The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set

Abstract

We have refined the analysis of the data from the FIRAS (Far InfraRed Absolute Spectrophotometer) on board the COBE (COsmic Background Explorer). The FIRAS measures the difference between the cosmic microwave background and a precise blackbody spectrum. We find new tighter upper limits on general deviations from a blackbody spectrum. The RMS deviations are less than 50 parts per million of the peak of the CMBR. For the Comptonization and chemical potential we find $|y|<15\times 10^{-6}$ and $|\mu |<9\times 10^{-5}$ (95\% CL). There are also refinements in the absolute temperature, 2.728 $\pm$ 0.004 K (95\% CL), and dipole direction, $(\ell ,b)=(264.14^{\circ }\pm 0.30,48.26^{\circ }\pm 0.30)$ (95\% CL), and amplitude, $3.372\pm 0.007$ mK (95\% CL). All of these results agree with our previous publications.

32 pages, LaTeX+aasms package, 6 figures as separate PostScript file. Submitted to Ap.J

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• Is there a need and another way to measure the Cosmic Microwave Background temperature more accurately?
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles
• Aberrating the CMB sky: fast and accurate computation of the aberration kernel
• Distances with <4% Precision from Type Ia Supernovae in Young Star-Forming Environments
• Integral Field Spectroscopy and multi-wavelength imaging of the nearby spiral galaxy NGC5668: an unusual flattening in metallicity gradient
• The CTA Sensitivity to Lorentz-Violating Effects on the Gamma-Ray Horizon
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Effective photon mass and (dark) photon conversion in the inhomogeneous Universe
• Big Bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves
• Probing relic neutrino decays with 21 cm cosmology
• Exploring the NANOGrav Signal and Planet-mass Primordial Black Holes through Higgs Inflation
• Cosmological Abundance of Colored Relics
• Detecting WIMPs in the Microwave Sky
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Refined approximations for the distortion visibility function and mu-type spectral distortions
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• Hadronic Axion Model in Gauge-Mediated Supersymmetry Breaking
• Inverse Compton scattering in mildly relativistic plasma
• Cosmological Dependence of Non-resonantly Produced Sterile Neutrinos
• Gravitational Waves and Primordial Black Holes from Supersymmetric Hybrid Inflation
• Tests of Dark MACHOs: Lensing, Accretion, and Glow
• Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history
• Consistency conditions and primordial black holes in single field inflation
• Testing dark matter interactions with CMB spectral distortions
• Serendipitous discovery of the long-sought AGN in Arp 299-A
• Signatures of Intergalactic Dust From the First Supernovae
• The Sunyaev-Zeldovich Background
• Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Anisotropy of the galaxy cluster X-ray luminosity-temperature relation
• Testing Inflation and Curvaton Scenarios with CMB Distortions
• First results from the WISPDMX radio frequency cavity searches for hidden photon dark matter
• Big Bang Nucleosynthesis with Matter--Antimatter Domains
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• The Sunyaev-Zel'dovich Effect by Cocoons of Radio Galaxies
• Constraining Gravitino Dark Matter with the Cosmic Microwave Background
• AGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy groups and clusters
• Spectral distortions to the Cosmic Microwave Background from the recombination of hydrogen and helium
• Cosmic microwave background and inflation in multi-fractional spacetimes
• Big-bang nucleosynthesis with sub-GeV massive decaying particles
• Cloud formation in the atomic and molecular phase: HI self absorption (HISA) towards a Giant Molecular Filament
• Searching for anisotropy in the distribution of binary black hole mergers
• NANOGrav signal as mergers of Stupendously Large Primordial Black Holes
• The nuclear starburst in Arp 299-A: From the 5.0 GHz VLBI radio light-curves to its core-collapse supernova rate
• Statistics of Sunyaev-Zel'dovich Cluster Surveys
• Non-thermal WIMPs as "Dark Radiation" in Light of ATACAMA, SPT, WMAP9 and Planck
• A Type II Supernova Hubble diagram from the CSP-I, SDSS-II, and SNLS surveys
• Ultra-bright CO and [CI] emission in a lensed z=2.04 submillimeter galaxy with extreme molecular gas properties
• Speed from light: growth rate and bulk flow at z ~ 0.1 from improved SDSS DR13 photometry
• Gauging the effect of Supermassive Black Holes feedback on Quasar host galaxies
• Sunyaev-Zeldovich Effect from Quasar-driven Blast-waves
• Axion Star Explosions: A New Source for Axion Indirect Detection
• The meso-inflationary QCD axion
• Primordial black holes in non-canonical scalar field inflation driven by quartic potential in the presence of bump
• SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
• Rich structure of non-thermal relativistic CMB spectral distortions from high energy particle cascades at redshifts $z\lesssim 2\times 10^5$
• Constraints on high-J CO emission lines in $z\sim 6$ quasars
• Cosmological Simulations of the Preheating Scenario for Galaxy Cluster Formation: Comparison to Analytic Models and Observations
• Sommerfeld Enhancement of DM Annihilation: Resonance Structure, Freeze-Out and CMB Spectral Bound
• The intergalactic medium temperature and Compton y parameter
• Constraining Antimatter Domains in the Early Universe with Big Bang Nucleosynthesis
• Radio Sources in the Nearby Universe
• The y-sky: diffuse spectral distortions of the cosmic microwave background
• Remarkable analytic relations among greybody parameters
• CMB $\mu$ distortion from primordial gravitational waves
• Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis
• Extragalactic Foregrounds of the Cosmic Microwave Background: Prospects for the MAP Mission
• Constraining Large Scale Structure Theories with the Cosmic Background Radiation
• Submillimeter Galaxy Number Counts and Magnification by Galaxy Clusters
• Non-thermal photons and H2 formation in the early Universe
• Mapping the relativistic electron gas temperature across the sky
• The Copernican principle in light of the latest cosmological data
• Cosmological solutions to the Lithium problem: Big-bang nucleosynthesis with photon cooling, $X$-particle decay and a primordial magnetic field
• On the relation between the isotropy of the CMB and the geometry of the universe
• Heating of Intracluster Gas by Jet Activities of AGN: Is the "Preheating" Scenario Realistic?
• Polarized anisotropic spectral distortions of the CMB: Galactic and extragalactic constraints on photon-axion conversion
• The Core-Collapse Supernova Rate in Arp299 Revisited
• A void in the Hubble tension? The end of the line for the Hubble bubble
• Missing one-loop contributions in secondary gravitational waves
• Temperature Fluctuations of the Cosmic Microwave Background Radiation: A Case of Nonextensivity?
• CMB Constraints On The Thermal WIMP Mass And Annihilation Cross Section
• The nature of supernovae 2010O and 2010P in Arp 299 - I. Near-infrared and optical evolution
• Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II
• Combining ILC and moment expansion techniques for extracting average-sky signals and CMB anisotropies
• Primordial black holes and secondary gravitational waves from generalized power-law non-canonical inflation with quartic potential
• Planck-LFI: Design and Performance of the 4 Kelvin Reference Load Unit
• Cosmic Microwave Background anisotropies generated by domain wall networks
• Anisotropic universe with anisotropic sources
• Growth of curvature perturbations for PBH formation \& detectable GWs in non-minimal curvaton scenario revisited
• Impact of calibration errors on CMB component separation using FastICA and ILC
• Constraints on hidden photons from current and future observations of CMB spectral distortions
• Gravitational waves from type II axion-like curvaton model and its implication for NANOGrav result
• On the Properties of Spectroscopically-Confirmed Ultra-Diffuse Galaxies Across Environment
• Precision constraints on radiative neutrino decay with CMB spectral distortion
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• Detecting Beyond the Standard Model Interactions of Solar Neutrinos in Low-Threshold Dark Matter Detectors
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Constraints on the Cluster Environments and Hot Spot Magnetic Field Strengths of the Radio Sources 3C254 and 3C280
• Gravitational Lensing of the X-Ray Background by Clusters of Galaxies
• Cosmicflows-3: Cold Spot Repeller?
• The role of soft photon injection and heating in 21 cm cosmology
• Effects of Long-lived 10 MeV Scale Sterile Neutrino on Primordial Elemental Abundances and Effective Neutrino Number
• How stable is the photon?
• Searching for Dark Matter Constituents with Many Solar Masses
• A New interpretation of chain galaxies at high redshift
• Imprints of Axion Superradiance in the CMB
• Comparing Cosmic Microwave Background Datasets
• A Chandra Search for X-Ray Jets in Redshift 6 Quasars
• The QCD phase transition behind a PBH origin of LIGO/Virgo events?
• The multipole expansion of the local expansion rate
• One $\mu$ to rule them all: CMB spectral distortions can probe domain walls, cosmic strings and low scale phase transitions
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• The mid-infrared Tully-Fisher relation: Spitzer Surface Photometry
• The Spin-Resolved Atomic Velocity Distribution and 21-cm Line Profile of Dark-Age Gas
• Cosmic Background dipole measurements with Planck-High Frequency Instrument
• SweetSpot: Near-Infrared Observations of Thirteen Type Ia Supernovae from a New NOAO Survey Probing the Nearby Smooth Hubble Flow
• Bayesian estimation of our local motion from the Planck-2018 CMB temperature map
• Constraining CSL strength parameter $\lambda$ from standard cosmology and spectral distortions of CMBR
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations
• Axion-photon-dark photon oscillation and its implication for 21 cm observation
• Cosmicflows-3: The South Pole Wall
• Herschel deep far-infrared counts through the Abell 2218 cluster-lens
• Dark Matter from Late Invisible Decays to/of Gravitinos
• Intragroup and Galaxy-Linked Diffuse X-ray Emission in Hickson Compact Groups
• Quasi-extremal primordial black holes are a viable dark matter candidate
• Mechanism of primordial black holes production and secondary gravitational waves in $\alpha$-attractor Galileon inflationary scenario
• Extracting foreground-obscured $\mu$-distortion anisotropies to constrain primordial non-Gaussianity
• Primordial black holes and induced gravitational waves from double-pole inflation
• On the recovery of Local Group motion from galaxy redshift surveys
• Kinetic Inductance Detectors for the OLIMPO experiment: design and pre-flight characterization
• Radio Wavelength Constraints on the Sources of the Far Infrared Background
• Sunyaev-Zel'dovich Predictions for the Planck Surveyor Satellite using the Hubble Volume Simulations
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• Early Preheating and Galaxy Formation
• Formulation and constraints on decaying dark matter with finite mass daughter particles
• Planck ISW-lensing likelihood and the CMB temperature
• Observational Constraints on the Primordial Curvature Power Spectrum
• Cosmological Alfvén waves in the recent CMB data, and the observational bound on the primordial vector perturbation
• Chandra Observations of Two High-Redshift Quasars
• Visible Sterile Neutrinos as the Earliest Relic Probes of Cosmology
• "Dark energy" in the Local Void
• Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination
• The Cosmic Microwave Background Spectrum and a Determination of Fractal Space Dimensionality
• Warm Gas and Ionizing Photons in the Local Group (ApJL version)
• Alternative Explanations of the Cosmic Microwave Background: A Historical and an Epistemological Perspective
• A method for testing the cosmic homogeneity with Shannon entropy
• A Dark Sink Enhances the Direct Detection of Freeze-in Dark Matter
• Primordial black holes formation and secondary gravitational waves in nonminimal derivative coupling inflation
• Testing isotropy in the Universe using photometric and spectroscopic data from the SDSS
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: 40 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• A joint study of early and late spectral distortions of the cosmic microwave background and of the millimetric foreground
• The SZ effect as a cosmological discriminator
• Post-Newtonian Celestial Dynamics in Cosmology: Field Equations
• Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018
• Is the diffuse gamma background radiation generated by galactic cosmic rays?
• Limits on Dust and Metallicity Evolution of Lya Forest Clouds from COBE
• Luminous Type II supernovae for their low expansion velocities
• Spectral distortions of the CMB dipole
• Probing correlations of early magnetic fields using mu-distortion
• Constraining the Initial Primordial Black Hole Clustering with CMB-distortion
• Pinning down the primordial black hole formation mechanism with gamma-rays and gravitational waves
• Type II Supernovae as Distance Indicators at Near-IR Wavelengths
• What if Planck's Universe isn't flat?
• Solving cosmological problem in universal extra dimension models by introducing Dirac neutrino
• Inflowing gas onto a compact obscured nucleus in Arp 299A: Herschel spectroscopic studies of H2O and OH
• Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation
• Easing cosmic tensions with an open and hotter universe
• The double Compton emissivity in a mildly relativistic thermal plasma within the soft photon limit
• Constraining dark photons and their connection to 21 cm cosmology with CMB data
• Physics of the cosmic microwave background anisotropy
• Cosmic Strings in Hidden Sectors: 2. Cosmological and Astrophysical Signatures
• Limits on Cosmic Matter--Antimatter Domains from Big Bang Nucleosynthesis
• The Nancay HI Zone of Avoidance survey of 2MASS bright galaxies
• Fermionic partner of Quintessence field as candidate for dark matter
• Exploring cosmic origins with CORE: effects of observer peculiar motion
• An Instrument to Measure the Temperature of the Cosmic Microwave Background Radiation at Centimeter Wavelengths
• Supersymmetry and Cosmology
• Supernovae evidence for foundational change to cosmological models
• Search for the stochastic gravitational-wave background induced by primordial curvature perturbations in LIGO's second observing run
• Effects of the galactic magnetic field upon large scale anisotropies of extragalactic Cosmic Rays
• Some clarifications about Lemaître-Tolman models of the Universe used to deal with the dark energy problem
• Effective conductance method for the primordial recombination spectrum
• Millicharged Relics Reveal Massless Dark Photons
• CMB constraints on mass and coupling constant of light pseudoscalar particles
• Hidden Photon Dark Matter Interacting via Axion-like Particles
• CMB distortion anisotropies due to the decay of primordial magnetic fields
• An Ultimate Target for Dark Matter Searches
• A simple parametric model for spherical galaxy clusters
• Evidence of a fast bar in the weakly-interacting galaxy NGC 4264 with MUSE
• Ionization history of the Universe as a test for Super Heavy Dark Matter particles
• Prospects for Constraining Cosmology with the Extragalactic Cosmic Microwave Background Temperature
• Detecting Dark Matter Substructures on Small Scales with Fast Radio Bursts
• Bianchi type I space and the stability of inflationary Friedmann-Robertson-Walker space
• Cosmological and astrophysical constraints on superconducting cosmic strings
• $\bar{T}$: A New Cosmological Parameter?
• A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
• An SZ Temperature Decrement - X-ray Luminosity Relation for Galaxy Clusters
• A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
• Primordial black holes from an inflationary potential valley
• A Massive Spiral Galaxy in the Zone of Avoidance
• The D/H ratio at z = 3.57 toward Q 1937-1009
• What Can the Cosmic Microwave Background Tell Us About the Outer Solar System?
• Clusters, Groups, and Filaments in the Chandra Deep Field-South up to Redshift 1
• Limits Due to Instrumental Polarisation in CMB Experiments at Microwave Wavelengths
• ASASSN-14dq: A fast-declining type II-P Supernova in a low-luminosity host galaxy
• Baryon Asymmetry in a Heavy Moduli Scenario
• Draining the Local Void
• CMB spectral distortions from the decay of causally generated magnetic fields
• New operator approach to the CMB aberration kernels in harmonic space
• I- A hydrodynamical CLONE of the Virgo cluster of galaxies to confirm observationally-driven formation scenarios
• CMB polarization constraints on radiative feedback
• Can residuals of the Solar system foreground explain low multipole anomalies of the CMB ?
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Sensitivity forecasts for the cosmological recombination radiation in the presence of foregrounds
• Probing large-scale magnetism with the Cosmic Microwave Background
• Minimal Dark Matter Freeze-in with Low Reheating Temperatures and Implications for Direct Detection
• CMB constraints on dark matter phenomenology via reheating in minimal plateau inflation
• Testing the mapping between redshift and cosmic scale factor
• Effects of CMB temperature uncertainties on cosmological parameter estimation
• The Standard Cosmological Model
• Spectral Distortion of the CMB by the Cumulative CO Emission from Galaxies throughout Cosmic History
• Late reionizations of the Universe and their manifestation in the CMB data
• WALLABY Pre-Pilot Survey: HI Content of the Eridanus Supergroup
• CMB Distortions from Damping of Acoustic Waves Produced by Cosmic Strings
• Cosmological Constraints on Dark Scalar
• Analytic solutions of scalar perturbations induced by scalar perturbations
• Antimatter Regions in the Early Universe and Big Bang Nucleosynthesis
• New insights into black bodies
• A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case
• Beyond the Boost: Measuring the intrinsic dipole of the CMB using the spectral distortions of the monopole and quadrupole
• Microwave Background Anisotropies Due to the Kinematic Sunyaev-Zel'dovich Effect of the Lyman-alpha Forest
• Estimation of the CMB temperature from atomic C\,{\sc i} and molecular CO lines in the interstellar medium of early galaxies
• Small-scale primordial fluctuations in the 21cm Dark Ages signal
• Dark Matter at the Fermi Scale
• Unlocking the synergy between CMB spectral distortions and anisotropies
• Cosmological Dependence of Resonantly Produced Sterile Neutrinos
• The Cosmology Large Angular Scale Surveyor Receiver Design
• Gamma-ray spectral modulations induced by photon-ALP-dark photon oscillations
• Constraints on Gravitino Decay and the Scale of Inflation using CMB spectral distortions
• Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data
• Cosmological foundations revisited with Pantheon+
• Analysis of the thin layer of Galactic warm ionized gas in the range 20 < l < 30 deg, -1.5 < b < +1.5 deg
• The imprint of cosmological hydrogen recombination lines on the power spectrum of the CMB
• The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment
• A Low Noise Thermometer Readout for Ruthenium Oxide Resistors
• New CMB spectral distortion constraints on decaying dark matter with full evolution of electromagnetic cascades before recombination
• Constraints on a Local Group X-ray Halo
• Spiral arms in CALIFA galaxies traced by non-circular velocities, abundances, and extinctions
• PopRatio: A program to calculate atomic level populations in astrophysical plasmas
• Using the COBE/DMR data as a test-bed for normality assessments
• Probing the Universe's Tilt with the Cosmic Infrared Background Dipole
• Phenomenology of quintessino dark matter -- Production of NLSP particles
• de Sitter as a Resonance
• The degenerate gravitino scenario
• Reconstructing the Primary CMB Dipole
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• Effects of Foreground Contamination on the Cosmic Microwave Background Anisotropy Measured by MAP
• Measuring primordial anisotropic correlators with CMB spectral distortions
• Spectral Distortion Anisotropy from Inflation for Primordial Black Holes
• Primordial black holes in scalar field inflation coupled to the Gauss-Bonnet term with fractional power-law potentials
• Breaking Be: a sterile neutrino solution to the cosmological lithium problem
• Non-Nucleosynthetic Constraints on the Baryon Density and Other Cosmological Parameters
• The Evolution of the Cosmic Microwave Background
• Cosmic Neutrino Last Scattering Surface
• What can we learn on the thermal history of the Universe from future CMB spectrum measures at long wavelengths?
• A numerical code for the solution of the Kompaneets equation in cosmological context
• Small-scale anisotropy of the cosmic background radiation and scattering by cloudy plasma
• Symmetry and anti-symmetry of the CMB anisotropy pattern
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Pre-discovery and Follow-up Observations of the Nearby SN 2009nr: Implications for Prompt Type Ia SNe
• Inflation in $F(R)$ gravity models revisited after ACT
• An information theory based search for homogeneity on the largest accessible scale
• Observational evidence favors a static universe
• Multiple scattering Sunyaev-Zeldovich signal I: lowest order effect
• The Performance and Scientific Rationale for an IR Imaging Fourier Transform Spectrograph on a Large Space Telescope
• Constraints on non-resonant photon-axion conversion from the Planck satellite data
• Primordial black holes generated by fast-roll mechanism in non-canonical natural inflation
• Can accreting primordial black holes explain the excess radio background?
• Magnetic reheating
• Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
• POX 186: A Dwarf Galaxy in the Process of Formation?
• Radiation in equilibrium with plasma and plasma effects on cosmic microwave background
• Lumped element kinetic inductance detectors maturity for space-borne instruments in the range between 80 and 180 GHz
• A Stimulating Explanation of the Extragalactic Radio Background
• Limits on the fluctuating part of $y$-type distortion monopole from Planck and SPT results
• Cosmological Bounds on sub-GeV Dark Vector Bosons from Electromagnetic Energy Injection
• Relativistic Corrections to the Sunyaev-Zeldovich Effect for Clusters of Galaxies. V. Effect of the Motion of the Observer
• Universe opacity and CMB
• Are we living near the center of a local void?
• The Cosmic Microwave Background: State of the Art
• Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT
• Sudden braking and turning with a two-field potential bump: primordial black hole formation
• Search for Possible Variation of the Fine Structure Constant
• A slow bar in the lenticular barred galaxy NGC 4277
• How heavy can the Fermions in Split Susy be? A study on Gravitino and Extradimensional LSP
• $\mu$-distortion around stupendously large primordial black holes
• Some Like It Hot: Linking Diffuse X-ray Luminosity, Baryonic Mass, and Star Formation Rate in Compact Groups of Galaxies
• Patchy Screening of the CMB from Dark Photons
• Cosmological constraints in the presence of ionizing and resonance radiation at recombination
• Calibration Method and Uncertainty for the Primordial Inflation Explorer (PIXIE)
• Constraints on the generalized tachyon field models from latest observational data
• WIMP and FIMP dark matter in the inert doublet plus singlet model
• Testing distance duality with CMB anisotropies
• Probing large scale homogeneity and periodicity in the LRG distribution using Shannon entropy
• Optimized in-flight absolute calibration for extended CMB surveys
• Generalisation of the Kaiser Rocket effect in general relativity in the wide-angle galaxy 2-point correlation function
• Generation of gravitational waves in dynamical Chern-Simons gravity
• A new method for testing isotropy with Shannon entropy
• Cosmological Dependence of Sterile Neutrino Dark Matter With Self-Interacting Neutrinos
• Cosmological Information Contents on the Light-Cone
• On the primordial black hole formation in hybrid inflation
• CMB anisotropies generated by cosmic string loops
• A Global ILC Approach in Pixel Space over Large Angular Scales of the Sky using CMB Covariance Matrix
• Minimal cosmography
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Refined modelling of the radio SZ signal: kinematic terms, relativistic temperature corrections and anisotropies in the radio background
• Thomson scattering: One rate to rule them all
• Was Entropy Conserved between BBN and Recombination?
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• Statistical Thermodynamics of Polymer Quantum Systems
• Chameleon-Photon Mixing in a Primordial Magnetic Field
• Astrophysical constraints on primordial black holes in Brans-Dicke theory
• On a possible nonequilibrium imprint in the cosmic background at low frequencies
• Review of Dark Matter
• A low Hubble Constant from galaxy distribution observations
• Time variations of narrow absorption lines in high resolution quasar spectra
• CMB spectral distortions from continuous large energy release
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• A novel approach to reconstructing signals of isotropy violation from a masked CMB sky
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• CMB Spectral Distortion Constraints on Thermal Inflation
• Accidental Inflation from Kähler Uplifting
• On the assembly history of massive galaxies. A pilot project with VEGAS deep imaging and M3G integral field spectroscopy
• Volumetric Star Formation Prescriptions in Vertically Resolved Edge-on Galaxies
• Anisotropic CMB distortions from non-Gaussian isocurvature perturbations
• A low-luminosity core-collapse supernova very similar to SN 2005cs
• Edges and Endpoints in 21-cm Observations from Resonant Photon Production
• Dynamics of Abell 3266 - I. An Optical View of a Complex Merging Cluster
• The Irrelevance of Primordial Black Hole Clustering in the LVK mass range
• Swampland Bounds on Dark Sectors
• The limits of cosmology: role of the Moon
• Cosmological moduli problem in large volume scenario and thermal inflation
• CMB Polarization and Temperature Power Spectra Estimation using Linear Combination of WMAP 5-year Maps
• Alleviation of anomalies from the non-oscillatory vacuum in loop quantum cosmology
• Catching Tidal Dwarf Galaxies at a Later Evolutionary Stage with ALFALFA
• Does Planck mass run on the cosmological horizon scale?
• The bar rotation rate as a diagnostic of dark matter content in the centre of disc galaxies
• Search for exotic interactions of solar neutrinos in the CDEX-10 experiment
• HAFFET: Hybrid Analytic Flux FittEr for Transients
• Monopole Fluctuation of the CMB and its Gauge Invariance
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• The first spectral line surveys searching for signals from the Dark Ages
• Measuring the Hubble constant from the cooling of the CMB monopole
• Resonant amplification of curvature perturbations in inflation model with periodical derivative coupling
• Testing isotropy in the Two Micron All-Sky redshift survey with information entropy
• Gravitational Waves from Incomplete Inflationary Phase Transitions
• Cosmic Flows surveys and CLUES simulations
• de Sitter Harmonies: Cosmological Spacetimes as Resonances
• Constraining the impact of standard model phase transitions on primordial black holes
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• A Review of One-Way and Two-Way Experiments to Test the Isotropy of the Speed of Light
• $\mathcal{O}(10)M_{\odot }$ primordial black holes and string axion dark matter
• Constraint on the early-formed dark matter halos using the free-free emission in the Planck foreground analysis
• Linearized iterative least-squares (LIL): A parameter fitting algorithm for component separation in multifrequency CMB experiments such as Planck
• Abundance and properties of dark radiation from the cosmic microwave background
• Comprehensive Constraints on Dark Radiation Injection After BBN
• How to measure CMB spectral distortions with an imaging telescope
• Cosmological limits on axions and axion-like particles
• Intensity Mapping without Cosmic Variance
• High-z Sudoku: A diagnostic tool for identifying robust (sub)mm redshifts
• Improved large scales interstellar dust foreground model and CMB solar dipole measurement
• Modification of the mean free path of very high energy photons due to a relativistic deformed kinematics
• Hunting long-lived gluinos at the Pierre Auger Observatory
• The Darkness of Spin-0 Dark Radiation
• A closer look at dark photon explanations of the excess radio background
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Astrophysical information from the Rayleigh-Jeans Tail of the CMB
• Constraining dark photon model with dark matter from CMB spectral distortions
• Why CMB physics?
• Sunyaev-Zeldovich effects, free-free emission, and imprints on the cosmic microwave background
• Impact of Dust on Spectral Distortion Measurements of the Cosmic Microwave Background
• X-ray Clusters of Galaxies as Cosmological Tools
• Exploring X-ray Binary Populations in Compact Group Galaxies with $Chandra$
• PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry
• Constraining ultra slow roll inflation using cosmological datasets
• Cosmological Constraints on Unstable Particles: Numerical Bounds and Analytic Approximations
• The role of $T_0$ in CMB anisotropy measurements
• Primordial black holes in non-minimal Gauss-Bonnet inflation in light of the PTA data
• A-B transition in superfluid ${}^3$He and cosmological phase transitions
• New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background
• Shaping Dark Photon Spectral Distortions
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Dark matter production through a non-thermal flavon portal
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• Recent developments in astrophysical and cosmological exploitation of microwave surveys
• Asymmetric capture of Dirac dark matter by the Sun
• Microwave Background Constraints on Decaying Defects
• CMB and 21cm bounds on early structure formation boosted by primordial black hole entropy fluctuations
• CMB spectral distortions in generic two-field models
• Cosmological constraints on dark energy
• The Tully-Fisher relation for flat galaxies
• Constraints on the Low-Energy Cutoff in the Electron Distribution of the PKS 0637-752 Jet
• Probing small-scale non-Gaussianity from anisotropies in acoustic reheating
• The COSmic Monopole Observer (COSMO)
• The Distortion of the Cosmic Microwave Background Spectrum Due to Intergalactic Dust
• External priors for the next generation of CMB experiments
• Cosmic transparency and acceleration
• Probing dark gauge boson with observations from neutron stars
• Dense Gas and Star Formation in Nearby Infrared Bright Galaxies: APEX survey of HCN and HCO+ J=2-1
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Distortion of Infall Regions in Redshift Space-I
• Signals of merging supermassive primordial black holes in pulsar timing arrays
• On Measuring the CMB Temperature at Redshift 0.89
• Sub-MeV Dark Sink Dark Matter
• One-loop corrections to the E-type $\alpha$-attractor models of inflation and primordial black hole production
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• The Sunyaev-Zel'dovich Effect: Results and Future Prospects
• Constraints on structure formation models from Sunyaev-Zel'dovich Effect
• SU(2)$_{\tiny\mbox{CMB}}$ at high redshifts and the value of $H_0$
• The Arecibo Galaxy Environment Survey XII : Optically dark HI clouds in the Leo I Group
• Cosmic Birefringence from Neutrino and Dark Matter Asymmetries
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Modern Cosmology, an Amuse-Gueule
• Robust μ-distortion constraints on primordial supermassive black holes from cubic (gNL) non-Gaussian perturbations
• Antimatter from the cosmological baryogenesis and the anisotropies and polarization of the CMB radiation
• Missing dust signature in the cosmic microwave background
• Exploring primordial black holes and gravitational waves with R-symmetric GUT Higgs inflation
• Euclid: Testing the Copernican principle with next-generation surveys
• Ultralight boson constraints from gravitational wave observations of spinning binary black holes
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Trading kinetic energy: How late kinetic decoupling of dark matter changes $N_{\text{eff}}$
• Camouflaged galactic CMB foregrounds: total and polarized contributions of the kinetic Sunyaev Zeldovich effect
• What have we learned from observational cosmology ?
• A study in scarlet -- I. Photometric properties of a sample of Intermediate Luminosity Red Transients
• Systematic effects in polarizing Fourier transform spectrometers for cosmic microwave background observations
• CMB Spectral $\mu$-Distortion of Multiple Inflation Scenario
• Constraining gravitational-wave backgrounds from conversions into photons in the Galactic magnetic field
• Modified dispersion relations and a potential explanation of the EDGES anomaly
• Detecting Planet 9 via Hawking radiation
• WALLABY Pilot Survey: Gas-Rich Galaxy Scaling Relations from Marginally-Resolved Kinematic Models
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracy
• Large-scale anisotropies of extragalactic cosmic rays below the ankle
• Self-annihilating dark matter and the CMB: reionizing the Universe and constraining cross sections
• GeV-scale dark matter with $p$-wave Breit-Wigner enhanced annihilation
• Bounds on Very Weakly Interacting Sub-eV Particles (WISPs) from Cosmology and Astrophysics
• Estimation of Full Sky Power Spectrum between Intermediate to Large Angular Scales from Partial Sky CMB Anisotropies using Artificial Neural Network
• Early Decay of Peccei-Quinn Fermion and the IceCube Neutrino Events
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Physics of the Cosmic Microwave Background Radiation
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Spiky CMB distortions from primordial bubbles
• An Unbiased Estimator of the Full-sky CMB Angular Power Spectrum at Large Scales using Neural Networks
• Interpreting Pulsar Timing Array data of Gravitational Waves with Ekpyrosis-Bouncing Cosmology
• Non-parametric maximum likelihood component separation for CMB polarization data
• Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Warm Hawking Relics From Primordial Black Hole Domination
• Analysis of residual spectra and the monopole spectrum for 3 K blackbody radiation by means of non-extensive thermostatistics
• Cosmic Microwave Background Spectral Distortions from Cosmic String Loops
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Non-thermal Sunyaev-Zeldovich signal from radio galaxy lobes
• Venus Observations at 40 and 90 GHz with CLASS
• Mild-split SUSY with flavor
• Magnetic fields and Sunyaev-Zel'dovich effect in galaxy clusters
• Decays of Long-Lived Relics and Their Signatures at IceCube
• Precision cosmology as a test for statistics
• Constraints on $N_{\mathrm{eff}}$ of high energy non-thermal neutrino injections upto $z\sim 10^8$ from CMB spectral distortions and abundance of light elements
• The maximum extent of the filaments and sheets in the cosmic web: an analysis of the SDSS DR17
• Testing kinetically coupled inflation models with CMB distortions
• Resilience and implications of adiabatic CMB cooling
• Testing homogeneity of the galaxy distribution in the SDSS using Renyi entropy
• Total power horn-coupled 150 GHz LEKID array for space applications
• t-channel dark matter at the LHC -- a whitepaper
• The impact of non-Planckian effects on cosmological radio backgrounds
• Sunyaev-Zel'dovich anisotropy due to Primordial black holes
• A New Blackbody Radiation Law Based on Fractional Calculus and its Application to NASA COBE Data
• Spectral Distortions from Axion Monodromy Inflation
• Primordial black holes and scalar induced gravitational waves from Higgs inflation with non-canonical kinetic term
• Cosmological constraints on spontaneous R-symmetry breaking models
• Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
• Ruling out a critical density baryonic universe
• Time-ordered data simulation and map-making for the PIXIE Fourier transform spectrometer
• Motion induced second order temperature and y-type anisotropies after the subtraction of linear dipole in the CMB maps
• The Measure of Cosmological Parameters
• The Homogeneity Scale of the universe
• Energy injection in pre-recombination era and EDGES detection
• A blackbody is not a blackbox
• Cosmological constraints for the Cosmic Defect theory
• Big Bang nucleosynthesis in a weakly non-ideal plasma
• On parton distributions in a photon gas
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Primordial black holes in SB SUSY Gauss-Bonnet inflation
• Is the local Hubble flow consistent with concordance cosmology?
• The spectral energy distribution of the Carina nebula from far infrared to radio wavelengths
• Cosmology with Recombination Spectrum
• Microwave Emission from the Edgeworth-Kuiper Belt and the Asteroid Belt Constrained from WMAP
• Polylogarithmic representation of radiative and thermodynamic properties of thermal radiation in a given spectral range: II. Real-body radiation
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
• Spatially-resolved spectroscopy of narrow-line Seyfert 1 host galaxies
• Spectral Distortion in a Radially Inhomogeneous Cosmology
• A Deep Chandra Observation of the Distant Galaxy Cluster MS1137.5+6625
• Cosmic Neutrino Decoupling and its Observable Imprints: Insights from Entropic-Dual Transport
• NMSSM with Gravitino Dark Matter to be tested at LHC
• Test of the Einstein equivalence principle with spectral distortions in the cosmic microwave background
• The parity-odd Intrinsic Bispectrum
• The Accelerated Recombination, and the ACBAR and WMAP data
• Matter Dipole and Hubble Tension due to Large Wavelength Perturbations
• A quantum mechanical relation connecting time, temperature, and cosmological constant of the universe: Gamow's relation revisited as a special case
• Disentangle Neutrino Electromagnetic Properties with Atomic Radiative Pair Emission
• Information Wells and the Emergence of Primordial Black Holes in a Cyclic Quantum Universe
• On the origin of the diffuse gamma-ray background radiation
• Anisotropic higher derivative gravity and inflationary universe
• Primordial black hole formation in $\alpha$-attractor models: an analysis using optimized peaks theory
• A New Uncertainty Scheme for Galaxy Distances from Flow Models
• Freezing-in Cannibal Dark Sectors
• Recent Developments in Degenerate Higher Order Scalar Tensor Theories
• Review of QCD, QGP, Heavy Quark Meson Production Enhancement and Suppression
• Different effects of the Lorentz and Gaussian bump functions on the formation of primordial black holes and secondary gravitational waves
• Peculiar velocity effects on the Hubble constant from time-delay cosmography
• Updated cosmological constraints on Macroscopic Dark Matter
• Can anisotropy in the galaxy distribution tell the bias?
• Measuring our peculiar velocity from spectroscopic redshift surveys
• Spectral Distortion Signatures of Step-like Inflationary Potential
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Probing the global 21-cm background by velocity-induced dipole and quadrupole anisotropies
• Effects of observer peculiar motion on the isotropic background frequency spectrum: from monopole to higher multipoles
• Statistical effects of the observer's peculiar velocity on source number counts
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Feebly-interacting dark matter
• Constraining broad photon spectrum injections from exotic and astrophysical sources
• Primordial black holes and scalar-induced gravitational waves from the polynomial attractor model
• Properties of the giant HII regions and bar in the nearby spiral galaxy NGC5430
• Olber's Paradox for Superluminal Neutrinos: Constraining Extreme Neutrino Speeds at TeV-ZeV Energies with the Diffuse Neutrino Background
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Revisiting constraints on primordial magnetic fields from spectral distortions of cosmic microwave background
• Primordial Black Holes and Second-order Gravitational Waves in Axion-like Hybrid Inflation
• Scaling Laws in High-Energy Inverse Compton Scattering. II. Effect of Bulk Motions
• Enhanced Small-Scale Structure in the Cosmic Dark Ages
• NGC 7679: an anomalous, composite Seyfert 1 galaxy whose, X-ray luminous AGN vanishes at optical wavelengths
• Cosmological consequences of statistical inhomogeneity
• Effects of boosting on extragalactic components: methods and statistical studies
• Effects on the CMB from magnetic field dissipation before recombination
• Assessment of Models of Galactic Thermal Dust Emission Using COBE/FIRAS and COBE/DIRBE Observations
• Predictions for the diffuse cosmic dipole at radio frequencies from reionization imprints
• Simulations and Observations of the Microwave Universe
• Non-BBN Constraints On The Key Cosmological Parameters
• Cosmological implications of neutrinos
• SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction
• CMB delensing with deep learning
• SPECTER: An Instrument Concept for CMB Spectral Distortion Measurements with Enhanced Sensitivity
• Revisiting the temperature evolution law of the CMB with gaussian processes
• On the Impact of Random Residual Calibration Error on the Gibbs ILC Estimates over Large Angular Scales
• Challenges and prospects for better measurements of the CMB intensity spectrum
• On an Improvement of the Planck radiation Energy Distribution
• Causal Set Phenomenology
• Monopole Fluctuations in Galaxy Surveys
• Revisiting Ryskin's Model of Cosmic Acceleration
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Reconstruction of full sky CMB $\mathbf{E}$ and $\mathbf{B}$ modes spectra removing $\mathbf{E}$-to-$\mathbf{B}$ leakage from partial sky using deep learning
• Updated constraints on the primordial power spectrum at sub-Mpc scales
• Perturbative instability of inflationary cosmology from quantum potentials
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• Note on Thermalization of Non-resonantly Produced Sterile Neutrinos
• Isotropy, entropy, and energy scaling
• Scrutinizing Fermionic Dark Matter in Scotogenic Model with Low Reheating Temperature
• ALP Dark Matter from Kinetic Fragmentation: Opening up the Parameter Window
• Magnetic fields from small-scale primordial perturbations
• Self-similar cosmological expansion of collisional gas
• Cosmic Microwave Background as a thermal gas of SU(2) photons: Implications for the high-z cosmological model and the value of $H_0$
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• The BaR-SPOrt Experiment
• Non-linear effects in early Universe cosmology
• An Instrument Error Budget for Space-Based Absolute Flux Measurements of the Sky Synchrotron Spectrum Below 20 MHz
• Sunyaev-Zeldovich Cluster Counts as a Probe of Intra-Supercluster Gas
• A Hidden Microwave Background? -- signatures of photon-WISP oscillations in the CMB
• Challenges to the cosmological constant model following results from the Dark Energy Survey
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• Formation of the First Stars and Quasars
• Fifty shades of grayness: parametrizations of spectral distortions and applications in cosmology
• Improving NASA/IPAC Extragalactic Database Redshift Calculations
• Cosmological Constraints on a Massive Neutrino
• A theory of intelligence: networked problem solving in animal societies
• Missing Components in ΛCDM from DESI Y1 BAO Measurements: Insights from Redshift Remapping
• Quantum Decoherence of Photons in the Presence of Hidden U(1)s
• Probing Dark Photons through Gravitational Decoupling of Mass-State Oscillations in Interstellar Media
• On observational signatures of multi-fractional theory
• Probing the last scattering surface through the recent and future CMB observations
• Monte Carlo Study on Distortion of the Space-Dimension in COBE Monopole Data
• Axion braneworld cosmology
• The CMB Dipole and Circular Galaxy Distribution
• Indirect detection of long-lived particles in a rich dark sector with a dark vector portal
• Constant-roll inflation and primordial black holes within Barrow entropic framework
• CMB lensing from early-formed dark matter halos
• Mixed Inflaton and Spectator Field Models: CMB constraints and $\mu$ distortion
• Is it possible to unify three kinds of Dark Matters into a Kaluza-Klein Neutrino?
• Constraining self-interacting ultrahigh-energy muon neutrinos by cosmic microwave background spectral distortion
• Physics beyond the Standard Model with the DSA-2000
• The Kaiser-Rocket effect: three decades and counting
• CMB polarization anisotropies from cosmological reionization: extension to B-modes
• Status of CMB observations in 2015
• The Radio and Microwave Sky as Seen by Juno on its Mission to Jupiter
• Primordial black holes and scalar induced gravitational waves from sound speed resonance in non-minimal derivative coupling inflation model
• On the radiative and thermodynamic properties of the cosmic radiations using Cobe Firas instrumental data: Sunyaev-Zeldovich distortion effect
• Primordial black holes and uncertainties in the choice of the window function
• Resolved properties of a luminous "hinge clump" in the compact group of galaxies NGC\,6845
• Axion production and CMB spectral distortion in cosmological tangled magnetic field
• Correlating Gravitational Wave and Gamma-ray Signals from Primordial Black Holes
• Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos
• Archeops, mapping the CMB sky from large to small angular scales
• Primordial magnetic non-Gaussianity with generic vacua and detection prospects in CMB spectral distortions
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• The FAST Hundred-Deg${}^2$ HI Deep (HD${}^2$) Survey: Early Results from the Pilot Survey
• Development of generic no-scale inflation
• The Cosmological Dipole in Tilted Anisotropic Universes
• Inelastic Dirac Dark Matter
• The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures
• Probing small-scale baryon and dark matter isocurvature perturbations with cosmic microwave background anisotropies
• Spectral distortions in the decaying QCD dark matter scenario
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane
• Cosmological constraints on the decay of heavy relics into neutrinos
• Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae
• Mathematical matrix theory of the field in n-dimensional metric space: rigorous derivation of the equations of the field with application in electromagnetic-gravitational fields
• Entropy and its relationship to allometry
• Cosmic microwave background spectral distortions from Rayleigh scattering at second order
• CMB Observational Techniques and Recent Results
• Dark matter with excitable levels
• Galaxy Clusters in Cosmology: Cluster Abundance as a Probe of Structure Formation