Making maps from Planck LFI 30 GHz data with asymmetric beams and cooler noise-Reference-Cited by-同舟云学术

Making maps from Planck LFI 30 GHz data with asymmetric beams and cooler noise

Published:2008-11-20 Issue:2 Volume:493 Page:753-783
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Ashdown M. A. J.,Baccigalupi C.,Bartlett J. G.,Borrill J.,Cantalupo C.,de Gasperis G.,de Troia G.,Górski K. M.,Hivon E.,Huffenberger K.,Keihänen E.,Keskitalo R.,Kisner T.,Kurki-Suonio H.,Lawrence C. R.,Natoli P.,Poutanen T.,Prézeau G.,Reinecke M.,Rocha G.,Sandri M.,Stompor R.,Villa F.,Wandelt B.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:200810381/pdf

Reference51 articles.

1. Making sky maps from Planck data

2. Making maps from Planck LFI 30 GHz data

3. First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Foreground Emission

4. Borrill, J. 1999, in Proceedings of the 5th European SGI/Gray MPP Workshop, Bologna, Italy [arXiv:astro-ph/9911389]

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