Beecroft Institute for Particle Astrophysics and Cosmology

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The formation of galaxy discs

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 324:2 (2001) 313-318
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The host galaxies of luminous radio-quiet quasars

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 322:4 (2001) 843-858

Authors:

WJ Percival, L Miller, RJ McLure, JS Dunlop
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The submaximal disk of NGC 4254

GALAXY DISKS AND DISK GALAXIES 230 (2001) 559-560

Authors:

T Kranz, A Slyz, HW Rix
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The trispectrum of the 4 year COBE DMR data

ASTROPHYSICAL JOURNAL 563:2 (2001) L99-L102

Authors:

M Kunz, AJ Banday, PG Castro, PG Ferreira, KM Górski
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From the time-ordered data to the Maximum-Likelihood temperature maps of the Cosmic Microwave Backgorund anisotropy

ArXiv astro-ph/0012418 (2000)

Authors:

R Stompor, A Balbi, J Borrill, P Ferreira, S Hanany, A Jaffe, A Lee, S Oh, B Rabii, P Richards, G Smoot, C Winant, J-HP Wu

Abstract:

We 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).
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