Fast computation of angular power spectra and covariances of high-resolution cosmic microwave background maps using the Toeplitz approximation (2020)
Attributed to:
Consolidated Grant Astronomy Observation and Theory 2019-2022
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2010.14344
Publication URI: https://arxiv.org/abs/2010.14344
Type: Other