Table 1.
Overview of BEYONDPLANCK and preliminary COSMOGLOBE papers.
Reference | Title |
---|---|
Pipeline | |
This paper | I. Global Bayesian analysis of the Planck Low Frequency Instrument data |
Keihänen et al. (2023) | II. CMB mapmaking through Gibbs sampling |
Galloway et al. (2023a) | III. Commander3 |
Brilenkov et al. (2023) | IV. On end-to-end simulations in CMB analysis – Bayesian versus frequentist statistics |
Instrument characterization | |
Herman et al. (2023) | V. Minimal ADC Corrections for Planck LFI |
Ihle et al. (2023) | VI. Noise characterization and modeling |
Gjerløw et al. (2023) | VII. Bayesian estimation of gain and absolute calibration for CMB experiments |
Galloway et al. (2023b) | VIII. Efficient Sidelobe Convolution and Correction through Spin Harmonics |
Svalheim et al. (2023a) | IX. Bandpass and beam leakage corrections |
Cosmological and astrophysical results | |
Basyrov et al. (2023) | X. Planck LFI frequency maps with sample-based error propagation |
Colombo et al. (2023) | XI. Bayesian CMB analysis with sample-based end-to-end error propagation |
Paradiso et al. (2023) | XII. Cosmological parameter estimation with end-to-end error propagation |
Andersen et al. (2023) | XIII. Intensity foregrounds, degeneracies and priors |
Svalheim et al. (2023b) | XIV. Polarized foreground emission between 30 and 70 GHz |
Herman et al. (2023) | XV. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP |
COSMOGLOBE | |
Gerakakis et al. (2023) | From BEYONDPLANCK to COSMOGLOBE: Open Science, reproducibility, and data longevity |
Watts et al. (2023) | From BEYONDPLANCK to COSMOGLOBE: Preliminary WMAP Q-band analysis |
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