The XMM-Newton/2dF survey - III. Comparison between optical and X-ray cluster detection methods

Monthly Notices of the Royal Astronomical Society

Volumn 351, Issue 3, 2004, Pages 989-996

  Basilakos, S ^a   Plionis, M ^a,b   Georgakakis, A ^a   Georgantopoulos, I ^a   Gaga, T ^a,c   Kolokotronis, V ^a   Stewart, G C ^d  

^a NATIONAL OBSERVATORY OF ATHENS   (Greece)

^b INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^c UNIVERSITY OF ATHENS   (Greece)

^d UNIVERSITY OF LEICESTER   (United Kingdom)

Author keywords

Cosmology: large scale structure of Universe; Cosmology: observations; Galaxies: clusters: general

Indexed keywords

GALAXIES; MATCHED FILTERS; SOLVENTS;

CLUSTER DETECTION; COSMOLOGY OBSERVATIONS; COSMOLOGY: LARGE SCALE STRUCTURE OF UNIVERSE; DETECTION METHODS; GALAXIES: CLUSTERS: GENERAL; OPTICAL TECHNIQUE; OPTICAL-; SLOAN DIGITAL SKY SURVEY; X-RAY TECHNIQUES; XMM-NEWTON;

SURVEYS;

EID: 3042814727     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07841.x     Document Type: Review

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