THE GAUSS–LEGENDRE SKY PIXELIZATION FOR THE CMB POLARIZATION (GLESP-POL) ERRORS DUE TO PIXELIZATION OF THE CMB SKY

DOI10.1142/S0218271811019219zbMath1219.85009arXiv0904.2517OpenAlexW3099870639MaRDI QIDQ3019455

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Publication date: 28 July 2011

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0904.2517

zbMATH Keywords

data analysiscosmic microwave background

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40) Statistical astronomy (85A35)

Related Items (2)

Needlet-Whittle estimates on the unit sphere ⋮ On the regularity of the covariance matrix of a discretized scalar field on the sphere

Cites Work

• Fast algorithms for spherical harmonic expansions. II.
• GAUSS–LEGENDRE SKY PIXELIZATION (GLESP) FOR CMB MAPS
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