From the time-ordered data to the Maximum-Likelihood temperature maps of the Cosmic Microwave Backgorund anisotropy

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dc.creatorStompor, R.
dc.creatorBalbi, A.
dc.creatorBorrill, J.
dc.creatorFerreira, P.
dc.creatorHanany, S.
dc.creatorJaffe, A.
dc.creatorLee, A.
dc.creatorOh, S.
dc.creatorRabii, B.
dc.creatorRichards, P.
dc.creatorSmoot, G.
dc.creatorWinant, C.
dc.creatorWu, J. -H. P.
dc.date2000-12-20
dc.date.accessioned2026-07-07T01:57:06Z
dc.date.available2026-07-07T01:57:06Z
dc.descriptionWe review selected methods of the Cosmic Microwave Background data analysis appropriate for the analysis of the largest currently available data sets. We focus on techniques of the time-ordered data manipulation and map making algorithms based on the maximum-likelihood approach. The presented methods have been applied to the MAXIMA data analysis (Hanany et al 2000) and the description of the algorithms is illustrated with the examples drawn from that experience. The more extensive presentation of the here-mentioned issues will be given in the forthcoming paper (Stompor et al 2001).
dc.description7 pages, no figures, uses eso.sty, to appear in Mining the Sky, ESO Astrophysics Symposia Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0012418
dc.identifierhttp://arxiv.org/abs/astro-ph/0012418
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2255
dc.subjectAstrophysics
dc.titleFrom the time-ordered data to the Maximum-Likelihood temperature maps of the Cosmic Microwave Backgorund anisotropy
dc.typetext

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