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Small scale entropy and adiabatic density perturbations ? Antimatter in the Universe
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The interaction of matter and radiation in a hot-model universe
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New horizons in cosmology with spectral distortions of the cosmic microwave background
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LiteBIRD: A Satellite for the Studies of B-Mode Polarization and Inflation from Cosmic Background Radiation Detection
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February 2019 |
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Large-scale structure, the cosmic microwave background and primordial non-Gaussianity
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Planck 2013 results. XXIII. Isotropy and statistics of the CMB
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Planck 2015 results : XXII. A map of the thermal Sunyaev-Zeldovich effect
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September 2016 |
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Planck 2015 results : XIII. Cosmological parameters
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September 2016 |
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Planck 2015 results : XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
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September 2016 |
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Planck intermediate results : XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
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December 2016 |
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Planck 2018 results: IV. Diffuse component separation
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September 2020 |
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Planck 2018 results: IX. Constraints on primordial non-Gaussianity
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September 2020 |
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A full sky, low foreground, high resolution CMB map from WMAP
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Spectral distortions of the microwave background radiation resulting from the damping of pressure waves
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The three-point correlation function of the cosmic microwave background in inflationary models
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Power spectrum constraints from spectral distortions in the cosmic microwave background
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Foregrounds and Forecasts for the Cosmic Microwave Background
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In the realm of the Hubble tension—a review of solutions *
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July 2021 |
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Scale-dependent non-Gaussianity probes inflationary physics
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A generalized local ansatz and its effect on halo bias
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The Primordial Inflation Explorer (PIXIE): a nulling polarimeter for cosmic microwave background observations
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The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes
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The Atacama Cosmology Telescope: likelihood for small-scale CMB data
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Constraints on μ-distortion fluctuations and primordial non-Gaussianity from Planck data
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Correlating CMB spectral distortions with temperature: what do we learn on inflation?
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December 2016 |
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Primordial non-Gaussianity with μ-type andy-type spectral distortions: exploiting Cosmic Microwave Background polarization and dealing with secondary sources
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Exploring cosmic origins with CORE: B -mode component separation
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April 2018 |
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Spectral distortion anisotropies from single-field inflation
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August 2018 |
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The Simons Observatory: science goals and forecasts
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February 2019 |
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The synergy between CMB spectral distortions and anisotropies
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February 2020 |
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The Websky extragalactic CMB simulations
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October 2020 |
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Breaking degeneracies with the Sunyaev-Zeldovich full bispectrum
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June 2021 |
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Primordial tensor bispectra in μ-CMB cross-correlations
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February 2022 |
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Combining ILC and moment expansion techniques for extracting average-sky signals and CMB anisotropies
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October 2020 |
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Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB E-mode and μ-distortion anisotropies
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Evolution of CMB spectral distortion anisotropies and tests of primordial non-Gaussianity
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December 2016 |
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Which spectral distortions does ΛCDM actually predict?
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Prospects for measuring cosmic microwave background spectral distortions in the presence of foregrounds
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The Python Sky Model: software for simulating the Galactic microwave sky
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May 2017 |
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Extracting foreground-obscured μ-distortion anisotropies to constrain primordial non-Gaussianity
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April 2018 |
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CMB μT cross correlations as a probe of primordial black hole scenarios
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August 2021 |
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Consistency conditions and primordial black holes in single field inflation
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Spectral distortion anisotropy from inflation for primordial black holes
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Nonlinear evolution of long-wavelength metric fluctuations in inflationary models
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Non-Gaussian aspects of thermal and kinetic Sunyaev-Zel’dovich effects
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High resolution foreground cleaned CMB map from WMAP
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Running non-Gaussianities in Dirac-Born-Infeld inflation
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Likelihood analysis of CMB temperature and polarization power spectra
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Scale-dependent bias of galaxies and μ -type distortion of the cosmic microwave background spectrum from single-field inflation with a modified initial state
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Cosmology from the thermal Sunyaev-Zel’dovich power spectrum: Primordial non-Gaussianity and massive neutrinos
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Probing the scale dependence of non-Gaussianity with spectral distortions of the cosmic microwave background
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June 2015 |
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Cosmological constraints from μ E cross correlations
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November 2016 |
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New Window on Primordial Non-Gaussianity
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July 2012 |
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CMB and SZ effect separation with constrained Internal Linear Combinations: CMB and SZ separation with constrained ILC
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A needlet internal linear combination analysis of WMAP 7-year data: estimation of CMB temperature map and power spectrum: A NILC analysis of WMAP 7-year data
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The evolution of CMB spectral distortions in the early Universe: CMB spectral distortions
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CMB at 2 × 2 order: the dissipation of primordial acoustic waves and the observable part of the associated energy release: Acoustic damping
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Unavoidable cmb Spectral Features and Blackbody Photosphere of our Universe
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June 2013 |