GAUSS–LEGENDRE SKY PIXELIZATION (GLESP) FOR CMB MAPS
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Publication:4680597
DOI10.1142/S0218271805006183zbMath1071.83506arXivastro-ph/0305537WikidataQ56573186 ScholiaQ56573186MaRDI QIDQ4680597
Per Rex Christensen, Pavel D. Naselsky, Oleg V. Verkhodanov, Dmitry I. Novikov, Li-Yuan Chiang, Andrei Georgievich Doroshkevich, Igor D. Novikov, V. I. Turchaninoff
Publication date: 7 June 2005
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0305537
Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05) Astrophysical cosmology (85A40)
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Nearly tight frames and space-frequency analysis on compact manifolds ⋮ The needlets bispectrum ⋮ PECULIARITIES OF PHASES OF THE WMAP QUADRUPOLE ⋮ A turning bands method for simulating isotropic Gaussian random fields on the sphere ⋮ Fast spin \(\pm \)2 spherical harmonics transforms and application in cosmology ⋮ SYMMETRIES OF THE GALACTIC FOREGROUNDS IN THE WMAP DATA ⋮ THE GAUSS–LEGENDRE SKY PIXELIZATION FOR THE CMB POLARIZATION (GLESP-POL) ERRORS DUE TO PIXELIZATION OF THE CMB SKY ⋮ CMB data analysis and sparsity ⋮ Practical wavelet design on the sphere ⋮ Statistical challenges in the analysis of cosmic microwave background radiation ⋮ On the regularity of the covariance matrix of a discretized scalar field on the sphere
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