaxy colors and clustering in a hierarchical Bayesian model $-$ Application to realistic $N$-body simulations
• Modelling and simulation of large-scale polarized dust emission over the southern Galactic cap using the GASS HI data
• The part and the whole: voids, supervoids, and their ISW imprint
• Filling in CMB map missing data using constrained Gaussian realizations
• Likelihood methods for the combined analysis of CMB temperature and polarisation power spectra
• Clues on void evolution III: Structure and dynamics in void shells
• Diffuse Neutrino and Gamma-ray Emissions of the Galaxy above the TeV
• Constraints on f_nl and g_nl from the analysis of the N-pdf of the CMB large scale anisotropies
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys
• What can be learned from the lensed cosmic microwave background B-mode polarization power spectrum?
• Searching for a dipole modulation in the large-scale structure of the Universe
• Anisotropy in the all-sky distribution of galaxy morphological types
• Covariance of CMB anomalies
• Directional detection of dark matter streams
• Mitigating Complex Dust Foregrounds in Future CMB Polarization Experiments
• The Accuracy of Weak Lensing Simulations
• Optical Cluster-Finding with An Adaptive Matched-Filter Technique: Algorithm and Comparison with Simulations
• A neural simulation-based inference approach for characterizing the Galactic Center $\gamma$-ray excess
• Hybrid Adaptive Ray-Moment Method (HARM${}^2$): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids
• Fermi/LAT discovery of gamma-ray emission from the flat-spectrum radio quasar PKS 1454-354
• Euclid preparation: XVI. Exploring the ultra low-surface brightness Universe with Euclid/VIS
• Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
• Optimized Beam Sculpting with Generalized Fringe-Rate Filters
• Clustering of photometric luminous red galaxies I : Growth of Structure and Baryon Acoustic Feature
• Galaxy Counts on the CMB Cold Spot
• Channeling in direct dark matter detection II: channeling fraction in Si and Ge crystals
• Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys
• Bayesian Model Comparison and Analysis of the Galactic Disk Population of Gamma-Ray Millisecond Pulsars
• Fast generation of ensembles of cosmological N-body simulations via mode-resampling
• Anomalous variance in the WMAP data and Galactic Foreground residuals
• Monte Carlo modelling of the propagation and annihilation of nucleosynthesis positrons in the Galaxy
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Unbiased methods for removing systematics from galaxy clustering measurements
• Dark Energy Survey Year 3 results: Magnification modeling and impact on cosmological constraints from galaxy clustering and galaxy-galaxy lensing
• 3DEX: a code for fast spherical Fourier-Bessel decomposition of 3D surveys
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• Matched filter optimization of kSZ measurements with a reconstructed cosmological flow field
• Gaia Data Release 3 Validating the classification of variable Young Stellar Object candidates
• Aberrating the CMB sky: fast and accurate computation of the aberration kernel
• Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect
• Improved constraints on primordial non-Gaussianity for the Wilkinson Microwave Anisotropy Probe 5-yr data
• Testing Isotropy in the Local Universe
• A Technique for Primary Beam Calibration of Drift-Scanning, Wide-Field Antenna Elements
• The Simons Observatory: Constraining inflationary gravitational waves with multi-tracer B-mode delensing
• Fast and Exact Spin-s Spherical Harmonic Transforms
• TORUS-3DPDR: A self-consistent code treating three-dimensional photoionization and photodissociation regions
• Constraints on direction-dependent cosmic birefringence from Planck polarization data
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Separating E and B types of polarization on an incomplete sky
• The integrated 3-point correlation function of cosmic shear
• Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background
• SKA Weak Lensing II: Simulated Performance and Survey Design Considerations
• Fast Radio Burst dispersion measures and rotation measures and the origin of intergalactic magnetic fields
• Gaia Data Release 2: Rotational modulation in late-type dwarfs
• The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey footprint. III. The South Galactic Cap Sample and the Quasar Luminosity Function at Cosmic Noon
• Detectability of tensor modes in the presence of foregrounds
• Unbiased pseudo-Cl power spectrum estimation with mode projection
• Destriping CMB temperature and polarization maps
• The Extremely Luminous Quasar Survey (ELQS) in the SDSS footprint I.: Infrared Based Candidate Selection
• Optically thick HI does not dominate dark gas in the local ISM
• Angular power spectrum of galaxies in the 2MASS Redshift Survey
• Model-independent analyses of non-Gaussianity in Planck CMB maps using Minkowski Functionals
• Maps of the Southern Millimeter-wave Sky from Combined 2500 deg${}^2$ SPT-SZ and Planck Temperature Data
• Milky Way Satellites Shining Bright in Gravitational Waves
• The geometry of the magnetic field in the Central Molecular Zone measured by PILOT
• The cut-sky cosmic microwave background is not anomalous
• Weak-lensing observables in relativistic N-body simulations
• Synthetic observations of star formation and the interstellar medium
• The polarization in the JVAS/CLASS flat-spectrum radio sources: II. A search for aligned radio polarizations
• Constraints on the topology of the Universe derived from the 7-year WMAP data
• Bayesian component separation and CMB estimation for the 5-year WMAP temperature data
• A fast particle-mesh simulation of non-linear cosmological structure formation with massive neutrinos
• Revisiting the WMAP - NVSS angular cross correlation. A skeptic's view
• Subtraction of point sources from interferometric radio images through an algebraic forward modeling scheme
• Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data
• Statistical description of dust polarized emission from the diffuse interstellar medium -- A RWST approach
• The cosmic radio dipole: Bayesian estimators on new and old radio surveys
• Accurate Analytic Model for the Weak Lensing Convergence One-Point Probability Distribution Function and its Auto-Covariance
• First Detection of the BAO Signal from Early DESI Data
• The roles of stellar feedback and galactic environment in star forming molecular clouds
• The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
• Improved limits on a stochastic gravitational-wave background and its anisotropies from Advanced LIGO O1 and O2 runs
• Testing a direction-dependent primordial power spectrum with observations of the Cosmic Microwave Background
• New 145-MHz Source Measurements by PAPER in the Southern Sky
• A minimal power-spectrum-based moment expansion for CMB B-mode searches
• Searching the Gamma-ray Sky for Counterparts to Gravitational Wave Sources: Fermi GBM and LAT Observations of LVT151012 and GW151226
• The joint large-scale foreground-CMB posteriors of the 3-year WMAP data
• HI, CO, and Dust in the Perseus Cloud
• Power Asymmetries in the Cosmic Microwave Background Temperature and Polarization patterns
• Search for Very High Energy Gamma Rays from the Northern $\text{Fermi}$ Bubble Region with HAWC
• Evidence of a truncated spectrum in the angular correlation function of the cosmic microwave background
• Explaining the GeV antiproton/$\gamma -$ray excesses and W-boson mass anomaly in an inert two Higgs doublet model
• TEASING: a fast and accurate approximation for the low multipole likelihood of the Cosmic Microwave Background temperature
• Foreground removal for Square Kilometre Array observations of the Epoch of Reionization with the Correlated Component Analysis
• MAXI investigation into the longterm X-ray variability from the very-high-energy gamma-ray blazar Mrk 421
• Can Ground-based Telescopes Detect The Oxygen 1.27 Micron Absorption Feature as a Biomarker in Exoplanets ?
• Orbital anisotropy in cosmological haloes revisited
• Constraints on Large-Scale Magnetic Fields in the Intergalactic Medium Using Cross-Correlation Methods
• WMAP 5-year constraints on fnl with wavelets
• Non-Gaussianity detections in the Bianchi VIIh corrected WMAP 1-year data made with directional spherical wavelets
• Diffuse Ionized Gas in Simulations of Multiphase, Star-Forming Galactic Disks
• Imaging Systematics and Clustering of DESI Main Targets
• Radiative transfer meets Bayesian statistics: where does a galaxy's [CII] emission come from?
• Estimates of Fast Radio Burst Dispersion Measures from Cosmological Simulations
• Directional dependence of CMB parity asymmetry
• Ring-like features in directional dark matter detection
• Reconstruction of high-resolution SZ maps from heterogeneous datasets using needlets
• The Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Errors due to pixelization of the CMB sky
• Loops and spurs: The angular power spectrum of the Galactic synchrotron background
• Euclid: Early Release Observations -- Dwarf galaxies in the Perseus galaxy cluster
• The Atacama Cosmology Telescope: Calibration with WMAP Using Cross-Correlations
• Impact of Galactic polarized emission on B-mode detection at low multipoles
• A Galaxy Model from 2MASS Star Counts in the Whole Sky Including the Plane
• Large-Angle CMB Suppression and Polarization Predictions
• Very fast stochastic gravitational wave background map making using folded data
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• Coincident detection significance in multimessenger astronomy
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• Microwave-Sky Simulations and Projections for Galaxy Cluster Detection with the Atacama Cosmology Telescope
• Combining radiative transfer and diffuse interstellar medium physics to model star formation
• CMB-S4: Iterative Internal Delensing and $r$ Constraints
• Searching for the continuum spectrum photons correlated to the 130 GeV gamma-ray line
• The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
• Angular clustering properties of the DESI QSO target selection using DR9 Legacy Imaging Surveys
• PARSEC: A Parametrized Simulation Engine for Ultra-High Energy Cosmic Ray Protons
• The Pan-STARRS1 $\mathbf{z}>5.6$ Quasar Survey: III. The $\mathbf{z}\approx 6$ Quasar Luminosity Function
• Simulating full-sky interferometric observations
• Signals of Statistical Anisotropy in WMAP Foreground-Cleaned Maps
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• Completeness of the Gaia-verse I: when and where were Gaia's eyes on the sky during DR2?
• Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz
• Lensing reconstruction from PLANCK sky maps: inhomogeneous noise
• Probing the Local Velocity Distribution of WIMP Dark Matter with Directional Detectors
• The Statistical Significance of the "Dark Flow"
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• Comparison of map-making algorithms for CMB experiments
• The bispectrum of polarized galactic foregrounds
• RascalC: A Jackknife Approach to Estimating Single and Multi-Tracer Galaxy Covariance Matrices
• In situ measurement of MWA primary beam variation using ORBCOMM
• Improved cosmic microwave background (de-)lensing using general spherical harmonic transforms
• A Scaling Index Analysis of the WMAP three year data: Signatures of non-Gaussianities and Asymmetries in the CMB
• 3D Dust Mapping Reveals that Orion Forms Part of a Large Ring of Dust
• GMOSS: All-sky model of spectral radio brightness based on physical components and associated radiative processes
• Deflections of UHECRs in the Galactic magnetic field
• Predictions of the LSST Solar System Yield: Near-Earth Objects, Main Belt Asteroids, Jupiter Trojans, and Trans-Neptunian Objects
• The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH)
• Simulations of the Pairwise Kinematic Sunyaev-Zel'dovich Signal
• Powellsnakes II: a fast Bayesian approach to discrete object detection in multi-frequency astronomical data sets
• Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
• Erasing the variable: Empirical foreground discovery for global 21 cm spectrum experiments
• Demonstration of magnetic field tomography with starlight polarization towards a diffuse sightline of the ISM
• The isotropic radio background revisited
• Can a primordial magnetic field originate large-scale anomalies in WMAP data?
• Cosmic-ray interactions with the Sun using the FLUKA code
• Magnetostriction in magnetic gels and elastomers as a function of the internal structure and particle distribution
• Complex data processing: fast wavelet analysis on the sphere
• HI filaments are cold and associated with dark molecular gas. HI4PI based estimates of the local diffuse CO-dark H2 distribution
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• The stellar content of the ROSAT all-sky survey
• Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies
• The galaxy cluster Ysz-Lx and Ysz-M relations from the WMAP 5-yr data
• Deriving the contribution of blazars to the Fermi-LAT Extragalactic $\gamma$-ray background at $E>10$ GeV with efficiency corrections and photon statistics
• The Power Spectra of Polarized, Dusty Filaments
• A Markov Chain Monte Carlo Algorithm for analysis of low signal-to-noise CMB data
• Isotropy of low redshift type Ia Supernovae: A Bayesian analysis
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• WMAP 7 year constraints on CPT violation from large angle CMB anisotropies
• A model-independent test for scale-dependent non-Gaussianities in the CMB
• Modeling the Atomic-to-Molecular Transition and Chemical Distributions of Turbulent Star-Forming Clouds
• Planck 2018 constraints on anisotropic birefringence and its cross-correlation with CMB anisotropy
• Production of secondary particles and nuclei in cosmic rays collisions with the interstellar gas using the FLUKA code
• Large-scale anomalies in the cosmic microwave background as signatures of non-Gaussianity
• Cosmic Shear: Inference from Forward Models
• Detecting a Stochastic Gravitational-Wave Background: The Overlap Reduction Function
• Comparison between hemisphere comparison method and dipole-fitting method in tracing the anisotropic expansion of the Universe use the Union2 dataset
• Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster
• Point-Source Power in 3 Year Wilkinson Microwave Anisotropy Probe Data
• Planck intermediate results. XXXIV. The magnetic field structure in the Rosette Nebula
• Building the Evryscope: Hardware Design and Performance
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• Insights into searches for anisotropies in the nanohertz gravitational-wave background
• Extragalactic Point Source Search in Five-year WMAP 41, 61 and 94 GHz Maps
• The NANOGrav 12.5-year Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries
• The Application of the Montage Image Mosaic Engine To The Visualization Of Astronomical Images
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• A comparison of cosmological filaments catalogues
• Star-galaxy classification in the Dark Energy Survey Y1 dataset
• Dissecting the inner Galaxy with $\gamma$-ray pixel count statistics
• Unraveling the origin of magnetic fields in galaxies
• A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
• Cross-correlation of the thermal Sunyaev-Zel'dovich effect and weak gravitational lensing: Planck and Subaru Hyper Suprime-Cam first-year data
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Large angular scale multipoles at redshift ~0.8
• Extreme Starlight Polarization in a Region with Highly Polarized Dust Emission
• A multi-band map of the natural night sky brightness including Gaia and Hipparcos integrated starlight
• The Galactic dynamics revealed by the filamentary structure in atomic hydrogen emission
• Polarization as an indicator of intrinsic alignment in radio weak lensing
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• Revisiting the distance to radio Loops I and IV using Gaia and radio/optical polarization data
• Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
• Unresolved Gamma-Ray Sky through its Angular Power Spectrum
• The first catalog of Fermi-LAT sources below 100 MeV
• Comparison of absolute gain photometric calibration between Planck/HFI and Herschel/SPIRE at 545 and 857 GHz
• Planck intermediate results. XLII. Large-scale Galactic magnetic fields
• Parametrizations of the global 21-cm signal and parameter estimation from single-dipole experiments
• Integrated approach to cosmology: Combining CMB, large-scale structure and weak lensing
• Timing, polarimetry and physics of the bright, nearby millisecond pulsar PSR J0437-4715 - a single-pulse perspective
• Modeling the Radio Foreground for detection of CMB spectral distortions from Cosmic Dawn and Epoch of Reionization
• KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
• First constraints on the running of non-Gaussianity
• COSMOSOMAS Observations of the CMB and Galactic Foregrounds at 11 GHz: Evidence for anomalous microwave emission at high Galactic Latitude
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• CMB E/B decomposition of incomplete sky: a pixel space approach
• Correcting for Fibre Assignment Incompleteness in the DESI Bright Galaxy Survey
• On the proper kinetic quadrupole CMB removal and the quadrupole anomalies
• Maximum likelihood, parametric component separation and CMB B-mode detection in suborbital experiments
• A search for point sources of EeV photons
• QuickPol: Fast calculation of effective beam matrices for CMB polarization
• Percent-Level Test of Isotropic Expansion Using Type Ia Supernovae
• Ruprecht 147 DANCe I. Members, empirical isochrone, luminosity and mass distributions
• CMB constraint on non-Gaussianity in isocurvature perturbations
• Tomographic analyses of the CMB lensing and galaxy clustering to probe the linear structure growth
• BeyondPlanck III. Commander3
• Testing the standard model of cosmology with the SKA: the cosmic radio dipole
• Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach
• Extracting the cold neutral medium from HI emission with deep learning: Implications for Galactic foregrounds at high latitude
• Dusting off the diffuse interstellar bands: DIBs and dust in extragalactic SDSS spectra
• Non-Gaussianity in the WMAP data using the peak-peak correlation function
• Impact of Polarized Galactic Foreground Emission on CMB Lensing Reconstruction and Delensing of B-Modes
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• IceCube search for neutrinos coincident with gravitational wave events from LIGO/Virgo run O3
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: I. Construction of all-sky thermal and kinetic SZ-maps
• Simulating the Galactic Multi-messenger Emissions with HERMES
• Searches for sterile neutrinos and axionlike particles from the Galactic halo with eROSITA
• Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman-$\alpha$ forest
• Searching for anisotropy in the distribution of binary black hole mergers
• Sky reconstruction from transit visibilities: PAON-4 and Tianlai Dish Array
• CMB reconstruction from the WMAP and Planck PR2 data
• Constraining the evolution of the CMB temperature with SZ measurements from Planck data
• Forming Super-Massive Black Hole Seeds under the Influence of a Nearby Anisotropic Multi-Frequency Source
• Instrumental and Analytic Methods for Bolometric Polarimetry
• Long-term variability of extragalactic radio sources in the Planck Early Release Compact Source Catalogue
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Magnification bias in galaxy surveys with complex sample selection functions
• Directional Variations of the Non-Gaussianity Parameter f_NL
• The Formation of Rapidly Rotating Black Holes in High Mass X-ray Binaries
• Searching for axion-like particles through CMB birefringence from string-wall networks
• The selection function of the RAVE survey
• Stochastic gravitational wave background: methods and Implications
• Polarization in Monte Carlo radiative transfer and dust scattering polarization signatures of spiral galaxies
• Search for TeV Gamma-Ray Emission from Point-like Sources in the Inner Galactic Plane with a Partial Configuration of the HAWC Observatory
• Spider Optimization: Probing the Systematics of a Large Scale B-Mode Experiment
• Earth as an Exoplanet: A Two-dimensional Alien Map
• No evidence for the cold spot in the NVSS radio survey
• Super-sample covariance approximations and partial sky coverage
• Shock and Splash: Gas and Dark Matter Halo Boundaries around LambdaCDM Galaxy Clusters
• Properties and use of CMB power spectrum likelihoods
• Correlating high-energy IceCube neutrinos with 5BZCAT blazars and RFC sources
• All-sky, all-frequency directional search for persistent gravitational-waves from Advanced LIGO's and Advanced Virgo's first three observing runs
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• ISW Imprint of Superstructures on Linear Scales
• Large scale anisotropy due to pre-inflationary phase of cosmic evolution
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Observational Constraints on Planet Nine: Cassini Range Observations
• Cross-correlation of weak lensing and gamma rays: implications for the nature of dark matter
• Search for Gravitational Waves in the CMB After WMAP3: Foreground Confusion and The Optimal Frequency Coverage for Foreground Minimization
• Direct collapse to supermassive black hole seeds: the critical conditions for suppression of ${\mathrm{H}}_2$ cooling
• Making Maps from Planck LFI 30GHz Data
• Detection of Quasar Feedback from the Thermal Sunyaev-Zel'dovich Effect in Planck
• Cleaning the USNO-B Catalog through automatic detection of optical artifacts
• The Diffuse Galactic Far-Ultraviolet Sky
• The POlarised GLEAM Survey (POGS) II: Results from an All-Sky Rotation Measure Synthesis Survey at Long Wavelengths
• Comparing Planck and WMAP: Maps, Spectra, and Parameters
• Did WMAP see Moving Local Structures?
• Persistent Homology and Non-Gaussianity
• The Long Wavelength Array Software Library
• Constraints on dark matter annihilations from diffuse gamma-ray emission in the Galaxy
• exocartographer: A Bayesian Framework for Mapping Exoplanets in Reflected Light
• Direct detection of the kinetic Sunyaev-Zel'dovich effect in galaxy clusters
• Putting Things Back Where They Belong: Tracing Cosmic-Ray Injection with H2
• Constraining primordial non-Gaussianity from DESI quasar targets and Planck CMB lensing
• Planck intermediate results. LIV. The Planck Multi-frequency Catalogue of Non-thermal Sources
• Identifying RR Lyrae Variable Stars in Six Years of the Dark Energy Survey
• Constraints on dark matter models from a Fermi LAT search for high-energy cosmic-ray electrons from the Sun
• The Angular Power Spectra of Photometric SDSS LRGs
• Patterns of primary beam non-redundancy in close-packed 21 cm array observations
• Kolmogorov cosmic microwave background sky
• Finding Quasars behind the Galactic Plane. I. Candidate Selections with Transfer Learning
• A Synthetic Roman Space Telescope High-Latitude Imaging Survey: Simulation Suite and the Impact of Wavefront Errors on Weak Gravitational Lensing
• Unidentified Gamma-ray Sources as Targets for Indirect Dark Matter Detection with the Fermi-Large Area Telescope
• Characterizing the Gravitational Wave Signature from Cosmic String Cusps
• Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey
• Multi-wavelength characterisation of z~2 clustered, dusty star forming galaxies discovered by Planck
• Polarization of the WMAP Point Sources
• Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
• CMB Faraday rotation as seen through the Milky Way
• Luminosity distance and anisotropic sky-sampling at low redshifts: a numerical relativity study
• Characterizing bias on large scale CMB $B$-modes after galactic foregrounds cleaning
• A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment's Sample-Variance Limited E-Mode Measurement
• The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center
• C-Band All-Sky Survey: A First Look at the Galaxy
• A test of the Poincare dodecahedral space topology hypothesis with the WMAP CMB data
• Probing cosmological isotropy with Planck Sunyaev-Zeldovich galaxy clusters
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data
• Simulated forecasts for primordial B-mode searches in ground-based experiments
• Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory
• Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey
• Harmonic space analysis of pulsar timing array redshift maps
• Cross-correlating radio continuum surveys and CMB lensing: constraining redshift distributions, galaxy bias and cosmology
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• Frequency Modulation of Directly Imaged Exoplanets: Geometric Effect as a Probe of Planetary Obliquity
• Polarized anisotropic spectral distortions of the CMB: Galactic and extragalactic constraints on photon-axion conversion
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• First detection of a virial shock with SZ data: implication for the mass accretion rate of Abell 2319
• Detecting the polarization induced by scattering of the microwave background quadrupole in galaxy clusters
• ICE-COLA: fast simulations for weak lensing observables
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• Abundance anomalies in metal-poor stars from Population III supernova ejecta hydrodynamics
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• Weak lensing magnification in the Dark Energy Survey Science Verification Data
• Mapping the relativistic electron gas temperature across the sky
• The dipole anisotropy of AllWISE galaxies
• A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 AU New Horizons-LORRI Data
• Two-point Correlation Function of WMAP 9 year data
• To the center of cold spot with Planck
• The WaZP galaxy cluster sample of the Dark Energy Survey Year 1
• Testing cosmic anisotropy with Pantheon sample and quasars at high redshifts
• Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments
• Temperature Fluctuations of the Cosmic Microwave Background Radiation: A Case of Nonextensivity?
• Using inpainting to construct accurate cut-sky CMB estimators
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• Anisotropic universe with anisotropic sources
• Allsky NICER and NICEST extinction maps based on the 2MASS near-infrared survey
• Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost
• Multiview Deep Learning for Predicting Twitter Users' Location
• Local primordial non-Gaussianity from the large-scale clustering of photometric DESI luminous red galaxies
• Impact of calibration errors on CMB component separation using FastICA and ILC
• Constraining the redshift evolution of the Cosmic Microwave Background black-body temperature with PLANCK data
• ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• First HAWC Observations of the Sun Constrain Steady TeV Gamma-Ray Emission
• Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II
• Establishing the X-ray Source Detection Strategy for eROSITA with Simulations
• Correlations in the (Sub)millimeter background from ACTxBLAST
• The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
• Bayesian analysis of the low-resolution polarized 3-year WMAP sky maps
• Is there evidence for anomalous dipole anisotropy in the large-scale structure?
• The SDSS-III Baryonic Oscillation Spectroscopic Survey: Constraints on the Integrated Sachs Wolfe effect
• Matrix-free Large Scale Bayesian inference in cosmology
• A search for concentric circles in the 7-year WMAP temperature sky maps
• Antenna beam characterisation for the global 21cm experiment LEDA and its impact on signal model parameter reconstruction
• NPTFit: A code package for Non-Poissonian Template Fitting
• Planck constraints on cross-correlations between anisotropic cosmic birefringence and CMB polarization
• Eliminating Primary Beam Effect in Foreground Subtraction of Neutral Hydrogen Intensity Mapping Survey with Deep Learning
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• Alignments of parity even/odd-only multipoles in CMB
• Magnetic Deflections of Ultra-High Energy Cosmic Rays from Centaurus A
• Mapping the Integrated Sachs-Wolfe Effect
• The BINGO Project II: Instrument Description
• Local variance asymmetries in Planck temperature anisotropy maps
• Polarized Sunyaev Zel'dovich tomography
• A Compton thick AGN in the barred spiral NGC 4785
• Predictions of polarized dust emission from interstellar clouds: spatial variations in the efficiency of radiative torque alignment
• First Data Release of the All-sky NOAO Source Catalog
• Clustering and Bias Measurements of SDSS Voids
• Combining ILC and moment expansion techniques for extracting average-sky signals and CMB anisotropies
• Characterisation of the non-Gaussianity of radio and IR point-sources at CMB frequencies
• Kolmogorov stochasticity parameter measuring the randomness in Cosmic Microwave Background
• Daily modulation due to channeling in direct dark matter crystalline detectors
• The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
• Identification of Spinning Dust in Halpha-Correlated Microwave Emission
• Search for anomalous alignments of structures in Planck data using Minkowski Tensors
• Lunar Orbit Measurement of Cosmic Dawn 21 cm Global Spectrum
• Mid-Infrared Properties of Disk Averaged Observations of Earth with AIRS
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• Optimal constraint on g_NL from CMB
• Large Covariance Matrices: Accurate Models Without Mocks
• From supernova to supernova remnant: comparison of thermonuclear explosion models
• DESI Early Data Release Milky Way Survey Value-Added Catalogue
• Towards automatic classification of all WISE sources
• On the Amplitude and Stokes Parameters of a Stochastic Gravitational-Wave Background
• Second-Generation Curvelets on the Sphere
• Reconstructing signals from noisy data with unknown signal and noise covariance
• The TeV Sun Rises: Discovery of Gamma rays from the Quiescent Sun with HAWC
• Constraining the Galactic millisecond pulsar population using Fermi Large Area Telescope
• The 37-month MAXI/GSC source catalog in the high Galactic-latitude sky
• Non-Equilibrium Chemistry and Destruction of CO by X-ray Flares
• Analyzing the cosmic variance limit of remote dipole measurements of the cosmic microwave background using the large-scale kinetic Sunyaev Zel'dovich effect
• Statistical challenges in the analysis of Cosmic Microwave Background radiation
• KiDS-1000 cosmology: Combined second- and third-order shear statistics
• Optimal filters for detecting cosmic bubble collisions
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• A Model-independent Test of Cosmic Isotropy with Low-z Pantheon Supernovae
• Bayesian Limits on Primordial Isotropy Breaking
• No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution
• Foreground Analysis Using Cross-Correlations of External Templates on the 7-year WMAP data
• Dim but not entirely dark: Extracting the Galactic Center Excess' source-count distribution with neural nets
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• The Sunyaev-Zel'dovich effect in WMAP data
• Completeness of the Gaia-verse IV: The Astrometry Spread Function of Gaia DR2
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• An optimal method for scheduling observations of large sky error regions for finding optical counterparts to transients
• Gravitational redshift and asymmetric redshift-space distortions for stacked clusters
• Libpsht - algorithms for efficient spherical harmonic transforms
• Hard and bright gamma-ray emission at the base of the Fermi bubbles
• Tensor Minkowski Functionals: first application to the CMB
• Probing magnetic helicity with synchrotron radiation and Faraday rotation
• A high-level analysis framework for HAWC
• Likelihood methods for CMB experiments
• Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
• Directional dependence of LCDM cosmological parameters
• Measurement of the high-energy gamma-ray emission from the Moon with the Fermi Large Area Telescope
• Constraining Polarized Foregrounds for EOR Experiments II: Polarization Leakage Simulations in the Avoidance Scheme
• Galactic foregrounds: Spatial fluctuations and a procedure of removal
• Map-making in small field modulated CMB polarisation experiments: approximating the maximum-likelihood method
• Revisiting dynamical friction: the role of global modes and local wakes
• Cosmic microwave background multipole alignments in slab topologies
• Urchin: A Reverse Ray Tracer for Astrophysical Applications
• The Topology and Size of the Universe from CMB Temperature and Polarization Data
• The effect of photoionising feedback on star formation in isolated and colliding clouds
• Poisson Denoising on the Sphere: Application to the Fermi Gamma Ray Space Telescope
• Spherical 3D Isotropic Wavelets
• A novel approach for accurate radiative transfer in cosmological hydrodynamic simulations
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• The multipole expansion of the local expansion rate
• When disorder looks like order: a new model to explain radial magnetic fields in young supernova remnants
• The distinct stellar metallicity populations of simulated Local Group dwarfs
• The Simons Observatory: Galactic Science Goals and Forecasts
• Polycyclic Aromatic Hydrocarbons, the Anomalous Microwave Emission, and Their Connection to the Cold Neutral Medium
• All sky CMB map from cosmic strings integrated Sachs-Wolfe effect
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
• The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
• Brute-Force Mapmaking with Compact Interferometers: A MITEoR Northern Sky Map from 128 MHz to 175 MHz
• Stacked CMB lensing and ISW signals around superstructures in the DESI Legacy Survey
• What can be learnt from UHECR anisotropies observations? Paper I : large-scale anisotropies and composition features
• Hemispherical power asymmetries in the WMAP 7-year low-resolution temperature and polarization maps
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• A $f(R)$-gravity model of the Sunyaev-Zeldovich profile of the Coma cluster compatible with {\it Planck} data
• Local Bubble contribution to the 353-GHz dust polarized emission
• CMB map derived from the WMAP data through Harmonic Internal Linear Combination
• Lensing reconstruction from a patchwork of polarization maps
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys IV: Characterizing Density and Pressure Clumping due to Infalling Substructures
• Magritte, a modern software library for 3D radiative transfer: I. Non-LTE atomic and molecular line modelling
• Wavemoth -- Fast spherical harmonic transforms by butterfly matrix compression
• Component separation with flexible models. Application to the separation of astrophysical emissions
• The Simons Observatory: pipeline comparison and validation for large-scale B-modes
• Intensity Mapping in the Presence of Foregrounds and Correlated Continuum Emission
• All-sky census of Galactic high-latitude molecular intermediate-velocity clouds
• On the computation of directional scale-discretized wavelet transforms on the sphere
• Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models
• Fermi GBM GRBs with characteristics similar to GRB 170817A
• Data challenges of time domain astronomy
• OSLO: On-the-Sphere Learning for Omnidirectional images and its application to 360-degree image compression
• CMB signal in WMAP 3yr data with FastICA
• Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments
• HI anisotropies associated with radio-polarimetric filaments. Steep power spectra associated with cold gas
• The First MAXI/GSC Catalog in the High Galactic-Latitude Sky
• A map-based method for eliminating systematic modes from galaxy clustering power spectra with application to BOSS
• Bayesian analysis of anisotropic cosmologies: Bianchi VII_h and WMAP
• Methods for pixel domain correction of EB leakage
• The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access
• Large scale alignment anomalies of CMB anisotropies: a new test for residuals applied to WMAP 5yr maps
• PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
• Quantifying Excess Power from Radio Frequency Interference in Epoch of Reionization Measurements
• Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamics Simulations
• The Second AGILE Catalog of Gamma-Ray Sources
• The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA
• First observational constraints on tensor non-Gaussianity sourced by primordial magnetic fields from cosmic microwave background
• Reconstructing Small Scale Lenses from the Cosmic Microwave Background Temperature Fluctuations
• Bayesian estimation of our local motion from the Planck-2018 CMB temperature map
• Polarized accretion shocks from the cosmic web
• The Topology and Size of the Universe from the Cosmic Microwave Background
• Cosmic Ray Small Scale Anisotropies and Local Turbulent Magnetic Fields
• Mapping the anisotropic Galactic stellar halo with Blue Horizontal Branch stars
• The Extremely Luminous Quasar Survey in the Pan-STARRS 1 Footprint (PS-ELQS)
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• The Atacama Cosmology Telescope: Detection of mm-wave transient sources
• The demographics of obscured AGN from X-ray spectroscopy guided by multiwavelength information
• Power spectrum modelling of galaxy and radio intensity maps including observational effects
• Optimal filters on the sphere
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Large scale directional anomalies in the WMAP 5yr ILC map
• Dust moments: towards a new modelling of the galactic dust emission for CMB B-modes analysis
• How to make a clean separation between CMB E and B modes with proper foreground masking
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Quadratic estimator for CMB cross-correlation
• Far-ultraviolet fluorescent molecular hydrogen emission map of the Milky Way Galaxy
• Non-Gaussianity analysis on local morphological measures of WMAP data
• On the large-scale angular distribution of short-Gamma ray bursts
• Introducing Mexican needlets for CMB analysis: Issues for practical applications and comparison with standard needlets
• Anisotropy expectations for ultra-high-energy cosmic rays with future high statistics experiments
• Extracting foreground-obscured $\mu$-distortion anisotropies to constrain primordial non-Gaussianity
• A spatial correlation analysis for a toroidal universe
• CMB polarization map derived from the WMAP 5 year data through Harmonic Internal Linear Combination
• Foreground Separation and Constraints on Primordial Gravitational Waves with the PICO Space Mission
• On the linear term correction for needlets/wavelets non-Gaussianity estimators
• Minkowski Functionals of SDSS-III BOSS : Hints of Possible Anisotropy in the Density Field?
• The RapidXMM Upper Limit Server: X-ray aperture photometry of the XMM-Newton archival observations
• Exploring Cosmic Origins with CORE: Cluster Science
• Lensed CMB temperature and polarization maps from the Millennium Simulation
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Deviation from Gaussianity in the cosmic microwave background temperature fluctuations
• Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era
• B-mode Detection with an Extended Planck Mission
• Directional spin wavelets on the sphere
• Can we detect Hot or Cold spots in the CMB with Minkowski Functionals?
• Observational Constraints on Planet Nine: Astrometry of Pluto and Other Trans-Neptunian Objects
• ForSE: a GAN based algorithm for extending CMB foreground models to sub-degree angular scales
• Iterative destriping and photometric calibration for Planck-HFI, polarized, multi-detector map-making
• An all-sky 3D dust map Based on Gaia and LAMOST
• Stochastic gravitational wave background constraints from Gaia DR3 astrometry
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• A new approach to determine optically thick H2 cooling and its effect on primordial star formation
• Lost Horizon: Quantifying the Effect of Local Topography on Global 21-cm Cosmology Data Analysis
• Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations
• Simulating the atomic and molecular content of molecular clouds using probability distributions of physical parameters
• LOC program for line radiative transfer
• INTEGRAL IBIS, SPI, and JEM-X observations of LVT151012
• Phase-coherent mapping of gravitational-wave backgrounds using ground-based laser interferometers
• Simulations of Galactic polarized synchrotron emission for Epoch of Reionization observations
• J-GEM Follow-Up Observations of The Gravitational Wave Source GW151226
• De-blending Deep Herschel Surveys: A Multi-wavelength Approach
• Testing LSST Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics
• J-GEM Follow-Up Observations to Search for an Optical Counterpart of The First Gravitational Wave Source GW150914
• TRIS III: the diffuse galactic radio emission at $\delta =+42^{\circ }$
• Search for primordial non-Gaussianity in the quasars of SDSS-III BOSS DR9
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• Millimeter and Submillimeter Excess Emission in M33 revealed by Planck and LABOCA
• The thermal Sunyaev-Zel'dovich Signature of Baryons in the Local Universe
• Circular polarization of the CMB: Foregrounds and detection prospects
• Detection of virial shocks in stacked Fermi-LAT clusters
• Reconstructing continuous distributions of 3D protein structure from cryo-EM images
• Constraints on the non-linear coupling parameter fnl with the Archeops data
• A novel multi-frequency technique for the detection of point sources in Cosmic Microwave Background maps
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• Random spherical hyperbolic diffusion
• Constraining spatial variations of the fine structure constant using clusters of galaxies and Planck data
• Validation of the HERA Phase I Epoch of Reionization 21 cm Power Spectrum Software Pipeline
• Void profile from Planck lensing potential map
• Direction dependence of the power spectrum and its effect on the Cosmic Microwave Background Radiation
• Spectral index of the Galactic foreground emission in the 50-87 MHz range
• GLASS: Generator for Large Scale Structure
• Synthetic Observations of 21cm HI Line Profiles from Inhomogeneous Turbulent Interstellar HI Gas with Magnetic Field
• The Nuclear Window to the Extragalactic Universe
• Planck intermediate results. XLIX. Parity-violation constraints from polarization data
• Anisotropies in the Diffuse Gamma-Ray Background from Dark Matter with Fermi LAT: a closer look
• Weak lensing peak statistics in the era of large scale cosmological surveys
• One-point fluctuation analysis of the high-energy neutrino sky
• Planck intermediate results. XXXVIII. E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium
• Planck's confirmation of the M31 disk and halo rotation
• Fast Generation of Covariance Matrices for Weak Lensing
• Micrometeoroid Events in LISA Pathfinder
• Precision Pointing of IBEX-Lo Observations
• Non-Gaussian Signatures in the five-year WMAP data as identified with isotropic scaling indices
• A faint halo star cluster discovered in the Blanco Imaging of the Southern Sky Survey
• Testing gamma-ray models of blazars in the extragalactic sky
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data
• Measuring cosmic magnetic fields by rotation measure-galaxy cross-correlations in cosmological simulations
• CMB lensing and primordial squeezed non-Gaussianity
• Producing a BOSS-CMASS sample with DES imaging
• A new approach for the statistical denoising of Planck interstellar dust polarization data
• Multifrequency radiation hydrodynamics simulations of H2 line emission in primordial, star-forming clouds
• DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Testing the Dipole Modulation Model in CMBR
• The study of topology of the universe using multipole vectors
• A Two-Point Correlation Function For Galactic Halo Stars
• Parity in the CMB: Space Oddity
• Instability of reconstruction of the low CMB multipoles
• Wavelet-Bayesian inference of cosmic strings embedded in the cosmic microwave background
• Cosmological Alfvén waves in the recent CMB data, and the observational bound on the primordial vector perturbation
• KiDS-1000 Cosmology: Constraints from density split statistics
• Cross-correlation cosmic shear with the SDSS and VLA FIRST surveys
• Planck ISW-lensing likelihood and the CMB temperature
• SOFIA/HAWC+ Far-InfraRed Polarimetric Large Area CMZ Exploration (FIREPLACE) Survey I: General Results from the Pilot Program
• Pearson's random walk in the space of the CMB phases: evidence for parity asymmetry
• Comparison of the Diffuse Halpha and FUV Continuum Backgrounds: On the Origins of the Diffuse Halpha Background
• Dust distributions in the Magellanic Clouds
• Measuring the redshift dependence of the CMB monopole temperature with PLANCK data
• Recovering the CMB Signal with Machine Learning
• Patchy Screening of the Cosmic Microwave Background by Inhomogeneous Reionization
• Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System
• Channeling in direct dark matter detection III: channeling fraction in CsI crystals
• Follow-up of astrophysical transients in real time with the IceCube Neutrino Observatory
• Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data
• Cold imprint of supervoids in the Cosmic Microwave Background re-considered with Planck and BOSS DR10
• On Minkowski Functionals of CMB polarization
• Tensor Minkowski Functionals for random fields on the sphere
• Rotational Spectral Unmixing of Exoplanets: Degeneracies between Surface Colors and Geography
• Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates
• The impact of the ionosphere on ground-based detection of the global Epoch of Reionisation signal
• A Measurement of Primordial Non-Gaussianity Using WMAP 5-Year Temperature Skewness Power Spectrum
• Structure, Kinematics, and Observability of the Large Magellanic Cloud's Dynamical Friction Wake in Cold vs. Fuzzy Dark Matter
• A possible common explanation for several cosmic microwave background (CMB) anomalies: A strong impact of nearby galaxies on observed large-scale CMB fluctuations
• Detecting and Characterizing Mg II absorption in DESI Survey Validation Quasar Spectra
• Optimal scan strategies for future CMB satellite experiments
• A sample of Fast Radio Bursts discovered and localised with MeerTRAP at the MeerKAT telescope
• Cygrid: A fast Cython-powered convolution-based gridding module for Python
• Visualisation of Multi-mission Astronomical Data with ESASky
• Local analyses of Planck maps with Minkowski Functionals
• Line-of-Sight Extrapolation Noise in Dust Polarization
• Mapping Milky Way disk perturbations in stellar number density and vertical velocity using Gaia DR3
• Tempestuous life beyond R500: X-ray view on the Coma cluster with SRG/eROSITA. II. Shock & Relic
• On Approximation for Fractional Stochastic Partial Differential Equations on the Sphere
• Analysis of non-Gaussian CMB maps based on the N-pdf. Application to WMAP data
• Messier 81's Planck view vs its halo mapping
• CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator
• A Map of Diffuse Radio Emission at 182 MHz to Enhance Epoch of Reionization Observations in the Southern Hemisphere
• One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
• The primordial magnetic field in our cosmic backyard
• SuperFaB: a fabulous code for Spherical Fourier-Bessel decomposition
• Giant Rings in the CMB Sky
• Understanding the WMAP Cold Spot mystery
• Efficient decomposition of cosmic microwave background polarization maps into pure E, pure B, and ambiguous components
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• Clustering of the IR Background Light with Spitzer: Contribution from Resolved Sources
• Detection of Spectral Variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: 40 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• Efficient Optimal Reconstruction of Linear Fields and Band-powers from Cosmological Data
• Producing Synthetic Maps of Dust Polarization using Velocity Channel Gradient Technique
• Gamma-Ray Emission from Molecular Clouds Generated by Penetrating Cosmic Rays
• Testing isotropy in the Universe using photometric and spectroscopic data from the SDSS
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• A Model For Polarised Microwave Foreground Emission From Interstellar Dust
• Tree-based solvers for adaptive mesh refinement code FLASH -- II: radiation transport module TreeRay
• CatNorth: An Improved Gaia DR3 Quasar Candidate Catalog with Pan-STARRS1 and CatWISE
• Lunar occultation of the diffuse radio sky: LOFAR measurements between 35 and 80 MHz
• A Search for Dark Matter Lines at the Galactic Center with 14 Years of Fermi Data
• Efficiency of pseudo-spectrum methods for estimation of Cosmic Microwave Background B-mode power spectrum
• Cataloging Accreted Stars within Gaia DR2 using Deep Learning
• Maps of the number of HI clouds along the line of sight at high galactic latitude
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz
• Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper look
• Magnification of Photometric LRGs by Foreground LRGs and Clusters in SDSS
• Evidence of Quasi-linear Super-Structures in the Cosmic Microwave Background and Galaxy Distribution
• On the origin of low escape fractions of ionizing radiation from massive star-forming galaxies at high redshift
• On-sky performance of the CLASS Q-band telescope
• Impact of modulation on CMB B-mode polarization experiments
• High significance detection of the tSZ effect relativistic corrections
• Dissecting the Stochastic Gravitational Wave Background with Astrometry
• No evidence for dust B-mode decorrelation in Planck data
• An optimal survey geometry of weak lensing survey: minimizing super-sample covariance
• Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
• Gravitational Wave Background Sky Maps from Advanced LIGO O1 Data
• BICEP2 / Keck Array VII: Matrix based E/B Separation applied to BICEP2 and the Keck Array
• Planck intermediate results. XLIII. The spectral energy distribution of dust in clusters of galaxies
• Radiation Hydrodynamics using Characteristics on Adaptive Decomposed Domains for Massively Parallel Star Formation Simulations
• A new equal-area isolatitudinal grid on a spherical surface
• Removal of two large scale Cosmic Microwave Background anomalies after subtraction of the Integrated Sachs Wolfe effect
• HIDE & SEEK: End-to-End Packages to Simulate and Process Radio Survey Data
• Weak lensing mass reconstruction using sparsity and a Gaussian random field
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• The Data Big Bang and the Expanding Digital Universe: High-Dimensional, Complex and Massive Data Sets in an Inflationary Epoch
• Free-moving Quantitative Gamma-ray Imaging
• The 7-year MAXI/GSC X-ray Source Catalog in the High Galactic-Latitude Sky (3MAXI)
• The Power of Halometry
• The All-Sky SignAl Short-Spacing INterferometer (ASSASSIN) I: Global sky measurements with the Engineering Development Array-2
• The Ultraviolet Extinction Map and Dust Property at High Galactic Latitude
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Removing Imaging Systematics from Galaxy Clustering Measurements with Obiwan : Application to the SDSS-IV extended Baryon Oscillation Spectroscopic Survey Emission Line Galaxy Sample
• The Weak Lensing Bispectrum Induced By Gravity
• SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release
• Search for Gamma-Ray Bursts and Gravitational Wave Electromagnetic Counterparts with High Energy X-ray Telescope of \textit{Insight}-HXMT
• The detection of the imprint of filaments on cosmic microwave background lensing
• Simulating the Legacy Survey of Space and Time stellar content with TRILEGAL
• A search for cosmic topology in the final WMAP data
• The halo light cone catalogues of \Abacus{AbacusSummit}
• The Integrated Sachs-Wolfe Signal from BOSS Super-Structures
• Measuring Coherent Motions in the Universe
• Long-term spectra of the blazars Mrk 421 and Mrk 501 at TeV energies seen by HAWC
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Measuring the hydrostatic mass bias in galaxy clusters by combining Sunyaev-Zel'dovich and CMB lensing data
• Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing
• Starlight-polarization-based tomography of the magnetized interstellar medium: PASIPHAE's line-of-sight inversion method
• Framework for performance forecasting and optimization of CMB B-mode observations in presence of astrophysical foregrounds
• Detecting the power spectrum turnover with HI intensity mapping
• Predictions of Cosmic Microwave Background Foregrounds Dust Polarization Using Velocity Gradients
• Observation number correlation in WMAP data
• A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys
• Fast and precise map-making for massively multi-detector CMB experiments
• An improved Compton parameter map of thermal Sunyaev-Zeldovich effect from Planck PR4 data
• The Atacama Cosmology Telescope: Weighing distant clusters with the most ancient light
• Variable star classification across the Galactic bulge and disc with the VISTA Variables in the Vía Láctea survey
• Cosmological constraints from the observed angular cross-power spectrum between Sunyaev-Zel'dovich and X-ray surveys
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• Constraining the regular Galactic Magnetic Field with the 5-year WMAP polarization measurements at 22 GHz
• CMB EB and TB cross-spectrum estimation via pseudo-spectrum techniques
• Frequency dependence of the thermal dust $E/B$ ratio and $EB$ correlation: insights from the spin-moment expansion
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• Large-scale analysis of the SDSS-III DR8 photometric luminous galaxies angular correlation function
• The interaction of Type Iax supernova ejecta with a helium companion star
• Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation
• Prospects for joint observations of gravitational waves and gamma rays from merging neutron star binaries
• Constraining the local variance of $H_0$ from directional analyses
• Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic Rays
• Bias in low-multipole CMB reconstructions
• BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors
• Signature of the first galaxies in JWST deep field observations
• The error budget of the Dark Flow measurement
• Measurement of the integrated Sachs-Wolfe effect using the AllWISE data release
• Impact on the tensor-to-scalar ratio of incorrect Galactic foreground modelling
• An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data
• Exploring cosmic origins with CORE: effects of observer peculiar motion
• Search for neutrinos in coincidence with gravitational wave events from the LIGO-Virgo O3a Observing Run with the Super-Kamiokande detector
• Validations and Corrections of the SFD and Planck Reddening Maps Based on LAMOST and Gaia Data
• LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
• A note on the large-angle anisotropies in the WMAP cut-sky maps
• Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115
• Detectability of modulated X-rays from LISA's supermassive black hole mergers
• Galactic PeVatrons and helping to find them: Effects of Galactic absorption on the observed spectra of very high energy $\gamma$-ray sources
• Hot and cold spots counts as probes of non-Gaussianity in the CMB
• Bulk flow of halos in ΛCDM simulation
• All sky angular power spectrum: I. Estimating brightness temperature fluctuations using TGSS 150 MHz survey
• Azimuthal asymmetry in cosmic-ray boosted dark matter flux
• The EBEX Balloon Borne Experiment - Detectors and Readout
• ArtDeco: A beam deconvolution code for absolute CMB measurements
• Taking measurements of the kinematic Sunyaev-Zel'dovich effect forward: including uncertainties from velocity reconstruction with forward modeling
• An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission
• Possible detection of the M31 rotation in WMAP data
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• Dipole Modulation of Cosmic Microwave Background Temperature and Polarization
• Detection of pairwise kSZ effect with DESI galaxy clusters and Planck
• High precision simulations of weak lensing effect on Cosmic Microwave Background polarization
• The cosmological principle is not in the sky
• Holographic Beam Mapping of the CHIME Pathfinder Array
• DART-Ray: a 3D ray-tracing radiative transfer code for calculating the propagation of light in dusty galaxies
• Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
• Searching for non-Gaussianity in the WMAP data
• Modelling the Galactic Foreground and Beam Chromaticity for Global 21-cm Cosmology
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Gaia Focused Product Release: Asteroid orbital solution. Properties and assessment
• Identification of RR Lyrae stars in multiband, sparsely-sampled data from the Dark Energy Survey using template fitting and Random Forest classification
• KaRMMa -- Kappa Reconstruction for Mass Mapping
• General Relativistic Corrections to the Weak Lensing Convergence Power Spectrum
• The angular two-point correlation of NVSS galaxies revisited
• Explicit Bayesian treatment of unknown foreground contaminations in galaxy surveys
• MillimeterDL: Deep Learning Simulations of the Microwave Sky
• Presto-Color: A Photometric Survey Cadence for Explosive Physics & Fast Transients
• INTEGRAL 11-year hard X-ray survey above 100 keV
• A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
• The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium
• First Investigation of the Combined Impact of Ionizing Radiation and Momentum Winds from a Massive Star on a Self-Gravitating Core
• On the universality of MOG weak field approximation at galaxy cluster scale
• Catalog of Long-Term Transient Sources in the First 10 Years of Fermi-LAT Data
• The behaviour of shape and velocity anisotropy in dark matter haloes
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• DUSTiER (DUST in the Epoch of Reionization): dusty galaxies in cosmological radiation-hydrodynamical simulations of the Epoch of Reionization with RAMSES-CUDATON
• Structures in the microwave background radiation
• Scale dependent non-Gaussianities in the CMB data identified with Minkowski Functionals and Scaling Indices
• Cleaning our own Dust: Simulating and Separating Galactic Dust Foregrounds with Neural Networks
• Hierarchical Bayesian Detection Algorithm for Early-Universe Relics in the Cosmic Microwave Background
• Reionization on Large Scales II: Detecting Patchy Reionization through Cross Correlation of the Cosmic Microwave Background
• Non-Gaussian modelling and statistical denoising of Planck dust polarization full-sky maps using scattering transforms
• Redshift requirements for cosmic shear with intrinsic alignment
• Cross-correlation of WMAP7 and the WISE Full Data Release
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• Magnetic Misalignment of Interstellar Dust Filaments
• Consistency of cosmic shear analyses in harmonic and real space
• Multi-resolution Bayesian CMB component separation through Wiener-filtering with a pseudo-inverse preconditioner
• On the Statistical Significance of the Bulk Flow Measured by the PLANCK Satellite
• Non Gaussian extrema counts for CMB maps
• Sky reconstruction for the Tianlai cylinder array
• Global Mapping of an Exo-Earth using Sparse Modeling
• Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
• Multi-Clustering Needlet-ILC for CMB B-modes component separation
• Toward $abinitio$ extremely metal poor stars
• Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
• Framework for analysis of next generation, polarised CMB data sets in the presence of galactic foregrounds and systematic effects
• Constraining Galactic dark matter with gamma-ray pixel counts statistics
• The peak-flux of GRB 221009A measured with GRBAlpha
• The triply-ionized carbon forest from eBOSS: cosmological correlations with quasars in SDSS-IV DR14
• Are stellar--mass binary black hole mergers isotropically distributed?
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• A Constraint On the Integrated Mass Power Spectrum out to z = 1100 from Lensing of the Cosmic Microwave Background
• Tight framelets and fast framelet filter bank transforms on manifolds
• Neutron Star$-$Neutron Star and Neutron Star$-$Black Hole Mergers: Multiband Observations and Early Warnings
• The Propagation of Cosmic Rays from the Galactic Wind Termination Shock: Back to the Galaxy?
• Comparison of delensing methodologies and assessment of the delensing capabilities of future experiments
• Detection prospects for high energy neutrino sources from the anisotropic matter distribution in the local universe
• In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications
• On the anisotropy in the arrival directions of ultra-high-energy cosmic rays
• CMB polarization constraints on radiative feedback
• Is the Cygnus Superbubble a Hypernova Remnant?
• The Atacama Cosmology Telescope: A search for Planet 9
• Searching for Planet Nine with Coadded WISE and NEOWISE-Reactivation Images
• Analyzing the Gamma-ray Sky with Wavelets
• A 3D model for CO molecular line emission as a potential CMB polarization contaminant
• Constraints on the spectral index of polarized synchrotron emission from WMAP and Faraday-corrected S-PASS data
• Machine Learning Based Real Bogus System for HSC-SSP Moving Object Detecting Pipeline
• A Cross-Correlation Study of High-energy Neutrinos and Tracers of Large-Scale Structure
• A survey of active galaxies at TeV photon energies with the HAWC gamma-ray observatory
• Faraday Rotation as a diagnostic of Galactic foreground contamination of CMB maps
• Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at $|b|<20°$
• The halo mass of optically-luminous quasars at z=1-2 measured via gravitational deflection of the cosmic microwave background
• Recovery of Large Angular Scale CMB Polarization for Instruments Employing Variable-delay Polarization Modulators
• The Atacama Cosmology Telescope: Map-Based Noise Simulations for DR6
• Non-gaussianity in the foreground-reduced CMB maps
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Direction dependence of cosmological parameters due to cosmic hemispherical asymmetry
• The Observational Anatomy of Externally Photoevaporating Planet-Forming Discs I: Atomic Carbon
• Steerable wavelet analysis of CMB structures alignment
• Harmonic in-painting of CMB sky by constrained Gaussian realization
• Can residuals of the Solar system foreground explain low multipole anomalies of the CMB ?
• PSZSPT: a joint Planck and SPT-SZ cluster catalog
• Astrochemical Correlations in Molecular Clouds
• Cosmic Polarization Rotation: an Astrophysical Test of Fundamental Physics
• The Validity of the Cosmic String Pattern Search with the Cosmic Microwave Background
• Stacked lensing estimators and their covariance matrices: Excess surface mass density vs. Lensing shear
• The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis
• Galactic googly: the rotation-metallicity bias in the inner stellar halo of the Milky Way
• Measuring the integrated Sachs-Wolfe effect from the low-density regions of the universe
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Entering the Era of Dark Matter Astronomy? Near to Long-Term Forecasts in X-Ray and Gamma-Ray Bands
• X-ray to gamma-ray virial shock signal from the Coma cluster
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• Ephemeris Errors and the Gravitational Wave Signal: Harmonic Mode Coupling in Pulsar Timing Array Searches
• Measuring HERA's primary beam in-situ: methodology and first results
• Statistical recovery of 21cm visibilities and their power spectra with Gaussian constrained realisations and Gibbs sampling
• Simulated catalogs and maps of radio galaxies at millimeter wavelengths in Websky
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• Characterization of the polarized synchrotron emission from Planck and WMAP data
• Spherical Cows in Dark Matter Indirect Detection
• Constraining the Distance to the North Polar Spur with Gaia DR2
• Numerical evolutions of fields on the 2-sphere using a spectral method based on spin-weighted spherical harmonics
• Data Processing Pipeline For Tianlai Experiment
• Dark Matter decay and annihilation in the Local Universe: CLUES from Fermi
• Sparse Bayesian mass-mapping with uncertainties: local credible intervals
• C3, A Command-line Catalogue Cross-match tool for large astrophysical catalogues
• Constraints on Patchy Reionization from Planck CMB Temperature Trispectrum
• Imaging sensitivity of a linear interferometer array on lunar orbit
• Completeness of the Gaia-verse V: Astrometry and Radial Velocity sample selection functions in Gaia EDR3
• Detection of Anomalous Microwave Emission in the Pleiades Reflection Nebula with WMAP and the COSMOSOMAS Experiment
• North-South non-Gaussian asymmetry in PLANCK CMB maps
• Measuring Planck beams with planets
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case
• The actual Rees--Sciama effect from the Local Universe
• CRT: A numerical tool for propagating ultra-high energy cosmic rays through Galactic magnetic field models
• The Impact of Beam Variations on Power Spectrum Estimation for 21-cm Cosmology I: Simulations of Foreground Contamination for HERA
• Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids
• BOOMERanG Constraints on Primordial Non-Gaussianity from Analytical Minkowski Functionals
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• A framework for testing isotropy with the cosmic microwave background
• Strategies for Finding Prompt Radio Counterparts to Gravitational Wave Transients with the Murchison Widefield Array
• SILC: a new Planck Internal Linear Combination CMB temperature map using directional wavelets
• Could multiple voids explain the Cosmic Microwave Background Cold Spot anomaly?
• Probing the statistical properties of CMB $B$-mode polarization through Minkowski Functionals
• Observations of the Cosmic Microwave Background and Galactic Foregrounds at 12-17 GHz with the COSMOSOMAS Experiment
• Clustering dark energy imprints on cosmological observables of the gravitational field
• The fast transient sky with Gaia
• The scalar perturbation spectral index n_s: WMAP sensitivity to unresolved point sources
• Quasar Host Environments: The view from Planck
• Measuring the Largest Angular Scale CMB B-mode Polarization with Galactic Foregrounds on a Cut Sky
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• Non-Gaussian Structure of B-mode Polarization after Delensing
• An alternative validation strategy for the Planck cluster catalog and $y$-distortion maps
• A common explanation of the Hubble tension and anomalous cold spots in the CMB
• Spatially Coherent 3D Distributions of HI and CO in the Milky Way
• Is the cold spot responsible for the CMB North-South asymmetry?
• Inpainting Galactic Foreground Intensity and Polarization maps using Convolutional Neural Network
• A Neural-Network based estimator to search for primordial non-Gaussianity in Planck CMB maps
• A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing Runs
• Understanding the faint red galaxy population using large-scale clustering measurements from SDSS DR7
• Minute-cadence Observations of the LAMOST Fields with the TMTS: I. Methodology of Detecting Short-period Variables and Results from the first-year Survey
• Forecasts on the contamination induced by unresolved point sources in primordial non-Gaussianity beyond Planck
• Faraday caustics: Singularities in the Faraday spectrum and their utility as probes of magnetic field properties
• Testing the Cosmological Principle in the radio sky
• Optimal filtering for CMB lensing reconstruction
• Deciphering Residual Emissions: Time-Dependent Models for the Non-Thermal Interstellar Radiation from the Milky Way
• How to detect gravitational waves through the cross-correlation of the galaxy distribution with the CMB polarization
• The Atacama Cosmology Telescope: Measurement and Analysis of 1D Beams for DR4
• A hybrid approach to CMB lensing reconstruction on all-sky intensity maps
• Cross-correlating 2D and 3D galaxy surveys
• CMB statistical anisotropy, multipole vectors and the influence of the dipole
• Minkowski Functionals of CMB polarisation intensity with Pynkowski: theory and application to Planck and future data
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• Too few spots in the cosmic microwave background
• Estimating the weak-lensing rotation signal in radio cosmic shear surveys
• Enhancing cosmic shear with the multi-scale lensing PDF
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• AKARI-CAS --- Online Service for AKARI All-Sky Catalogues
• Bulk Flow Motion Detection in the Local Universe with Pantheon$+$ Type Ia Supernovae
• Primordial non-Gaussian signatures in CMB polarization
• The Efficacy of Event Isotropy as an Event Shape Observable
• Localization of Binary Black-Hole Mergers with Known Inclination
• Average fractional polarization of extragalactic sources at Planck frequencies
• BICEP / Keck XVI: Characterizing Dust Polarization through Correlations with Neutral Hydrogen
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• CMB Aberration and Doppler Effects as a Source of Hemispherical Asymmetries
• The cosmic shallows I: interaction of CMB photons in extended galaxy halos
• Local non-Gaussianity in the Cosmic Microwave Background the Bayesian way
• Searching for hidden mirror symmetries in CMB fluctuations from WMAP 7 year maps
• Rapid localization of gravitational wave sources from compact binary coalescences using deep learning
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
• Constraints on general primordial non-Gaussianity using wavelets for the Wilkinson Microwave anisotropy probe 7-year data
• CMB constraints on running non-Gaussianity
• Separating polarized cosmological and galactic emissions for CMB B-mode polarization experiments
• Fermi bubble edges: spectrum and diffusion function
• Distortion of the ultrahigh energy cosmic ray flux from rare transient sources in inhomogeneous extragalactic magnetic fields
• Single frequency CMB B-mode inference with realistic foregrounds from a single training image
• Planck view of the M82 galaxy
• Non-Gaussianity in WMAP Data Due to the Correlation of CMB Lensing Potential with Secondary Anisotropies
• Detection/estimation of the modulus of a vector. Application to point source detection in polarization data
• DELVE-ing into the Jet: a thin stellar stream on a retrograde orbit at 30 kpc
• Constraining gravity at large scales with the 2MASS Photometric Redshift catalogue and Planck lensing
• Preparing to discover the unknown with Rubin LSST -- I: Time domain
• Search for 10--1000 GeV neutrinos from Gamma Ray Bursts with IceCube
• Updated galactic radio constraints on Dark Matter
• Characterising the Gaia Radial Velocity sample selection function in its native photometry
• Relating the inhomogeneous power spectrum to the CMB hemispherical anisotropy
• Tessellated Mapping of Cosmic Background Radiation Correlations and Source Distributions
• The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope
• Measuring Bulk Flow of Galaxy Clusters using Kinematic Sunyaev-Zel'dovich effect: Prediction for Planck
• Angular clustering of point sources at 150 MHz in the TGSS survey
• Effect of Template Uncertainties on the WMAP and Planck Measures of the Optical Depth Due To Reionization
• Polarized wavelets and curvelets on the sphere
• A linear filter to reconstruct the ISW effect from CMB and LSS observations
• Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
• Dark Energy Survey Year 3 results: imprints of cosmic voids and superclusters in the Planck CMB lensing map
• Patchy Kinetic Sunyaev-Zel'dovich Effect with Controlled Reionization History and Morphology
• Large scale CMB anomalies from thawing cosmic strings
• Planck revealed bulk motion of Centaurus A lobes
• Wavelet reconstruction of E and B modes for CMB polarisation and cosmic shear analyses
• The Great Wave: Evidence of a large-scale vertical corrugation propagating outwards in the Galactic disc
• Identification of point sources in gamma rays using U-shaped convolutional neural networks and a data challenge
• HI Intensity Mapping for Clustering-Based Redshift Estimation
• Fundamental uncertainty levels of 21cm power spectra from a delay analysis
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Evidence of Ultra-faint Radio Frequency Interference in Deep 21~cm Epoch of Reionization Power Spectra with the Murchison Widefield Array
• 21cm Signal Recovery via the Robust Principle Component Analysis
• A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Galaxy with DELVE Early Data Release 3
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter
• A case study for measuring the relativistic dipole of a galaxy cross-correlation with the Dark Energy Spectroscopic Instrument
• The Parkes Galactic Meridian Survey (PGMS): observations and CMB polarization foreground analysis
• The remnant radio galaxy associated with NGC 1534
• Broadband spectral energy distributions of SDSS-selected quasars and of their host galaxies: intense activity at the onset of AGN feedback
• COMAP Early Science: VI. A First Look at the COMAP Galactic Plane Survey
• On the Detection of CMB B-modes from Ground at Low Frequency
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q Band
• Anisotropic infall in the outskirts of OmegaWINGS galaxy clusters
• The effects of varying depth in cosmic shear surveys
• Growth-rate measurement with type-Ia supernovae using ZTF survey simulations
• Constraining Primordial Non-Gaussianities from the WMAP2 2-1 Cumulant Correlator Power Spectrum
• Pre-merger sky localization of gravitational waves from binary neutron star mergers using deep learning
• Zodiacal Light Emission in the PLANCK mission
• MINOT: Modeling the intracluster medium (non-)thermal content and observable prediction tools
• Hard X-ray Luminosity Function of Tidal Disruption Events: First Results from MAXI Extragalactic Survey
• Topology beyond the horizon: how far can it be probed?
• Global Mapping of the Surface Composition on an Exo-Earth using Color Variability
• Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts
• Magritte, a modern software library for 3D radiative transfer: II. Adaptive ray-tracing, mesh construction and reduction
• How does an incomplete sky coverage affect the Hubble Constant variance?
• Using angular two-point correlations to self-calibrate the photometric redshift distributions of DECaLS DR9
• The Evolution of the Cosmic Microwave Background
• The effect of asymmetric beams in the Wilkinson Microwave Anisotropy Probe experiment
• Higgsino Dark Matter Confronts 14 years of Fermi Gamma Ray Data
• Effect of Cosmic UV Background on Star Formation in High Redshift Galaxies
• An Isotropy Measurement with Gravitational Wave Observations
• QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• Avoiding bias in reconstructing the largest observable scales from partial-sky data
• Scientific verification of Faraday Rotation Modulators: Detection of diffuse polarized Galactic emission
• Integrated Cosmological Probes: Extended Analysis
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. II. Second year of LP15 observations
• The Dark Ages of the Universe and Hydrogen Reionization
• Multibaseline gravitational wave radiometry
• An Improved Diffuse Foreground Subtraction by ILC method: CMB Map and Angular Power Spectrum using Planck and WMAP Observations
• Dust polarization spectral dependence from Planck HFI data. Turning point on CMB polarization foregrounds modelling
• Inadequacy of internal covariance estimation for super-sample covariance
• Cosmological Applications of the Gaussian Kinematic Formula
• Wiener filtering and pure E/B decomposition of CMB maps with anisotropic correlated noise
• The MeerKAT Pulsar Timing Array: Maps of the gravitational-wave sky with the 4.5 year data release
• A Simple Proposal for Radial 3D Needlets
• A Coincidence Search for Cosmic Neutrino and Gamma-Ray Emitting Sources Using IceCube and Fermi LAT Public Data
• Chandra Observations of the Planck ESZ Sample: A Re-Examination of Masses and Mass Proxies
• Measuring ISW with next-generation radio surveys
• Genus Topology and Cross-Correlation of BICEP2 and Planck 353 GHz B-Modes: Further Evidence Favoring Gravity Wave Detection
• Convolutional Neural Network-reconstructed velocity for kinetic SZ detection
• Exploring cosmic origins with CORE: mitigation of systematic effects
• Measuring gravitational lensing of the cosmic microwave background using cross correlation with large scale structure
• Large-scale three-dimensional Gaussian process extinction mapping
• The Cosmic Neutrino Background Anisotropy - Linear Theory
• Searching for gamma-ray emission from galaxy clusters at low redshift
• Large Scale Plane-Mirroring in the Cosmic Microwave Background WMAP5 Maps
• Parameter Estimation from Improved Measurements of the CMB from QUaD
• Earthshine as an Illumination Source at the Moon
• Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
• Fast generation of isotropic Gaussian random fields on the sphere
• Identifying Host Galaxies of Supermassive Black Hole Binaries Found by PTAs
• Unified mapmaking for an anisotropic stochastic gravitational wave background
• Beamforming Errors in Murchison Widefield Array Phased Array Antennas and their effects on Epoch of Reionization Science
• Exploring Simulated Early Star Formation in the Context of the Ultrafaint Dwarf Galaxies
• Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
• An imaging algorithm for a lunar orbit interferometer array
• On the impact of large angle CMB polarization data on cosmological parameters
• Runaway and Hypervelocity Stars from Compact Object Encounters in Globular Clusters
• Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters
• A new method to perform data/model comparison in Fermi-LAT analysis
• Towards a soft magnetoelastic twist actuator
• Gamma-ray anisotropies from dark matter in the Milky Way: the role of the radial distribution
• Deep learning for Sunyaev-Zel'dovich detection in Planck
• Dominant Multipoles in WMAP5 Mosaic Data Correlation Maps
• Statistical Characterization of the Chandra Source Catalog
• Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey
• Dust polarization modeling at large-scale over the Northern Galactic cap using EBHIS and Planck data
• Exploring two-spin internal linear combinations for the recovery of the CMB polarization
• Pure E and B polarization maps via Wiener filtering
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Stellar winds and photoionization in a spiral arm
• Preferred axis of CMB parity asymmetry in the masked maps
• On Preferred Axes in WMAP Cosmic Microwave Background Data after Subtraction of the Integrated Sachs-Wolfe Effect
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky
• Probing frequency-dependent half-wave plate systematics for CMB experiments with full-sky beam convolution simulations
• Testing physical models for dipolar asymmetry: from temperature to k space to lensing
• Residual foreground contamination in the WMAP data and bias in non-Gaussianity estimation
• Imprint of Inhomogeneous and Anisotropic Primordial Power Spectrum on CMB Polarization
• Theoretical and numerical perspectives on cosmic distance averages
• Delensing the CMB with the cosmic infrared background: the impact of foregrounds
• Lack-of-correlation anomaly in CMB large scale polarisation maps
• Cosmological parameter estimation: impact of CMB aberration
• Tidal Effects on the Radial Velocities of V723 Mon: Additional Evidence for a Dark $3M_{\odot }$ Companion
• Symmetry and anti-symmetry of the CMB anisotropy pattern
• Foreground model recognition through Neural Networks for CMB B-mode observations
• Planck intermediate results. XLI. A map of lensing-induced B-modes
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• Planck Lensing and Cosmic Infrared Background Cross-Correlation with Fermi-LAT: Tracing Dark Matter Signals in the Gamma-Ray Background
• Towards a full $w$CDM map-based analysis for weak lensing surveys
• Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
• Simulating the Large-Scale Structure of HI Intensity Maps
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Studies of Systematic Uncertainties for Simons Observatory: Detector Array Effects
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• The impact of extragalactic foregrounds on internal delensing of CMB B-mode polarization
• CENN: A fully convolutional neural network for CMB recovery in realistic microwave sky simulations
• Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
• Radiation transport methods in star formation simulations
• CMB component separation in the pixel domain
• Cosmic string induced CMB maps
• The Kullback-Leibler Divergence as an Estimator of the Statistical Properties of CMB Maps
• Triangulum galaxy viewed by Planck
• Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
• Intensity-Corrected Herschel Observations of Nearby Isolated Low-Mass Clouds
• Dark matter spin determination with directional direct detection experiments
• Bayesian power-spectrum inference with foreground and target contamination treatment
• Blind correction of the EB-leakage in the pixel domain
• Bayesian Dynamic Mapping of an Exo-Earth from Photometric Variability
• DeepSphere: a graph-based spherical CNN
• Stochastic gravitational-wave background searches and constraints on neutron-star ellipticity
• DESI Legacy Imaging Surveys Data Release 9: Cosmological Constraints from Galaxy Clustering and Weak Lensing using the Minimal Bias Model
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
• Simulating the Detection of the Global 21 cm Signal with MIST for Different Models of the Soil and Beam Directivity
• Towards Accurate Field-Level Inference of Massive Cosmic Structures
• Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
• Optimal Estimation of the Binned Mask-Free Power Spectrum, Bispectrum, and Trispectrum on the Full Sky: Scalar Edition
• KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
• Characterising cosmic birefringence in the presence of galactic foregrounds and instrumental systematic effects
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagation
• Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• Bayesian inference of three-dimensional gas maps: II. Galactic HI
• Determination of Polarization Angles in CMB Experiments and Application to CMB Component Separation Analyses
• Impact of survey geometry and super-sample covariance on future photometric galaxy surveys
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• A measurement of the scale of homogeneity in the Early Universe
• Modeling Redshift-Space Clustering with Abundance Matching
• CMB Mode Coupling with Isotropic Polarization Rotation
• Linking nearby stellar streams to more distant halo overdensities
• Radio Galaxy Zoo: New Giant Radio Galaxies in the RGZ DR1catalogue
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Clustering of Local Extrema in Planck CMB maps
• Spherically Restricted Random Hyperbolic Diffusion
• Quantifying EoR delay spectrum contamination from diffuse radio emission
• High mass and halo resolution from fast low resolution simulations
• Bounds on WIMP dark matter from galaxy clusters at low redshift
• ESASky : A Science-Driven Discovery Portal for Space-Based Astronomy Missions
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region
• Measuring Linear and Non-linear Galaxy Bias Using Counts-in-Cells in the Dark Energy Survey Science Verification Data
• Simulated reconstruction of the remote dipole field using the kinetic Sunyaev Zel'dovich effect
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• Cosmological-scale coherent orientations of quasar optical polarization vectors in the $Planck$ era Investigating the Galactic dust contamination scenario
• The dipole anisotropy of WISE x SuperCOSMOS number counts
• Sparse image reconstruction on the sphere: analysis and synthesis
• Making maps of Cosmic Microwave Background polarization for B-mode studies: the POLARBEAR example
• Lensing Bias to CMB Measurements of Compensated Isocurvature Perturbations
• Spin-SILC: CMB polarisation component separation with spin wavelets
• Galaxy clustering with photometric surveys using PDF redshift information
• A New Maximum-Likelihood Technique for Reconstructing Cosmic-Ray Anisotropy at All Angular Scales
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• Limits on the fluctuating part of $y$-type distortion monopole from Planck and SPT results
• A new polarisation amplitude bias reduction method
• Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
• Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
• Far-Ultraviolet Observations of the Spica Nebula and the Interaction Zone
• General CMB bispectrum analysis using wavelets and separable modes
• Optimal bispectrum estimator and simulations of the the CMB Lensing-ISW non-Gaussian signal
• Large-scale anomalies of the CMB in the curvaton scenario
• Testing Homogeneity with Galaxy Star Formation Histories
• Template fitting of WMAP 7-year data: anomalous dust or flattening synchrotron emission?
• Constraining the topology of the Universe using the polarised CMB maps
• Are There Echoes From The Pre-Big Bang Universe? A Search for Low Variance Circles in the CMB Sky
• Statistical Characterization of Temperature Patterns in Anisotropic Cosmologies
• Residual noise covariance for Planck low-resolution data analysis
• WMAP anomalous signal in the ecliptic plane
• Likelihood Methods for the Detection and Characterization of Gamma-ray Pulsars with the Fermi Large Area Telescope
• HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4
• Dual Polarization Measurements of MWA Beampatterns at 137 MHz
• Numerical Models for the Diffuse Ionized Gas in Galaxies. II. Three-dimensional radiative transfer in inhomogeneous interstellar structures as a tool for analyzing the diffuse ionized gas
• The Hot and Cold Spots in Five-Year WMAP Data
• Earth as an Exoplanet. II. Earth's Time-variable Thermal Emission and Its Atmospheric Seasonality of Bioindicators
• Search for anisotropies in cosmic-ray positrons detected by the PAMELA experiment
• PReBeaM for Planck: A Polarized Regularized Beam Deconvolution Map-Making Method
• Molecular gas properties of Planck-selected protocluster candidates at z~1.3-3
• Probing Large-Angle Correlations with the Microwave Background Temperature and Lensing Cross Correlation
• Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimation
• Peculiarities of phases of the WMAP quadrupole
• A Search for Correlation of Ultra-High Energy Cosmic Rays with IRAS-PSCz and 2MASS-6dF Galaxies
• Synthetic spectra for Lyman-$\alpha$ forest analysis in the Dark Energy Spectroscopic Instrument
• Polarized Synchrotron Foreground Assessment for CMB Experiments
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Null stream analysis of Pulsar Timing Array data: localisation of resolvable gravitational wave sources
• Combining neutrino experimental light-curves for pointing to the next Galactic Core-Collapse Supernova
• Identification of Patterns in Cosmic-Ray Arrival Directions using Dynamic Graph Convolutional Neural Networks
• Mapping the large-angle deviation from Gaussianity in simulated CMB maps
• Systematic Distortion in Cosmic Microwave Background Maps
• Gaia Focused Product Release: Sources from Service Interface Function image analysis -- Half a million new sources in omega Centauri
• CMB seen through random Swiss Cheese
• The conventions for the polarization angle
• hammurabi X: Simulating Galactic Synchrotron Emission with Random Magnetic Fields
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Designing an Optimal LSST Deep Drilling Program for Cosmology with Type Ia Supernovae
• CMB polarization as a probe of the anomalous nature of the Cold Spot
• Implications on Spatial Models of Interstellar Gamma-Ray Inverse-Compton Emission from Synchrotron Emission Studies in Radio and Microwaves
• Correlations between age, kinematics, and chemistry as seen by the RAVE survey
• Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods
• Polarised emission from aligned dust grains in nearby galaxies: predictions from the Auriga simulations
• The Tiered Radio Extragalactic Continuum (T-RECS) simulation II: HI emission and continuum-HI cross-correlation
• Influence of local structure on relic neutrino abundances and anisotropies
• Give Me a Few Hours: Exploring Short Timescales in Rubin Observatory Cadence Simulations
• The Sensitivity of Future Gamma-Ray Telescopes to Primordial Black Holes
• Harmonic Inpainting of the Cosmic Microwave Background Sky: Formulation and Error Estimate
• Wavelet-Based Techniques for the Gamma-Ray Sky
• Eigenspectra: A Framework for Identifying Spectra from 3D Eclipse Mapping
• Planck/SDSS Cluster Mass and Gas Scaling Relations for a Volume-Complete redMaPPer Sample
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• Cosmic Flow Measurement and Mock Sampling Algorithm of Cosmicflows-4 Tully-Fisher Catalogue
• Fermi-LAT gamma-ray study of the interstellar medium and cosmic rays in the Chamaeleon Molecular-Cloud Complex: A look at the dark gas as optically thick HI
• Extragalactic sources in Cosmic Microwave Background maps
• Lensing simulations by Taylor expansion -- not so inefficient after all
• Analytic Light Curves in Reflected Light: Phase Curves, Occultations, and Non-Lambertian Scattering for Spherical Planets and Moons
• The variance of the CMB temperature gradient: a new signature of a multiply connected Universe
• A Deep, High-Angular Resolution 3D Dust Map of the Southern Galactic Plane
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• QUBIC II: Spectro-Polarimetry with Bolometric Interferometry
• Polarisation properties of Milky-Way-like galaxies
• The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ~0.7
• No evidence for anomalously low variance circles on the sky
• Collision Chains among the Terrestrial Planets. II. An Asymmetry between Earth and Venus
• New insights into foreground analysis of the WMAP five-year data using FASTICA
• The Response of Metal Rich Gas to X-Ray Irradiation from a Massive Black Hole at High Redshift: Proof of Concept
• Local properties of WMAP Cold Spot
• A multi-level solver for Gaussian constrained CMB realizations
• A Bayesian approach to high fidelity interferometric calibration II: demonstration with simulated data
• Bianchi VII_h models and the cold spot texture
• WMAP Observations of Planck ESZ Clusters
• Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization
• Scalable angular adaptivity for Boltzmann transport
• Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues
• Minkowski Functionals in Joint Galaxy Clustering & Weak Lensing Analyses
• H.E.S.S. follow-up observations of Binary Black Hole Coalescence events during the second and third Gravitational Waves observing runs of Advanced LIGO and Advanced Virgo
• Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Years of Data from the IceCube Observatory
• Local Group Dwarf Galaxy Detection Limit in the CSST survey
• On the statistics of the polarized submillimetre emission maps from thermal dust in the turbulent, magnetized, diffuse ISM
• Scale-dependent non-Gaussianities in the WMAP data as identified by using surrogates and scaling indices
• Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
• Implementation of a Fourier Matched Filter in CMB Analyses. Application to ISW Studies
• Searching for planar signatures in WMAP
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• Constraining the $\bar{p}/p$ Ratio in TeV Cosmic Rays with Observations of the Moon Shadow by HAWC
• Upper limits on persistent gravitational waves using folded data and the full covariance matrix from Advanced LIGO${}^{\prime }$s first two observing runs
• On the nature of LOFAR RMs and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios
• A spatially dependent correction of Gaia EDR3 parallax zero-point offset based on 0.3 million LAMOST DR8 giant stars
• Catalog-based pseudo-$C_{\ell }$s
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• A matched filter approach for blind joint detection of galaxy clusters in X-ray and SZ surveys
• Cosmological Parameter Estimation and Inference using Deep Summaries
• The new Herschel/PACS Point Source Catalogue
• A Global ILC Approach in Pixel Space over Large Angular Scales of the Sky using CMB Covariance Matrix
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• High-frequency asymptotics for Lipschitz-Killing curvatures of excursion sets on the sphere
• Full-sky beam convolution for cosmic microwave background applications
• Optical follow-up of gravitational wave triggers with DECam during the first two LIGO/VIRGO observing runs
• Skewness and Kurtosis as Indicators of Non-Gaussianity in Galactic Foreground Maps
• Analysis of Spatial Structure of the SPica H II Region
• Angular Resolution of the Search for Anisotropic Stochastic Gravitational-Wave Background with Terrestrial Gravitational-Wave Detectors
• Precision measurements of large scale structure with future type Ia supernova surveys
• On the dipole straylight contamination in spinning space missions dedicated to CMB anisotropy
• Correlation between galactic HI and the Cosmic Microwave Background
• The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: an application to lensing-matter clustering statistics
• Isotropy statistics of CMB hot and cold spots
• Radiation-driven turbulent accretion onto massive black holes
• Correlated Component Analysis for diffuse component separation with error estimation on simulated Planck polarization data
• DeepSphere: towards an equivariant graph-based spherical CNN
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• A roadmap to cosmological parameter analysis with third-order shear statistics III: Efficient estimation of third-order shear correlation functions and an application to the KiDS-1000 data
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• The White Dwarf Luminosity Functions from the Pan-STARRS 1 3π Steradian Survey
• Non-Gaussian Foreground Residuals of the WMAP First Year Maps
• MAXI upper limits of the electromagnetic counterpart of GW170817
• Hemispherical power asymmetry: parameter estimation from CMB WMAP5 data
• The Correspondence between Convergence Peaks from Weak Lensing and Massive Dark Matter Haloes
• Tomographic local 2D analyses of the WISExSuperCOSMOS all-sky galaxy catalogue
• A new method for testing isotropy with Shannon entropy
• Search for Extended Sources of Neutrino Emission in the Galactic Plane with IceCube
• Observing relativistic features in large-scale structure surveys -- II: Doppler magnification in an ensemble of relativistic simulations
• Dynamical Surface Imaging of lambda Andromedae
• CMB low multipole alignments in the $\mathbf{\Lambda }$CDM and Dipolar models
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• Mapping dark matter on the celestial sphere with weak gravitational lensing
• Dark Matter Distribution Induced by a Cosmic String Wake in the Nonlinear Regime
• Gaia predicted brown dwarf detection rates around FGK stars in astrometry, radial velocity, and photometric transits
• Semi-blind Bayesian inference of CMB map and power spectrum
• High-resolution CMB bispectrum estimator with flexible modal basis
• A Photodissociation Region study of NGC 4038
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• SPEAR far UV spectral imaging of highly ionized emission from the North Galactic Pole Region
• Improving stochastic estimates with inference methods: calculating matrix diagonals
• Data analysis methods for the cosmic microwave background
• Gas and Dust Properties in the Chamaeleon Molecular Cloud Complex based on the Optically Thick HI
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• The Vera C. Rubin Observatory Data Preview 1
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• Integrated Sachs-Wolfe map recovery from NVSS and WMAP 7yr data
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• 3D simulations of AGB stellar winds -- II. Ray-tracer implementation and impact of radiation on the outflow morphology
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• Intergalactic baryon-rich regions at high redshift
• Joint Modelling of Dust Scattering and Thermal Emission: The Spider Complex
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• Consistency of cosmic microwave background temperature measurements in three frequency bands in the 2500-square-degree SPT-SZ survey
• Probing Cosmic Strings with Satellite CMB measurements
• Turbulent power distribution in the local interstellar medium
• Multichannel Poisson denoising and deconvolution on the sphere : Application to the Fermi Gamma Ray Space Telescope
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• The H.E.S.S. Gravitational Wave Rapid Follow-up Program
• Density Weighted Angular Redshift Fluctuations: a New Cosmological Observable
• Predicting Interstellar Object Chemodynamics with Gaia
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• Detection of cross-correlation between CMB Lensing and low-density points
• Parametrizing the Reionization History with the Redshift Midpoint, Duration, and Asymmetry
• Planck Observations of M33
• Searching for Moving Objects in HSC-SSP: Pipeline and Preliminary Results
• Galactic Diffuse Neutrino Emission from Sources beyond the Discovery Horizon
• The sensitivity of Cherenkov telescopes to dark matter and astrophysical anisotropies in the diffuse gamma-ray background
• Weak Gravitational Lensing Shear Estimation with Metacalibration for the Roman High-Latitude Imaging Survey
• Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions
• A panoptic view of the Taurus molecular cloud I. The cloud dynamics revealed by gas emission and 3D dust
• Cosmological Particle Production and Pairwise Hotspots on the CMB
• CMASS galaxy sample and the ontological status of the cosmological principle
• An update on Fermi-LAT transients in the Galactic plane, including strong activity of Cygnus X-3 in mid-2020
• Impact of early dark energy on the Planck SZ cluster sample
• A novel approach to reconstructing signals of isotropy violation from a masked CMB sky
• Simulating image coaddition with the Nancy Grace Roman Space Telescope: I. Simulation methodology and general results
• Towards the ICRF3: astrometric comparison of the USNO 2016A VLBI solution with ICRF2 and Gaia DR1
• Star cluster formation and feedback in different environments of a Milky Way-like galaxy
• Angular power spectrum analysis on current and future high-energy neutrino data
• Bandpass mismatch error for satellite CMB experiments I: Estimating the spurious signal
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Analysis of WMAP 7-year Temperature Data: Astrophysics of the Galactic Haze
• Tomography of the Reionization Epoch with Multifrequency CMB Observations
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Magnetically induced elastic deformations of magnetic gels and elastomers containing particles of mixed size
• Detecting chiral gravity with the pure pseudospectrum reconstruction of the cosmic microwave background polarized anisotropies
• The CMB Cold Spot as predicted by foregrounds around nearby galaxies
• Statistics of Bipolar Representation of CMB maps
• On the origin of the Cold Spot
• Estimating the tensor-to-scalar ratio and the effect of residual foreground contamination
• $S^2$Net: Accurate Panorama Depth Estimation on Spherical Surface
• Observational Scan Induced Artificial CMB Anisotropy
• A Challenge to Identify an Optical Counterpart of the Gravitational Wave Event GW151226 with Hyper Suprime-Cam
• Detailed study of the microwave emission of the supernova remnant 3C 396
• Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
• The Impact of Anisotropic Redshift Distributions on Angular Clustering
• White dwarf deflagrations for Type Iax supernovae: Polarisation signatures from the explosion and companion interaction
• 3D cosmic shear: numerical challenges, 3D lensing random fields generation and Minkowski Functionals for cosmological inference
• Testing Gaussianity on Archeops Data
• Constraining the WMAP9 bispectrum and trispectrum with needlets
• Statistical Anisotropic Gaussian Simulations of the CMB Temperature Field
• Testing anisotropic Hubble expansion
• A numerical study of observational systematic errors in lensing analysis of CMB polarization
• Impact of Point Spread Function Higher Moments Error on Weak Gravitational Lensing II: A Comprehensive Study
• The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
• Foreground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year data
• Data compression on the sphere
• Dark matter implications of the WMAP-Planck Haze
• Induced CMB quadrupole from pointing offsets
• On the optimality of the spherical Mexican hat wavelet estimator for the primordial non-Gaussianity
• Enabling catalog simulations of transient and variable sources based on LSST cadence strategies
• Spinning nano-carbon grains: Viable origin for anomalous microwave emission
• Can one reconstruct masked CMB sky?
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust
• Removing beam asymmetry bias in precision CMB temperature and polarisation experiments
• An Examination of Galactic Polarization with Application to the Planck TB Correlation
• Expected constraints on the Galactic magnetic field using PLANCK data
• Cross-Correlation of Far-Infrared Background Anisotropies and CMB Lensing from Herschel and Planck satellites
• The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
• Accurate field-level weak lensing inference for precision cosmology
• Detection of WHIM in the Planck data using Stack First approach
• Galactic Magnetic Field Bias on Inferences from UHECR Data
• Ionospheric Attenuation of Polarized Foregrounds in 21 cm Epoch of Reionization Measurements: A Demonstration for the HERA Experiment
• Searching for patchy reionization from cosmic microwave background with hybrid quadratic estimators
• The Simulated Catalogue of Optical Transients and Correlated Hosts (SCOTCH)
• The effects of the antenna power pattern uncertainty within a global 21 cm experiment
• Requirements for future CMB satellite missions: photometric and band-pass response calibration
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• All Sky Modelling Requirements for Bayesian 21 cm Power Spectrum Estimation with BayesEoR
• GRB Sky Distribution Puzzles
• Synthetic observations of spiral arm tracers of a simulated Milky Way analog
• Galactic Faraday rotation effect on polarization of 21 cm lines from the epoch of reionization
• Minute-Cadence Observations of the LAMOST Fields with the TMTS: II. Catalogues of Short-Period Variable Stars from the First Two-Year Surveys
• Asymmetric velocity anisotropies in remnants of collisionless mergers
• Monitoring Atmospheric Dust Spring Activity at High Southern Latitudes on Mars using OMEGA
• Application of the Kolmogorov-Smirnov test to CMB data: Is the universe really weakly random?
• The galaxy power spectrum from TGSS ADR1 and the effect of flux calibration systematics
• HEALPix Alchemy: Fast All-Sky Geometry and Image Arithmetic in a Relational Database for Multimessenger Astronomy Brokers
• Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
• Hemispherical Power Asymmetry in intensity and polarization for Planck PR4 data
• Hierarchical Bayesian CMB Component Separation with the No-U-Turn Sampler
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Robust Limits from Upcoming Neutrino Telescopes and Implications on Minimal Dark Matter Models
• The nature of non-Gaussianity and statistical isotropy of the 408 MHz Haslam synchrotron map
• ECLIPSE: a fast Quadratic Maximum Likelihood estimator for CMB intensity and polarization power spectra
• Peeling off the late Universe: Reconstructing the ISW map with galaxy surveys
• A Compound Poisson Generator approach to Point-Source Inference in Astrophysics
• CMB Polarization and Temperature Power Spectra Estimation using Linear Combination of WMAP 5-year Maps
• Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
• Joint measurement of the galaxy cluster pressure profile with Planck and SPT-SZ
• Joint Bayesian analysis of large angular scale CMB temperature anomalies
• Selection functions of large spectroscopic surveys
• HAFFET: Hybrid Analytic Flux FittEr for Transients
• Morphological Analysis of the Polarized Synchrotron Emission with WMAP and Planck
• Efficient ILC analysis on polarization maps after EB leakage correction
• The ISW effect and the lack of large-angle CMB temperature correlations
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• A hybrid map-$C_{\ell }$ component separation method for primordial CMB $B$-mode searches
• Simultaneous determination of the cosmic birefringence and miscalibrated polarisation angles from CMB experiments
• TREVR: A general $Nlo{g}^{2}N$ radiative transfer algorithm
• Needatool: A Needlet Analysis Tool for Cosmological Data Processing
• QUIJOTE Scientific results. III. Microwave spectrum of intensity and polarization in the Taurus molecular cloud Complex and L1527
• Optical validation and characterization of \Planck\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
• IVOA Recommendation: HiPS - Hierarchical Progressive Survey
• Covariant polarized radiative transfer on cosmological scales for investigating large-scale magnetic field structures
• Analysis of NILC performance on B-modes data of sub-orbital experiments
• Large Scale Traces of Solar System Cold Dust on CMB Anisotropies
• Kolmogorov analysis detecting radio and Fermi gamma-ray sources in cosmic microwave background maps
• Inpainting CMB maps using Partial Convolutional Neural Networks
• The star formation history in the last 10 billion years from CIB cross-correlations
• Effect of Foregrounds on the CMBR Multipole Alignment
• Testing CMB Anomalies in E-mode Polarization with Current and Future Data
• Beyond optical depth: Future determination of ionization history from the CMB
• A proposed deep sea Neutrino Observatory in the Nanhai
• A new model of the microwave polarized sky for CMB experiments
• Expansion-maximization-compression algorithm with spherical harmonics for single particle imaging with X-ray lasers
• Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models
• E and B families of the Stokes parameters in the polarized synchrotron and thermal dust foregrounds
• All-sky, narrowband, gravitational-wave radiometry with folded data
• Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster
• Filamentary Dust Polarization and the Morphology of Neutral Hydrogen Structures
• The Steady-State Multi-TeV Diffuse Gamma-Ray Emission Predicted with GALPROP and Prospects for the Cherenkov Telescope Array
• Optimal cosmic microwave background map-making in the presence of cross-correlated noise
• A Dictionary Approach to EBSD Indexing
• Using CMB data to constrain non-isotropic Planck-scale modifications to Electrodynamics
• Helicity in the Large-Scale Galactic Magnetic Field
• What the Milky Way's Dwarfs tell us about the Galactic Center extended excess
• A Search for Neutrino Point-Source Populations in 7 Years of IceCube Data with Neutrino-count Statistics
• nazgul: A statistical approach to gamma-ray burst localization. Triangulation via non-stationary time-series models
• The link between E-B polarization modes and gas column density from interstellar dust emission
• Probing CMB Cold Spot through Local Minkowski Functionals
• Testing isotropy in the Two Micron All-Sky redshift survey with information entropy
• Searching for Dark Matter Sub-structure with HAWC
• Evidence for Neutrino Emission from X-Ray-bright Active Galactic Nuclei with IceCube
• Momentum space sampling of neutrinos in $N$-body simulations
• Atomic line radiative transfer with MCFOST I. Code description and benchmarking
• Beam profile sensitivity of the WMAP CMB power spectrum
• Spin characterisation of systematics in CMB surveys -- a comprehensive formalism
• A Global Astrometric Solution for Pan-STARRS referenced to ICRF2
• Detection and Removal of B-mode Dust Foregrounds with Signatures of Statistical Anisotropy
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• The spectral index of polarized diffuse Galactic emission between 30 and 44 GHz
• The SOUX AGN Sample: SDSS-XMM-Newton Optical, Ultraviolet and X-ray selected active galactic nuclei spanning a wide range of parameter space -- Sample definition
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Expansion History using the Genus Amplitude as a Standard Ruler
• Ultra high energy cosmic rays from super-heavy dark matter in the context of large exposure observatories
• Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
• An angular power spectrum analysis of the DRAO 1.4 GHz polarization survey: implications for CMB observations
• Cosmology with the Planck cluster sample
• Isolated pulsar population synthesis with simulation-based inference
• The impact of dipole straylight contamination on the alignment of low multipoles of CMB anisotropies
• Channeling in solid Xe, Ar and Ne direct dark matter detectors
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Shape of the Matter Power Spectrum
• Integrated Sachs-Wolfe map reconstruction in the presence of systematic errors
• On the suspected timing error in WMAP map-making
• BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP
• Measuring the Expansion of the Universe Through Changes in the CMB Photosphere
• A Well-Posed UV Completion for Simulating Scalar Galileons
• Sparse Bayesian mass-mapping with uncertainties: peak statistics and feature locations
• Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources
• LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB
• Searching for concentric low variance circles in the cosmic microwave background
• Global Far-Ultraviolet Properties of the Cygnus Loop
• Application of Contour Minkowski Tensor and $\mathcal{D}$ Statistic to the Planck $E$-mode data
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Foreground Bias From Parametric Models of Far-IR Dust Emission
• Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Constraining low redshift [CII] Emission by Cross-Correlating FIRAS and BOSS Data
• A Cross-correlation Study between IceCube Neutrino Events and the Fermi Unresolved Gamma-ray Sky
• New Constraints on Spatial Variations of the Fine Structure Constant from Clusters of Galaxies
• Reassessment of the dipole in the distribution of quasars on the sky
• INTEGRAL observations of GW170104
• Topology of Large-Scale Structures of Galaxies in Two Dimensions - Systematic Effects
• Extended analysis of CMB constraints on non-Gaussianity in isocurvature perturbations
• QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
• Hot pixel contamination in the CMB correlation function?
• CMB-S4 and the Hemispherical Variance Anomaly
• Spider Optimization II: Optical, Magnetic and Foreground Effects
• Quasar UV Luminosity Function at $3.5<z<5.0$ from SDSS Deep Imaging Data
• Revisiting constraints on (pseudo)conformal Universe with Planck data
• Euclid: Covariance of weak lensing pseudo-$C_{\ell }$ estimates. Calculation, comparison to simulations, and dependence on survey geometry
• Exact joint likelihood of pseudo-$C_{\ell }$ estimates from correlated Gaussian cosmological fields
• Towards detecting super-GeV dark matter via annihilation to neutrinos
• Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches
• Templated Anisotropic Analyses of the LISA Galactic Foreground
• The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-Sky Catalog Based on Gaia DR3
• Impact of the 1/f noise and the asymmetric beam on non-Gaussianity searches with Planck
• Identifying nearby sources of ultra-high-energy cosmic rays with deep learning
• Far-Ultraviolet Cooling Features of the Antlia Supernova Remnant
• Structure Generation by Irradiation: What can GLIMPSE teach us about the ISM structure?
• Weak Lensing Skew-Spectrum
• Fast CMB lensing using statistical interpolation on the sphere
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• New limit on pseudoscalar-photon mixing from WMAP Observations
• Non-Gaussianity of diffuse Galactic synchrotron emission at 408 MHz
• Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background
• Far-infrared excess emission as a tracer of disk-halo interaction
• Linearized iterative least-squares (LIL): A parameter fitting algorithm for component separation in multifrequency CMB experiments such as Planck
• Simulations for a next-generation UHECR observatory
• High-precision Monte-Carlo modelling of galaxy distribution
• Galaxy power spectrum and biasing results from the LOFAR Two-metre Sky Survey (first data release)
• TRINITY: a three-dimensional time-dependent radiative transfer code for in-vivo near-infrared imaging
• THOR: An Algorithm for Cadence-Independent Asteroid Discovery
• Probabilistic Cross-Identification in Crowded Fields as an Assignment Problem
• High-resolution HI and CO observations of high-latitude intermediate-velocity clouds
• Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross correlations
• Contribution of Radio Halos to the Foreground for SKA EoR Experiments
• Large angular scale fluctuations of near infrared extragalactic background light based on the IRTS observations
• Stochastic gravitational wave background mapmaking using regularised deconvolution
• No longer ballistic, not yet diffusive--the formation of cosmic ray small-scale anisotropies
• Rotating baryonic dark halos
• Morphology of CMB fields -- effect of weak gravitational lensing
• Galaxy blending effects in deep imaging cosmic shear probes of cosmology
• Galactic halo bubble magnetic fields and UHECR deflections
• Re-evaluating evidence for Hawking points in the CMB
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• Rapid localization of gravitational wave hosts with FIGARO
• The cosmic microwave background Cold Spot anomaly: the impact of sky masking and the expected contribution from the Integrated Sachs-Wolfe effect
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Testing for spectral index variations in polarised CMB foregrounds
• Constraints on ${\tau }_{\mathrm{NL}}$ from Planck temperature and polarization
• Wilkinson Microwave Anisotropy Probe 7-yr constraints on fNL with a fast wavelet estimator
• Cosmic microwave anisotropies in an inhomogeneous compact flat universe
• A new probe of magnetic fields in the pre-reionization epoch: II. Detectability
• Gamma-Ray Polarimetry of the Crab Pulsar Observed by POLAR
• Spin-induced offset stream self-crossing shocks in tidal disruption events
• Scale-dependent dipolar modulation and the quadrupole-octopole alignment in the CMB temperature
• LSST Survey Strategy in the Galactic Plane and Magellanic Clouds
• Probing the Diffuse Lyman-alpha Emission on Cosmological Scales: Lyα Emission Intensity Mapping Using the Complete SDSS-IV eBOSS Survey
• Testing the isotropy of high energy cosmic rays using spherical needlets
• A quantitative comparison of lunar orbital neutron data
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Hickson-like compact groups inhabiting different environments
• QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey
• Differentiable and accelerated spherical harmonic and Wigner transforms
• The first comprehensive Milky Way stellar mock catalogue for the Chinese Space Station Telescope Survey Camera
• Tomographic redshift dipole: Testing the cosmological principle
• A Novel CMB Component Separation Method: Hierarchical Generalized Morphological Component Analysis
• Real Space Approach to CMB deboosting
• Polarized Spots in Anisotropic Open Universes
• The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from MWA drift scan observations I: Validation and preliminary results
• The precision and accuracy of early Epoch of Reionization foreground models: comparing MWA and PAPER 32-antenna source catalogs
• Generative models of astrophysical fields with scattering transforms on the sphere
• A new map-making algorithm for CMB polarisation experiments
• Improved measurements of the TeV-PeV extragalactic neutrino spectrum from joint analyses of IceCube tracks and cascades
• Time-average based methods for multi-angular scale analysis of cosmic-ray data
• Impact of modelling foreground uncertainties on future CMB polarization satellite experiments
• Constraints on Neutrino Emission from Nearby Galaxies Using the 2MASS Redshift Survey and IceCube
• The most uniform distribution of points on the sphere
• The effect of the linear term on the wavelet estimator of primordial non-Gaussianity
• Planck intermediate results. LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect
• Cosmoglobe: Simulating zodiacal emission with ZodiPy
• Optical and UV surface brightness of translucent dark nebulae: Dust albedo, radiation field and fluorescence emission by H2
• Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB $E$-mode and $\mu$-distortion anisotropies
• Testing statistical Isotropy in Cosmic Microwave Background Polarization maps
• Magnetic elastomers as specific soft actuators -- predicting particular modes of deformation from selected configurations of magnetizable inclusions
• Jointly setting upper limits on multiple components of an anisotropic stochastic gravitational-wave background
• A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• The kinematic contribution to the cosmic number count dipole
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Constraints on primordial non-Gaussianity from the cross-correlation of DESI Luminous Red Galaxies and $Planck$ CMB lensing
• Quantifying the Interstellar Medium and Cosmic Rays in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop using Fermi-LAT Gamma-ray Observations
• Reconsidering seismological constraints on the available parameter space of macroscopic dark matter
• Searching For Fermi GRB Optical Counterparts With The Prototype Gravitational-Wave Optical Transient Observer (GOTO)
• Consistency of a needlet spectral estimator on the sphere
• Simulating the LOcal Web (SLOW) -- III: Synchrotron emission from the local cosmic web
• Cosmic-ray-induced H${}_2$ line emission: Astrochemical modeling and implications for JWST observations
• Modeling the cross power spectrum of Sunyaev-Zel'dovich and X-ray surveys
• Spin Needlets for Cosmic Microwave Background Polarization Data Analysis
• Gaia Data Release 1: The archive visualisation service
• A bimodal distribution of haze in Pluto's atmosphere
• Self-consistent redshift estimation using correlation functions without a spectroscopic reference sample
• Radiance Cascades: A Novel High-Resolution Formal Solution for Multidimensional Non-LTE Radiative Transfer
• Recent developments in astrophysical and cosmological exploitation of microwave surveys
• Angular distribution of cosmological parameters as a probe of inhomogeneities: a kinematic parametrisation
• High circular polarization of near infrared light induced by micron-size dust grains
• Direct reconstruction of spherical harmonics from interferometer observations of the CMB polarization
• Systematic effects induced by Half Wave Plate precession into Cosmic Microwave Background polarization measurements
• Local patch analysis for testing statistical isotropy of the Planck convergence map
• Cosmic microwave background anomalies viewed via Gumbel Statistics
• Metal Lines Associated with the Lyman-alpha Forest from eBOSS Data
• Impact of SZ cluster residuals in CMB maps and CMB-LSS cross-correlations
• What can be learnt from UHECR anisotropies observations Paper II: intermediate-scale anisotropies
• The Global Magneto-Ionic Medium Survey (GMIMS): The brightest polarized region in the Southern sky at 75cm and its implications for Radio Loop II
• Bayesian analysis of white noise levels in the 5-year WMAP data
• Local alignments of parsec-scale AGN radiojets
• Improved large scales interstellar dust foreground model and CMB solar dipole measurement
• Orthogonal BipoSH measures : Scrutinizing sources of isotropy violation
• Ray-tracing 3D dust radiative transfer with DART-Ray: code upgrade and public release
• Open high-level data formats and software for gamma-ray astronomy
• Three-Dimensional Modelling of Ionized Gas. I. Did very massive stars of different metallicities drive the second cosmic reionization?
• Planck intermediate results. VI: The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters
• Gravitational lensing of the cosmic microwave background by nonlinear structures
• Implementation of an efficient Bayesian search for gravitational wave bursts with memory in pulsar timing array data
• Testing the statistical isotropy of large scale structure with multipole vectors
• Non-Parametric Cell-Based Photometric Proxies for Galaxy Morphology: Methodology and Application to the Morphologically-Defined Star Formation -- Stellar Mass Relation of Spiral Galaxies in the Local Universe
• Harnessing the Population Statistics of Subhalos to Search for Annihilating Dark Matter
• Evidence for large-scale excesses associated with low HI column densities in the sky I. Dust excess
• The integrated angular bispectrum of weak lensing
• HIR4: Cosmological signatures imprinted on the cross correlation between 21-cm map and galaxy clustering
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Exploring suppressed long-distance correlations as the cause of suppressed large-angle correlations
• C IV Emission-line Detection of the Supernova Remnant RCW 114
• Do Cosmological Perturbations Have Zero Mean?
• Lensed CMB power spectrum biases from masking extragalactic sources
• The SPIIR online coherent pipeline to search for gravitational waves from compact binary coalescences
• Marginal distributions for cosmic variance limited CMB polarization data
• A Perturbative Analysis of Synchrotron Spectral Index Variation over Microwave Sky
• On the Coherence of WMAP and Planck Temperature Maps
• Diffuse Far-ultraviolet Observation of the Lupus Loop Region
• A method for reconstructing the Galactic magnetic field using dispersion of fast radio bursts and Faraday rotation of radio galaxies
• Symmetry of the CMB sky as a new test of its statistical isotropy. Non Cosmological Octupole?
• Kinematics of the Milky Way from the Gaia EDR3 red giants and sub-giants
• Direct Optimal Mapping for 21cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization Array
• Recovering the Tidal Field in the Projected Galaxy Distribution
• On the Measurement of the Helicity of Intergalactic Magnetic Fields Using Ultra-High-Energy Cosmic Rays
• Astrometric Weak Lensing with Gaia DR3 and Future Catalogs: Searches for Dark Matter Substructure
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• Testing isotropy of cosmos with WMAP and PLANCK data
• UHECR Echoes from the Council of Giants
• The Impact of Planetary Rotation Rate on the Reflectance and Thermal Emission Spectrum of Terrestrial Exoplanets Around Sun-like Stars
• A survey of lens spaces and large-scale CMB anisotropy
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Recent extensions to GALPROP
• Morphology of Weak Lensing Convergence Maps
• Ultrahigh energy cosmic rays from nearby starburst galaxies
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Searching for High Energy Neutrino counterpart signals; The case of the Fermi Bubbles signal and of Dark Matter annihilation in the inner Galaxy
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Noncommutative Geometry and the Primordial Dipolar Imaginary Power Spectrum
• Improving the LSST dithering pattern and cadence for dark energy studies
• Search for point sources of ultra-high energy photons with the Telescope Array surface detector
• Cosmological Parameters from CMB Maps without Likelihood Approximation
• Statistical isotropy violation in WMAP CMB maps resulting from non-circular beams
• Cosmic shear calibration with forward modeling
• Combining strong and weak lensing estimates in the Cosmos field
• Impact of Galactic dust non-Gaussianity on searches for B-modes from inflation
• Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• The PICASSO map-making code: application to a simulation of the QUIJOTE northern sky survey
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Fingerprint of Galactic Loop I on polarized microwave foregrounds
• Synchrotron emission from virial shocks around stacked OVRO-LWA galaxy clusters
• Impact of nonlinear growth of the large-scale structure on CMB B-mode delensing
• Isotropic non-Gaussian $g_{\mathrm{NL}}$-like toy models that reproduce the cosmic microwave background anomalies
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• 21-cm foreground removal using AI and frequency-difference technique
• A Blueprint for the Milky Way's Stellar Populations. IV. A String of Pearls $-$ the Galactic Starburst Sequence
• The effect of systematics on polarized spectral indices
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• Influence of Planck foreground masks in the large angular scale quadrant CMB asymmetry
• Forecasts of CMB lensing reconstruction of AliCPT-1 from the foreground cleaned polarization data
• Introducing constrained matched filters for improved separation of point sources from galaxy clusters
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Improved Dark Energy Detection through the Polarization-assisted WMAP-NVSS ISW Correlation
• Polar ionospheric currents and high temporal resolution geomagnetic field models
• SAGUARO: Time-domain Infrastructure for the Fourth Gravitational-wave Observing Run and Beyond
• CMB Anisotropy Induced by a Moving Straight Cosmic String
• Testing the ABS method with the simulated Planck temperature maps
• Box Replication Effects in Weak Lensing Light-cone Construction
• Search for multi-messenger signals in NOvA coincident with LIGO/Virgo detections
• The Kinematic Structure of Magnetically Aligned HI Filaments
• A weakly random Universe?
• Asymmetry of the CMB map: local and global anomalies
• The CMB cold spot under the lens: ruling out a supervoid interpretation
• Multi-Component Imaging of the Fermi Gamma-ray Sky in the Spatio-spectral Domain
• Growing Supermassive Black Holes by Chaotic Accretion
• Towards a robust estimation of orientation parameters between ICRF and $Gaia$ celestial reference frames
• Joint Minkowski Functionals and Bispectrum Constraints on Non-Gaussianity in the CMB
• Impact of extragalactic point sources on the low-frequency sky spectrum and cosmic dawn global 21-cm measurements
• Galaxy cluster SZ detection with unbiased noise estimation: an iterative approach
• A study of Dipolar Signal in distant Quasars with various observables
• Statistical properties of polarized CMB foreground maps
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• A Strong Test of the Dark Matter Origin of the 1.4 TeV DAMPE Signal Using IceCube Neutrinos
• Harmonic analysis of isotropic fields on the sphere with arbitrary masks
• BeyondPlanck X. Planck LFI frequency maps with sample-based error propagation
• Posterior sampling for inverse imaging problems on the sphere in seismology and cosmology
• A Generalized Doppler and Aberration Kernel for Frequency-Dependent Cosmological Observables
• Uniform Modelling of the Stellar Density of Thirteen Tidal Streams within the Galactic Halo
• Can supernova shells feed supermassive black holes in galactic nuclei?
• Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
• Constraints on Equivalence Principle Violation from Gamma Ray Bursts
• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• Optimized Large-Scale CMB Likelihood And Quadratic Maximum Likelihood Power Spectrum Estimation
• How real-time cosmology can distinguish between different anisotropic models
• Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach
• Modeling the non-recycled Fermi gamma-ray pulsar population
• Iterative map-making with two-level preconditioning for polarized Cosmic Microwave Background data sets
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• Galactic Magnetic Turbulence from Radio data
• Efficient least-squares basket-weaving
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• Coincident SZ and $\gamma$-ray signals from cluster virial shocks
• Adaptive Langevin Sampler for Separation of t-Distribution Modelled Astrophysical Maps
• The halo bias for number counts on the light cone from relativistic N-body simulations
• Galaxy shapes in Magneticum. I. Connecting stellar and dark matter shapes to dynamical and morphological galaxy properties and the large-scale structure
• B-mode constraints from Planck low multipole polarisation data
• Temperature and Polarization Patterns in Anisotropic Cosmologies
• Revisiting the large-scale CMB anomalies: The impact of the SZ signal from the Local Universe
• Modelling the spinning dust emission from LDN 1780
• Main-belt and Trojan Asteroid Phase Curves from the ATLAS Survey
• Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
• QUIJOTE Scientific Results -- XVII. Studying the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
• Dust Scattering In Turbulent Media: Correlation Between The Scattered Light and Dust Column Density
• Symmetries of CMB Temperature Correlation at Large Angular Separations
• Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
• Identifying RR Lyrae in the ZTF DR3 dataset
• Large-Scale Polarized Foreground Component Separation for Planck
• Multipole vectors of completely random microwave skies for $l\le 50$
• Accelerating Cosmic Microwave Background map-making procedure through preconditioning
• Cross-Correlation analysis of WMAP and EGRET in Wavelet Space
• Data calibration for the MASCARA and bRing instruments
• Testing the isotropy of the log N - log S slope for the NVSS radio catalogue
• The Cosmic Foreground Explorer (COFE): A balloon-borne microwave polarimeter to characterize polarized foregrounds
• The Dust Extinction Curve: Beyond R(V)
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Ellipticity of Structures in CMB Sky Maps
• BeyondPlanck VIII. Efficient Sidelobe Convolution and Correction through Spin Harmonics
• Detection of new point-sources in WMAP Cosmic Microwave Background (CMB) maps at high Galactic latitude. A new technique to extract point sources from CMB maps
• A tomographic spherical mass map emulator of the KiDS-1000 survey using conditional generative adversarial networks
• Weak Lensing Trispectrum and Kurt-Spectra
• Footprints of Doppler and Aberration Effects in CMB Experiments: Statistical and Cosmological Implications
• MAXI/SSC All-sky maps from 0.7 keV to 4 keV
• ESASky SSOSS: Solar System Object Search Service and the case of Psyche
• Cosmic Covariance and the Low Quadrupole Anisotropy of the Wilkinson Microwave Anisotropy Probe (WMAP) Data
• A Comparison of Popular Point Configurations on ${\mathbb{S}}^2$
• Spherical harmonic transform with GPUs
• The Photo-Astrometric Vertical Tracer Density of the Milky Way I: The Method
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• An unbiased method of measuring the ratio of two data sets
• Cosmic ray acceleration to ultrahigh energy in radio galaxies
• Global distribution of far-ultraviolet emissions from highly ionized gas in the Milky Way
• The density distributions of cosmic structures: impact of the local environment on weak-lensing convergence
• Euclid preparation. LIX. Angular power spectra from discrete observations
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• The geometrical meaning of statistical isotropy of smooth random fields in two dimensions
• Stellar Reddening Based Extinction Maps for Cosmological Applications
• Statistical nature of non-Gaussianity from cubic order primordial perturbations: CMB map simulations and genus statistic
• Optimal machine-driven acquisition of future cosmological data
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• Improving initialization and evolution accuracy of cosmological neutrino simulations
• Optimal analysis of azimuthal features in the CMB
• Cosmic Sculpture: A new way to visualise the Cosmic Microwave Background
• Reconstruction of CMB Temperature Anisotropies with Primordial CMB Induced Polarization in Galaxy Clusters
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Sparse point-source removal for full-sky CMB experiments: application to WMAP 9-year data
• Enabling discovery of solar system objects in large alert data streams
• Validation Solutions to the Full-Sky Radio Interferometry Measurement Equation for Diffuse Emission
• Testing for foreground residuals in the Planck foreground cleaned maps: A new method for designing confidence masks
• Using the 2-MASS Photometric Redshift Survey to optimize LIGO Follow-Up Observations
• Can galactic dark matter substructure contribute to the cosmic gamma-ray anisotropy?
• Global Optimization for Future Gravitational Wave Detectors' Sites
• Possible signature of distant foreground in the Planck data
• Observatory/data centre partnerships and the VO-centric archive: The JCMT Science Archive experience
• Core orientations and magnetic fields in isolated molecular clouds
• The BINGO Project IX: Search for Fast Radio Bursts -- A Forecast for the BINGO Interferometry System
• Fast analytical calculation of the random pair counts for realistic survey geometry
• Testing the Cosmological Principle: On the Time Dilation of Distant Sources
• Near-infrared extinction with discretised stellar colours
• Model of the polarized foreground diffuse Galactic emissions from 33 to 353 GHz
• Planck intermediate results. LV. Reliability and thermal properties of high-frequency sources in the Second Planck Catalogue of Compact Sources
• Cosmological constraints from low redshift 21 cm intensity mapping with machine learning
• The Milky Way as Seen by Classical Cepheids I: Distances Based on Mid-infrared Photometry
• Search for line signal candidates in the Fermi-LAT data
• The Kolmogorov-Smirnov test for the CMB
• Foreground removal with ILC methods for AliCPT-1
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data
• Functional Penalised Basis Pursuit on Spheres
• A Pixel Space Method for Testing Dipole Modulation in the CMB Polarization
• The integrated angular bispectrum
• QUIJOTE scientific results -- V. The microwave intensity and polarisation spectra of the Galactic regions W49, W51 and IC443
• Toward a test of Gaussianity of a gravitational wave background
• Data driven foreground clustering approach to component separation in multifrequency CMB experiments: A new Planck CMB map
• Electromagnetic counterparts to gravitational wave events from Gaia
• Biparametric Adaptive Filter: detection of compact sources in complex microwave backgrounds
• Camouflaged galactic CMB foregrounds: total and polarized contributions of the kinetic Sunyaev Zeldovich effect
• Observation of Cosmic-Ray Anisotropy in the Southern Hemisphere with 12 yr of Data Collected by the IceCube Neutrino Observatory
• How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
• CMB Lensing and Giant Rings
• The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra
• Deep view of the intracluster light in the Coma cluster of galaxies
• The completeness of the open cluster census towards the Galactic anticentre
• Connecting the time domain community with the Virtual Astronomical Observatory
• Growth and anisotropy of ionization fronts near high redshift quasars in the MassiveBlack simulation
• A Blueprint for the Milky Way's Stellar Populations. V. 3D Local Dust Extinction
• Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Far-Ultraviolet Spectral Images of the Vela Supernova Remnant: Supplements and Comparisons with other Wavelength Images
• The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Structures in the Planck map of the CMB
• The Mysterious Sickle Object in the Carina Nebula: A stellar wind induced bow shock grazing a clump?
• Tree-based solvers for adaptive mesh refinement code FLASH -- III: a novel scheme for radiation pressure on dust and gas and radiative transfer from diffuse sources
• A Deep Learning Earth System Model for Efficient Simulation of the Observed Climate
• Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
• Local properties of the large-scale peaks of the CMB temperature
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• The PAU Survey: Narrow-band image photometry
• A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra
• eROSITA narrowband maps at the energies of soft X-ray emission lines
• Rapid Development of Interferometric Software Using MIRIAD and Python
• SCONCE: A cosmic web finder for spherical and conic geometries
• Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• A Search for Cosmic Neutrino and Gamma-Ray Emitting Transients in 7.3 Years of ANTARES and Fermi LAT Data
• Angular distribution of cosmological parameters as a probe of space-time inhomogeneities
• HCGrid: A Convolution-based Gridding Framework for RadioAstronomy in Hybrid Computing Environments
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Non-parametric maximum likelihood component separation for CMB polarization data
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Correlation properties of the maps of the NVSS survey and WMAP ILC
• Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
• Forecast of foreground cleaning strategies for AliCPT-1
• An Unbiased Estimator of the Full-sky CMB Angular Power Spectrum at Large Scales using Neural Networks
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Solving linear equations with messenger-field and conjugate gradients techniques - an application to CMB data analysis
• The First MAXI/SSC Catalog of X-ray Sources in 0.7--7.0~keV
• Multi-Messenger Astrophysics with the Cosmic Neutrino Background
• All-sky analysis of astrochronometric signals induced by gravitational waves
• Untargeted Bayesian search of anisotropic gravitational-wave backgrounds through the analytical marginalization of the posterior
• A Fast and Accurate Algorithm for Spherical Harmonic Analysis on HEALPix Grids with Applications to the Cosmic Microwave Background Radiation
• Modelling the WMAP large-angle anomalies as an effect of a local density inhomogeneity
• Fast scalar quadratic maximum likelihood estimators for the CMB B-mode power spectrum
• A close examination of cosmic microwave background mirror-parity after Planck
• Scalar quadratic maximum likelihood estimators for the CMB cross power spectrum
• Isotropy-Violation Diagnostics for $B$-mode Polarization Foregrounds to the Cosmic Microwave Background
• Simulating image coaddition with the Nancy Grace Roman Space Telescope: II. Analysis of the simulated images and implications for weak lensing
• Consistency of CMB experiments beyond cosmic variance
• DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations
• Extragalactic Fields Optimized for Adaptive Optics
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Optimising LSST Observing Strategy for Weak Lensing Systematics
• Estimation of Full Sky Power Spectrum between Intermediate to Large Angular Scales from Partial Sky CMB Anisotropies using Artificial Neural Network
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• The Second Catalog of Interplanetary Network Localizations of Konus Short Duration Gamma-Ray Bursts
• BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics
• Future magnetic fields studies using the Planck Surveyor experiment
• Search for Sources of High Energy Neutrons with Four Years of Data from the IceTop Detector
• Fully data-driven time-delay interferometry with time-varying delays
• Inference of the optical depth to reionization $\tau$ from $\text{Planck}$ CMB maps with convolutional neural networks
• Sparse Inpainting and Isotropy
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• Spectropolarimetry and spectral decomposition of high-accreting Narrow Line Seyfert 1 galaxies
• Clustering at 74 MHz
• Galaxy clusters as probes for cosmology and dark matter
• Synthetic dust polarization emission maps at 353 GHz for an observer placed inside a Local Bubble-like cavity
• Joint Bayesian estimation of tensor and lensing B-modes in the power spectrum of CMB polarization data
• Intensity-Coupled-Polarization in Instruments with a Continuously Rotating Half-Wave Plate
• Compactified Cosmological Simulations of the Infinite Universe
• RGB photometric calibration of 15 million Gaia stars
• Technologies for supporting high-order geodesic mesh frameworks for computational astrophysics and space sciences
• Bayesian foreground analysis with CMB data
• One-point fluctuation analysis of IceCube neutrino events outlines a significant unassociated isotropic component and constrains the Galactic contribution
• CMB map restoration
• Accurate estimation of angular power spectra for maps with correlated masks
• ISW in $\Lambda$CDM or something else?
• Scalar quantities as detectors of non-Gaussianity on CMB maps
• Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars
• A search for nontoroidal topological lensing in the Sloan Digital Sky Survey quasar catalog
• Search for non-Gaussianities in the WMAP data with the Scaling Index Method
• Towards a more robust reconstruction method for IceCube's real-time program
• Foreground Maps in WMAP frequency bands
• Probing supervoids with weak lensing
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Aspect ratios of far-infrared and H i filaments in the diffuse interstellar medium at high Galactic latitudes
• A multifrequency angular power spectrum analysis of the Leiden polarization surveys
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Observing small-scale $\gamma$-ray anisotropies with the Cherenkov Telescope Array
• Fast, exact (but unstable) spin spherical harmonic transforms
• The CMB lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog
• Planck CO revisited: Improved CO line emission maps from Planck space mission observations
• The C-Band All-Sky Survey (C-BASS): New Constraints on the Integrated Radio Spectrum of M 31
• GWOPS: A VO-technology Driven Tool to Search for the Electromagnetic Counterpart of Gravitational Wave Event
• Large- and Medium-Scale Anisotropies in the Arrival Directions of Cosmic Rays observed with KASCADE-Grande
• CMB statistical isotropy confirmation at all scales using multipole vectors
• Radio-loudness statistics of quasars from Quaia-VLASS
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
• Estimation of Expected Euler Characteristic Curves of Nonstationary Smooth Gaussian Random Fields
• Simulated Predictions for HI at $z=3.35$ with the Ooty Wide Field Array (OWFA) -- II: Foreground Avoidance
• Hemispherical Variance Anomaly and Reionization Optical Depth
• ARC: Adaptive Ray-tracing with CUDA, a New Ray Tracing Code for Parallel GPUs
• High Speed Source Localization in Searches for Gravitational Waves from Compact Object Collisions
• Parity in Planck full-mission CMB temperature maps
• BeyondPlanck II. CMB map-making through Gibbs sampling
• Statistics of non-polarized points in the CMB polarization maps
• A Spherical Harmonic Analysis of the Ooty Wide Field Array (OWFA) Visibility Signal
• A forecast of the sensitivity on the measurement of the optical depth to reionization with the GroundBIRD experiment
• Study of systematics effects on the Cross Power Spectrum of 21 cm Line and Cosmic Microwave Background using Murchison Widefield Array Data
• High-resolution CARMA Observation of Molecular Gas in the North America and Pelican Nebulae
• The embedded ring-like feature and star formation activities in G35.673-00.847
• Detecting Electron Density Fluctuations from Cosmic Microwave Background Polarization using a Bispectrum Approach
• Angular systematics-free cosmological analysis of galaxy clustering in configuration space
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• A selection function toolbox for subsets of astronomical catalogues
• A Joint Ranking Statistic for Multi-messenger Astronomical Searches with Gravitational Waves
• Anomalies in the topology of the temperature fluctuations in the cosmic microwave background: An analysis of the $\text{NPIPE}$ and $\text{FFP10}$ data releases
• Analysis of the Amplitude of the Sunyaev-Zel'dovich Effect out to Redshift z=0.8
• Preconditioner-free Wiener filtering with a dense noise matrix
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey
• Testing synchrotron models and frequency resolution in BINGO 21 cm simulated maps using GNILC
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Galaxy-galaxy and galaxy-cluster lensing with the SDSS and FIRST surveys
• Searching for high-energy gamma-ray counterparts to Gravitational Wave sources with Fermi-LAT: a needle in a haystack
• Orbital parallax of binary systems compared to GAIA DR3 and the parallax zero-point offset at bright magnitudes
• Treasure Maps for Detections of Extreme Energy Cosmic Rays
• Model-independent search for anisotropies in stochastic gravitational-wave backgrounds and application to LIGO-Virgo's first three observing Runs
• The Tracking Tapered Gridded Estimator (TTGE) for the power spectrum from drift scan observations
• Caustic-like Structures in UHECR Flux after Propagation in Turbulent Intergalactic Magnetic Fields
• Extracting the gamma-ray source-count distribution below the Fermi-LAT detection limit with deep learning
• Field-level multiprobe analysis of the CMB, integrated Sachs-Wolfe effect, and the galaxy density maps
• Systematic error mitigation for the PIXIE Fourier transform spectrometer
• Estimating SI violation in CMB due to non-circular beam and complex scan in minutes
• Search for continuous gravitational waves directed at sub-threshold radiometer candidates in O3 LIGO data
• Protostellar disk accretion in turbulent filaments
• Primordial Non-Gaussianities of inflationary step-like models
• Forecast of CMB TB and EB correlations for AliCPT-1
• Sensitivity of Bayesian 21 cm power spectrum estimation to foreground model errors
• Detecting the tensor-to-scalar ratio with the pure pseudospectrum reconstruction of $B$-mode
• On the contributions of extragalactic CO emission lines to ground-based CMB observations
• Diffuse Synchrotron Emission from Galactic Cosmic Ray Electrons
• The magnetic field of the Radcliffe Wave: starlight polarization at nearest approach to the Sun
• FSH3D: 3D Representation via Fibonacci Spherical Harmonics
• An Independent Measure of the Kinematic Dipole from SDSS
• Confirming the Tidal Tails of the Young Open Cluster Blanco 1 with TESS Rotation Periods
• The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium
• The Q/U Imaging Experiment: Polarization Measurements of Radio Sources at 43 and 95 GHz
• Euclid: Relativistic effects in the dipole of the 2-point correlation function
• Simulating image coaddition with the Nancy Grace Roman Space Telescope: III. Software improvements and new linear algebra strategies
• Correlating Fourier phase information with real-space higher order statistics
• A Differentiable, End-to-End Forward Model for 21 cm Cosmology: Estimating the Foreground, Instrument, and Signal Joint Posterior
• Map-level baryonification: unified treatment of weak lensing two-point and higher-order statistics
• Using CMB polarization to constrain the anomalous nature of the Cold Spot with an incomplete sky-coverage
• Exploring local fNL estimators based on the binned bispectrum
• Non-Gaussianity and CMB aberration and Doppler
• Towards efficient and optimal analysis of CMB anisotropies on a masked sky
• A search for concentric rings with unusual variance in the 7-year WMAP temperature maps using a fast convolution approach
• Cosmological Parameters from a re-analysis of the WMAP-7 low resolution maps
• Forecasting Supernova Observations with the CSST: I. Photometric Samples
• Search for UHE Photons from Gravitational Wave Sources with the Pierre Auger Observatory
• Astrophysical interpretation of the medium scale clustering in the ultra-high energy sky
• On the Galactic Halos Rotation by Planck Data
• QUIJOTE scientific results -- VI. The Haze as seen by QUIJOTE
• Bayesian noise estimation for non-ideal CMB experiments
• Parallel Spherical Harmonic Transforms on heterogeneous architectures (GPUs/multi-core CPUs)
• Mitigating Bias in CMB B-modes from Foreground Cleaning Using a Moment Expansion
• J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools II. Second data release and machine learning methodology
• Impact of thermal SZ effect on cross-correlations between Planck CMB lensing and SDSS galaxy density fields
• Signatures of Recent Cosmic-Ray Acceleration in the High-Latitude $\gamma$-Ray Sky
• Characterising solar surface convection using Doppler measurements
• Semianalytical Approach for Sky Localization of Gravitational Waves
• Revised planet brightness temperatures using the Planck/LFI 2018 data release
• Simulating instrumental systematics of Cosmic Microwave Background experiments with s4cmb
• The primordial non-Gaussianity of local type (f_NL) in the WMAP 5-year data: the length distribution of CMB skeleton
• The evolution of Luminous Red Galaxies in the Sloan Digital Sky Survey 7th data release
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Optimal strategy for polarization modulation in the LSPE-SWIPE experiment
• Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
• Enabling Radiative Transfer on AMR grids in CRASH
• Efficient Catalog Matching with Dropout Detection
• Studies of the UHECR propagation in the Galactic Magnetic Field
• Machine Learning Etudes in Astrophysics: Selection Functions for Mock Cluster Catalogs
• Identification of galaxy clusters in cosmic microwave background maps using the Sunyaev-Zel'dovich effect
• Limits on Semiclassical Fluctuations in the Primordial Universe
• The Kinetic Sunyaev-Zel'dovich Effect Due to the Electrons of Our Galaxy
• Predicting CMB dust foreground using galactic 21 cm data
• Suppressing the thermal SZ-induced variance in CMB-cluster lensing estimators
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• Spectral imaging of the thermal Sunyaev-Zel'dovich effect in X-COP galaxy clusters: method and validation
• The 8-parameter Fisher-Bingham distribution on the sphere
• Mapping the Milky Way in 5-D with 170 Million Stars
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• On the impact of the galaxy window function on cosmological parameter estimation
• Detecting Extraterrestrial Civilizations That Employ an Earth-level Deep Space Network
• Cosmic topology. Part IVa. Classification of manifolds using machine learning: a case study with small toroidal universes
• Diversity of new Martian crater clusters informs meteoroid atmospheric interactions
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Redshift drift in a universe with structure III: Numerical relativity
• Sensitivity Estimation for Dark Matter Subhalos in Synthetic Gaia DR2 using Deep Learning
• An analytical model for the magnetic field in the thick shell of Galactic bubbles with uniform initial conditions
• Imaging the positron annihilation line with 20 years of INTEGRAL/SPI observations
• Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
• Clustering properties of the CatWISE2020 quasar catalogue and their impact on the cosmic dipole anomaly
• ARKCoS: Artifact-Suppressed Accelerated Radial Kernel Convolution on the Sphere
• Full sky Integrated Sachs-Wolfe maps for the MICE Grand Challenge lightcone simulation
• Simultaneous determination of the cosmic birefringence and miscalibrated polarization angles II: Including cross frequency spectra
• Generation of high circular polarization of interstellar Lyman $\alpha$ radiation triggering biological homochirality
• Hawaii Two-0: High-redshift galaxy clustering and bias
• Estimates of unresolved point sources contribution to WMAP 5
• Testing Quadratic Maximum Likelihood estimators for forthcoming Stage-IV weak lensing surveys
• CO Component Estimation Based on the Independent Component Analysis
• Gravitational wave effects on astrometric observables
• Precise self-calibration of interloper bias in spectroscopic surveys
• DES Science Portal: Creating Science-Ready Catalogs
• Multi-Resolution HEALPix Maps for Multi-Wavelength and Multi-Messenger Astronomy
• General solutions of the leakage in integral transforms and applications to the EB-leakage and detection of the cosmological gravitational wave background
• Significant foreground unrelated non-acoustic anisotropy on the one degree scale in WMAP 5-year observations
• Seeing the halo rotation of nearby spiral galaxies using Planck data
• A search for cosmological anisotropy using the Lyman alpha forest from SDSS quasar spectra
• High-Significance Detection of Correlation Between the Unresolved Gamma-Ray Background and the Large Scale Cosmic Structure
• Point Source Detection with Fully-Convolutional Networks: Performance in Realistic Simulations
• Multiscale analysis of the CMB temperature derivatives
• Time variability of TeV cosmic ray sky map
• An Intermediate Velocity HI Cloud Falling to the Galactic Disk; Possible Evidence for Low Metallicity HI Gas Originated Outside the Galactic Disk
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• MAPPRAISER: A massively parallel map-making framework for multi-kilo pixel CMB experiments
• Partial CMB maps: bias removal and optimal binning of the angular power spectrum
• Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
• Lensing Bias to CMB Polarization Measurements of Compensated Isocurvature Perturbations
• Geographic and seasonal influences on optical followup of gravitational wave events
• Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane?
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
• Orbifold Line Topology and the Cosmic Microwave Background
• Tracing the magnetic field morphology of the LDN 1172/1174 cloud complex
• The White Mountain Polarimeter Telescope and an Upper Limit on CMB Polarization
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• Accurate Kappa Reconstruction Algorithm for masked shear catalog (AKRA)
• Footprints of Loop I on Cosmic Microwave Background Maps
• The effect of cosmic variance on the characteristics of dust polarization power spectra
• Co-estimation of core and lithospheric magnetic fields by a maximum entropy method
• Fast and precise way to calculate the posterior for the local non-Gaussianity parameter $f_{\text{nl}}$ from cosmic microwave background observations
• Joint deconvolution and unsupervised source separation for data on the sphere
• AuriDESI: Mock Catalogues for the DESI Milky Way Survey
• The kinetic Sunyaev-Zel'dovich effect from the diffuse gas in the Local Group
• A statistical analysis of a Galactic all sky survey at 1.4 GHz
• The FLAMINGO project: cosmology with the redshift dependence of weak gravitational lensing peaks
• Discovery of the Goat Horn complex: a $\sim 1000$ deg${}^2$ diffuse X-ray source connected to radio loop XII
• Gas and Cosmic-Ray Properties in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop as Revealed by HI Line Profiles, Dust, and Gamma-Ray Data
• WHIM-hunting through cross-correlation of optical and SZ effect data in the Virgo cluster filaments
• A deconvolution map-making method for experiments with circular scanning strategies
• Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
• Galactic foregrounds and CMB polarization
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• Baryon Pasting the Uchuu Lightcone Simulation
• The first direct measurement of gravitational potential decay rate at cosmological scales and improved dark energy constraint
• Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution
• A Constrained NILC method for CMB B mode observations
• HLC2: a highly efficient cross-matching framework for large astronomical catalogues on heterogeneous computing environments
• Anisotropy of TeV and PeV cosmic rays with IceCube and IceTop
• Testing inhomogeneous cosmography in our cosmic neighborhood using CosmicFlows-4
• The spectral energy distribution of the Carina nebula from far infrared to radio wavelengths
• Masking versus removing point sources in CMB data: the source corrected WMAP power spectrum from new extended catalogue
• The Statistics of Extended Debris Disks Measured with Gaia and Planck
• Smoothing methods comparison for CMB E- and B-mode separation
• A Bayesian estimate of the CMB-large-scale structure cross-correlation
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• All-Sky Search for Transient Astrophysical Neutrino Emission with 10 Years of IceCube Cascade Events
• The interplay of CMB temperature lensing power reconstruction with primordial non-Gaussianity of local type
• The anomaly of the CMB power with the latest Planck data
• Comparing the Photometric Calibration of DESI Imaging and Gaia Synthetic Photometry
• The distribution of ultra-high-energy cosmic rays along the supergalactic plane measured at the Pierre Auger Observatory
• On the effect of projections on convergence peak counts and Minkowski functionals
• Taller in the saddle: constraining CMB physics using saddle points
• Bayesian decomposition of the Galactic multi-frequency sky using probabilistic autoencoders
• Impact of Galactic magnetic field modelling on searches of point sources via UHECR-Neutrino correlations
• The Simons Observatory: Assessing the Impact of Dust Complexity on the Recovery of Primordial $B$-modes
• Vizic: A Jupyter-based Interactive Visualization Tool for Astronomical Catalogs
• Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science: Incremental Templates in Year 1
• Is the local Hubble flow consistent with concordance cosmology?
• Unbiased estimation of gravitational-wave anisotropies from noisy data
• Searching for All-Scale Anisotropies in the Arrival Directions of Cosmic Rays above the Ankle
• The Orion-Taurus ridge: a synchrotron radio loop at the edge of the Orion-Eridanus superbubble
• The Cherenkov Telescope Array Will Test Whether Pulsars Generate the Galactic Center Gamma-Ray Excess
• Determining the Scale Length and Height of the Milky Way's Thick Disc Using RR~Lyrae
• The T-E correlation coefficient of Planck legacy data
• A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• Blind Map Level Systematics Cleaning: A Quadratic Estimator Approach
• A High-Significance Measurement of Correlation Between Unresolved IRAS Sources and Optically-Selected Galaxy Clusters
• Spherical framelets from spherical designs
• Statistical estimation of full-sky radio maps from 21cm array visibility data using Gaussian constrained realizations
• Probing Cosmology beyond $\Lambda$CDM using the SKA
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• Future Radio Continuum Cosmology Clustering Surveys
• Magnetic fields and young stellar objects in cometary cloud LDN 1616
• Global Mapping of Surface Composition on an Exo-Earth Using Sparse Modeling
• Three-dimensional modeling of ionized gas. II. Spectral energy distributions of massive and very massive stars in stationary and time-dependent modeling of the ionization of metals in HII regions
• On the structure of galactic halos and the microwave temperature maps
• Polarization of Cosmic Microwave Background
• Dynamical considerations for life in multihabitable planetary systems
• Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: II. Anisotropic large-scale coherence in hot gas, galaxies, and dark matter
• Constraints on fNL from Wilkinson Microwave Anisotropy Probe 7-year data using a neural network classifier
• Tracing PAH Emission in $\lambda$-Orionis Using COBE/DIRBE Data
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure
• The bandmerged Planck Early Release Compact Source Catalogue: Probing sub-structure in the molecular gas at high Galactic latitude
• An Accurate Reconstruction of CMB E Mode Signal over Large Angular Scales using Prior Information of CMB Covariance Matrix in ILC Algorithm
• Holographic Beam Measurements of the Canadian Hydrogen Intensity Mapping Experiment (CHIME)
• Effects of observer peculiar motion on the isotropic background frequency spectrum: from monopole to higher multipoles
• A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimators
• The Polarization Signature of Local Bulk Flows
• FaVeST: Fast Vector Spherical Harmonic Transforms
• Narrow-line HI and cold structures in the ISM
• Model Independent Foreground Power Spectrum Estimation using WMAP 5-year Data
• Reconstruction of Missing Data using Iterative Harmonic Expansion
• Characterization of Extragalactic Point-Sources on E- and B-mode Maps of the CMB Polarization
• Searching for Stringy Topologies in the Cosmic Microwave Background
• Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
• A CMB Gibbs sampler for localized secondary anisotropies
• Axion signals from neutron star populations
• The signature of the Warm Hot Intergalactic Medium in WMAP and the forthcoming PLANCK data
• Cross-Observatory Coordination with tilepy: A Novel Tool for Observations of Multi-Messenger Transient Events
• Searching for Radio Transients with Inverted Spectra in Epoch 1 of VLASS and VCSS, and Identification of a Sample of Candidate Relativistic Nuclear Transients
• The 4MOST-Cosmology Redshift Survey: Target Selection of Bright Galaxies and Luminous Red Galaxies
• The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance
• Optimal Follow-Up of Gravitational-Wave Events with the UltraViolet EXplorer (UVEX)
• Level correlations of the CMB temperature angular power spectrum
• PRIN/SPRIN: On Extracting Point-wise Rotation Invariant Features
• Efficient data structures for masks on 2D grids
• Determining our peculiar velocity from the aberration in the cosmic microwave background
• VIDE: The Void IDentification and Examination toolkit
• The Kinetic Sunyaev-Zel'dovich effect of the Milky Way Halo
• Position-Dependent Correlation Function of Weak Lensing Convergence
• Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data
• The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
• A new look at the integrated radio/microwave continuum spectrum of Galactic supernova remnant IC443
• Doppler imaging combined with high-cadence photometry. I. Revisiting the surface of a pre-main-sequence flare star
• Probing the astrophysical origin of high-energy cosmic-ray electrons with Monte Carlo simulation
• The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voids
• Searching for Anisotropy in the Gravitational Wave Background Using the Parkes Pulsar Timing Array
• Constraints on primordial non-Gaussianity from Quaia
• Exploring the Solar System with the NOIRLab Source Catalog I: Detecting Objects with CANFind
• New evidence for lack of CMB power on large scales
• Optimal estimator for the amplitude of the bispectrum from IR sources
• A New Galactic Extinction Map in High Ecliptic Latitudes
• The SDSS DR7 Galaxy Angular Power Spectrum: Volume-Limits and Galaxy Morphology
• Cross-correlating IceCube neutrinos with a large set of galaxy samples around redshift z ~ 1
• Associating LOFAR Galactic Faraday structures with the warm neutral medium
• Phase-resolved gamma-ray spectroscopy of the Crab pulsar observed by POLAR
• Spherical cap discrepancy of perturbed lattices under the Lambert projection
• Can anisotropy in the galaxy distribution tell the bias?
• Testing Gaussianity in the WMAP data of OT foreground reduced map
• Dynamic Zoom Simulations: a fast, adaptive algorithm for simulating lightcones
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• A 20 GHz bright sample for δ > +72°: I. Catalogue
• A spatial-correlation analysis of the cubic 3-torus topology based on the Planck 2013 data
• Cross-correlating Planck with VST ATLAS LRGs: a new test for the ISW effect in the Southern Hemisphere
• The MeerKAT Absorption Line Survey (MALS) data release 3: Cold atomic gas associated with the Milky Way
• Scanning the Universe for Large-Scale Structures using Gamma-Ray Bursts
• Morphometry on the sphere: Cartesian and irreducible Minkowski tensors explained and implemented
• The Galactic interstellar medium has a preferred handedness of magnetic misalignment
• Revisiting the Local Interstellar Radiation Field using Gaia DR3
• Solid confirmation of the broad DIB around 864.8 nm using stacked Gaia-RVS spectra
• Constraining the average magnetic field in galaxy clusters with current and upcoming CMB surveys
• Modelling LAEs in the Epoch of Reionization with OBELISK
• Reflection Spectra of Accretion Disks Illuminated by an Off-Axis Corona
• Examining statistical isotropy of CMB low multipoles from Planck PR4 data
• Detection of an orthogonal alignment between parsec scale AGN jets and their host galaxies
• Distribution of Maximal Luminosity of Galaxies in the Sloan Digital Sky Survey
• Expanded Generalized Needlet Internal Linear Combination (eGNILC) Framework for the 21-cm Foreground Removal
• AKRA 2.0: Accurate Kappa Reconstruction Algorithm for masked shear catalog
• On the regularity of the covariance matrix of a discretized scalar field on the sphere
• Phase statistics of the WMAP 7 year data
• Foreground removal from WMAP 7yr polarization maps using an MLP neural network
• YOLO-CL cluster detection in the Rubin/LSST DC2 simulation
• Measuring our peculiar velocity from spectroscopic redshift surveys
• Joint inference of multiplicative and additive systematics in galaxy density fluctuations and clustering measurements
• Far-ultraviolet Emission-line Morphologies of the Supernova Remnant G65.3+5.7
• Recoiling Ion-Channeling in Direct Dark Matter Detectors
• Probing large-scale structures with the two-point function and the power spectrum: insights into cosmic clustering evolution
• Polarization and variability of compact sources measured in Planck time-ordered data
• QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $\rho$\,Ophiuchi, Perseus and W43
• Images of the Ultra-High Energy Cosmic Rays from Point Sources
• High-Performance Astrophysical Simulations and Analysis with Python
• Test for anisotropy in the mean of the CMB temperature fluctuation in spherical harmonic space
• Pixel space convolution for cosmic microwave background experiments
• Cross-Power Spectrum and Its Application on Window Functions in the WMAP data
• Study on the filters of atmospheric contamination in ground based CMB observation
• Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT
• Constraining a Model of the Radio Sky Below 6 MHz Using the Parker Solar Probe/FIELDS Instrument in Preparation for Upcoming Lunar-based Experiments
• Reconstruction of weak lensing mass maps for non-Gaussian studies in the celestial sphere
• Uncertainties of the 30-408 MHz Galactic emission as a calibration source for radio detectors in astroparticle physics
• Simulations of systematic effects arising from cosmic rays in the LiteBIRD space telescope, and effects on the measurements of CMB $B$-modes
• Relativistic matter bispectrum of cosmic structures on the light cone
• Imaging parity-violation in the CMB
• The RTApipe framework for the gamma-ray real-time analysis software development
• Detecting and characterizing pulsar haloes with the Cherenkov Telescope Array
• CU-JADE: A Method for Traversing Extinction Jumps along the Line of Sight
• Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 Data
• Consequences of constant elevation scans for instrumental systematics in Cosmic Microwave Background Experiments
• Triggered Population III star formation: the effect of H${}_2$ self-shielding
• The Universe is Brighter in the Direction of Our Motion: Galaxy Counts and Fluxes are Consistent with the CMB Dipole
• All-sky reconstruction of the primordial scalar potential from WMAP temperature data
• Maximum likelihood kinetic Sunyaev Zel'dovich velocity reconstruction
• The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey
• Detecting anomalies in CMB maps: a new method
• The STATiX pipeline for the detection of X-ray transients in three dimensions
• Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps
• QUIJOTE scientific results -- IX. Radio sources in the QUIJOTE-MFI wide survey maps
• Detecting Cosmic 21 cm Global Signal Using an Improved Polynomial Fitting Algorithm
• Simulation of the cosmic ray effects for the LiteBIRD satellite observing the CMB B-mode polarization
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• Ki-Pode: Keypoint-based Implicit Pose Distribution Estimation of Rigid Objects
• Spherical harmonics analysis of Fermi gamma-ray data and the Galactic dark matter halo
• Constraining the Anomalous Microwave Emission Mechanism in the S140 Star Forming Region with Spectroscopic Observations Between 4 and 8 GHz at the Green Bank Telescope
• CMB likelihood approximation for banded probability distributions
• Signature of a Cosmic String Wake at $z=3$
• The C-Band All-Sky Survey (C-BASS): Total intensity point-source detection over the northern sky
• A Bayesian ILC method for CMB B-mode posterior estimation and reconstruction of primordial gravity wave signal
• Cosmic microwave background constraints on the tensor-to-scalar ratio
• Extended Delta-map: a map-based foreground removal method for CMB polarization observations
• NeuralPDR: Neural Differential Equations as surrogate models for Photodissociation Regions
• Resolving Individual Signals in the Presence of Stochastic Background in Future Pulsar Timing Arrays
• Unifying supervised learning and VAEs -- coverage, systematics and goodness-of-fit in normalizing-flow based neural network models for astro-particle reconstructions
• Consistency tests for Planck and WMAP in the low multipole domain
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• Development of 2MASS Catalog Server Kit
• All-sky neutrino point-source search with IceCube combined track and cascade data
• Non-Gaussianity in the HILC foreground-reduced three-year WMAP CMB map
• An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples
• Self-supervised component separation for the extragalactic submillimeter sky
• Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission
• Polycomp: efficient and configurable compression of astronomical timelines
• Anisotropies in the diffuse gamma-ray background measured by Fermi LAT
• Bright stars observed by FIMS/SPEAR
• Hemispheric handedness in the Galactic synchrotron polarization foreground
• A new method to subdivide a spherical surface into equal-area cells
• First astrometric constraints on parity-violation in the gravitational wave background
• An evaluation of the LLC4320 global ocean simulation based on the submesoscale structure of modeled sea surface temperature fields
• Cosmic Ray contribution to the WMAP polarization data on the Cosmic Microwave Background
• Model independent variance cancellation in CMB lensing cross-correlations
• Tail Behaviour of Mexican Needlets
• ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network
• TeV Observations of the Galactic Plane with HAWC and Joint Analysis of GeV Data from Fermi
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Effects of boosting on extragalactic components: methods and statistical studies
• Constraints on the Emission of Gamma Rays from M31 with HAWC
• Statistical properties of Galactic synchrotron temperature and polarization maps -- a multi-frequency comparison
• Neural style transfer of weak lensing mass maps
• CMB Anomalies from Imperfect Dark Energy: Confrontation with the Data
• Estimating accurate reddening values of LAMOST M dwarfs
• A New Tidal Stream Discovered in Gaia DR3
• The Dark Matter Contribution to Galactic Diffuse Gamma Ray Emission
• The Australian Space Eye: studying the history of galaxy formation with a CubeSat
• Zonal Modes of Cosmic Microwave Background Temperature Maps
• Deep Needlet: A CNN based full sky component separation method in Needlet space
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Sparse estimation of model-based diffuse thermal dust emission
• Testing cosmological models with large-scale power modulation using microwave background polarization observations
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• AMON Searches for Jointly-Emitting Neutrino + Gamma-Ray Transients
• Photometric Catalogue for Space and Ground Night-Time Remote-Sensing Calibration: RGB Synthetic Photometry from Gaia DR3 Spectrophotometry
• X-ray upper limits of GW151226 with MAXI
• Prospects of detecting a large-scale anisotropy of ultra-high-energy cosmic rays from a nearby source with the K-EUSO orbital telescope
• Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution
• The two-and three-point correlation functions of the polarized five-year WMAP sky maps
• Sparse Isotropic Regularization for Spherical Harmonic Representations of Random Fields on the Sphere
• Constraints on primordial non-Gaussianity from Planck PR4 data
• Relevance of Ion-Channeling for Direct DM Detection
• On the interaction of a Bonnor-Ebert sphere with a stellar wind
• A Note on Spherical Needlets
• Improved Gibbs samplers for Cosmic Microwave Background power spectrum estimation
• Galactic foreground constraints on primordial $B$-mode detection for ground-based experiments
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Quasar Pairs as Large--Scale Structure tracers
• Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-Point Statistics
• The impact of beam deconvolution on noise properties in CMB measurements: Application to Planck LFI
• Excess ellipticity of hot and cold spots in the WMAP data?
• The CMB Derivatives of Planck's Beam Asymmetry
• Isotropy in the two-point angular correlation function of the CMB
• Tree-based solvers for adaptive mesh refinement code FLASH -- IV: An X-ray radiation scheme to couple discrete and diffuse X-ray emission sources to the thermochemistry of the interstellar medium
• SETI@home: Data Analysis and Findings
• Mapping possible non-Gaussianity in the Planck maps
• Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis
• Study of the Cosmic Rays and Interstellar Medium in Local HI Clouds using Fermi-LAT Gamma-Ray Observations
• On Stellar Migration from Andromeda to the Milky Way
• CMB-PAInT: An inpainting tool for the cosmic microwave background
• The optical system of the Tenerife Microwave Spectrometer: a window for observing the 10-20 GHz sky spectra
• Exploring the MeV Sky with a Combined Coded Mask and Compton Telescope: The Galactic Explorer with a Coded Aperture Mask Compton Telescope (GECCO)
• Quadrant asymmetry in the angular distribution of the Cosmic Microwave Background in the Planck satellite data
• CMB constraints on noncommutative geometry during inflation
• Accelerating linear system solvers for time domain component separation of cosmic microwave background data
• Effect of redshift bin mismatch on cross correlation between DESI Legacy Imaging Survey and Planck CMB lensing potential
• Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
• Accelerated direct demodulation method for image reconstruction with spherical data from Hard X-ray Modulation Telescope
• A Broker Integrated Algorithm for Gravitational Wave - Electromagnetic Counterpart Searches in O4a and O4b Runs
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• A Bayesian method for point source polarization estimation
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: III. CMB Temperature Anomalies
• The cross correlation of the ABS and ACT maps
• Cosmic Kite: Auto-encoding the Cosmic Microwave Background
• Long-term impact of the magnetic-field strength on the evolution and electromagnetic emission by neutron-star merger remnants
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• A Minkowski Functional Analysis of the Cosmic Microwave Background Weak Lensing Convergence
• Application of Genetic Algorithm to Estimate the Large Angular Scale Features of Cosmic Microwave Background
• On the evolution of irradiated turbulent clouds: A comparative study between modes of triggered star-formation
• Dark Matter constraints from Planck observations of the Galactic polarized synchrotron emission
• From few to many maps: A fast map-level emulator for extreme augmentation of CMB systematics datasets
• A three-dimensional model for the reversal in the local large-scale interstellar magnetic field
• Distinguishing Monochromatic Signals in LISA and Taiji: Ultralight Dark Matter versus Gravitational Waves
• A roadmap for searching cosmic rays correlated with the extraterrestrial neutrinos seen at IceCube
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Sensitivity of BEACON to Ultra-High Energy Diffuse and Transient Neutrinos
• GReX: An Instrument Overview and New Upper Limits on the Galactic FRB Population
• Environment-based selection effects of Planck clusters
• SPECTER: An Instrument Concept for CMB Spectral Distortion Measurements with Enhanced Sensitivity
• Impact of Large-Scale Structure Systematics on Cosmological Parameter Estimation
• Search for neutrino signals correlated with LHAASO diffuse Galactic emission
• On the tomographic cluster clustering as a cosmological probe
• Evidence of .Ia Supernova Detonations in 3D Hydrodynamical Simulations of Double Degenerate Mergers
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
• Cosmic rays: interstellar gamma-ray and radio emission
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Correlations between Ultrahigh Energy Cosmic Rays and AGNs
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
• Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: II. Angular Power Spectra and Likelihood
• Synthesis imaging with a lunar orbit array: I. global sky map and its systematics
• Reconstructing redshift distributions with photometric galaxy clustering
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• CMB low multipole alignments across WMAP and \emph{Planck} data releases
• Foreground removal and angular power spectrum estimation of 21 cm signal using harmonic space ILC method
• Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events
• The FLAMINGO simulations data release
• Searching for continuous gravitational waves in the Parkes Pulsar Timing Array Data Release 3
• Enhancing Compton telescope imaging with maximum a posteriori estimation: a modified Richardson-Lucy algorithm for the Compton Spectrometer and Imager
• Modeling Local Bubble analogs II: Synthetic Faraday rotation maps
• A New Probe of Gaussianity and Isotropy applied to the CMB Maps
• Efficient prescription to search for linear gravitational wave memory from hyperbolic black hole encounters and its application to the NANOGrav 12.5-year dataset
• Technosignature Searches with Real-time Alert Brokers
• The Morphology of the Anomalous Microwave Emission in the Planck 2015 data release
• Simulations of Sparse Static Detector Networks for City-Scale Radiological/Nuclear Detection
• Searching for Particle Dark Matter with eROSITA Early Data
• Messier 90 galactic halo rotation in the microwaves
• Forecasts of effects of beam systematics and deprojection on the third-generation ground-based cosmic microwave background experiment
• SIToolBox : A package for Bayesian estimation of the isotropy violation in the CMB sky
• Mapping on the HEALPix grid
• Variable gamma-ray sky at 1 GeV
• Polarized CMB recovery with sparse component separation
• 3D Correlations in the Lyman-$\alpha$ Forest from Early DESI Data
• Stacking catalog sources in WMAP data
• Modelling non-Gaussianity from foreground contaminants
• CMB delensing with deep learning
• Sidelobe Modeling and Mitigation for a Three Mirror Anastigmat Cosmic Microwave Background Telescope
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Spectral Variations of the Sky: Constraints on Alternate Universes
• Homology reveals significant anisotropy in the cosmic microwave background
• Globally optimal and scalable $N$-way matching of astronomy catalogs
• Accelerating spherical harmonic transforms for a large number of sky maps
• Cosmoglobe: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations
• Constraints on the gamma-ray emission from Small Solar System Bodies with the Fermi Large Area Telescope data
• An exact result concerning the $1/f$ noise contribution to the large-angle error in CMB temperature and polarization maps
• Does stellar mass assembly history vary with environment?
• Nature of M31 gamma-ray halo in relation to dark matter annihilation
• Polarization fraction of Planck Galactic cold clumps and forecasts for the Simons Observatory
• The Optical Depth of Foregrounds for the Highest Redshift 21 cm Signals
• Baryon density extraction and isotropy analysis of Cosmic Microwave Background using Deep Learning
• The Earth Mover's Pinball Loss: Quantiles for Histogram-Valued Regression
• The Quest for the Missing Dust: I -- Restoring Large Scale Emission in Herschel Maps of Local Group Galaxies
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Reconstruction of full sky CMB $\mathbf{E}$ and $\mathbf{B}$ modes spectra removing $\mathbf{E}$-to-$\mathbf{B}$ leakage from partial sky using deep learning
• Directional Neutrino Searches for Galactic Center Dark Matter at Large Underground LArTPCs
• The spherical Fast Multipole Method (sFMM) for Gravitational Lensing Simulation
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• Combined $13\times 2$-point analysis of the Cosmic Microwave Background and Large-Scale Structure: implications for the $S_8$-tension and neutrino mass constraints
• Characterizing the Expected Behavior of Non-Poissonian Template Fitting
• Antarctic Survey Telescope 3-3: Overview, System Performance and Preliminary Observations at Yaoan, Yunnan
• MAXI : Monitor of All-sky X-ray Image
• Radiation Driven Implosion and Triggered Star Formation
• Boltzmann-Poisson-like approach to simulating the galactic halo response to satellite accretion Dependence on the halo density profile
• Numerical Analysis of the Primordial Power Spectrum for (Small Field) Inflationary Potentials
• Cross-correlating 2MRS galaxies with UHECR flux from Pierre Auger Observatory
• Maximizing Survey Volume for Large-Area Multi-Epoch Surveys with Voronoi Tessellation
• Angular Momentum Inheritance from the Schwinger Effect in (Chromo)electromagnetic Fields
• The GALPROP Cosmic-ray Propagation and Non-thermal Emissions Framework: Release v57
• The linear bias of radio galaxies at z~0.3 via cosmic microwave background lensing
• Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology
• Improving the low-energy transient sensitivity of AMEGO-X using single-site events
• From top-hat masking to smooth transitions: P-filter and its application to polarized microwave sky maps
• Anomalies of Cosmic Anisotropy from Holographic Universality of Great-Circle Variance
• Halo Pressure Profile through the Skew Cross-Power Spectrum of Sunyaev-Zel'dovich Effect and CMB Lensing in $\text{Planck}$
• Fast map-based simulations of systematics in CMB surveys including effects of the scanning strategy
• Iterative Residual Fitting for Spherical Harmonic Transform of Band-Limited Signals on the Sphere: Generalization and Analysis
• Optimization of the half wave plate configuration for the LSPE-SWIPE experiment
• Model-independent constraints on clustering and growth of cosmic structures from BOSS DR12 galaxies in harmonic space
• Application of beam deconvolution technique to power spectrum estimation for CMB measurements
• Cosmological Simulations of Number Counts
• Searching for ring-like structures in the Cosmic Microwave Background
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Galaxy-galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
• A Measurement of Gas Temperatures in Galaxy Clusters using the Relativistic Sunyaev-Zeldovich Effect
• Gas Inflow and Star Formation near Supermassive Black Holes: The Role of Nuclear Activity
• Multiple Sound Source Localisation with Steered Response Power Density and Hierarchical Grid Refinement
• Spherical Transformer: Adapting Spherical Signal to CNNs
• SRoll3: A neural network approach to reduce large-scale systematic effects in the Planck High Frequency Instrument maps
• Test of cosmic isotropy in the Planck era
• Spectrum of the Anomalous Microwave Emission in the North Celestial Pole with WMAP 7-Year data
• A Square Equal-area Map Projection with Low Angular Distortion, Minimal Cusps, and Closed-form Solutions
• A Study of Gaussianity in CMB band maps
• Excessive shift of the CMB acoustic peaks of the Cold Spot area
• Inverse Compton gamma-rays from Galactic dark matter annihilation: Anisotropy signatures
• Confirmation of the detection of B-modes in the Planck polarization maps
• On the Impact of Random Residual Calibration Error on the Gibbs ILC Estimates over Large Angular Scales
• Exploring the anisotropic gravitational wave background from all-sky mock gravitational wave event catalogues
• GARFIELD, a toolkit for interpreting ultrafast electron diffraction data of imperfect quasi-single crystals
• The LSPE-Strip Pointing Reconstruction and Star Tracker
• Sky localization of gravitational waves from eccentric binaries
• The Bayesian Global Sky Model (B-GSM): Validation of a Data Driven Bayesian Simultaneous Component Separation and Calibration Algorithm for EoR Foreground Modelling
• Violation of Bell inequalities from Cosmic Microwave Background data
• Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
• Delensing for Precision Cosmology: Optimizing Future CMB B-mode Surveys to Constrain r
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Galaxy-cluster-stacked Fermi-LAT II: extended central hadronic signal
• Pixelization effects in cosmic shear angular power spectra
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Validation of standardized data formats and tools for ground-level particle-based gamma-ray observatories
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Constraining the polarisation flux density and angle of point sources by training a convolutional neural network
• Dipole-independent measurements of nearly-zero CMB correlation: a possible symmetry of primordial causal quantum coherence
• Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
• Bayesian recalibration of flux scale factors in diffuse radio maps using low-resolution absolute radiometers
• Where is Population II?
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• A CMB lensing analysis of the extended mass distribution of clusters
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• A Partial-Sky Gibbs ILC Approach for the Estimation of CMB Posterior over Large Angular Scales of the Sky
• Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Extreme Digitisation For Ground-Based Cosmic Microwave Background Experiments
• Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA
• Learning sparse representations on the sphere
• Answers from the void: VIDE and its applications
• Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
• The Planck submillimeter properties of Galactic high-mass star forming regions: dust temperatures, luminosities, masses and Star Formation Efficiency
• Interplanetary Dust as a Foreground for the LiteBIRD CMB Satellite Mission
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Halo detection via large-scale Bayesian inference
• Constraining primordial non-Gaussianity using Neural Networks
• Tracing the high-z cosmic web with Quaia: catalogues of voids and clusters in the quasar distribution
• Needlets and foreground removal for SKAO hydrogen intensity maps
• A New Estimator for Phase Statistics
• SymPix: A spherical grid for efficient sampling of rotationally invariant operators
• Pixel domain multi-resolution minimum variance painting of CMB maps
• Fréchet Vectors as sensitive tools for blind tests of CMB anomalies
• A Foreground Model Independent Bayesian CMB Temperature and Polarization Signal Reconstruction and Cosmological Parameter Estimation over Large Angular Scales
• No Flavor Anisotropy in the High-Energy Neutrino Sky Upholds Lorentz Invariance
• SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane
• Dynamical Evolution of Voids with Surrounding Gravitational Tidal Field
• Imaging reionization's last phases with I-front Lyman-$\alpha$ emissions
• A characterization of the diffuse Galactic emissions in the anti-center of the Galaxy
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• An isotropic full-sky sample of optically selected blazars
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Non-Gaussianities in the local curvature of the 5-year WMAP data
• Challenging a binary neutron star merger interpretation of GW230529
• A New Search Pipeline for Short Gamma Ray Bursts in Fermi/GBM Data -- A 50% Increase in the Number of Detections
• The calibrations of DAMPE $\gamma$-ray effective area
• Requirements on bandpass resolution and measurement precision for LiteBIRD
• The Angular Power Spectrum of Heavy Ion Collisions
• Fast generation of mock maps from realistic catalogs of astrophysical objects
• Searching for Extremal Spots in Planck Lensing Maps
• Impact of a binary companion in AGB outflows on CO spectral lines
• SILCC -- IX. The multi-phase interstellar medium at low metallicity
• Obtaining non-linear galaxy bias constraints from galaxy-lensing phase differences
• An approach for the detection of point-sources in very high resolution microwave maps
• Exoplanet Cartography using Convolutional Neural Networks
• Optimal-Dimensionality Sampling on the Sphere: Improvements and Variations
• Position-space curved-sky anisotropy quadratic estimation
• The large-scale monopole of the power spectrum in a Euclid-like survey: wide-angle effects, lensing, and the `finger of the observer'
• On the Energy Distribution of the Galactic Center Excess' Sources
• A geomagnetic filter for the Fermi-LAT background
• Betti Functionals as a Probe for Cosmic Topology
• Go with the Flow: The Self-Similar and Non-Linear Behaviour of Large-Scale In- and Outflows and the Impact of Accretion Shocks from Galaxies to Galaxy Clusters
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• The Lyman-$\alpha$ Forest from LBGs: First 3D Correlation Measurement with DESI and Prospects for Cosmology
• Tidal disruption events as the origin of the eROSITA and Fermi bubbles
• Compressed convolution
• Linear perturbations in spherically symmetric dust cosmologies including a cosmological constant
• The International Virtual Observatory Alliance in 2019
• Classifying Unidentified Gamma-ray Sources
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• Clustering of the extreme: A theoretical description of weak lensing critical points power spectra in the mildly nonlinear regime
• Excess B-modes extracted from the Planck polarization maps
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• Statistics of CMB polarization angles
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• Effect of Fourier filters in removing periodic systematic effects from CMB data
• Beamforming approaches toward detecting the 21-cm global signal from Cosmic Dawn with radio array telescopes
• Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise
• Robust Likelihoods for Inflationary Gravitational Waves from Maps of Cosmic Microwave Background Polarization
• Improved Method for Detecting Local Discontinuities in CMB data by Finite Differencing
• Far-infrared to centimeter emission of very nearby galaxies with archival data
• Number counts, confusion, mapping issues and sky coverage analysis for radio continuum surveys through EMU Early Science, EMU-ASKAP, and WODAN especially for cosmology science goals
• CNNs based Viewpoint Estimation for Volume Visualization
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Calibration and Applications of the All-Sky Camera at the Ali Observatory in Tibet
• The comptonization parameter from simulations of single-frequency, single-dish, dual-beam, cm-wave observations of galaxy clusters and mitigating CMB confusion using the Planck sky survey
• Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking
• Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs
• Probing the last scattering surface through the recent and future CMB observations
• Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions
• Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
• Cluster optical depth and pairwise velocity estimation using machine learning
• Analyzing billion-objects catalog interactively: Apache Spark for physicists
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• Construction of a far ultraviolet all sky map from an incomplete survey: Application of a deep learning algorithm
• Optimizing point-source parameters for scanning satellite surveys
• Testing for directionality in the Planck polarization and lensing data
• Modeling optical systematics for the Taurus CMB experiment
• Chaotic Behavior of Trapped Cosmic Rays
• On the role of dust in the microwave emission of galactic halos
• Probing the spatial and velocity anisotropies in stellar halos from the Aquarius simulations
• Wind-mediated Eddington-limited emission in a $10^4{M}_{\odot }$ Black Hole Tidal Disruption Event
• The Crab Nebula as a Calibrator for wide-beam Cosmic Microwave Background polarization surveys
• The impact of lunar topography on the 21-cm power spectrum for grid-based arrays : Insights for the Dark-ages EXplorer (DEX)
• Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
• Fermi-bubble bulk and edge analysis reveals dust, cooling breaks, and cosmic-ray diffusion, facilitating a self-consistent model
• Thermal Sunyaev-Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes
• Ring Type Structures in the Planck map of the CMB
• Resolving the formation of cold HI filaments in the high velocity cloud complex C
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies
• A coordinate-independent technique for detecting globally inhomogeneous flat topologies
• The CMB angular power spectrum via component separation: a study on Planck data
• Eridanus IV: an Ultra-Faint Dwarf Galaxy Candidate Discovered in the DECam Local Volume Exploration Survey
• What exactly did the Transformer learn from our physics data?
• Probing Galactic Diffuse TeV Gamma-Ray Emission with the HAWC Observatory
• Simultaneously unveiling the EBL and intrinsic spectral parameters of gamma-ray sources with Hamiltonian Monte Carlo
• The Luminosity of the Darkness: Schechter function in dark sirens
• A Redistribution Tool for Long-Term Archive of Astronomical Observation Data
• A Fast Algorithm for Finding Point Sources in the Fermi Data Stream: FermiFAST
• Deblending the MIGHTEE-COSMOS survey with XID+: The resolved radio source counts to $S_{1.4}\approx 5\mu$Jy
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Angular Power Spectrum in Modular Invariant Inflation Model
• The Python Sky Model 3 software
• Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials
• Observation of Anisotropy in the Arrival Direction Distribution of Cosmic Rays above TeV Energies with Icecube
• Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
• CMB lensing tomography with clustering estimation of lens redshift distributions
• On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• Multi-frequency point source detection with fully convolutional networks: Performance in realistic microwave sky simulations
• B-mode polarization forecasts for GreenPol
• A Simulation Framework for the LiteBIRD Instruments
• Imaging the Southern Sky at 159MHz using Spherical Harmonics with the Engineering Development Array 2
• The double detonation of a double degenerate system, from Type Ia supernova explosion to its supernova remnant
• Quantification of propagation modes in an astronomical instrument from its radiation pattern
• Photometric Selection of a Massive Galaxy Catalog with $z\ge 0.55$
• Joint Bayesian separation and restoration of CMB from convolutional mixtures
• The effect of a scanning flat fold mirror on a CMB B-mode experiment
• Neutrino anisotropy as a probe of extreme astrophysical accelerators
• Sample Variance for Supernovae Distance Measurements and the Hubble tension
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• System design and calibration of SITARA -- a global 21 cm short spacing interferometer prototype
• Systematic Investigation of Dust and Gaseous CO in 12 Nearby Molecular Clouds
• A Bayesian approach to high fidelity interferometric calibration I: mathematical formalism
• Mitigating Cosmic Microwave Background Shadow Degradation of Tensor-to-scalar Ratio Measurements through Map-based Studies
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Optimal data compression for Lyman-$\alpha$ forest cosmology
• Ring of attraction: overlapping directions of the dipole modulation of the CMB, the parity asymmetry, and kinematic dipole percolation zone
• Optimal map-making with singularities
• Removing the mask -- reconstructing a scalar field on the sphere from a masked field
• Null-stream-based Bayesian Unmodeled Framework to Probe Generic Gravitational-wave Polarizations
• Searching for non-Gaussianity in the Planck data
• An updated and improved thermal SZ $y$-map from Planck PR4 data
• Scale-discretised ridgelet transform on the sphere
• Simulating a full-sky high resolution Galactic synchrotron spectral index map using neural networks
• Recovering 21cm Monopole Signals Without Smoothness
• Radial derivatives as a test of pre-Big-Bang events on the Planck data
• Resolving Exo-Continents with Einstein Ring Deconvolution
• Validating dark energy models using polarised Sunyaev-Zel'dovich effect with large-angle CMB temperature and E-mode polarization anisotropies
• Non-Gaussianity in Cosmology: from Inflation to the CMB
• Correlation of IceCube neutrinos with the 2MASS Redshift Survey
• The satellite population around luminous red galaxies in the 25 square degree DESI Legacy Imaging Surveys Early Data Release
• The orbit of Planet Nine
• Multi-tracer analysis of straight depolarisation canals in the surroundings of the 3C 196 field
• Lya2pcf: an efficient pipeline to estimate two- and three-point correlation functions of the Lyman-$\alpha$ forest
• Beam-deconvolved Planck LFI maps
• Sentinel of the extraordinary: the IceCube alert system for neutrino flares
• Channeling Effects in Direct Dark Matter Detectors
• Exploring realistic nanohertz gravitational-wave backgrounds
• Assessing membership projection errors in star forming regions
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• A blind search for intraday gamma-ray transients with Fermi-LAT: Detections of GRB and solar emissions
• Extreme value statistics of CMB lensing deflection angles
• Learning Equivariant Representations
• Systematic effects on lensing reconstruction from a patchwork of CMB polarization maps
• FuGa3D: Fast full-sky analysis of Galaxy catalogs in 3D
• Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking
• Detection of polarized Fermi-bubble synchrotron and dust emission
• A 3D Monte Carlo calculation of the inverse Compton emission from the Sun and stars in presence of magnetic and electric fields
• Advanced modelling of Night Sky Background light for Imaging Atmospheric Cherenkov Telescopes
• A numerically stable comoving frame solver for line radiative transfer
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Counts-in-Cells Statistics
• Encapsulating Textual Contents into a MOC data Structure for Advanced Applications
• CMB line-of-sight integrators for nearly-isotropic cosmological models
• Investigating the origin of the Milky Way streams. A revised look at their orbital pole distribution in light of precession effects
• Optimal method for reconstructing polychromatic maps from broadband observations with an asymmetric antenna pattern
• Probing CMB Polarization Gaussianity with the Statistics of Unpolarized Points: Non-Gaussianity of Planck Data and Prospects for Future B-Mode Measurements
• Fast Bayesian analysis of individual binaries in pulsar timing array data
• The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science
• Comparison of the Planck 2018 CMB polarization maps in the BICEP2/Keck region
• Removing systematics-induced 21-cm foreground residuals by cross-correlating filtered data
• Extending Galactic foreground emission with neural networks
• Advancing weak lensing mass mapping with a mask-aware HEALPix transformer
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• Ultraluminous X-ray sources in the first eROSITA survey I. Candidate catalogs
• A Monte Carlo Implementation of Galactic Free-Free Emission for the EoR Foreground Models
• Measurement of High Energy Gamma Rays from 200 MeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
• Joint deconvolution and blind source separation on the sphere with an application to radio-astronomy
• Test of the Statistical Isotropy of the Universe using Gravitational Waves
• Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
• Explaining the UHECR spectrum, composition and large-scale anisotropies with radio galaxies
• Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices
• Non-Gaussian likelihood of weak lensing power spectra
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• Dark Energy Survey Year 3 Results: Three-Point Shear Correlations and Mass Aperture Moments
• Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx
• Local bandpower diagnostics for the hemispherical power asymmetry in CMB E-mode polarization
• Measuring peculiar velocity and tomographic redshift dipole with DESI DR1 catalogs
• Probing dipole and quadrupole anisotropy in Gamma-ray bursts from Swift dataset
• Exploring the nature of Galactic unassociated sources detected by the Fermi-LAT
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• IVOA HiPS Implementation in the Framework of WorldWide Telescope
• Accurate and efficient likelihood modeling for large-scale CMB data
• Clustering properties of TGSS radio sources
• Testing the cosmological principle with quasars
• The Ellis and Baldwin test of the Cosmic Dipole: Exploring the impact of multiple flux density cuts
• ChebLieNet: Invariant Spectral Graph NNs Turned Equivariant by Riemannian Geometry on Lie Groups
• Self-Supervised ConvLSTM for Fermi Large Area Telescope Transient Detection
• VarWISE: Infrared Variability via NEOWISE Single Exposure Photometry
• Monitoring the TeV sky on hours long timescales with HAWC
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Destriping Cosmic Microwave Background Polarimeter data
• Ray-traced weak lensing convergence in screened modified gravity theories
• Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy
• A new magnitude--redshift relation based on Type Ia supernovae
• Probabilistic Cross-identification of Multiple Catalogs in Crowded Fields
• Measurements of the diffuse Galactic synchrotron spectral index and curvature from MeerKLASS pilot data
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• The Impact of Observing Strategy on Reliable Classification of Standard Candle Stars: Detection of Amplitude, Period, and Phase Modulation (Blazhko Effect) of RR Lyrae Stars with LSST
• CMB lensing reconstruction from the WMAP 7-year data
• Spectral Map Making with SPHEREx
• Perturbative and numerical study of nonlinear relativistic effects in weak lensing
• The Radio and Microwave Sky as Seen by Juno on its Mission to Jupiter
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Statical properties of CMB B-mode polarisation in a partial sky analysis
• Echoes of the past: ultra-high energy cosmic rays accelerated by radio galaxies, scattered by starburst galaxies
• Semiclassical Length Measure from a Quantum-Gravity Wave Function
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• DIAPHANE: a Portable Radiation Transport Library for Astrophysical Applications
• Towards detecting Primordial non-Gaussianity in the CMB using Spherical Convolutional Neural Networks
• AutoKnots: Adaptive Knot Allocation for Spline Interpolation
• Detectability of Galactic Faraday Rotation in Multi-wavelength CMB Observations: A Cross-Correlation Analysis of CMB and Radio Maps
• Comparison of maximum likelihood mapping methods for gravitational-wave backgrounds
• Weak Lensing Low Multipoles
• The Kaiser-Rocket effect: three decades and counting
• Local environmental dependence on weak-lensing shear statistics
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Integrated Sachs-Wolfe maps from the Gower Street $w$CDM simulations
• A novel Cosmic Filament catalogue from SDSS data
• QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon
• A study of an energy-dependent anisotropy of cosmic rays beyond the GZK cut-off with deep neural networks
• Foreground Mitigation for CMB Lensing with the Global Minimum Variance Quadratic Estimator
• NVST data archiving system based on fastbit nosql database
• Estimating fiber orientation distribution from diffusion MRI with spherical needlets
• Modeling Tangential Vector Fields on a Sphere
• Skykatana: a scalable framework to construct sky masks for the Vera Rubin Observatory and large astronomical surveys
• Constraints on the dark energy dipole from large-scale structures
• Systematics mitigation for catalogue-based angular power spectra
• A new approach of estimating the Galactic thermal dust and synchrotron polarized emission template in the microwave bands
• Search for Diffuse Galactic Neutrinos with the Full ANTARES Telescope Dataset
• Deep learning with hybrid frequency differencing and principal component analysis for 21-cm foreground and beam mitigation
• Efficient Search for Detection Candidates Using a Peak Finder Strategy for All-Sky-All-Frequency Gravitational Wave Radiometer
• Probing gravity with non-linear clustering in redshift space
• $\text{SBi3PCF:}$ Simulation-based inference with the integrated 3PCF
• Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae
• Score-based generative emulation of impact-relevant Earth system model outputs
• Forecasts of constraining isotropic cosmic birefringence on AliCPT-1
• Ultra-high energy cosmic rays with UFA-15 source model in Bumblebee gravity theory
• Using the large scale quasar clustering to constrain flat quintessential universes
• Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions
• Clustering analysis of medium-band selected high-redshift galaxies
• On the detection of point sources in Planck LFI 70 GHz CMB maps based on cleaned K-map
• Extragalactic Searches for Dark Matter Annihilation
• It's Always Darkest Before the Cosmic Dawn: Early Results from Novel Tools and Telescopes for 21 cm Cosmology
• Using hybrid GPU/CPU kernel splitting to accelerate spherical convolutions
• Investigating non-Gaussianity in Cosmic Microwave Background Temperature Maps using Spherical Harmonic Phases
• Scaling pair count to next galaxy surveys
• Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach
• Incorporating curved geometry in cosmological simulations
• Accidental deep field bias in CMB T and SNe $z$ correlation
• Large-angle non-Gaussianity in simulated high-resolution CMB maps
• Supervised Extraction of the Thermal Sunyaev$-$Zel'dovich Effect with a Three-Dimensional Convolutional Neural Network
• Generative modeling of convergence maps based on predicted one-point statistics
• A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
• Circumventing Cosmic Variance via Remote Quadrupole Measurements
• A comparative study of non-Gaussianity in ILC-7yr CMB map