A full-sky prediction of the Sunyaev-Zeldovich effect from diffuse hot gas in the local universe and the upper limit from the WMAP data

Monthly Notices of the Royal Astronomical Society

Volumn 361, Issue 3, 2005, Pages 753-762

  Hansen, F K ^a   Branchini, E ^b   Mazzotta, P ^c,d   Cabella, P ^c   Dolag, K ^e  

^a UNIVERSITY OF OSLO   (Norway)

^b ROMA TRE UNIVERSITY   (Italy)

^c UNIVERSITY OF ROME TOR VERGATA   (Italy)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmology: cosmic microwave background; Cosmology: observations; Methods: data analysis; Methods: statistical; Techniques: image processing

Indexed keywords

GALAXIES; GASES; IMAGE PROCESSING;

COSMIC MICROWAVES BACKGROUND; COSMOLOGY OBSERVATIONS; COSMOLOGY: COSMIC MICROWAVE BACKGROUND; HOT GAS; LARGE-SCALES; METHODS. DATA ANALYSIS; METHODS:STATISTICAL; SUNYAEV-ZELDOVICH EFFECTS; TECHNIQUES: IMAGE PROCESSING; UPPER LIMITS;

COSMOLOGY;

EID: 23844531943     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09210.x     Document Type: Article

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