COSMOGLOBE DR1 results-I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
We present COSMOGLOBE Data Release 1, which implements the first joint analysis of
WMAP and Planck LFI time-ordered data, processed within a single Bayesian end-to-end …
WMAP and Planck LFI time-ordered data, processed within a single Bayesian end-to-end …
COSMOGLOBE DR1 results-III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
We present the first model of full-sky polarized synchrotron emission that is derived from all
WMAP and Planck LFI frequency maps. The basis of this analysis is the set of end-to-end …
WMAP and Planck LFI frequency maps. The basis of this analysis is the set of end-to-end …
From BeyondPlanck to Cosmoglobe: Preliminary WMAP Q-band analysis
We present the first application of the COSMOGLOBE analysis framework by analyzing nine-
year WMAP time-ordered observations that uses similar machinery to that of …
year WMAP time-ordered observations that uses similar machinery to that of …
COSMOGLOBE DR1 results-II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data
Cosmic birefringence is a parity-violating effect that might have rotated the plane of the
linearly polarized light of the cosmic microwave background (CMB) by an angle β since its …
linearly polarized light of the cosmic microwave background (CMB) by an angle β since its …
Assessing consistency between WMAP 9-year and Planck 2015 temperature power spectra
Y Huang, GE Addison, JL Weiland… - arXiv preprint arXiv …, 2018 - arxiv.org
We perform a comparison of WMAP 9-year (WMAP9) and Planck 2015 cosmic microwave
background (CMB) temperature power spectra across multipoles $30\leq\ell\leq1200 $. We …
background (CMB) temperature power spectra across multipoles $30\leq\ell\leq1200 $. We …
Point-source power in 3 year Wilkinson Microwave Anisotropy Probe data
KM Huffenberger, HK Eriksen… - The Astrophysical …, 2006 - iopscience.iop.org
Using a set of multifrequency cross spectra computed from the 3 year WMAP sky maps, we
fit for the unresolved point-source contribution. For a white-noise power spectrum, we find a …
fit for the unresolved point-source contribution. For a white-noise power spectrum, we find a …
Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: final maps and results
CL Bennett, D Larson, JL Weiland… - The Astrophysical …, 2013 - iopscience.iop.org
We present the final nine-year maps and basic results from the Wilkinson Microwave
Anisotropy Probe (WMAP) mission. The full nine-year analysis of the time-ordered data …
Anisotropy Probe (WMAP) mission. The full nine-year analysis of the time-ordered data …
A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
U Natale, L Pagano, M Lattanzi, M Migliaccio… - Astronomy & …, 2020 - aanda.org
We present a cosmic microwave background (CMB) large-scale polarization dataset
obtained by combining Wilkinson Microwave Anisotropy Probe (WMAP) in the K, Q, and V …
obtained by combining Wilkinson Microwave Anisotropy Probe (WMAP) in the K, Q, and V …
Diagnosing timing error in WMAP data
H Liu, SL Xiong, TP Li - Monthly Notices of the Royal …, 2011 - academic.oup.com
The Doppler dipole signal dominates the cosmic microwave background (CMB) anisotropy
maps obtained by the Wilkinson Microwave Anisotropy Probe (WMAP) mission, and plays a …
maps obtained by the Wilkinson Microwave Anisotropy Probe (WMAP) mission, and plays a …
First-year wilkinson microwave anisotropy probe (wmap)* observations: Data processing methods and systematic error limits
G Hinshaw, C Barnes, CL Bennett… - The Astrophysical …, 2003 - iopscience.iop.org
We describe the calibration and data processing methods used to generate full-sky maps of
the cosmic microwave background (CMB) from the first year of Wilkinson Microwave …
the cosmic microwave background (CMB) from the first year of Wilkinson Microwave …