Showing 1–20 of 22 results
/ Date/ Name
Jun 11, 2024COMAP Pathfinder -- Season 2 results II. Updated constraints on the CO(1-0) power spectrumNov 11, 2020BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument dataMay 20, 2022From BeyondPlanck to Cosmoglobe: Open Science, Reproducibility, and Data LongevityAug 20, 2024Cosmoglobe DR2. I. Global Bayesian analysis of COBE-DIRBEMay 3, 2023Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI dataJun 27, 2023Cosmoglobe: Towards end-to-end CMB cosmological parameter estimation without likelihood approximationsJan 12, 2026Cosmoglobe DR2. IV. Modelling starlight in DIRBE with Gaia and WISEOct 20, 2023Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI dataJan 20, 2022BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priorsJun 3, 2024Cosmoglobe DR2. II. CIB monopole measurements from COBE-DIRBE through global Bayesian analysisOct 27, 2025Separation of gain fluctuations and continuum signals in total power spectrometers with application to COMAPJan 15, 2026Cosmoglobe DR2. VI. Disentangling hot and cold thermal dust emission with Planck HFIAug 20, 2024Cosmoglobe DR2. III. Improved modelling of zodiacal light with COBE-DIRBE through global Bayesian analysisJun 11, 2024COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"Mar 27, 2025Three-Dimensional Stacking as a Line Intensity Mapping StatisticJan 12, 2026Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBEMay 13, 2024Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmakingJun 11, 2024COMAP Pathfinder -- Season 2 results I. Improved data selection and processingMar 14, 2023Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysisFeb 24, 2022From BeyondPlanck to Cosmoglobe: Preliminary $\mathit{WMAP}$ $\mathit Q$-band analysis