SCOPUS 정보 검색 플랫폼

Monthly Notices of the Royal Astronomical Society

Volumn 376, Issue 1, 2007, Pages 343-347

Can a large-scale structure probe cosmic microwave background-constrained non-Gaussianity?

(3) Kang, X a,c Norberg, P b Silk, Joseph a

a UNIVERSITY OF OXFORD (United Kingdom)

b UNIVERSITY OF EDINBURGH (United Kingdom)

c The Scottish Universities Physics Alliance (United Kingdom)

Author keywords

Cosmology: theory; Galaxies: clusters: general; Large scale structure of Universe

Indexed keywords

DISTRIBUTION FUNCTIONS; GALAXIES; PROBABILITY DENSITY FUNCTION; PROBES;

COSMIC MICROWAVES BACKGROUND; COSMOLOGY: THEORY; FIRST YEAR; GALAXIES: CLUSTERS: GENERAL; HIGH-REDSHIFT; LARGE SCALE STRUCTURE OF UNIVERSE; LARGE-SCALE STRUCTURE; NONGAUSSIANITY; PRIMORDIAL NON-GAUSSIANITY; WILKINSON MICROWAVE ANISOTROPY PROBE;

COSMOLOGY;

EID: 33947236367 PISSN: 00358711 EISSN: 13652966 Source Type: Journal
DOI: 10.1111/j.1365-2966.2007.11435.x Document Type: Article

Times cited : (38)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.