Showing 1–20 of 40 results
/ Date/ Name
Aug 19, 2024In-Flight Performance of Spider's 280 GHz ReceiversSep 9, 2022BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statisticsNov 12, 2020BeyondPlanck VI. Noise characterization and modellingJan 12, 2026Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBEJan 10, 2022BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAPJul 13, 2020A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimatorsDec 22, 2020Design and pre-flight performance of SPIDER 280 GHz receiversNov 16, 2020BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experimentsNov 11, 2020BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument dataNov 11, 2020BeyondPlanck II. CMB map-making through Gibbs samplingJan 10, 2022BeyondPlanck X. Bandpass and beam leakage correctionsMay 20, 2022BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagationAug 30, 2022BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagationFeb 10, 2023Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurationsOct 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 analysisJan 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 analysisOct 2, 2020Planck constraints on the tensor-to-scalar ratio