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Article Dans Une Revue Monthly Notices of the Royal Astronomical Society Année : 2010

Partial CMB maps: bias removal and optimal binning of the angular power spectrum

Résumé

We present a semi-analytical method to investigate the systematic effects and statistical uncertainties of the calculated angular power spectrum when incomplete spherical maps are used. The computed power spectrum suffers in particular a loss of angular frequency resolution, which can be written as \delta_l ~ \pi/\gamma_max, where \gamma_max is the effective maximum extent of the partial spherical maps. We propose a correction algorithm to reduce systematic effects on the estimated C_l, as obtained from the partial map projection on the spherical harmonic Ylm(l,m) basis. We have derived near optimal bands and weighting functions in l-space for power spectrum calculation using small maps, and a correction algorithm for partially masked spherical maps that contain information on the angular correlations on all scales.
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Dates et versions

hal-00424694 , version 1 (19-10-2009)
hal-00424694 , version 2 (02-10-2010)

Identifiants

Citer

R. Ansari, C. Magneville. Partial CMB maps: bias removal and optimal binning of the angular power spectrum. Monthly Notices of the Royal Astronomical Society, 2010, 405 (3), pp.1421-1430. ⟨10.1111/j.1365-2966.2010.16561.x⟩. ⟨hal-00424694v2⟩
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