Showing 1–20 of 20 results
/ Date/ Name
Nov 10, 2021COMAP Early Science: IV. Power Spectrum Methodology and ResultsNov 10, 2021COMAP Early Science: VII. Prospects for CO Intensity Mapping at ReionizationNov 10, 2021COMAP Early Science: III. CO Data ProcessingNov 10, 2021COMAP Early Science: V. Constraints and Forecasts at $z \sim 3$Nov 10, 2021COMAP Early Science: II. Pathfinder InstrumentNov 10, 2021COMAP Early Science: VI. A First Look at the COMAP Galactic Plane SurveyApr 22, 2021A model of spectral line broadening in signal forecasts for line-intensity mapping experimentsNov 10, 2021COMAP Early Science: I. OverviewApr 19, 2023COMAP Early Science: VIII. A Joint Stacking Analysis with eBOSS QuasarsMay 7, 2024COMAP Galactic Science I: Observations of Spinning Dust Emission at 30GHz in Dark Clouds Surrounding the λ-Orionis Hii RegionOct 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 priorsJan 15, 2026Cosmoglobe DR2. VI. Disentangling hot and cold thermal dust emission with Planck HFIJun 11, 2024COMAP Pathfinder -- Season 2 results II. Updated constraints on the CO(1-0) power spectrumSep 9, 2022BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statisticsJan 12, 2026Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBEFeb 24, 2022From BeyondPlanck to Cosmoglobe: Preliminary $\mathit{WMAP}$ $\mathit Q$-band analysisJan 12, 2026Cosmoglobe DR2. VII. Towards a concordance model of large-scale thermal dust emission for microwave and infrared frequenciesAug 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 data