The Temperature of the Cosmic Microwave Background

Abstract

The FIRAS data are independently recalibrated using the WMAP data to obtain a CMB temperature of 2.7260 +/- 0.0013. Measurements of the temperature of the cosmic microwave background are reviewed. The determination from the measurements from the literature is cosmic microwave background temperature of 2.72548 +/- 0.00057 K.

6 Pages 3 figures

References in corpus (1)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

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• 7Be charge exchange between 7Be3+ ion and exotic long-lived negatively charged massive particle in big bang nucleosynthesis
• Least response method to separate CMB spectral distortions from foregrounds
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• Model-Independent Measurement of the Matter-Radiation Equality Scale in DESI 2024
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Bounds on sterile neutrino lifetime and mixing angle with active neutrinos by global 21 cm signal
• How does pressure gravitate? Cosmological constant problem confronts observational cosmology
• Interplay of CMB Temperature, Space Curvature, and Expansion Rate Parameters
• Modelling the spinning dust emission from LDN 1780
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Misalignment production of vector boson dark matter from axion-SU(2) inflation
• Sardinia Radio Telescope observations of the Coma Cluster
• The Kolmogorov-Smirnov test for the CMB
• QUIJOTE scientific results -- V. The microwave intensity and polarisation spectra of the Galactic regions W49, W51 and IC443
• The influence of the effective number of active and sterile neutrinos on the determination of the values of cosmological parameters
• Missing dust signature in the cosmic microwave background
• Casimir cosmology
• Modern Cosmology, an Amuse-Gueule
• Binomial Line Cox Processes: Statistical Characterization and Applications in Wireless Network Analysis
• The long duration cryogenic system of the OLIMPO balloon--borne experiment: design and in--flight performance
• Stokes parameters spectral distortions due to the Sunyaev-Zel'dovich effect and an independent estimation of the CMB low multipoles
• Features of the gamma-ray pulsar halo HESS J1831$-$098
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Optical inverse-Compton emission from clusters of galaxies
• Impact of half-wave plate systematics on the measurement of CMB $B$-mode polarization
• Cosmological constrains on fast transition Unified Dark Energy/Matter models
• Modified dispersion relations and a potential explanation of the EDGES anomaly
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Statistical Uncertainties of the $N_{\text{DW}}=1$ QCD Axion Mass Window from Topological Defects
• Confirming ALMA Calibration using Planck and ACT Observations
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude
• Radiative transfer of Lyman-$\alpha$ photons at cosmic dawn with realistic gas physics
• Re-Examination of Globally Flat Space-Time
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• Halos in Dark Ages: formation and chemistry
• GeV-scale dark matter with $p$-wave Breit-Wigner enhanced annihilation
• Constraining gravitational-wave backgrounds from conversions into photons in the Galactic magnetic field
• Separation of CMB $\mu$ spectral distortions from foregrounds with poorly defined spectral shapes
• Unveiling the Universe with Emerging Cosmological Probes
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Fast and Flexible Neutrino Decoupling Part I: The Standard Model
• 0.3-to-1.5-GHz LNA with Wideband Noise and Power Matching for Radio Astronomy
• Finite temperature effects in modular cosmology
• Initial Li Abundances in the Protogalaxy and Globular Clusters Based upon the Chemical Separation and Hierarchical Structure Formation
• The Atacama Cosmology Telescope: Flux Upper Limits from a Targeted Search for Extragalactic Transients
• The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
• On the Galactic radio signal from stimulated decay of axion dark matter
• Testing the wavelength dependence of cosmological redshift down to $\Delta z\sim 10^{-6}$
• Cosmological impact of microwave background temperature measurements
• The Superhorizon Test of Future B-mode Experiments
• Resilience and implications of adiabatic CMB cooling
• Protonated hydrogen cyanide as a tracer of pristine molecular gas
• Integrated Sachs-Wolfe tomography with orthogonal polynomials
• A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
• $\Lambda$CDM cosmology with a quiescent anisotropy in a higher dimensional steady state universe
• Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
• PTOLEMY's test of generalized neutrino interactions: unveiling challenges and constraints
• Test of the Einstein equivalence principle with spectral distortions in the cosmic microwave background
• Casimir force in the Gödel space-time and its possible induced cosmological inhomogeneity
• Entropy methods for CMB analysis of anisotropy and non-Gaussianity
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• Coupled quintessence inspired by warm inflation
• Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution
• Reconstructing the early-universe expansion and thermal history
• Loop Quantum Cosmology with a noncommutative quantum deformed photon gas
• Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
• Clear sky atmosphere at cm-wavelengths from climatology data
• The spatial correlation between CN line and dust continuum emitting regions in high-mass star-forming cloud
• Helium diffusion during formation of the first galaxies
• Examining statistical isotropy of CMB low multipoles from Planck PR4 data
• Spectral features of non-equilibrium antineutrinos of primordial nucleosynthesis
• Variation of the baryon-to-photon ratio due to decay of dark matter particles
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Low-cost, Low-loss, Ultra-wideband Compact Feed for Interferometric Radio Telescopes
• Thermodynamics of the Primordial Universe
• Particle dispersion in the classical vector dark matter background
• Widespread subsonic turbulence in Ophiuchus North 1
• CMB two-point angular correlation function in the Ellipsoidal Universe
• Hearing Higgs with Gravitational Wave Detectors
• Level correlations of the CMB temperature angular power spectrum
• A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimators
• Effects of observer peculiar motion on the isotropic background frequency spectrum: from monopole to higher multipoles
• The establishment of the Standard Cosmological Model through observations
• The origin and evolution of the [CII] deficit in HII regions and star-forming molecular clouds
• Predictions for the diffuse cosmic dipole at radio frequencies from reionization imprints
• On spacetime structure and electrodynamics
• Escape from the swamp with spectator
• Can we constrain structure growth from galaxy proper motions?
• Coleman-Weinberg dynamics of ultralight scalar dark matter and GeV-scale right-handed neutrinos
• A relook at the GZK Neutrino-Photon Connection: Impact of Extra-galactic Radio Background & UHECR properties
• Giant lobes of Centaurus A as seen in radio and gamma-ray images obtained with the Fermi-LAT and Planck satellites
• Impact of Dark Sector Preheating on CMB Observables
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• A frequentist view on the two-body decaying dark matter model
• A neutral hydrogen absorption study of cold gas in the outskirts of the Magellanic Clouds using the GASKAP-HI survey
• Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
• What did the seahorse swallow? APEX 170 GHz observations of the chemical conditions in the Seahorse infrared dark cloud
• Non-thermal photons and direct photodissociation of H2, HD and HeH+ in the chemistry of the primordial Universe
• Characterising the physical and chemical properties of a young Class 0 protostellar core embedded in the Orion B9 filament
• Real-time thermal photon-photon interactions in the mixed space
• Revisiting the temperature evolution law of the CMB with gaussian processes
• What laboratory experiments can teach us about cosmology: A chameleon example
• Absorption of Photons from Distant Gamma-Ray Sources
• Microwave Observations of Venus with CLASS
• An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results
• SPECTER: An Instrument Concept for CMB Spectral Distortion Measurements with Enhanced Sensitivity
• Primordial nucleosynthesis constraints on high-z energy releases
• ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
• Violation of Bell inequalities from Cosmic Microwave Background data
• On the Deepest Search for Galactic Center Pulsars and an Examination of an Intriguing Millisecond Pulsar Candidate
• How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis
• Infrared galaxies detected by the Atacama Cosmology Telescope
• Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
• Monopole Fluctuations in Galaxy Surveys
• Challenges and prospects for better measurements of the CMB intensity spectrum
• On the correspondence between energy conservation and energy-momentum tensor conservation in cosmology
• Galactic abundances as a relic neutrino detection scheme
• Universal Peaks Ratio In The Spectral Energy Density Of Double Hump Blazars, Gamma Ray Bursts, And Microquasars
• A physical mechanism of the generation of stable positive kinetic energy systems and a qualitative explanation of the proportions of the four ingredients in the universe
• An exact solution of the higher-order gravity in standard radiation-dominated era
• Flat Space, Dark Energy, and the Cosmic Microwave Background
• Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe
• Constraining nonminimal f(T) gravity from Primordial Nucleosynthesis to Late-Universe observations
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Evolution of linear matter perturbations with error-bounded bundle physics-informed neural networks
• The EDIBLES survey. X. The 6196 Å diffuse interstellar band: Identification of side DIBs as an indication of a small carrier molecule
• Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
• Gravitational Ionization by Schwarzschild Primordial Black Holes
• Neutrino masses from CMB B-mode polarization and cosmic growth rate
• Does Cosmological Evolution Select for Technology?
• MeV cosmic-ray electrons modify the TeV pair-beam plasma instability
• Fluids in cosmology
• Thermal Sunyaev-Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes
• The gas distribution in the high-redshift cluster MS 1054-0321
• Horndeski in motion
• Can dark-matter Q-balls grow to the mass gap masses?
• The Universe at the MeV era: neutrino evolution and cosmological observables
• Limits on Dark Matter Annihilation from the Shape of Radio Emission in M31
• Cross bispectra and trispectra of the non-linear integrated Sachs-Wolfe effect and the tracer galaxy density field
• Evidence against Ryskin's model of cosmic acceleration
• Far-infrared to centimeter emission of very nearby galaxies with archival data
• Observational Imprints of Our Lost Twin Anti-Universe
• Gravitational wave emission from the CMB and other thermal fields
• ILC sensitivity for leptophilic scalar dark matter
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• Constraining Tsallis Corrections to Photon Reheating from Electron-Positron Annihilation: A Phenomenological Approach
• Systematic Light Propagation Bias from the Heliosphere and Its Impact on the Hubble Tension
• Cosmic microwave background temperature cosmography
• Implications of the cosmological 21-cm absorption profile for high-redshift star formation and deep JWST surveys
• Cosmology with the SZ spectrum: measuring the Universe's temperature with galaxy clusters
• Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario
• The GPSP Atlas: High-resolution Galactic Photon Survival Probability Atlas for Very-High- and Ultra-High-Energy Gamma-Ray Astronomy
• Redshift Dependence of CMB Temperature in BSBM $\alpha$-Varying Theories
• Boomerang mechanism explaining the excess radio background
• The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science
• Testing the cosmological principle on gigaparsec scales
• Exiting Inflation with a Smooth Scale Factor
• On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
• An empirical model of the extragalactic radio background
• The 107 GHz methanol transition is a dasar in G0.253+0.016
• Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions