MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics

Abstract

We present further development and the first public release of our multimodal nested sampling algorithm, called MultiNest. This Bayesian inference tool calculates the evidence, with an associated error estimate, and produces posterior samples from distributions that may contain multiple modes and pronounced (curving) degeneracies in high dimensions. The developments presented here lead to further substantial improvements in sampling efficiency and robustness, as compared to the original algorithm presented in Feroz & Hobson (2008), which itself significantly outperformed existing MCMC techniques in a wide range of astrophysical inference problems. The accuracy and economy of the MultiNest algorithm is demonstrated by application to two toy problems and to a cosmological inference problem focussing on the extension of the vanilla $\Lambda$CDM model to include spatial curvature and a varying equation of state for dark energy. The MultiNest software, which is fully parallelized using MPI and includes an interface to CosmoMC, is available at http://www.mrao.cam.ac.uk/software/multinest/. It will also be released as part of the SuperBayeS package, for the analysis of supersymmetric theories of particle physics, at http://www.superbayes.org

14 pages, 9 figures

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• Magellan/M2FS Spectroscopy of the Reticulum 2 Dwarf Spheroidal Galaxy
• Primordial Black Hole Evaporation and Dark Matter Production: II. Interplay with the Freeze-In/Out Mechanism
• AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration
• Assessing tension metrics with Dark Energy Survey and Planck data
• First Observational Tests of Eternal Inflation
• What next for the CMSSM and the NUHM: Improved prospects for superpartner and dark matter detection
• Hunting Down the Best Model of Inflation with Bayesian Evidence
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• A comparison of exoplanet spectroscopic retrieval tools
• Global Study of the Simplest Scalar Phantom Dark Matter Model
• Gemini Near Infrared Field Spectrograph Observations of the Seyfert 2 Galaxy Mrk 573: In Situ Acceleration of Ionized and Molecular Gas Off Fueling Flows
• Gluino-driven Radiative Breaking, Higgs Boson Mass, Muon $\mathbf{g}-2$, and the Higgs Diphoton Decay in SUGRA Unification
• A High False Positive Rate for Kepler Planetary Candidates of Giant Stars using Asterodensity Profiling
• Optical phase curve of the ultra-hot Jupiter WASP-121b
• Apparent cosmic acceleration from type Ia supernovae
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• CEERS Key Paper IV: Galaxies at $4<z<9$ are Bluer than They Appear -- Characterizing Galaxy Stellar Populations from Rest-Frame $\sim 1$ micron Imaging
• Awesome SOSS: Transmission Spectroscopy of WASP-96b with NIRISS/SOSS
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• The Hunt for Exomoons with Kepler (HEK): III. The First Search for an Exomoon around a Habitable-Zone Planet
• Bayesian model selection without evidences: application to the dark energy equation-of-state
• 3D stellar kinematics at the Galactic center: measuring the nuclear star cluster spatial density profile, black hole mass, and distance
• Towards a more complex description of chemical profiles in exoplanets retrievals: A 2-layer parameterisation
• An Analysis of Chandra Deep Follow-up GRBs: Implications for Off-Axis Jets
• The GJ 504 system revisited. Combining interferometric, radial velocity, and high contrast imaging data
• Model selection applied to reconstruction of the Primordial Power Spectrum
• The Roasting Marshmallows Program with IGRINS on Gemini South I: Composition and Climate of the Ultra Hot Jupiter WASP-18 b
• The POLAR Gamma-Ray Burst Polarization Catalog
• Detection and Bulk Properties of the HR 8799 Planets with High Resolution Spectroscopy
• Foreground Mismodeling and the Point Source Explanation of the Fermi Galactic Center Excess
• Low-mass right-handed sneutrino dark matter: SuperCDMS and LUX constraints and the Galactic Centre gamma-ray excess
• High-z galaxies with JWST and local analogues -- it is not only star formation
• A General Bayesian Framework for Foreground Modelling and Chromaticity Correction for Global 21cm Experiments
• Prospects for dark matter searches in the pMSSM
• The Transiting System GJ1214: High-Precision Defocused Transit Observations and a Search for Evidence of Transit Timing Variation
• Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Global fits of the dark matter-nucleon effective interactions
• A population of dust-enshrouded objects orbiting the Galactic black hole
• Scaling Relations for Dark Matter Annihilation and Decay Profiles in Dwarf Spheroidal Galaxies
• A search for HI absorption in nearby radio galaxies using HIPASS
• A Census of Baryons and Dark Matter in an Isolated, Milky Way-sized Elliptical Galaxy
• COLDz: A High Space Density of Massive Dusty Starburst Galaxies ~1 Billion Years after the Big Bang
• The First Tidally Disrupted Ultra-Faint Dwarf Galaxy? - Spectroscopic Analysis of the Tucana III Stream
• Dark Energy Survey Year 3 Results: Optimizing the Lens Sample in Combined Galaxy Clustering and Galaxy-Galaxy Lensing Analysis
• Comparison of sampling techniques for Bayesian parameter estimation
• The 96 GeV Diphoton Excess in the Seesaw Extensions of the Natural NMSSM
• Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
• Implications for New Physics in $b\to s\mu \mu$ transitions after recent measurements by Belle and LHCb
• A Survey of the Molecular ISM Properties of Nearby Galaxies using the Herschel FTS
• Wind of Change: retrieving exoplanet atmospheric winds from high-resolution spectroscopy
• ARES I: WASP-76 b, A Tale of Two HST Spectra
• The impact of glitches on young pulsar rotational evolution
• ACCESS & LRG-BEASTS: a precise new optical transmission spectrum of the ultrahot Jupiter WASP-103b
• First gas-phase metallicity gradients of $0.1\lesssim z\lesssim 0.8$ galaxies with MUSE
• ARES II: Characterising the Hot Jupiters WASP-127 b, WASP-79 b and WASP-62 b with HST
• Lense-Thirring frame dragging induced by a fast-rotating white dwarf in a binary pulsar system
• The UTMOST pulsar timing programme II: Timing noise across the pulsar population
• An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
• Larger mutual inclinations for the shortest-period planets
• The pMSSM10 after LHC Run 1
• Early Low-Mass Galaxies and Star-Cluster Candidates at z~6-9 Identified by the Gravitational Lensing Technique and Deep Optical/Near-Infrared Imaging
• Optimizing searches for electromagnetic counterparts of gravitational wave triggers
• WIMP Dark Matter in a Well-Tempered Regime: A case study on Singlet-Doublets Fermionic WIMP
• The Return of the Templates: Revisiting the Galactic Center Excess with Multi-Messenger Observations
• Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
• GUT-constrained supersymmetry and dark matter in light of the new $(g-2{)}_{\mu }$ determination
• Global fits of the cMSSM including the first LHC and XENON100 data
• Proper Motions of Stellar Streams Discovered in the Dark Energy Survey
• Oscillation mode linewidths of main-sequence and subgiant stars observed by Kepler
• Galactic cosmic-ray propagation in the light of AMS-02: I. Analysis of protons, helium, and antiprotons
• An Empirical Model for the Star Formation History in Dark Matter Halos
• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
• Fermion Masses and Mixing from Double Cover and Metaplectic Cover of $A_5$ Modular Group
• Hubble WFC3 Spectroscopy of the Habitable-zone Super-Earth LHS 1140 b
• Unveiling cloudy exoplanets: the influence of cloud model choices on retrieval solutions
• Full parameter scan of the Zee model: exploring Higgs lepton flavor violation
• Predicted Number, Multiplicity, and Orbital Dynamics of TESS M Dwarf Exoplanets
• Aurora: A Generalised Retrieval Framework for Exoplanetary Transmission Spectra
• Drifting Oscillations in Axion Monodromy
• Accurate cosmic shear errors: do we need ensembles of simulations?
• The Kepler Dichotomy in Planetary Disks: Linking Kepler Observables to Simulations of Late-Stage Planet Formation
• Three-Flavoured Non-Resonant Leptogenesis at Intermediate Scales
• The High-Energy Tail of the Galactic Center Gamma-Ray Excess
• Comparison of algorithms for determination of rotation measure and Faraday structure I. 1100 - 1400 MHz
• Retrieval survey of metals in six ultra-hot Jupiters: Trends in chemistry, rain-out, ionisation and atmospheric dynamics
• Substructure in the lens HE 0435-1223
• Atmospheric Retrieval of Exoplanets
• BAHAMAS: new SNIa analysis reveals inconsistencies with standard cosmology
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Axion astronomy with microwave cavity experiments
• Accelerating astronomical and cosmological inference with Preconditioned Monte Carlo
• Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays
• Investigating the Binarity of S0-2: Implications for its Origins and Robustness as a Probe of the Laws of Gravity around a Supermassive Black Hole
• Comparison of statistical sampling methods with ScannerBit, the GAMBIT scanning module
• The inert doublet model in the light of Fermi-LAT gamma-ray data: a global fit analysis
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• Diurnal variations in the stratosphere of the ultrahot giant exoplanet WASP-121b
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• A comprehensive approach to dark matter studies: exploration of simplified top-philic models
• Dark matter astrophysical uncertainties and the neutrino floor
• First Observational Tests of Eternal Inflation: Analysis Methods and WMAP 7-Year Results
• The Occurrence Rate of Terrestrial Planets Orbiting Nearby Mid-to-late M Dwarfs from TESS Sectors 1-42
• Planck Constraints on Monodromy Inflation
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Spectrophotometric templates for core collapse supernovae and their application in simulations of time-domain surveys
• Interpreting the Global 21-cm Signal from High Redshifts. II. Parameter Estimation for Models of Galaxy Formation
• Circularly polarized radio emission from the repeating fast radio burst source FRB 20201124A
• Searches for the BSM scenarios at the LHC using decision tree based machine learning algorithms: A comparative study and review of Random Forest, Adaboost, XGboost and LightGBM frameworks
• A remarkable long-term light curve, and deep, low-state spectroscopy: Swift & XMM-Newton monitoring of the NLS1 galaxy Mkn 335
• TRADES: A new software to derive orbital parameters from observed transit times and radial velocities. Revisiting Kepler-11 and Kepler-9
• Localized correlated features in the CMB power spectrum and primordial bispectrum from a transient reduction in the speed of sound
• Developing Atmospheric Retrieval Methods for Direct Imaging Spectroscopy of Gas Giants in Reflected Light I: Methane Abundances and Basic Cloud Properties
• On the Feasibility of Intense Radial Velocity Surveys for Earth-twin Discoveries
• HD 1397b: a transiting warm giant planet orbiting a V = 7.8 mag sub-giant star discovered by TESS
• HD 213885b: A transiting 1-day-period super-Earth with an Earth-like composition around a bright ($V=7.9$) star unveiled by TESS
• Spurious Point Source Signals in the Galactic Center Excess
• Fitting $f(Q,T)$ gravity models with a $\Lambda$CDM limit using H(z) and Pantheon data
• KiDS-1000: cosmic shear with enhanced redshift calibration
• A fast and precise methodology to search for and analyse strongly lensed gravitational-wave events
• Dark matter annihilation and decay profiles for the Reticulum II dwarf spheroidal galaxy
• Constraining new physics with searches for long-lived particles: Implementation into SModelS
• Bounds on secret neutrino interactions from high-energy astrophysical neutrinos
• Detecting eccentric supermassive black hole binaries with pulsar timing arrays: Resolvable source strategies
• Electroweak phase transition with composite Higgs models: calculability, gravitational waves and collider searches
• Analysis of the 4-year IceCube high-energy starting events
• Primordial Features from Linear to Nonlinear Scales
• Reconstruction of the Dark Energy equation of state
• Near-Infrared Transmission Spectroscopy of HAT-P-18b with NIRISS: Disentangling Planetary and Stellar Features in the Era of JWST
• The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
• Investigating dark matter substructure with pulsar timing: I. Constraints on ultracompact minihalos
• Quantifying the Bayesian Evidence for a Planet in Radial Velocity Data
• A simple and robust method for automated photometric classification of supernovae using neural networks
• Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies
• Searching for Beyond the Standard Model Physics with COHERENT Energy and Timing Data
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• WASP-127b: A misaligned planet with a partly cloudy atmosphere and tenuous sodium signature seen by ESPRESSO
• Ships Passing in the Night: Spectroscopic Analysis of Two Ultra-Faint Satellites in the Constellation Carina
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot
• Dark matter or correlated errors: Systematics of the AMS-02 antiproton excess
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).IX. The effects of ram pressure stripping down to the scale of individual HII regions in the dwarf galaxy IC 3476
• Flavor anomalies and dark matter in SUSY with an extra U(1)
• Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
• Independent Cosmological Constraints from high-z HII Galaxies
• The discovery and mass measurement of a new ultra-short-period planet: EPIC~228732031b
• Multiple Chemodynamic Stellar Populations of the Ursa Minor Dwarf Spheroidal Galaxy
• Resolving Quiescent Galaxies at $z\gtrsim 2$: I. Search for Gravitationally Lensed Sources and Characterization of their Structure, Stellar Populations, and Line Emission
• HyDRA-H: Simultaneous Hybrid Retrieval of Exoplanetary Emission Spectra
• Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
• ARES V: No Evidence For Molecular Absorption in the HST WFC3 Spectrum of GJ 1132 b
• HAT-P-44b, HAT-P-45b, and HAT-P-46b: Three Transiting Hot Jupiters in Possible Multi-Planet Systems
• Strong Ly$\alpha$ Emission in an Overdense Region at $z=6.8$: A Very Large ($R\sim 3$ physical Mpc) Ionized Bubble in COSMOS?
• Double-lined Spectroscopic Binary Stars in the Radial Velocity Experiment Survey
• Witnessing the onset of reionisation via Lyman-$\alpha$ emission at redshift 13
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• 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
• Deciphering Contributions to the Extragalactic Gamma-Ray Background from 2 GeV to 2 TeV
• Constraining Monodromy Inflation
• Spatially-resolving the terminator: Variation of Fe, temperature and winds in WASP-76 b across planetary limbs and orbital phase
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• An optical transmission spectrum of the ultra-hot Jupiter WASP-33b. First indication of AlO in an exoplanet
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• The NINJA-2 project: Detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations
• EXONEST: Bayesian Model Selection Applied to the Detection and Characterization of Exoplanets Via Photometric Variations
• Planet populations inferred from debris discs: insights from 178 debris systems in the ISPY, LEECH and LIStEN planet-hunting surveys
• Nitrogen-enriched, highly-pressurized nebular clouds surrounding a super star cluster at cosmic noon
• The mass of our Galaxy from satellite proper motions in the Gaia era
• Inverse Primakoff Scattering as a Probe of Solar Axions at Liquid Xenon Direct Detection Experiments
• Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data
• An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• Modular Invariant $A_4$ Models for Quarks and Leptons with Generalized CP Symmetry
• Large Interferometer For Exoplanets (LIFE): III. Spectral resolution, wavelength range and sensitivity requirements based on atmospheric retrieval analyses of an exo-Earth
• Large Interferometer For Exoplanets (LIFE): V. Diagnostic potential of a mid-infrared space-interferometer for studying Earth analogs
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• An 8.8 minute orbital period eclipsing detached double white dwarf binary
• Enabling rootless Linux Containers in multi-user environments: the udocker tool
• WIMP astronomy and particle physics with liquid-noble and cryogenic direct-detection experiments
• Directional axion detection
• Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. II. Spatially Resolved Mass Outflow Rates for the QSO2 Markarian 34
• A Search for Stellar-Mass Black Holes via Astrometric Microlensing
• Time-Resolved GRB Polarization with POLAR and GBM
• Uncertainties in the Galactic dark matter distribution: an update
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• An Analytic Model for Rotational Modulations in the Photometry of Spotted Stars
• Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. III. Results for the Seyfert 2 Galaxies Markarian 3, Markarian 78, and NGC 1068
• Gravitational-wave detection and parameter estimation for accreting black-hole binaries and their electromagnetic counterpart
• The 5 - 10 keV AGN luminosity function at 0.01<z<4.0
• Profile likelihood maps of a 15-dimensional MSSM
• Estimating the sensitivity of pulsar timing arrays
• How Well Can Future CMB Missions Constrain Cosmic Inflation?
• Low energy SUSY confronted with new measurements of W-boson mass and muon g-2
• The tidal remnant of an unusually metal-poor globular cluster
• The Enigmatic Galactic Center Excess: Spurious Point Sources and Signal Mismodeling
• The 12CO/13CO isotopologue ratio of a young, isolated brown dwarf. Possibly distinct formation pathways of super-Jupiters and brown dwarfs
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Awesome SOSS: Atmospheric Characterisation of WASP-96 b using the JWST Early Release Observations
• Evidence for the volatile-rich composition of a 1.5-$R_{\oplus }$ planet
• Galaxy gas as obscurer: I. GRBs x-ray galaxies and find a N_H ~ M* relation
• The Spectral Energy Distribution of Powerful Starburst Galaxies I: Modelling the Radio Continuum
• Extragalactic fast X-ray transient candidates discovered by Chandra (2000-2014)
• Gamma-ray Timing of Redback PSR J2339-0533: Hints for Gravitational Quadrupole Moment Changes
• Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen Poor Low Mass White Dwarf
• Searching for Oscillations in the Primordial Power Spectrum: Perturbative Approach (Paper I)
• Cosmic ray propagation and dark matter in light of the latest AMS-02 data
• Search for a Variation of the Fine Structure around the Supermassive Black Hole in Our Galactic Center
• The Metal-Rich Atmosphere of the Neptune HAT-P-26b
• On The Compatibility of Ground-based and Space-based Data: WASP-96 b, An Example
• A Unified Analysis of Four Cosmic Shear Surveys
• Pippi - painless parsing, post-processing and plotting of posterior and likelihood samples
• A robust estimate of the Milky Way mass from rotation curve data
• WASP-127b transmission spectrum]{Abundance measurements of H${}_2$O and carbon-bearing species in the atmosphere of WASP-127b confirm its super-solar metallicity
• AIC, BIC, Bayesian evidence against the interacting dark energy model
• Accelerator and reactor complementarity in coherent neutrino scattering
• Tracing the Gas to the Virial Radius (R100) in a Fossil Group
• Supervised deep learning in high energy phenomenology: a mini review
• The power of Bayesian evidence in astronomy
• A comparison of chemical models of exoplanet atmospheres enabled by TauREx 3.1
• Triple system HD 201433 with a SPB star component seen by BRITE-Constellation: Pulsation, differential rotation, and angular momentum transfer
• Compatibility of Planck and BICEP2 in the Light of Inflation
• Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation
• The BACCO simulation project: biased tracers in real space
• Modeling microlensing events with MulensModel
• Neutrino tomography of the Earth
• Non-standard interactions with high-energy atmospheric neutrinos at IceCube
• JWST reveals a possible $z\sim 11$ galaxy merger in triply-lensed MACS0647$-$JD
• Mode-by-mode Relative Binning: Fast Likelihood Estimation for Gravitational Waveforms with Spin-Orbit Precession and Multiple Harmonics
• HARPS-N radial velocities confirm the low densities of the Kepler-9 planets
• LHS 1140 b is a potentially habitable water world
• Sampling Errors in Nested Sampling Parameter Estimation
• Unveiling the Gamma-ray Source Count Distribution Below the Fermi Detection Limit with Photon Statistics
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• Characterizing the Nature of the Unresolved Point Sources in the Galactic Center
• Constraining mornings & evenings on distant worlds: a new semi-analytical approach and prospects with transmission spectroscopy
• A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329
• On Atmospheric Retrievals of Exoplanets with Inhomogeneous Terminators
• Model independent determination of the dark matter mass from direct detection experiments
• Transmission spectroscopy and Rossiter-McLaughlin measurements of the young Neptune orbiting AU Mic
• Signatures of Nitrogen Chemistry in Hot Jupiter Atmospheres
• Distinguishing Dark Matter from Unresolved Point Sources in the Inner Galaxy with Photon Statistics
• Atmospheric retrievals with petitRADTRANS
• Information Gain on Reheating: the One Bit Milestone
• Bayesian optimal reconstruction of the primordial power spectrum
• A tentative detection of He I in the atmosphere of GJ 1214b
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• Constraints on a mixed model of dark matter particles and primordial black holes from the Galactic 511 keV line
• No Conclusive Evidence for Transits of Proxima b in MOST photometry
• Leptogenesis from Low Energy $CP$ Violation
• Solving the mode identification problem in asteroseismology of F stars observed with Kepler
• Light dark Higgs boson in minimal sub-GeV dark matter scenarios
• Studying the solar system with the International Pulsar Timing Array
• Implications of Lithium to Oxygen AMS-02 spectra on our understanding of cosmic-ray diffusion
• Neutrino Portal to FIMP Dark Matter with an Early Matter Era
• ARES III: Unveiling the Two Faces of KELT-7 b with HST WFC3
• The Ariel Target List: The Impact of TESS and the Potential for Characterising Multiple Planets Within a System
• Star Formation and Stellar Mass Assembly in Dark Matter Halos: From Giants to Dwarfs
• Super-Solar Metallicity Stars in the Galactic Center Nuclear Star Cluster: Unusual Sc, V, and Y Abundances
• A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776
• A combined radio and GeV gamma-ray view of the 2012 and 2013 flares of Mrk 421
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• The ALMA REBELS Survey: Efficient Ly$\alpha$ Transmission of UV-Bright z$\simeq$7 Galaxies from Large Velocity Offsets and Broad Line Widths
• TOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star
• Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour
• A search for 21 cm HI absorption in AT20G compact radio galaxies
• The Knotted Sky II: Does BICEP2 require a nontrivial primordial power spectrum?
• Current and Future Neutrino Oscillation Constraints on Leptonic Unitarity
• 2D Bayesian automated tilted-ring fitting of disk galaxies in large HI galaxy surveys: 2DBAT
• A Systematic Study of the Stochastic Gravitational-Wave Background due to Stellar Core Collapse
• Low star formation efficiency in typical galaxies at z=5-6
• MIGHTEE-HI: The baryonic Tully-Fisher relation over the last billion years
• Two temperate Earth-mass planets orbiting the nearby star GJ1002
• Bayesian Approach to Probabilistic Design Space Characterization: A Nested Sampling Strategy
• Quartz Clouds in the Dayside Atmosphere of the Quintessential Hot Jupiter HD 189733 b
• Masses and radii for the three super-Earths orbiting GJ 9827, and implications for the composition of small exoplanets
• UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1
• An empirical study of dust properties at the earliest epochs
• Bayesian Asteroseismology of 23 Solar-Like Kepler Targets
• Outstanding Challenges of Exoplanet Atmospheric Retrievals
• The GCE in a New Light: Disentangling the $\gamma$-ray Sky with Bayesian Graph Convolutional Neural Networks
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Promoting single-file DNA translocations through nanopores using electroosmotic flow
• A statistically significant lack of debris discs in medium separation binary systems
• Prospects for direct detection of dark matter in an effective theory approach
• The Influence of Stellar Contamination on the Interpretation of Near Infrared Transmission Spectra of Sub-Neptune Worlds around M-Dwarfs
• Neural posterior estimation for exoplanetary atmospheric retrieval
• JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy
• Bayesian global analysis of neutrino oscillation data
• Interpreting High-Resolution Spectroscopy of Exoplanets Using Cross-Correlations and Supervised Machine Learning
• A dichotomy between the hard state spectral properties of black hole and neutron star X-ray~binaries
• Is the $H_0$ tension suggesting a 4th neutrino's generation?
• Cosmological constraints with self-interacting sterile neutrinos
• Identifying the Theory of Dark Matter with Direct Detection
• Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
• The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane
• nestcheck: diagnostic tests for nested sampling calculations
• A Gaia DR 2 and VLT/FLAMES search for new satellites of the LMC
• Hints of a sulfur-rich atmosphere around the 1.6 R${}_{\oplus }$ Super-Earth L98-59 d from JWST NIRSpec G395H transmission spectroscopy
• Low fine tuning in the MSSM with higgsino dark matter and unification constraints
• MultiModeCode: An efficient numerical solver for multifield inflation
• Challenges testing the no-hair theorem with gravitational waves
• Should we still believe in constrained supersymmetry?
• Global fits of the Non-Universal Higgs Model
• The Knotted Sky I: Planck constraints on the primordial power spectrum
• A light NMSSM pseudoscalar Higgs boson at the LHC redux
• The White Dwarf Opportunity: Robust Detections of Molecules in Earth-like Exoplanet Atmospheres with the James Webb Space Telescope
• On the Existence of the Plateau Emission in High-Energy Gamma-Ray Burst LightCurves observed byFermi-LAT
• VLT Spectroscopy of Ultra-Faint Dwarf Galaxies. 1. Boötes I, Leo IV, Leo V
• Importance nested sampling with normalising flows
• A transiting warm giant planet around the young active star TOI-201
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• Explanation of the knee-like feature in the DAMPE cosmic $e^{-}+e^{+}$ energy spectrum
• Discovery of an Ultra-Faint Stellar System near the Magellanic Clouds with the DECam Local Volume Exploration (DELVE) Survey
• Bayesian Analysis of Inflation III: Slow Roll Reconstruction Using Model Selection
• Strong first-order phase transitions in the NMSSM --- a comprehensive survey
• Bayesian inflationary reconstructions from Planck 2018 data
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Removing degeneracy and multimodality in gravitational wave source parameters
• SDSS-IV MaNGA: Stellar initial mass function variation inferred from Bayesian analysis of the integral field spectroscopy of early type galaxies
• Testing the validity of the single-spin approximation in inspiral-merger-ringdown waveforms
• Quantifying lost information due to covariance matrix estimation in parameter inference
• ULYSSES: Universal LeptogeneSiS Equation Solver
• A model explaining neutrino masses and the DAMPE cosmic ray electron excess
• 2D Retrieval Frameworks for Hot Jupiter Phase Curves
• A machine learning approach to galaxy properties: joint redshift-stellar mass probability distributions with Random Forest
• WASP-52b. The effect of starspot correction on atmospheric retrievals
• Dark Matter properties through cosmic history
• A Transiting Jupiter Analog
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• The Zwicky Transient Facility Type Ia supernova survey: first data release and results
• On the direct detection of multi-component dark matter: sensitivity studies and parameter estimation
• Identifying WIMP dark matter from particle and astroparticle data
• Bayesian evidence for the tensor-to-scalar ratio $r$ and neutrino masses $m_{\nu }$: Effects of uniform vs logarithmic priors
• Statistical aspects of nuclear mass models
• Pinning down the mass of Kepler-10c: the importance of sampling and model comparison
• The variable and non-variable X-ray absorbers in Compton-thin type-II Active Galactic Nuclei
• Dark Matter Interferometry
• Blinding multi-probe cosmological experiments
• Light Fermionic WIMP Dark Matter with Light Scalar Mediator
• On the Application of Bayesian Leave-One-Out Cross-Validation to Exoplanet Atmospheric Analysis
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• Statistical Measurement of the Gamma-ray Source-count Distribution as a Function of Energy
• Cosmology with gravitationally lensed repeating Fast Radio Bursts
• Use of event-level neutrino telescope data in global fits for theories of new physics
• A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• A novel 3D technique to study the kinematics of lensed galaxies
• Statistical Analyses of Higgs- and Z-Portal Dark Matter Models
• Atmospheric retrievals suggest the presence of a secondary atmosphere and possible sulfur species on L 98-59 d from JWST NIRSpec G395H transmission spectroscopy
• TOI-481 b & TOI-892 b: Two long period hot Jupiters from the Transiting Exoplanet Survey Satellite
• Directional detection of dark matter streams
• Mapping stellar surfaces II: An interpretable Gaussian process model for light curves
• A novel approach to visibility-space modelling of interferometric gravitational lens observations at high angular resolution
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685
• Taming astrophysical bias in direct dark matter searches
• Cold dark matter plus not-so-clumpy dark relics
• Constraints on the binary black hole nature of GW151226 and GW170608 from the measurement of spin-induced quadrupole moments
• NGC 300 ULX1: A test case for accretion torque theory
• The Extremely High Dark Matter Halo Concentration of the Relic Compact Elliptical Galaxy Mrk 1216
• Amplitude and lifetime of radial modes in red giant star spectra observed by Kepler
• Statistical Issues in Astrophysical Searches for Particle Dark Matter
• Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
• Early Insights for Atmospheric Retrievals of Exoplanets using JWST Transit Spectroscopy
• A global fit of the $\gamma$-ray galactic center excess within the scalar singlet Higgs portal model
• A multi-epoch kinematic study of the remote dwarf spheroidal galaxy Leo II
• A Search for a Surviving White Dwarf Companion in SN 1006
• Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed
• Discovery of a dual active galactic nucleus with ~ 8 kpc separation
• The XXL Survey: VI. The 1000 brightest X-ray point sources
• KiDS-1000: Cosmology with improved cosmic shear measurements
• The Hubble WFC3 Emission Spectrum of the Extremely-Hot Jupiter, KELT-9b
• Explaining temporal variations in the jet position angle of the blazar OJ 287 using its binary black hole central engine model
• Bayesian constraints on the origin and geology of exo-planetary material using a population of externally polluted white dwarfs
• The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis
• Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey
• Parameter Estimation of Gravitational Waves from Nonprecessing BH-NS Inspirals with higher harmonics: Comparing MCMC posteriors to an Effective Fisher Matrix
• Dust attenuation evolution in $z\sim 2$-$12$ JWST galaxies
• Retrieving the C and O Abundances of HR 7672~AB: a Solar-Type Primary Star with a Benchmark Brown Dwarf
• Ultracompact minihalos as probes of inflationary cosmology
• Bayesian Model Comparison and Analysis of the Galactic Disk Population of Gamma-Ray Millisecond Pulsars
• Fast methods for training Gaussian processes on large data sets
• Global Fit of Modified Quark Couplings to EW Gauge Bosons and Vector-Like Quarks in Light of the Cabibbo Angle Anomaly
• Binary populations in Milky Way satellite galaxies: constraints from multi-epoch data in the Carina, Fornax, Sculptor and Sextans dwarf spheroidal galaxies
• Synchrotron Radiation Dominates the Extremely Bright GRB 221009A
• Towards rapid transient identification and characterization of kilonovae
• Joint resonant CMB power spectrum and bispectrum estimation
• Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-Dwarf Companion in the Hyades
• Nonlinear seismic scaling relations
• The Star Formation History of the Milky Way's Nuclear Star Cluster
• The CARMENES search for exoplanets around M dwarfs. Characterization of the nearby ultra-compact multiplanetary system YZ Ceti
• The Magellan-TESS Survey I: Survey Description and Mid-Survey Results
• A revisit of PSR J1909$-$3744 with 15-year high-precision timing
• Angular power spectrum of galaxies in the 2MASS Redshift Survey
• First constraints on the AGN X-ray luminosity function at $z\sim 6$ from an eROSITA-detected quasar
• Stellar Companions to TESS Objects of Interest: A Test of Planet-Companion Alignment
• Two ultimate tests of constrained supersymmetry
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• On the contamination of the global 21~cm signal from polarized foregrounds
• Bayesian Implications of Current LHC and XENON100 Search Limits for the Constrained MSSM
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Assessment of Supervised Machine Learning for Atmospheric Retrieval of Exoplanets
• Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling
• Extragalactic FXT Candidates Discovered by Chandra (2014-2022)
• Investigating the gamma-ray burst from decaying MeV-scale axion-like particles produced in supernova explosions
• Strong lensing reveals jets in a sub-microJy radio quiet quasar
• Search for Quantum Gravity Using Astrophysical Neutrino Flavour with IceCube
• Caught in the Act: Core-powered Mass-loss Predictions for Observing Atmospheric Escape
• A minimal power-spectrum-based moment expansion for CMB B-mode searches
• Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South
• Asymmetric spatial distribution of sub-solar metallicity stars in the Milky Way nuclear star cluster
• Illuminating the past 8 billion years of cold gas towards two gravitationally lensed quasars
• Neutrino Mass Priors for Cosmology from Random Matrices
• Do joint CMB and HST data support a scale invariant spectrum?
• Characterization of Kepler-91b and the Investigation of a Potential Trojan Companion Using EXONEST
• Perspective of monochromatic gamma-ray line detection with the High Energy cosmic-Radiation Detection (HERD) facility onboard China's Space Station
• (Lack of) Cosmological evidence for dark radiation after Planck
• The ELIXR Galaxy Survey. II: Baryons and Dark Matter in an Isolated Elliptical Galaxy
• The Most Metal-poor Stars in the Magellanic Clouds are $r$-process Enhanced
• A resonant pair of warm giant planets revealed by TESS
• Efficient reconstruction of CMSSM parameters from LHC data - A case study
• On parametrised cold dense matter equation of state inference
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Retrieval Study of Brown Dwarfs Across the L-T Sequence
• ISPY -- NACO Imaging Survey for Planets around Young stars: Survey description and results from the first 2.5 years of observations
• The stellar metallicities of massive quiescent galaxies at 1.0 < z < 1.3 from KMOS+VANDELS
• On the halo-mass and radial scale dependence of the lensing is low effect
• Electroweak baryogenesis and gravitational waves in a composite Higgs model with high dimensional fermion representations
• The Commensal Real-time ASKAP Fast Transient incoherent-sum survey
• A reproducible method to determine the meteoroid mass index
• Bayesian parameter constraints for neutron star masses and radii using X-ray timing observations of accretion-powered millisecond pulsars
• Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues
• XZ: Deriving redshifts from X-ray spectra of obscured AGN
• The Post-Pericenter Evolution of the Galactic Center Source G2
• Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
• Black hole spectroscopy horizons for current and future gravitational wave detectors
• ARES IV: Probing the atmospheres of the two warm small planets HD 106315 c and HD 3167 c with the HST/WFC3 camera
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• Simplified Models for Higgs Physics: Singlet Scalar and Vector-like Quark Phenomenology
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Powellsnakes II: a fast Bayesian approach to discrete object detection in multi-frequency astronomical data sets
• Eccentric Companions to Kepler-448b and Kepler-693b: Clues to the Formation of Warm Jupiters
• Exomoon Candidates from Transit Timing Variations: Eight Kepler systems with TTVs explainable by photometrically unseen exomoons
• A direct measurement of tomographic lensing power spectra from CFHTLenS
• Probing the Local Velocity Distribution of WIMP Dark Matter with Directional Detectors
• JADES: Primaeval Lyman-$\alpha$ emitting galaxies reveal early sites of reionisation out to redshift $z\sim 9$
• HST PanCET Program: A Complete Near-UV to Infrared Transmission Spectrum for the Hot Jupiter WASP-79b
• Global 21-cm Signal Extraction from Foreground and Instrumental Effects II: Efficient and Self-Consistent Technique for Constraining Nonlinear Signal Models
• The eROSITA Final Equatorial-Depth Survey (eFEDS): Characterization of Morphological Properties of Galaxy Groups and Clusters
• Effective Field Theory of Dark Matter: a Global Analysis
• TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• Detection of missing baryons in galaxy groups with kinetic Sunyaev-Zel'dovich effect
• Dissecting the inner Galaxy with $\gamma$-ray pixel count statistics
• Decoding spectral energy distributions of dust-obscured starburst-AGN
• Isotropy of low redshift type Ia Supernovae: A Bayesian analysis
• A warm Jupiter transiting an M dwarf: A TESS single transit event confirmed with the Habitable-zone Planet Finder
• Global fits of axion-like particles to XENON1T and astrophysical data
• Exploring the GRB population: Robust afterglow modelling
• A Second Look at 12 Candidate Dual AGNs using $\mathtt{BAYMAX}$
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• Discovery of a Transiting Planet Near the Snow-Line
• Kinematic Modelling of Disc Galaxies using Graphics Processing Units
• Parametrizations of the global 21-cm signal and parameter estimation from single-dipole experiments
• On statistical uncertainty in nested sampling
• Considerations for Atmospheric Retrieval of High-Precision Brown Dwarf Spectra
• BAMBI: blind accelerated multimodal Bayesian inference
• A Highly Eccentric Warm Jupiter Orbiting TIC 237913194
• Priors on Lagrangian bias parameters from galaxy formation modelling
• A global analysis strategy to resolve neutrino NSI degeneracies with scattering and oscillation data
• Effective $J$-factors for Milky Way dwarf spheroidal galaxies with velocity-dependent annihilation
• Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
• Probabilistic Catalogs for Crowded Stellar Fields
• Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy
• The ESO SupJup Survey I: Chemical and isotopic characterisation of the late L-dwarf DENIS J0255-4700 with CRIRES${}^{+}$
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements
• Superplot: a graphical interface for plotting and analysing MultiNest output
• The vertical structure of debris disks and the impact of gas
• A Comprehensive Analysis of WASP-17b's Transmission Spectrum from Space-Based Observations
• The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
• FLASH Early Science -- Discovery of an intervening HI 21-cm absorber from an ASKAP survey of the GAMA 23 field
• PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
• Complementarity of direct and indirect Dark Matter detection experiments
• Gravitational Redshift of Galaxies in Clusters from the Sloan Digital Sky Survey and the Baryon Oscillation Spectroscopic Survey
• Differentiating Modern and Prebiotic Earth Scenarios for TRAPPIST-1e: High-resolution Transmission Spectra and Predictions for JWST
• Cosmic microwave background and inflation in multi-fractional spacetimes
• Likelihood Analysis of the Minimal AMSB Model
• Inferring gas-phase metallicity gradients of galaxies at the seeing limit: A forward modelling approach
• A Sensitive Search for Supernova Emission Associated with the Extremely Energetic and Nearby GRB 221009A
• Epoch of Reionisation 21cm Forecasting From MCMC-Constrained Semi-Numerical Models
• Clear and Cloudy Exoplanet Forecasts for JWST: Maps, Retrieved Composition and Constraints on Formation with MIRI and NIRCam
• The ESO SupJup Survey III: Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+
• Improving Orbit Estimates for Incomplete Orbits with a New Approach to Priors -- with Applications from Black Holes to Planets
• Suppressing the Scattering of WIMP DM with Nucleons in Supersymmetric Theories
• Aura-3D: A Three-dimensional Atmospheric Retrieval Framework for Exoplanet Transmission Spectra
• Extremely late photometry of SN~2011fe
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Electron and Muon Anomalous Magnetic Moments in the Inverse Seesaw Extended NMSSM
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Detecting Dark Matter Cores in Galaxy Clusters with Strong Lensing
• KELT-11 b: Abundances of water and constraints on carbon-bearing molecules from the Hubble transmission spectrum
• Neutralino and gravitino dark matter with low reheating temperature
• Nuclear uncertainties in the spin-dependent structure functions for direct dark matter detection
• 21cmEMU: an emulator of 21cmFAST summary observables
• CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators
• Higgs Physics and Supersymmetry
• Muon g-2 and related phenomenology in constrained vector-like extensions of the MSSM
• Retrieval study of cool, directly imaged exoplanet 51 Eri b
• Spectral energy distribution and radio halo of NGC 253 at low radio frequencies
• Bayesian naturalness of the CMSSM and CNMSSM
• The Optical/Near-Infrared Extinction Law In Highly Reddened Regions
• Evidence for profile changes in PSR J1713+0747 using the uGMRT
• Extracting Majorana Properties in the Throat of Neutrinoless Double Beta Decay
• Is the atmosphere of the ultra-hot Jupiter WASP-121b variable?
• Discovery of a Supercluster in the eROSITA Final Equatorial Depth Survey: X-ray Properties, Radio Halo, and Double Relics
• MUSE sneaks a peek at extreme ram-pressure stripping events - IV. Hydrodynamic and gravitational interactions in the Blue Infalling Group
• Constraining the kinetically dominated Universe
• Bayesian Comparison of Interacting Scenarios
• The misaligned orbit of the Earth-sized planet Kepler-408b
• Electroweak and Higgs Boson Internal Bremsstrahlung: General considerations for Majorana dark matter annihilation and application to MSSM neutralinos
• Dynamics and cosmological constraints on Brans-Dicke cosmology
• The Giant Accreting Protoplanet Survey (GAPlanetS) -- Results from a Six Year Campaign to Image Accreting Protoplanets
• An exploration of model degeneracies with a unified phase curve retrieval analysis: The light and dark sides of WASP-43 b
• Triggering the Untriggered: The First Einstein Probe-Detected Gamma-Ray Burst 240219A and Its Implications
• Understanding WIMP-baryon interactions with direct detection: A Roadmap
• Where intermediate-mass black holes could hide in the Galactic Centre: A full parameter study with the S2 orbit
• Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations
• Accounting for Cosmic Variance in Studies of Gravitationally-Lensed High-Redshift Galaxies in the Hubble Frontier Field Clusters
• The unexpected narrowness of eccentric debris rings: a sign of eccentricity during the protoplanetary disc phase
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• The Tucana dwarf spheroidal galaxy: not such a massive failure after all
• Revealing the Formation of the Milky Way Nuclear Star Cluster via Chemo-Dynamical Modeling
• The VANDELS survey: A strong correlation between Ly$\alpha$ equivalent width and stellar metallicity at $3\le \mathbf{z}\le 5$
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• Testing the accuracy of the ionospheric Faraday rotation corrections through LOFAR observations of bright northern pulsars
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Cosmic Inflation at the Crossroads
• Searching for primordial localized features with CMB and LSS spectra
• Analysis of the theoretical bias in dark matter direct detection
• Simplified Dark Matter Models Confront the Gamma Ray Excess
• Near-infrared transmission spectrum of TRAPPIST-1 h using Hubble WFC3 G141 observations
• Predictable patterns in planetary transit timing variations and transit duration variations due to exomoons
• Alleviating the tension at low multipole through Axion Monodromy
• A Bayesian comparison of U(1) lepton flavour models
• JWST/NIRCam discovery of the first Y+Y brown dwarf binary: WISE J033605.05$-$014350.4
• Revisiting the atmosphere of the exoplanet 51 Eridani b with VLT/SPHERE
• A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096
• Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3
• The Galactic Center: Improved Relative Astrometry for Velocities, Accelerations, and Orbits near the Supermassive Black Hole
• SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
• The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres. No evidence of enhanced evaporation in young planets
• Accelerated Bayesian inference using deep learning
• Constraining the neutron star equation of state using Pulse Profile Modeling
• Forbidden frozen-in dark matter
• Retrieval Analysis of the Emission Spectrum of WASP-12b: Sensitivity of Outcomes to Prior Assumptions and Implications for Formation History
• Low frequency view of GRB 190114C reveals time varying shock micro-physics
• GAMBIT and its Application in the Search for Physics Beyond the Standard Model
• The challenge of measuring the phase function of debris disks. Application to HR\,4796
• Neural network reconstructions for the Hubble parameter, growth rate and distance modulus
• The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
• Indirect and direct detection prospect for TeV dark matter in the MSSM-9
• Application of a Bayesian Method to Absorption Spectral-Line Finding in Simulated ASKAP Data
• Inflation Model Selection meets Dark Radiation
• Investigating ULX accretion flows and cyclotron resonance in NGC 300 ULX1
• HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone
• An Atmospheric Retrieval of the Brown Dwarf Gliese 229B
• NPTFit: A code package for Non-Poissonian Template Fitting
• The Orbital Eccentricities of Directly Imaged Companions Using Observable-Based Priors: Implications for Population-level Distributions
• ExoReL${}^{\Re }$: A Bayesian Inverse Retrieval Framework For Exoplanetary Reflected Light Spectra
• The Problem with False Vacuum Higgs Inflation
• What $\xi$? Cosmological constraints on the non-minimal coupling constant
• Antenna beam characterisation for the global 21cm experiment LEDA and its impact on signal model parameter reconstruction
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Moderate-Resolution $K$-Band Spectroscopy of Substellar Companion $\kappa$ Andromedae b
• Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Radio and Far-IR Emission Associated with a Massive Star-forming Galaxy Candidate at z$\simeq$6.8: A Radio-Loud AGN in the Reionization Era?
• CMSSM, naturalness and the "fine-tuning price" of the Very Large Hadron Collider
• Global fit of pseudo-Nambu-Goldstone Dark Matter
• SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• K2-231 b: A sub-Neptune exoplanet transiting a solar twin in Ruprecht 147
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• Global limits and interference patterns in dark matter direct detection
• Loose Ends for the Exomoon Candidate Host Kepler-1625b
• Measuring the mass of the black widow PSR J1555-2908
• How Much Information Does the Sodium Doublet Encode? Retrieval Analysis of Non-LTE Sodium Lines at Low and High Spectral Resolutions
• A search for multi-planet systems with TESS using a Bayesian N-body retrieval and machine learning
• Improving timing sensitivity in the microhertz frequency regime: limits from PSR J1713$+$0747 on gravitational waves produced by super-massive black-hole binaries
• CUORE Sensitivity to $0\nu \beta \beta$ Decay
• Is there evidence for additional neutrino species from cosmology?
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Stellar Density Profiles of Dwarf Spheroidal Galaxies
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• H- and Dissociation in Ultra-hot Jupiters: A Retrieval Case Study of WASP-18b
• Electroweak baryogenesis in the Z3-invariant NMSSM
• A non-parametric method for measuring the local dark matter density
• A multi-wavelength analysis of a collection of short-duration GRBs observed between 2012-2015
• Cosmic-Ray Positrons Strongly Constrain Leptophilic Dark Matter
• Fitting flavour symmetries: the case of two-zero neutrino mass textures
• CNO Solar Neutrinos in Next-Generation Dark Matter Experiments
• Renormalization Group Running of Fermion Observables in an Extended Non-Supersymmetric SO(10) Model
• Testing non-minimally coupled inflation with CMB data: a Bayesian analysis
• Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
• Lensed: a code for the forward reconstruction of lenses and sources from strong lensing observations
• Ground-Based Transmission Spectroscopy with FORS2: A featureless optical transmission spectrum and detection of H${}_2$O for the ultra-hot Jupiter WASP-103b
• Brightest galaxies as halo centre tracers in SDSS DR7
• Contamination of the Epoch of Reionization power spectrum in the presence of foregrounds
• Direct Constraints on the Extremely Metal-Poor Massive Stars Underlying Nebular C IV Emission from Ultra-Deep HST/COS Ultraviolet Spectroscopy
• Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
• Convolutional neural networks as an alternative to Bayesian retrievals
• Simultaneous enhancement in gamma.gamma, b.b-bar and tau+.tau- rates in the NMSSM with nearly degenerate scalar and pseudoscalar Higgs bosons
• Towards a framework for testing general relativity with extreme-mass-ratio-inspiral observations
• The Gaia-ESO Survey: Dynamical models of flattened, rotating globular clusters
• Stellar chemo-kinematics of the Cetus dwarf spheroidal galaxy
• Binary companions of nearby supernova remnants found with Gaia
• Variations in the Fundamental constants in the QSO Host J1148+5251 at z = 6.4 and the BR1202-0725 System at z = 4.7
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- I. The Richness-Mass Relation
• Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
• Bayesian evidence for $\alpha$-attractor dark energy models
• Joint estimation of the Epoch of Reionization power spectrum and foregrounds
• Bayesian data analysis tools for atomic physics
• ACCESS: A Visual to Near-infrared Spectrum of the Hot Jupiter WASP-43b with Evidence of ${\mathrm{H}}_2\mathrm{O}$, but no evidence of Na or K
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8
• Warm and Cold Molecular Gas Conditions Modeled in 87 Galaxies Observed by the Herschel SPIRE Fourier Transform Spectrometer
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• Sunyaev-Zel'dovich observation of the Bullet-like cluster Abell 2146 with the Arcminute Microkelvin Imager
• Detection of Na in WASP-21b's lower and upper atmosphere
• Apprentice for Event Generator Tuning
• Cloud-by-cloud, multiphase, Bayesian modeling: Application to four weak, low ionization absorbers
• Dim but not entirely dark: Extracting the Galactic Center Excess' source-count distribution with neural nets
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Complementarity of dark matter direct detection: the role of bolometric targets
• Hubble Space Telescope Observations of [O~III] Emission in Nearby QSO2s: Physical Properties of the Ionised Outflows
• TOI-1231 b: A Temperate, Neptune-Sized Planet Transiting the Nearby M3 Dwarf NLTT 24399
• HI emission and absorption in nearby, gas-rich galaxies II. -- sample completion and detection of intervening absorption in NGC 5156
• A black widow population dissection through HiPERCAM multi-band light curve modelling
• Testing dark matter with Cherenkov light -- prospects of H.E.S.S. and CTA for exploring minimal supersymmetry
• Fortifying the characterization of binary mergers in LIGO data
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Bayesian Analysis of Molecular Emission and Dust Continuum of Protoplanetary Disks
• The HARPS search for southern extra-solar planets. XXXIX. HD175607 b, the most metal-poor G dwarf with an orbiting sub-Neptune
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• The chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of $\mathrm{HC}{\mathrm{O}}^{+}$
• Information content of JWST-NIRSPEC transmission spectra of warm Neptunes
• Effects of intermediate scales on renormalization group running of fermion observables in an SO(10) model
• The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18
• HST/STIS transmission spectrum of the ultra-hot Jupiter WASP-76 b confirms the presence of sodium in its atmosphere
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• Leptonic Unitarity Triangles
• CMB constraints on $\beta$-exponential inflationary models
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: I. Gas Properties
• Large Exomoons unlikely around Kepler-1625 b and Kepler-1708 b
• Discovery of a disrupting open cluster far into the Milky Way halo: a recent star formation event in the leading arm of the Magellanic stream?
• Bayesian analysis of anisotropic cosmologies: Bianchi VII_h and WMAP
• Testing Realistic $SO(10)$ SUSY GUTs with Proton Decay and Gravitational Waves
• Cosmological parameter estimation with Genetic Algorithms
• Characterising the rotational irregularities of the Vela pulsar from 21 yr of phase-coherent timing
• Probing WIMP particle physics and astrophysics with direct detection and neutrino telescope data
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• TOI-150b and TOI-163b: two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9979b
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- I. The importance of redshift-space distortions for galaxy number counts
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection
• Integrating light-curve and atmospheric modelling of transiting exoplanets
• Collider signatures of a light NMSSM pseudoscalar in neutralino decays in the light of LHC results
• The new $(g-2{)}_{\mu }$ result and the $\mu \nu$SSM
• Dark matter interpretations of ATLAS searches for the electroweak production of supersymmetric particles in $\sqrt{s}=8$ TeV proton-proton collisions
• Identification of Sagittarius stream members in Angular Momentum space with Gaussian mixture techniques
• What can(not) be measured with ton-scale dark matter direct detection experiments
• Cosmological model with decaying vacuum energy law from principles of quantum mechanics
• Testing gravity on cosmological scales with cosmic shear, cosmic microwave background anisotropies, and redshift-space distortions
• DAMPE squib? Significance of the 1.4 TeV DAMPE excess
• ZTF J1901+5309: A 40.6-Minute Orbital Period Eclipsing Double White Dwarf System
• COMET: Clustering Observables Modelled by Emulated perturbation Theory
• HATS-54b-HATS-58Ab: five new transiting hot Jupiters including one with a possible temperate companion
• Reticulum II: Particle Dark Matter and Primordial Black Holes Limits
• A comparison of optimisation algorithms for high-dimensional particle and astrophysics applications
• LBT transmission spectroscopy of HAT-P-12b: confirmation of a cloudy atmosphere with no significant alkali features
• Testing gamma-ray models of blazars in the extragalactic sky
• Anomalous Muon Magnetic Moment in the Inverse Seesaw Extended Next-to-Minimal Supersymmetric Standard Model
• Charming Dark Matter
• SHARP -- VI. Evidence for CO (1-0) molecular gas extended on kpc-scales in AGN star forming galaxies at high redshift
• A comparative study of WASP-67b and HAT-P-38b from WFC3 data
• Searching for Oscillations in the Primordial Power Spectrum with CMB and LSS Data
• A new measure of tension between experiments
• A sub-Earth-mass planet orbiting Barnard's star
• Wide-band Profile Domain Pulsar Timing Analysis
• Likelihood Analysis of the Sub-GUT MSSM in Light of LHC 13-TeV Data
• A formal method for identifying distinct states of variability in time-varying sources: SgrA* as an example
• GJ357: A low-mass planetary system uncovered by precision radial-velocities and dynamical simulations
• An External Shock Origin of GRB $\text{141028A}$
• GRAVITY K-band spectroscopy of HD 206893 B: brown dwarf or exoplanet
• A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals
• Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
• Fast Bayesian inference for slow-roll inflation
• Bayesian inference for pulsar timing models
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• A Physical Background Model for the Fermi Gamma-ray Burst Monitor
• Complementarity of Indirect and Accelerator Dark Matter Searches
• Searching for Supersymmetry: The $\mu \nu$SSM
• Bayesian Inference for Radio Observations
• Searches for Shapiro delay in seven binary pulsars using the MeerKAT telescope
• Naturalness of the relaxion mechanism
• A Bayesian analysis of sneutrino DM in the NMSSM with Type-I seesaw mechanism
• Reconstructing the three-dimensional local dark matter velocity distribution
• Axion global fits with Peccei-Quinn symmetry breaking before inflation using GAMBIT
• RELICS: Properties of z>5.5 Galaxies Inferred from Spitzer and Hubble Imaging Including A Candidate z~6.8 Strong [OIII] Emitter
• Testing the universality of cosmic-ray nuclei from protons to oxygen with AMS-02
• A Bayesian Analysis of SDSS J0914+0853, a Low-Mass Dual AGN Candidate
• Search for Surviving Companions of Progenitors of Young LMC Type Ia Supernova Remnants
• Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
• TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf
• Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars
• Determining the presence of characteristic fragmentation length-scales in filaments
• Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c
• Incorporating Astrochemistry into Molecular Line Modelling via Emulation
• Superposition Enhanced Nested Sampling
• x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data
• Concordance Cosmology?
• Quintessential Cosmological Tensions
• Modeling gravitational waves from exotic compact objects
• Using High-Energy Neutrinos As Cosmic Magnetometers
• Probing the Physics of Star-Formation (ProPStar): II. The first systematic search for streamers toward protostars
• Exploring H${}_2$O Prominence in Reflection Spectra of Cool Giant Planets
• Tycho-B: an unlikely companion for SN 1572
• WASP-117 b: an eccentric hot-Saturn as a future complex chemistry laboratory
• Running of Fermion Observables in Non-Supersymmetric SO(10) Models
• A Bayesian study of the primordial power spectrum from a novel closed universe model
• The Scientific Reach of Multi-Ton Scale Dark Matter Direct Detection Experiments
• MIGHTEE-HI: The first MeerKAT HI mass function from an untargeted interferometric survey
• Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling
• The Quintuplet Cluster: Extended Structure and Tidal Radius
• Consistency check of ΛCDM phenomenology
• The seven sisters DANCe IV. Bayesian hierarchical model
• Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
• Planetary system around LTT 1445A unveiled by ESPRESSO: Multiple planets in a triple M-dwarf system
• The Herschel-ATLAS: magnifications and physical sizes of $500\mu$m-selected strongly lensed galaxies
• A Bayesian analysis of inflationary primordial spectrum models using Planck data
• Discovery of the luminous X-ray ignition eRASSt J234402.9$-$352640; I. Tidal disruption event or a rapid increase in accretion in an active galactic nucleus?
• The Mysterious Dimmings of the T Tauri Star V1334 Tau
• Radiative Driving of the AGN Outflows in the Narrow-Line Seyfert 1 Galaxy NGC 4051
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Nested sampling cross-checks using order statistics
• Model selection for spectro-polarimetric inversions
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Interferometry of $\epsilon$ Aurigae: Characterization of the asymmetric eclipsing disk
• The 2-10 keV unabsorbed luminosity function of AGN from the XMM-Newton LSS, CDFS and COSMOS surveys
• A transmission spectrum of the sub-Earth planet L98-59~b in 1.1-1.7 $\mu$m
• The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
• DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
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• New determination of the production cross section for secondary positrons and electrons in the Galaxy
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• Supernovae evidence for foundational change to cosmological models
• Bayesian Model Averaging in Astrophysics: A Review
• Detailed SZ study of 19 LoCuSS galaxy clusters: masses and temperatures out to the virial radius
• A Bayesian quantification of consistency in correlated datasets
• Bayesian model comparison in cosmology with Population Monte Carlo
• The quadrupole in the local Hubble parameter: first constraints using Type Ia supernova data and forecasts for future surveys
• A new method for extending solutions to the self-similar relativistic magnetohydrodynamics equations for black hole outflows
• Evidence of a Clear Atmosphere for WASP-62b: the Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone
• Bayesian estimation of non-Gaussianity in pulsar timing analysis
• Variational Inference as an alternative to MCMC for parameter estimation and model selection
• Parametrizing the local dark matter speed distribution: a detailed analysis
• Bayesian parameter estimation in $\chi$EFT using Hamiltonian Monte Carlo
• Montblanc: GPU accelerated Radio Interferometer Measurement Equations in support of Bayesian Inference for Radio Observations
• Mapping the Likelihood of GW190521 with Diverse Mass and Spin Priors
• Bayesian analysis of inflationary features in Planck and SDSS data
• A 62-minute orbital period black widow binary in a wide hierarchical triple
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Hubble WFC3 Spectroscopy of the Terrestrial Planets L~98-59~c \& d: No Evidence for a Clear Hydrogen Dominated Primary Atmosphere
• Bayesian evidence for two companions orbiting HIP 5158
• The ESO SupJup Survey II: The 12C/13C ratios of three young brown dwarfs with CRIRES${}^{+}$
• Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
• The chemical structure of young high-mass star-forming clumps: (I) Deuteration
• Testing for New Physics: Neutrinos and the Primordial Power Spectrum
• Constraints on sneutrino dark matter from LHC Run 1
• Simple and statistically sound recommendations for analysing physical theories
• Hierarchical Bayesian Detection Algorithm for Early-Universe Relics in the Cosmic Microwave Background
• CKS IX: Revisiting the Minimum-Mass Extrasolar Nebula with Precise Stellar Parameters
• Gravitational lensing by wave dark matter halos
• HI emission and absorption in nearby, gas-rich galaxies
• Cosmic Swarms: A search for Supermassive Black Holes in the LISA data stream with a Hybrid Evolutionary Algorithm
• Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies
• Charged Higgs boson in the $W^{\pm }$ Higgs channel at the Large Hadron Collider
• Lensing Model of MACS J1149.5+2223 - I. Cluster mass reconstruction
• Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD235088 b (TOI-1430 b) with CARMENES
• Constraining holographic inflation with WMAP
• A simple parametric model for spherical galaxy clusters
• Radial Stellar Pulsation and Three-Dimensional Convection. II. Two-Dimensional Convection In Full Amplitude Radial Pulsation
• Signatures of dark Higgs boson in light fermionic dark matter scenarios
• Fast and robust Bayesian Inference using Gaussian Processes with GPry
• Phenomenology of SUSY with General Flavour Violation
• The REASONS Survey: Resolved Millimeter Observations of a Large Debris Disk Around the Nearby F Star HD 170773
• The cosmic evolution of the stellar mass$-$velocity dispersion relation of early-type galaxies
• Bayesian analysis of capture reactions ${}^3\mathrm{He}(\alpha ,\gamma {)}^7\mathrm{Be}$ and ${}^3\mathrm{H}(\alpha ,\gamma {)}^7\mathrm{Li}$
• Consistency of cosmic shear analyses in harmonic and real space
• Measuring the duration of inflation with the curvaton
• Probabilistic detection of spectral line components
• Transmission spectroscopy of the ultra-hot Jupiter MASCARA-4 b: Disentangling the hydrostatic and exospheric regimes of ultra-hot Jupiters
• Strong constraints on a simple self-interacting neutrino cosmology
• Constraining Galactic dark matter with gamma-ray pixel counts statistics
• Two-component scalar dark matter in $Z_{2n}$ scenarios
• Texture-zero patterns of lepton mass matrices from modular symmetry
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• Self-calibration and robust propagation of photometric redshift distribution uncertainties in weak gravitational lensing
• Constraining a companion of the galactic center black hole, Sgr A*
• Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at $z\gtrsim 1$
• Probing $L_{\mu }-L_{\tau }$ models with CE$\nu$NS: A new look at the combined COHERENT CsI and Ar data
• The SCUBA-2 850 $\mu m$ follow-up of WISE-selected, luminous dust-obscured quasars
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• Gaussian processes for radial velocity modeling Better rotation periods and planetary parameters with the quasi-periodic kernel and constrained priors
• Photo-Dynamical Analysis of Three Kepler Objects of Interest with Significant Transit Timing Variations
• Should we doubt the cosmological constant?
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• A new method for measuring the meteor mass index: application to the 2018 Draconid meteor shower outburst
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• Nested sampling with any prior you like
• Selection between foreground models for global 21-cm experiments
• Revisit cosmic ray propagation by using ${}^1$H, ${}^2$H, ${}^3$He and ${}^4$He
• The Most Metal-poor Stars in the Inner Bulge
• Solar fusion III: New data and theory for hydrogen-burning stars
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• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• Generative pulsar timing analysis
• Evidence for chromium hydride in the atmosphere of Hot Jupiter WASP-31b
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• A retrieval challenge exercise for the Ariel mission
• JWST-TST High Contrast: Living on the Wedge, or, NIRCam Bar Coronagraphy Reveals CO${}_2$ in the HR 8799 and 51 Eri Exoplanets' Atmospheres
• ACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques
• Analysing the SEDs of protoplanetary disks with machine learning
• Recovering the Physical Properties of Molecular Gas in Galaxies from CO SLED Modeling
• Around The Way: Testing $\Lambda$CDM with Milky Way Stellar Stream Constraints
• Proximal nested sampling for high-dimensional Bayesian model selection
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• DAMPE proton spectrum indicates a slow-diffusion zone in the nearby ISM
• A framework for testing isotropy with the cosmic microwave background
• Golden galactic binaries for LISA: mass-transferring white dwarf black hole binaries
• A Generalized Bayesian Approach to Model Calibration
• An enhanced slope in the transmission spectrum of the hot Jupiter WASP-104b
• A New Method For Studying Exoplanet Atmospheres Using Planetary Infrared Excess
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• Multi-lepton signatures at LHC from sneutrino dark matter
• The Possible Moon of Kepler-90g is a False Positive
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• Detection of l=4 and l=5 modes in 12 years of solar VIRGO-SPM data --- Tests on Kepler observations of 16 Cyg A and B
• GRB 110715A: The peculiar multiwavelength evolution of the first afterglow detected by ALMA
• Likelihood Analysis of Supersymmetric SU(5) GUTs
• What galaxy masses perturb the local cosmic expansion?
• Detection of Paschen $\beta$ absorption in the atmosphere of KELT-9 b: A new window into the atmospheres of ultra-hot Jupiters
• Near-IR imaging of T Cha: evidence for scattered-light disk structures at solar system scales
• Impact of LHC data on muon $g-2$ solutions in vector-like extension of the Constrained MSSM
• Detection prospects of light NMSSM Higgs pseudoscalar via cascades of heavier scalars from vector boson fusion and Higgs-strahlung
• Inverse Seesaw Model with a Modular $S_4^{}$ Symmetry: Lepton Flavor Mixing and Warm Dark Matter
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• Extended $\Lambda$CDM model
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• Large Interferometer For Exoplanets (LIFE): IX. Assessing the Impact of Clouds on Atmospheric Retrievals at Mid-Infrared Wavelengths with a Venus-Twin Exoplanet
• EXPRES. III. Revealing the Stellar Activity Radial Velocity Signature of $\epsilon$ Eridani with Photometry and Interferometry
• Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters
• Euclid: The Early Release Observations Lens Search Experiment
• On cosmological bias due to the magnification of shear and position samples in modern weak lensing analyses
• TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Cosmological foundations revisited with Pantheon+
• Determining Dark Matter properties with a XENONnT/LZ signal and LHC-Run3 mono-jet searches
• Singlino-dominated dark matter in $Z_3$-NMSSM
• Effective neutrino masses in KATRIN and future tritium beta-decay experiments
• Comparing compact binary parameter distributions I: Methods
• Korali: Efficient and Scalable Software Framework for Bayesian Uncertainty Quantification and Stochastic Optimization
• Stellar Populations in the Central 0.5 pc of Our Galaxy III: The Dynamical Sub-structures
• Evidence of a Decreased Binary Fraction for Massive Stars Within 20 Milliparsecs of the Supermassive Black Hole at the Galactic Center
• Borexino results on neutrinos from the Sun and Earth
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanet
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- II. A case study for magnification bias and radio continuum surveys
• Bayesian constraints on dark matter halo properties using gravitationally-lensed supernovae
• Stellar Spins in the Pleiades, Praesepe, and M35 Open Clusters
• Evidence for SiO cloud nucleation in the rogue planet PSO J318
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• Bayesian Model Selection with Future 21cm Observations of The Epoch of Reionisation
• Robust model comparison tests of DAMA/LIBRA annual modulation
• X-PSI Parameter Recovery for Temperature Map Configurations Inspired by PSR J0030+0451
• Bayesian evidence for non-zero theta_13 and CP-violation in neutrino oscillations
• Revisiting Radial Velocity Measurements of the K2-18 System with the Line-by-Line Framework
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• Impact of recent $(g-2{)}_{\mu }$ measurement on the light CP-even Higgs scenario in general Next-to-Minimal Supersymmetric Standard Model
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems
• Singlino-dominated dark matter in general NMSSM
• The polytropic state of the intracluster medium in the X-COP cluster sample
• Evidence for TiO in the atmosphere of the hot Jupiter HAT-P-65 b
• SPECIES II. Stellar parameters of the EXPRESS program giant star sample
• Multi-Dimensional Effective Field Theory Analysis for Direct Detection of Dark Matter
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years
• Weak lensing by triaxial galaxy clusters
• Karl G. Jansky Very Large Array observations of cold dust and molecular gas in starbursting quasar host galaxies at z~4.5
• Multivariate Rational Approximation
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Transmission spectroscopy of WASP-52 b with JWST NIRISS: Water and helium atmospheric absorption, alongside prominent star-spot crossings
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• A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger
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• Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
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• Squeezing $f_{\mathrm{NL}}$ out of the matter bispectrum with consistency relations
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• A search for lensed gamma-ray bursts in 11 years of observations by Fermi GBM
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• Spatial Anisotropy of Galaxy Kinematics in Sloan Digital Sky Survey Galaxy Clusters
• Evidence for Substructure in Ursa Minor Dwarf Spheroidal Galaxy using a Bayesian Object Detection Method
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• The transmission spectrum of WASP-17 b from the optical to the near-infrared wavelengths: combining STIS, WFC3 and IRAC datasets
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• Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS
• ALMA [N ıı] 205 μm Imaging Spectroscopy of the Lensed Submillimeter galaxy ID 141 at redshift 4.24
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• The coupling of an EUV coronal wave and ion acceleration in a Fermi-LAT behind-the-limb solar flare
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• Inferring the morphology of AGN torus using X-ray spectra: A reliability study
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• Stellar Populations in the Transition Region of Nuclear Star Cluster and Nuclear Stellar Disc
• Robust predictions for an oscillatory bispectrum in Planck 2015 data from transient reductions in the speed of sound of the inflaton
• Astrophysical interpretation of the anisotropies in the unresolved gamma-ray background
• Global Analysis of Dark Matter Simplified Models with Leptophobic Spin-One Mediators using MasterCode
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Masses of Kepler-46b, c from Transit Timing Variations
• PdBI U/LIRG Survey (PULS): Dense Molecular Gas in Arp 220 and NGC 6240
• The Exoplanet Simple Orbit Fitting Toolbox (ExoSOFT): An Open-Source Tool for Efficient Fitting of Astrometric and Radial Velocity Data
• PSR J1231-1411 revisited: Pulse Profile Analysis of X-ray Observation
• Extended Cosmology in Palatini f(R)-theories
• Zooming into the Cosmic Horseshoe: new insights on the lens profile and the source shape
• Measuring dust in core-collapse supernovae with a Bayesian approach to line profile modelling
• Measuring Tracers of Planet Formation in the Atmosphere of WASP-77A b: Sub-stellar O/H and C/H ratios, with a stellar C/O ratio and a potentially Super-stellar Ti/H ratio
• Indirect dark-matter detection with MadDM v3.2 -- Lines and Loops
• Spatially Resolved Outflows in a Seyfert Galaxy at z = 2.39
• Complex angular structure of three elliptical galaxies from high-resolution ALMA observations of strong gravitational lenses
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• LESSER: A Catalogue of Spectroscopically selected sample of Lyman-$\alpha$ Emitters Lensed By Galaxies
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• Confronting Kähler moduli inflation with CMB data
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Bayesian Comparison of the Cosmic Duality Scenarios
• Constraining quantum collapse inflationary models with current data: The semiclassical approach
• An investigation of the circumgalactic medium around z~2.2 AGN with ACA and ALMA
• Reconstructing WIMP properties through an interplay of signal measurements in direct detection, Fermi-LAT, and CTA searches for dark matter
• Time Resolved Absorption of Six Chemical Species With MAROON-X Points to Strong Drag in the Ultra Hot Jupiter TOI-1518 b
• On the radial velocity detection of additional planets in transiting, slowly rotating M-dwarf systems: the case of GJ 1132
• Forecasts on interacting dark energy with standard sirens
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• Transit Origami: A Method to Coherently Fold Exomoon Transits in Time Series Photometry
• Implications of a possible TeV break in the cosmic-ray electron and positron flux
• Constraining particle dark matter using local galaxy distribution
• Surrogate Models for Direct Dark Matter Detection
• Bayesian analysis and naturalness of (Next-to-)Minimal Supersymmetric Models
• The non-evolving internal structure of early-type galaxies: the case study SDSS J0728+3835 at z = 0.206
• The Luminous X-Ray Halos of Two Compact Elliptical Galaxies
• TASTE V. A new ground-based investigation of orbital decay in the ultra-hot Jupiter WASP-12b
• K2-263b: A 50-day period sub-Neptune with a mass measurement using HARPS-N
• Resolving the blazar CGRaBS J0809+5341 in the presence of telescope systematics
• JWST Observations of the Enigmatic Y Dwarf WISE 1828+2650: I. Limits to a Binary Companion
• Correlation of normal neutrino mass ordering with upper octant of ${\theta }_{23}^{}$ and third quadrant of $\delta$ via RGE-induced $\mu$-$\tau$ symmetry breaking
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• Dark Matter in Split SUSY with Intermediate Higgses
• VLTI/GRAVITY Observations and Characterization of the Brown Dwarf Companion HD 72946 B
• A formally motivated retrieval framework applied to the high resolution transmission spectrum of HD 189733 b
• A search for transit timing variations within the exomoon corridor using Kepler data
• Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 M${}_J$
• Dark Matter in 3D
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• Dark Matter versus h into gamma gamma and h into gamma Z with supersymmetric triplets
• On the determination of uncertainties in parton densities
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• Combining Photometry From Kepler and TESS to Improve Short-Period Exoplanet Characterization
• Measuring the Orbits of the Arches and Quintuplet Clusters using HST and Gaia: Exploring Scenarios for Star Formation Near the Galactic Center
• Evidence Networks: simple losses for fast, amortized, neural Bayesian model comparison
• Discovery of an Edge-on Circumstellar Debris Disk Around BD+45${}^{\circ }$598: a Newly Identifed Member of the $\beta$ Pictoris Moving Group
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• WASP-121b's transmission spectrum observed with JWST/NIRSpec G395H reveals thermal dissociation and SiO in the atmosphere
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• Atmospheric characterization of the super-Jupiter HIP 99770 b with KPIC
• Bayesian sparse reconstruction: a brute-force approach to astronomical imaging and machine learning
• Euclid: A complete Einstein ring in NGC 6505
• Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems
• The HARPS search for southern extra-solar planets. XLVI: 12 super-Earths around the solar type stars HD39194, HD93385, HD96700, HD154088, and HD189567
• Reconciling stellar dynamical and hydrostatic X-ray mass measurements of an elliptical galaxy with gas rotation, turbulence and magnetic fields
• Dynamical Surface Imaging of lambda Andromedae
• The Swansong of the Galactic Center Source X7: An Extreme Example of Tidal Evolution near the Supermassive Black Hole
• Scalable inference with Autoregressive Neural Ratio Estimation
• Mean shift cluster recognition method implementation in the nested sampling algorithm
• Pandora: A fast open-source exomoon transit detection algorithm
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• An independent assessment of significance of annual modulation in COSINE-100 data
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• Analysis of the planetary mass uncertainties on the accuracy of atmospherical retrieval
• VVV-WIT-08: the giant star that blinked
• Combining and comparing neutrinoless double beta decay experiments using different nuclei
• Efficient Estimation of Highly Structured Posteriors of Gravitational-Wave Signals with Markov-Chain Monte Carlo
• Fibre inflation and precision CMB data
• Probing protoneutron stars with gamma-ray axionscopes
• Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• Far beyond stacking: Fully bayesian constraints on sub-microJy radio source populations over the XMM-LSS-VIDEO field
• Evidence for stellar contamination in the transmission spectra of HAT-P-12b
• Bayesian evidence of non-standard inflation: isocurvature perturbations and running spectral index
• Active learning BSM parameter spaces
• Measuring the HI mass function below the detection threshold
• Reflected spectroscopy of small exoplanets III: probing the UV band to measure biosignature gasses
• Nonperturbative infrared finiteness in super-renormalisable scalar quantum field theory
• Accelerating Bayesian microseismic event location with deep learning
• An ice giant exoplanet interpretation of the anomaly in microlensing event OGLE-2011-BLG-0173
• The Weird Detector: Flagging periodic, coherent signals of arbitrary shape in time series photometry
• Nested sampling with plateaus
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• New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing
• Modelling of the Complex CASSOWARY/SLUGS Gravitational Lenses
• A million-solar-mass object detected at cosmological distance using gravitational imaging
• A statistical measurement of the HI spin temperature in DLAs at cosmological distances
• Terminus: A Versatile Simulator for Space-based Telescopes
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• Testing galaxy formation models with galaxy stellar mass functions
• Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars
• A Study of Stellar Spins in 15 Open Clusters
• A dynamical approach in exploring the unknown mass in the Solar system using pulsar timing arrays
• Searches for Cosmic-String Gravitational-Wave Bursts in Mock LISA Data
• Cross-Comparison of Sampling Algorithms for Pulse Profile Modeling of PSR J0740+6620
• The HARPS search for southern extra-solar planets XL. Searching for Neptunes around metal-poor stars
• The lost sunspot cycle: New support from Be10 measurements
• Axino dark matter with low reheating temperature
• Investigating subphotospheric dissipation in gamma-ray bursts using joint Fermi-Swift observations
• Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data
• Knobs and dials of retrieving JWST transmission spectra. I. The importance of p-T profile complexity
• The GALAH Survey: Using Galactic Archaeology to Refine our Knowledge of TESS Target Stars
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Dark matter substructure cannot explain properties of the Fermi Galactic Centre excess
• The Unusually High Halo Concentration of the Fossil Group NGC 6482: Evidence for Weak Adiabatic Contraction
• The Exceptional X-ray Evolution of SN1996cr in High Resolution
• An absolute mass, precise age, and hints of planetary winds for WASP-121 A and b from a JWST NIRSpec phase curve
• K2-113b: A dense hot-Jupiter transiting a solar analogue
• Improvement of the Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Inversion Code
• Further Sunyaev-Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager
• The optically-selected 1.4-GHz quasar luminosity function below 1 mJy
• Multi-Mask Least-Squares Deconvolution: Extracting RVs using tailored masks
• Toward Solving the Puzzle: Dissecting the Complex Merger A521 with Multi-wavelength Data
• Relativistic reflection from accretion disks in the population of Active Galactic Nuclei at z=0.5-4
• Halo-independence with quantified maximum entropy at DAMA/LIBRA
• Exploring black-hole scaling relations via the ensemble variability of Active Galactic Nuclei
• Tracking the footprints of the radio pulsar B1727$-$47: proper motion, host supernova remnant, and the glitches
• A systematic validation of hot Neptunes in TESS data
• AMI observations of ten CLASH galaxy clusters: SZ and X-ray data used together to determine cluster dynamical states
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• Inferring dark energy properties from the scale factor parametrisation
• Wolf-Rayet galaxies in SDSS-IV MaNGA. II. Metallicity dependence of the high-mass slope of the stellar initial mass function
• The spectacular cluster chain Abell 781 as observed with LOFAR, GMRT, and XMM-Newton
• Robust profile decomposition for large extragalactic spectral-line surveys
• Pulse Profile Modeling of Thermonuclear Burst Oscillations I: The Effect of Neglecting Variability
• Helioseismic and Neutrino Data Driven Reconstruction of Solar Properties
• The ESO SupJup Survey VII: Clouds and line asymmetries in CRIRES${}^{+}$ J-band spectra of the Luhman 16 binary
• AMI SZ observations and Bayesian analysis of a sample of six redshift-one clusters of galaxies
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Sunyaev--Zel'dovich profile fitting with joint AMI-Planck analysis
• A multi-planetary system orbiting the early-M dwarf TOI-1238
• The role of stochastic and smooth processes in regulating galaxy quenching
• A 5% measurement of the gravitational constant in the Large Magellanic Cloud
• MFV Reductions of MSSM Parameter Space
• Semi-analytic spectral fitting: simultaneously modelling the mass accumulation and chemical evolution in MaNGA spiral galaxies
• Cold Dark Matter Hypotheses in the MSSM
• Monochromatic neutrino lines from sneutrino dark matter
• Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H
• Long lived charginos in Natural SUSY?
• Bayesian evidence estimation from posterior samples with normalizing flows
• Classifying LISA gravitational wave burst signals using Bayesian evidence
• Understanding and improving the timing of PSR J0737-3039B
• Competing chemical signatures in the atmosphere of TOI-270 d: Inference of sulfur and carbon chemistry
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• A robust constraint on cosmic textures from the cosmic microwave background
• Highly structured inner planetary system debris around the intermediate age Sun-like star TYC 8830 410 1
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• The impact of neutron star spin on X-ray spectra
• Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore
• Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
• Constraints on the Tensor-to-Scalar ratio for non-power-law models
• Flavor constraints for a Vector-like quark of Nelson-Barr type
• MIRI-LRS spectrum of a cold exoplanet around a white dwarf: water, ammonia, and methane measurements
• On the importance of direct detection combined limits for spin independent and spin dependent dark matter interactions
• Uncovering the Invisible: A Study of Gaia18ajz, a Candidate Black Hole Revealed by Microlensing
• A new approach to modelling gamma-ray burst afterglows: Using Gaussian processes to account for the systematics
• New determination of the production cross section for $\gamma$ rays in the Galaxy
• The Nested_fit data analysis program
• The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
• Do stellar-mass and super-massive black holes have similar dining habits?
• Revisiting the Transit Timing Variations in the TrES-3 and Qatar-1 systems with TESS data
• Isolated pulsar population synthesis with simulation-based inference
• Impact of RGE-induced $\mu -\tau$ Reflection Symmetry Breaking on the Effective Majorana Neutrino Mass in $0\nu \beta \beta$ Decay
• EasyScan_HEP: a tool for connecting programs to scan the parameter space of physics models
• Model discrimination in pseudoscalar-meson photoproduction
• The cosmological analysis of X-ray cluster surveys; III. 4D X-ray observable diagrams
• An Efficient Interpolation Technique for Jump Proposals in Reversible-Jump Markov Chain Monte Carlo Calculations
• Flat spectrum radio quasars and BL Lacs dominate the anisotropy of the unresolved gamma-ray background
• EXPRES. II. Searching for Planets Around Active Stars: A Case Study of HD 101501
• Allesfitter: Flexible Star and Exoplanet Inference From Photometry and Radial Velocity
• Viability of exact tri-bimaximal, golden-ratio and bimaximal mixing patterns and renormalization-group running effects
• A Search for Neutrino Point-Source Populations in 7 Years of IceCube Data with Neutrino-count Statistics
• Supersymmetry Searches in GUT Models with Non-Universal Scalar Masses
• Uncovering axion-like particles in supernova gamma-ray spectra
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• ACCESS: An optical transmission spectrum of the high-gravity, hot Jupiter HAT-P-23b
• Galaxy blending effects in deep imaging cosmic shear probes of cosmology
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Kepler-1708 b-i is likely undetectable with HST
• Fundamental Physics with ESPRESSO, Constraining a simple parametrisation for varying $\alpha$
• Analyzing Exoplanet Phase Curve Information Content: Toward Optimized Observing Strategies
• Estimation of singly-transiting K2 planet periods with Gaia parallaxes
• Higgs Quark Flavor Violation: Simplified Models and Status of General Two-Higgs-Doublet Model
• Exploring phase space with Nested Sampling
• EXONEST: The Bayesian Exoplanetary Explorer
• RV-exoplanet eccentricities: Good, Beta, and Best
• $\mu -\tau$ Reflection Symmetry and Its Explicit Breaking for Leptogenesis in a Minimal Seesaw Model
• Obscuration properties of mid-IR selected AGN
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• Impacts of high-contrast image processing on atmospheric retrievals
• Polarized radiation from an accretion shock in accreting millisecond pulsars using exact Compton scattering formalism
• Unrecognized Astrometric Confusion in the Galactic Centre
• Prospects for Distinguishing Dark Matter Models Using Annual Modulation
• Use Model Averaging instead of Model Selection in Pulsar Timing
• 3D Radiative Transfer Modelling and Virial Analysis of Starless Cores in the B10 Region of the Taurus Molecular Cloud
• Thermal dark matter implies new physics not far above the weak scale
• Free-form modelling of galaxy clusters: a Bayesian and data-driven approach
• Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
• Toward a multidimensional analysis of transmission spectroscopy. Part III: Modelling 2D effects in retrievals with TauREx
• Detection of Na and K in the atmosphere of the hot Jupiter HAT-P-1b with P200/DBSP
• The multi-epoch X-ray tale of I Zwicky 1 outflows
• A Circumplanetary Dust Ring May Explain the Extreme Spectral Slope of the 10 Myr Young Exoplanet K2-33b
• Exploring the single-pulse behaviours of PSR J0628+0909 with FAST
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Introducing the Texas Euclid Survey for Lyman Alpha (TESLA) Survey: Initial Study Correlating Galaxy Properties to Lyman-Alpha Emission
• The Chemical Composition of Extreme-Velocity Stars
• IGRINS observations of WASP-127 b: H${}_2$O, CO, and super-Solar atmospheric metallicity in the inflated sub-Saturn
• One Fits All: A Unified Synchrotron Model Explains GRBs with FRED-Shaped Pulses
• Stop-mass prediction in naturalness scenarios within MSSM-25
• Bayes-X: a Bayesian inference tool for the analysis of X-ray observations of galaxy clusters
• Broad, weak 21 cm absorption in an early type galaxy: spectral-line finding and parametrization for future surveys
• Monitoring clumpy wind accretion in supergiant fast X-ray transients with XMM-Newto
• Constraining the formation of WASP-39b using JWST transit spectroscopy
• On The Distribution of Bayesian Evidences
• Stellar kinematics using a third integral of motion: method and application on the Andromeda galaxy
• Constraining $f(R)$ Gravity with a $k$-cut Cosmic Shear Analysis of the Hyper Suprime-Cam First-Year Data
• WASP-35 and HAT-P-30/WASP-51: re-analysis using TESS and ground-based transit photometry
• The EDGES measurement disfavors an excess radio background during the cosmic dawn
• The Global Magneto-Ionic Medium Survey (GMIMS): The brightest polarized region in the Southern sky at 75cm and its implications for Radio Loop II
• The hot interstellar medium towards 4U 1820-30: a Bayesian analysis
• ISPY -- NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• Demographics of the M-star Multiple Population in the Orion Nebula Cluster
• A blind detection of a large, complex, Sunyaev--Zel'dovich structure
• A precise blue-optical transmission spectrum from the ground: Evidence for haze in the atmosphere of WASP-74b
• Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• TD-CARMA: Painless, accurate, and scalable estimates of gravitational-lens time delays with flexible CARMA processes
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• Earth as an Exoplanet. III. Using Empirical Thermal Emission Spectra as an Input for Atmospheric Retrieval of an Earth-twin Exoplanet
• Validation of HD 183579b using archival radial velocities: a warm-neptune orbiting a bright solar analog
• Radiative Corrections to the Solar Lepton Mixing Sum Rule
• Measuring glitch recoveries and braking indices with Bayesian model selection
• Bayesian Model Testing of Ellipsoidal Variations on Stars due to Hot Jupiters
• Tentative detection of titanium oxide in the atmosphere of WASP-69 b with a 4m ground-based telescope
• Rotational and radio emission properties of PSR J0738-4042 over half a century
• Designing Decisive Detections
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Bayesian evidence-driven likelihood selection for sky-averaged 21-cm signal extraction
• Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array
• Pulse Profile Modelling of Thermonuclear Burst Oscillations II: Handling variability
• A hierarchical Bayesian approach for reconstructing the Initial Mass Function of Single Stellar Populations
• Evidence for thermal X-ray emission from the synchrotron dominated shocks in Tycho's supernova remnant
• The viability of ultralight bosonic dark matter in dwarf galaxies
• Detection of the 2175Å UV Bump at z>7: Evidence for Rapid Dust Evolution in a Merging Reionisation-Era Galaxy
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Determination of neutrino mass ordering in future ${}^{76}$Ge-based neutrinoless double-beta decay experiments
• Comparison of cosmological parameter inference methods applied to supernovae lightcurves fitted with SALT2
• Information geometry in cosmological inference problems
• Behind the Spotlight: A systematic assessment of outshining using NIRCam medium-bands in the JADES Origins Field
• Fast likelihood-free inference in the LSS Stage IV era
• The Chinese pulsar timing array data release I. Polarimetry for 56 millisecond pulsars
• Impact of leptonic unitarity and dark matter direct detection experiments on the NMSSM with inverse seesaw mechanism
• Additional JWST/NIRSpec Transits of the Rocky M Dwarf Exoplanet GJ 1132 b Reveal a Featureless Spectrum
• A detailed temperature map of the archetypal protostellar shocks in L1157
• OGLE-2013-BLG-0132Lb and OGLE-2013-BLG-1721Lb: Two Saturn-mass Planets Discovered around M-dwarfs
• Bayesian Model comparison of Higgs couplings
• An Empirical Bayesian Approach to Limb-darkening in Modeling WASP-121b Transit Light Curves
• BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN
• Dark matter candidates in the NMSSM with RH neutrino superfields
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• Dipole-induced anomalous top quark couplings at the LHC
• LRG-BEASTS: Evidence for clouds in the transmission spectrum of HATS-46 b
• Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of $\alpha$ Cen A. I. Observations, Orbital and Physical Properties, and Exozodi Upper Limits
• Interpreting the Fermi-LAT gamma ray excess in the simplified framework
• The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary
• A MeerKAT view of the double pulsar eclipses -- Geodetic precession of pulsar B and system geometry
• Supersymmetry With Prejudice: Fitting the Wrong Model to LHC Data
• Scintillating bolometers: a key for determining WIMP parameters
• Enabling Robust Exoplanet Atmospheric Retrievals with Gaussian Processes
• Gravitational-Wave Geodesy: A New Tool for Validating Detection of the Stochastic Gravitational-Wave Background
• GPU-accelerated LISA parameter estimation with full time domain response
• Astronomy and astrophysics with gravitational waves in the Advanced Detector Era
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
• A spectroscopic map of the Galactic centre -- Observations and resolved stars
• Thermal Emission from the hot Jupiter WASP-103b in J and Ks Bands
• Dark Matter, Sparticle Spectroscopy and Muon $(g-2)$ in $SU(4{)}_c\times SU(2{)}_L\times SU(2{)}_R$
• Nuclear Level Density and $\gamma$-ray Strength Function of ${}^{67}\mathrm{Ni}$ and the impact on the i-process
• Optimising Inflationary Features the Bayesian Way
• Measuring the baryonic Tully-Fisher relation below the detection threshold
• Dark lens candidates from Gaia Data Release 3
• NGC 1266: Characterization of the Nuclear Molecular Gas in an Unusual SB0 Galaxy
• Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
• Investigating time variability of X-ray absorption in Swift GRBs
• Uniform Modelling of the Stellar Density of Thirteen Tidal Streams within the Galactic Halo
• Measuring Star-Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams I: Model Definition and Mock Tests
• Constraints on Equivalence Principle Violation from Gamma Ray Bursts
• Resolving the mass--anisotropy degeneracy of the spherically symmetric Jeans equation I: theoretical foundation
• Machine Learning Model of the Swift/BAT Trigger Algorithm for Long GRB Population Studies
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: II. Dark Matter and Baryon Fraction
• Detecting and Characterizing Water Vapor in the Atmospheres of Earth Analogs through Observation of the 0.94 Micron Feature in Reflected Light
• Refractory and Volatile Species in the UV-to-IR Transmission Spectrum of Ultra-hot Jupiter WASP-178b with HST and JWST
• The Effect of $\alpha$-Vacua on the Scalar and Tensor Spectral Indices: Slow-Roll Approximation
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• A Population Analysis of 20 Exoplanets Observed from the Optical to the Near-infrared Wavelengths with HST: Evidence for Widespread Stellar Contamination
• Quintessential Implications of the presence of AdS in the Dark Energy sector
• Entanglement masquerading in the CMB
• Flow Matching for Atmospheric Retrieval of Exoplanets: Where Reliability meets Adaptive Noise Levels
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Weighing the Local Interstellar Medium using Gamma Rays and Dust
• Physical modelling of galaxy clusters detected by Planck
• Study of the $B^0\to \rho (770{)}^0{K}^{\ast }(892{)}^0$ decay with an amplitude analysis of $B^0\to ({\pi }^{+}{\pi }^{-})(K^{+}{\pi }^{-})$ decays
• Direct Measurement of Extinction in a Planet-Hosting Gap
• Discovery of the variable optical counterpart of the redback pulsar PSR J2055+1545
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• Mitigating baryonic effects with a theoretical error covariance
• Bayesian model selection for electromagnetic kaon production on the nucleon
• Cosmological bounds on neutrino statistics
• The peculiar physics of GRB 170817A and their implications for short GRBs
• Benchmark tests of transmission spectroscopy using transiting white dwarfs
• Extreme winds on the emerging dayside of an ultrahot Jupiter
• $\pi$ Earth: a 3.14-day Earth-sized Planet from $\text{K2}$'s Kitchen Served Warm by the SPECULOOS Team
• Diversity in the haziness and chemistry of temperate sub-Neptunes
• Detectability of Rocky-Vapour Atmospheres on Super-Earths with Ariel
• Model-independent determination of cosmic curvature based on Padé approximation
• A highly mutually-inclined, compact warm-Jupiter system KOI-984 ?
• Compact source detection in multi-channel microwave surveys: from SZ clusters to polarized sources
• Pursuing Truth: Improving Retrievals on Mid-Infrared Exo-Earth Spectra with Physically Motivated Water Abundance Profiles and Cloud Models
• AMOEBA: Automated Molecular Excitation Bayesian Line-Fitting Algorithm
• The Orbit and Companion of PSR J1622-0315: Variable Asymmetry and a Massive Neutron Star
• Quantifying torque from the Milky Way bar using Gaia DR2
• Towards fast machine-learning-assisted Bayesian posterior inference of microseismic event location and source mechanism
• Measuring the alpha-abundance of subsolar-metallicity stars in the Milky Way's central half-parsec: testing globular cluster and dwarf galaxy infall scenarios
• Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping:Monte Carlo Simulations
• A search for X-ray absorbed sources in the 3XMM catalogue, using photometric redshifts and Bayesian spectral fits
• Non-holomorphic modular flavor symmetry and odd weight polyharmonic Maaß form
• Rocks, Water and Noble Liquids: Unfolding the Flavor Contents of Supernova Neutrinos
• The ESO SupJup Survey VIII. Chemical fingerprints of young L dwarf twins
• Revisiting the Architecture of the KOI-89 System
• A minimal inverse seesaw model with $S_4$ flavour symmetry
• Evidence That Hydra I is a Tidally Disrupting Milky Way Dwarf Galaxy
• Methods and stability tests associated with the sterile neutrino search using improved high-energy ${\nu }_{\mu }$ event reconstruction in IceCube
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• Global Optimization for Future Gravitational Wave Detectors' Sites
• Enhanced lines and box-shaped features in the gamma-ray spectrum from annihilating dark matter in the NMSSM
• Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267
• The Radius of PSR J0437-4715 from NICER Data
• An unusually large gaseous transit in a debris disc
• The inflated, eccentric warm Jupiter TOI-4914 b orbiting a metal-poor star, and the hot Jupiters TOI-2714 b and TOI-2981 b
• Stochastic determination of matrix determinants
• R-parity violating chargino decays at the LHC
• The curse of clouds
• Comparing transit spectroscopy pipelines at the catalogue level: evidence for systematic differences
• Dark Energy Survey Year 3 Results: Cosmological constraints from second and third-order shear statistics
• Generalized Blind Spots for Dark Matter Direct Detection in the 2HDM
• Tentative sensitivity of future $0\nu \beta \beta$-decay experiments to neutrino masses and Majorana CP phases
• The 31-year Rotation History of the Millisecond Pulsar J1939+2134 (B1937+21)
• Coupled-channels treatment of ${}^7\mathrm{Be}(p,\gamma {)}^8\mathrm{B}$ in effective field theory
• TIC~257060897b: an inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star
• New BRITE-Constellation observations of the roAp star Alpha Circini
• Implications of Pulsar Timing Array Results for High Frequency Gravitational Waves
• Quantifying the tension between the Higgs mass and (g-2)_mu in the CMSSM
• Comparing the frequentist and Bayesian periodic signal detection: rates of statistical mistakes and sensitivity to priors
• ARES VI: Viability of one-dimensional retrieval models for transmission spectroscopy characterization of exo-atmospheres in the era of JWST and Ariel
• NICMOS Kernel-Phase Interferometry I: Catalogue of Brown Dwarfs Observed in F110W and F170M
• Trans-Planckian Effects in Warm Inflation
• Retrieving planet formation parameters of WASP-77Ab using SimAb
• Evidence for a brief appearance of gamma-ray periodicity after a compact star merger
• The Cosmic Background Imager 2
• Learn-As-You-Go Acceleration of Cosmological Parameter Estimates
• An HST Transmission Spectrum of the Closest M-Dwarf Transiting Rocky Planet LTT 1445Ab
• Histogram comparison as a powerful tool for the search of new physics at LHC. Application to CMSSM
• Dynamical Modeling of NGC 6809: Selecting the best model using Bayesian Inference
• CombineHarvesterFlow: Joint Probe Analysis Made Easy with Normalizing Flows
• Computing Entropies With Nested Sampling
• A Systematic Study of Projection Biases in Weak Lensing Analysis
• Cloudy mornings and clear evenings on a gas giant exoplanet
• Is there evidence for CIDER in the Universe?
• Time delay interferometry with minimal null frequencies
• Two-Point Separation Functions for Modeling Wide Binary Systems in Nearby Dwarf Galaxies
• Effects of periodicity in observation scheduling on parameter estimation of pulsar glitches
• Testing Higgs boson scenarios in the phenomenological NMSSM
• Detecting molecules in Ariel low resolution transmission spectra
• Constraining Orbital Periods from Nonconsecutive Observations: Period Estimates for Long-Period Planets in Six Systems Observed by K2 During Multiple Campaigns
• An Expanded Chemo-dynamical Sample of Red Giants in the Bar of the Large Magellanic Cloud
• Narrow Band X-ray Photometry as a Tool for Studying Galaxy and Cluster Mass Distributions
• Discrimination of anisotropy in dark matter velocity distribution with directional detectors
• CROCODILE \\ Incorporating medium-resolution spectroscopy of close-in directly imaged exoplanets into atmospheric retrievals via cross-correlation
• AMI SZ observation of galaxy-cluster merger CIZA J2242+5301: perpendicular flows of gas and dark matter
• The intrinsic X-ray luminosity distribution of an optically-selected SDSS quasar population
• Enhancing noise characterization with robust time delay interferometry combination
• Unveiling the Cosmic Gems Arc at $z\sim 10$ with JWST NIRCam
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Low-mass neutralino dark matter in supergravity scenarios: phenomenology and naturalness
• The GALAH Survey: Improving our understanding of confirmed and candidate planetary systems with large stellar surveys
• Measurement of the charged pion mass using a low-density target of light atoms
• Searching for high-energy gamma-ray counterparts to Gravitational Wave sources with Fermi-LAT: a needle in a haystack
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
• NGTS-21b: An Inflated Super-Jupiter Orbiting a Metal-poor K dwarf
• Prospects for disentangling dark matter with weak lensing
• Kernel Phase and Kernel Amplitude in Fizeau Imaging
• Coupling quintessence kinetics to electromagnetism
• DeepGlow: an efficient neural-network emulator of physical afterglow models for gamma-ray bursts and gravitational-wave events
• The effect of spectroscopic binning on atmospheric retrievals
• Spatially resolving polycyclic aromatic hydrocarbons in Herbig Ae disks with VISIR-NEAR at the VLT
• Near-instantaneous Atmospheric Retrievals and Model Comparison with FASTER
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• The decisive future of inflation
• On The Synergy Between Ariel And Ground-Based High-Resolution Spectroscopy
• Planet-star interactions with precise transit timing. IV. Probing the regime of dynamical tides for GK host stars
• Stage IV baryonic feedback correction for non-Gaussianity inference
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• Detecting and Monitoring Tidal Dissipation of Hot Jupiters in the Era of SiTian
• ALMA's view of the M-dwarf GSC 07396-00759's edge-on debris disc: AU Mic's coeval twin
• Horizontal and vertical exoplanet thermal structure from a JWST spectroscopic eclipse map
• Evidence of Titanate Clouds in the Day-side Atmosphere of the Ultra-Hot Jupiter WASP-121b
• HST Transmission Spectra of the Hot-Neptune HD 219666 b: Detection of Water and the Challenge of Constraining Both Water and Methane
• Consistent explanation for the cosmic-ray positron excess in $p$-wave Breit-Wigner enhanced dark matter annihilation
• Non-equilibrium in the Solar Neighbourhood using dynamical modelling with Gaia DR2
• A Comprehensive Study of the Young Cluster IRAS 05100+3723: Properties, Surrounding Interstellar Matter, and Associated Star Formation
• Constraining fine tuning in Composite Higgs Models with partially composite leptons
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
• A grand-design spiral galaxy 1.5 billion years after the Big Bang with JWST
• Probing intractable beyond-standard-model parameter spaces armed with Machine Learning
• ACCESS: Tentative detection of H${}_2$O in the ground-based optical transmission spectrum of the low-density hot Saturn HATS-5b
• Reducing instrumental errors in Parkes Pulsar Timing Array data
• Gaussian Mixture Models for Blended Photometric Redshifts
• A Wide Orbit Exoplanet OGLE-2012-BLG-0838Lb
• GausSN: Bayesian Time-Delay Estimation for Strongly Lensed Supernovae
• Exact SU(5) Yukawa matrix unification in the General Flavour Violating MSSM
• Bayesian pulsar timing and noise analysis with Vela.jl: an overview
• Universality of the halo mass function in screened gravity theories
• The SPAN512 mid-latitude pulsar survey at the Nançay Radio Telescope
• Disentangling disc and atmospheric signatures of young brown dwarfs with JWST/NIRSpec
• Baryonic Ecosystem in Galaxies (BEINGMgII) -- II. Unveiling the Nature of Galaxies Harboring Cool Gas Reservoirs
• Bayesian recalibration of Planck galaxy cluster scaling relations including relativistic Sunyaev-Zel'dovich corrections
• Gravitational Wave Astronomy: Needle in a Haystack
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• Gravitational Microlensing Event Statistics for the Zwicky Transient Facility
• A Comprehensive Investigation of Gamma-Ray Burst Afterglows Detected by TESS
• Nested Sampling for Non-Gaussian Inference in SLAM Factor Graphs
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Grid-based exploration of cosmological parameter space with Snake
• Improving pulsar-timing solutions through dynamic pulse fitting
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• Simultaneous multicolour transit photometry of hot Jupiters HAT-P-19b, HAT-P-51b, HAT-P-55b, and HAT-P-65b
• Inferring properties of neutron stars born in short gamma-ray bursts with a plerion-like X-ray plateau
• Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes
• Replica exchange nested sampling
• Status of negative coupling modifiers for extended Higgs sectors
• GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems
• Type Ia supernova constraints on compact object dark matter
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• Masses of the Kepler-419 Planets from Transit Timing Variations Analysis
• Bayesian Methods for Exoplanet Science
• The Similar Seven: A set of very-alike exoplanets to test correlations between system parameters and atmospheric properties
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• A Detailed Investigation of HD 209458 b HST & JWST Transmission Spectra with SANSAR
• Impact of lensing magnification on the analysis of galaxy clustering in redshift space
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• Detecting episodes of star formation using Bayesian model selection
• LHC and dark matter phenomenology of the NUGHM
• Effects of supersymmetric threshold corrections on the Yukawa matrix unification
• The role of cloud particle properties on WASP-39b transmission spectrum based on JWST/NIRSpec observations
• Can Dark Stars account for the star formation efficiency excess at very high redshifts?
• Detectability of Polycyclic Aromatic Hydrocarbons in the Atmosphere of WASP-6 b with JWST NIRSpec PRISM
• Equation-of-state-informed pulse profile modeling
• Bayes-factor of the ATLAS diphoton excess
• A reanalysis of the LHS 1140 b atmosphere observed with the Hubble Space Telescope
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• A super-Earth and a mini-Neptune around Kepler-59
• Impostor Among $\nu$s: Dark Radiation Masquerading as Self-Interacting Neutrinos
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Constraining a Model of the Radio Sky Below 6 MHz Using the Parker Solar Probe/FIELDS Instrument in Preparation for Upcoming Lunar-based Experiments
• Data Analysis and Phenomenological Cosmology
• A method to calculate gravitational accelerations within discrete localised regions in the Milky Way
• Beyond Fisher Forecasting for Cosmology
• Data Analysis Challenges for the Einstein Telescope
• archNEMESIS: an open-source Python package for analysis of planetary atmospheric spectra
• Informed total-error-minimizing priors: Interpretable cosmological parameter constraints despite complex nuisance effects
• Hierarchical Bayesian inference of the Initial Mass Function in Composite Stellar Populations
• Pulsar timing irregularities and the Neutron Star interior in the era of SKA: An Indian Outlook
• Geminga contribution to the cosmic-ray positron excess according to the gamma-ray observations
• Alternative Renormalizable Minimal SO(10) GUTs and Data Fitting
• Simultaneous multicolour optical and near-IR transit photometry of GJ 1214b with SOFIA
• Resolving the mass--anisotropy degeneracy of the spherically symmetric Jeans equation II: optimum smoothing and model validation
• Dark Matter Freeze-out during $\mathrm{SU}(2{)}_{\mathrm{L}}$ Confinement
• A re-analysis of equilibrium chemistry in five hot Jupiters
• DIAMONDS: A new Bayesian nested sampling tool
• Period change of massive binaries from combined photometric and spectroscopic data in Cygnus OB2
• Global fits of SUSY at future Higgs factories
• A Transiting Super-Earth in the Radius Valley and An Outer Planet Candidate Around HD 307842
• A Comprehensive Analysis of the Panchromatic Transmission Spectrum of the Hot-Saturn WASP-96 b: Nondetection of Haze, Possible Sodium Limb Asymmetry, Stellar Characterization, and Formation History
• On a possible cosmological evolution of galaxy cluster $Y_{\mathrm{X}}-Y_{\mathrm{SZE}}$ scaling relation
• A heavy neutral gauge boson near the Z boson mass pole via third generation fermions at the LHC
• A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models
• 2HDM singlet portal to dark matter
• Dark Matter in the CP-violating NMSSM
• Calculating Bayesian evidence for inflationary models using CONNECT
• A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses
• Data Compression and Covariance Matrix Inspection: Cosmic Shear
• Bayesian Active Search on Parameter Space: a 95 GeV Spin-0 Resonance in the ($B-L$)SSM
• Surrogate models for lightcurves and photosphere properties of Type II supernovae
• Numerical Exploration of Soliton Creation
• Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• The origin of the coherent radio flash potentially associated with GRB 201006A
• Optimizing future dark energy surveys for model selection goals
• A growing braking index and spin-down swings for the pulsar PSR B0540-69
• SAFARI I: A SPHERE discovery of a super metal-rich M dwarf companion to the star HD 86006
• Star formation histories of massive red spiral galaxies in the local universe
• Gauge $SU(2{)}_f$ flavour transfers
• Automatic detection of long-duration transients in Fermi-GBM data
• Gaussbock: Fast parallel-iterative cosmological parameter estimation with Bayesian nonparametrics
• Doomed Worlds II: Reassessing Suggestions of Orbital Decay for TrES-5 b
• HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen
• A joint effort to discover and characterize two resonant mini Neptunes around TOI-1803 with TESS, HARPS-N and CHEOPS
• A Polarization Pipeline for Fast Radio Bursts Detected by CHIME/FRB
• Impact sculpting of the early martian atmosphere
• New Constraints on Anisotropic Expansion from Supernovae Type Ia
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods II: Population inference
• Precise radial velocities of giant stars -- XVII. Distinguishing planets from intrinsically induced radial velocity signals in evolved stars
• A Global Fit of Non-Relativistic Effective Dark Matter Operators Including Solar Neutrinos
• Supersymmetry after the Higgs
• Applying Bayesian Inference to Galileon Solutions of the Muon Problem
• Aerosols and hydrocarbons in the atmosphere of a white dwarf planet
• How to Find a Planet from Transit Variations
• Magellan/M2FS Spectroscopy of Galaxy Clusters: Stellar Population Model and Application to Abell 267
• Detection of CO${}_2$, CO, and H${}_2$O in the atmosphere of the warm sub-Saturn HAT-P-12b
• Unveiling the nature of the Einstein Probe transient EP 241021a
• Complementarity of direct detection experiments in search of light Dark Matter
• Bayesian technique to combine independently-trained Machine-Learning models applied to direct dark matter detection
• A Close-in Planet Orbiting Giant Star HD 167768
• Majorana phases in high-scale mixings unification hypotheses
• Effect of Centrifugal Force on Transmission Spectroscopy of Exoplanet Atmospheres
• A Bayesian blind survey for cold molecular gas in the Universe
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Robust parameter estimation from pulsar timing data
• Modern Bayesian Sampling Methods for Cosmological Inference: A Comparative Study
• The CHEOPS view on the climate of WASP-3 b
• Beyond LambdaCDM: How the Hubble tension challenges early universe physics
• A Venus in the Making? Predictions for JWST Observations of the Ultracool M-Dwarf planet LP 890-9 c
• Right-handed sneutrino and gravitino multicomponent dark matter in light of neutrino detectors
• Light dark matter around 100 GeV from the inert doublet model
• Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Global Chemistry and Thermal Structure Models for the Hot Jupiter WASP-43b and Predictions for JWST
• Bayes and present dark matter direct search status
• Cosmology with shear ratios: a joint study of weak lensing and spectroscopic redshift datasets
• TrES-1 b: A Case Study in Detecting Secular Evolution of Exoplanet Orbits
• A Preference for Cold Dark Matter over Superfluid Dark Matter in Local Milky Way Data
• Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate
• Asteroseismic Data Analysis with DIAMONDS
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods I: Spectral analysis
• A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054
• Bayesian analysis for a class of $\alpha$-attractor inflationary models
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
• Impact of Accretion Assumptions on Pulse Profile Modelling of Superburst Oscillations in 4U 1636-536
• Knobs and dials of retrieving JWST transmission spectra. II. Impacts of pipeline-level differences on retrieval posteriors
• ZTF SN~Ia DR2: Cosmology-independent constraints on Type Ia supernova standardisation from supernova siblings
• Reionization in Protocluster Environments at $z>7$ with JWST/NIRSpec
• A Two-limb Explanation for the Optical-to-infrared Transmission Spectrum of the Hot Jupiter HAT-P-32Ab
• Characterizing the Expected Behavior of Non-Poissonian Template Fitting
• A study of radial self-similar non-relativistic MHD outflow models: parameter space exploration and application to the water fountain W43A
• Time delay interferometry with minimal null frequencies and shortened time span
• Radio Galaxy Detection in the Visibility Domain
• A systematic study of projection biases in the Weak Lensing analysis of cosmic shear and the combination of galaxy clustering and galaxy-galaxy lensing
• Parameter constraints for accreting millisecond pulsars with synthetic NICER data
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• AMI-CL J0300+2613: a Galactic anomalous-microwave-emission ring masquerading as a galaxy cluster
• Dark matter properties implied by gamma ray interstellar emission models
• OrbDot: A Python package for studying the secular evolution of exoplanet orbits
• From gas to stars: MUSEings on the internal evolution of IC 1613
• Pulse profile modelling of the accretion-powered millisecond pulsar SAX J1808.4-3658 using NICER data from its 2019 and 2022 outbursts
• Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
• Structure and Dynamics of the Young Massive Star Cluster Westerlund 1
• Evidence of the association of repeating fast-radio-burst sources with fast-spinning super-twisted magnetars
• Probing chromatic onsets of gravitational wave overtones
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• H I absorption line and anomalous dispersion in the radio pulses of PSR B1937+21
• Data Analysis Methods for Testing Alternative Theories of Gravity with LISA Pathfinder
• A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
• Detection of a Millisecond Periodicity in BATSE Short Gamma-Ray Bursts
• Revisiting wideband pulsar timing measurements
• Beetroots: spatially-regularized Bayesian inference of physical parameter maps -- Application to Orion
• Disentangling Atmospheric Compositions of K2-18 b with Next Generation Facilities
• KRONOS I: The $1-2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c
• HyDRo: Atmospheric Retrieval of Rocky Exoplanets in Thermal Emission
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces
• Inferring the Gas-to-Dust Ratio in the Main Planet-Forming Region of Disks
• The GAPS programme at TNG LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
• Status of ${\mathbb{Z}}_3$-NMSSM featuring a light bino-dominated LSP and a light singlet-like scalar under the LZ Experiment
• $SO(10)$ models with $A_4$ modular symmetry
• Impact of the LZ Experiment on the DM Phenomenology and Naturalness in the MSSM
• Low-energy electrons in GRB afterglow models
• Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
• Thermal emission spectra of the ultra-hot Jupiter WASP-33 b
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b
• Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission
• Kilonova Light Curve Parameter Estimation Using Likelihood-Free Inference
• Two unseen massive white dwarf candidates in close binaries
• Constraining the light Higgs bosons in the GNMSSM with recent Higgs data
• Gaia-GIC-1: An Evolving Catastrophic Planetesimal Collision Candidate
• Flavored gauge mediation in the Peccei-Quinn NMSSM
• Multi-epoch afterglow rebrightenings in GRB 250129A: Evidence for successive shock interactions
• MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z\sim 1$ star-forming galaxies
• Hot Rocks Survey V: Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI
• Breaking of the tetra-maximal neutrino mixing pattern
• A new look into the atmospheric composition of WASP-39 b
• Improving INTEGRAL/SPI data analysis of GRBs
• Model-independent approach for incorporating interference effects in collider searches for new resonances
• Predicting Sunyaev-Zel'dovich effect observations of galaxy cluster cavities with the Square Kilometre Array
• Revisiting the atmosphere of HAT-P-70b with CARMENES high-resolution transmission spectroscopy
• Exploring Synergies between Twinkle and Ariel: a Pilot Study
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk
• A New Parameterization for Finding Solutions for Microlensing Exoplanet Light Curves
• Deep JWST spectroscopy of galaxies in a candidate ionized bubble at $z=8.7$: probing reionization at pMpc scales with Ly$\alpha$ emission
• X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
• Methane on the temperate exo-Saturn TOI-199b
• Kinematics of the Sagittarius Dwarf Spheroidal core: A 5D Analysis for a 6D Methodology with Gaia DR3
• Is there a tilt in the fundamental (hyper)plane?
• Misidentification of Short GRBs as Magnetars in Nearby Galaxies
• TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data
• Inferring planet occurrence rates from radial velocities
• A transiting hot Jupiter with two outer siblings orbiting an intermediate-mass post main-sequence star
• Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics
• Towards a Field Based Bayesian Evidence Inference from Nested Sampling Data
• Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones
• Exposure-averaged Gaussian Processes for Combining Overlapping Datasets
• Joint Optical-HI mock catalogues and prospects for upcoming HI surveys
• Baryonic Ecosystem IN Galaxies (BEINGMgII) -- III. Cool gas reservoirs at $0.3\le z\le 1.6$ in the Dark Energy Survey
• A nuclear disc at Cosmic Noon: evidence of early bar-driven galaxy evolution
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Using Statistical Emulation and Knowledge of Grain-Surface Diffusion for Bayesian Inference of Reaction Rate Parameters: An Application to a Glycine Network
• Geometric nested sampling: sampling from distributions defined on non-trivial geometries
• Possible favored Great Oxidation Event scenario on exoplanets around M-Stars with the example of TRAPPIST-1e
• Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation
• Detailed Characterization of Heartbeat Stars and their Tidally Excited Oscillations
• The effect of JWST/NIRSpec data reduction on the retrieval of WASP-39b atmospheric properties
• A precessing jet from a supermassive black hole: multi-wavelength observations of S5 1044+71
• Towards simulating a realistic data analysis with an optimised angular power spectrum of spectroscopic galaxy surveys
• Optimisation of the Population Monte Carlo algorithm: Application to constraining isocurvature models with cosmic microwave background data
• Sample Variance Denoising in Cylindrical 21-cm Power Spectra
• Revisiting early afterglows of gamma-ray bursts with finite-thickness ejecta: Implications from XRF 080330 and GRB 080710
• Disentangling auroral, cloud and magnetic spot driven variability in three early L-dwarfs with HST/WFC3
• The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries
• Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
• Bayesian evidence and model selection approach for time-dependent dark energy
• Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared
• The HUSTLE Program: The UV to Near-IR Transmission Spectrum of the Hot Jupiter KELT-7b
• On the dark matter origin of an LDMX signal
• Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration
• APES: Approximate Posterior Ensemble Sampler
• Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
• Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling
• Two Higgs doublet model fitting and $t\bar{t}b\bar{b}$ signal at the ILC
• PAStar: a model for stellar surface from the Sun to active stars
• Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario
• Gravitational-Wave Geodesy: Defining False Alarm Probabilities with Respect to Correlated Noise
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• A planetary-mass candidate imaged in the Young Suns Exoplanet Survey
• Improving exoplanet mass characterisation with Bayesian model selection using the Learned Harmonic Mean Estimator
• Time-resolved JWST Retrieval Analysis of the Coldest Brown Dwarf: Temperature and Chemical Variations in WISE 0855-07
• Searching for Gluino LSP at the LHC
• Sector-Resolved Bayesian Model Averaging for DESI-Era Cosmology
• Piercing through the Haze: Characterizing Titan-like terrestrial exoplanets with JWST
• Information content on Venusian aerosols in VIRTIS-M infrared data
• Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5$-$704014
• Resonances in reflective Hamiltonian Monte Carlo
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• $\text{Exoformer}$: Accelerating Bayesian atmospheric retrievals with transformer neural networks
• Probing gravity with non-linear clustering in redshift space
• Non-halo structures and their effects on gravitationally lensed galaxies
• Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities
• Determining Frequentist Confidence Limits Using a Directed Parameter Space Search
• TOI-333b: A Neptune Desert planet around a F7V star
• RGE-induced $\mu$-$\tau$ symmetry breaking: an analysis of the latest T2K results
• Planets or asteroids? A geochemical method to constrain the masses of White Dwarf pollutants
• Assessment of a Physics-based Retrieval of Exoplanet Atmospheric Temperatures from Infrared Emission Spectra
• Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies
• Light and compressed gluinos at the LHC via string theory
• 30 parameter version of the MSSM in light of the $B_s\to {\mu }^{+}{\mu }^{-}$ observation
• Tidal Disruption of Super Star Clusters as the origin of Bluish Light at the inner region of the Perseus Cluster Central Galaxy
• Searching for stop LSP at the LHC
• What We Have Learned from NICER About Neutron Star Radii
• Redshift Evolution of the HII Galaxy $L$-$\sigma$ Relation: Gaussian Process Analysis and Cosmological Implications
• A constant pressure model for the warm absorber in Mrk 509
• Constraining the AGN tori at cosmic noon using high-resolution JWST imaging and simultaneous SED fitting
• Particle production during inflation: A Bayesian analysis with CMB data from Planck 2018
• Limits on the axion-photon coupling from Chandrayaan-2 observations