Probing the large-scale structure with the REFLEX cluster survey

被引：0

作者：

Böhringer, H ^{[1
]}

Guzzo, L ^{[1
]}

Collins, CA ^{[1
]}

Schuecker, P ^{[1
]}

Schindler, S ^{[1
]}

Voges, W ^{[1
]}

Neumann, DM ^{[1
]}

Cruddace, R ^{[1
]}

DeGrandi, S ^{[1
]}

Chincarini, G ^{[1
]}

Reiprich, TH ^{[1
]}

Edge, AC ^{[1
]}

MacGillivray, HT ^{[1
]}

Shaver, P ^{[1
]}

机构：

[1] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany

来源：

FROM EXTRASOLAR PLANETS TO COSMOLOGY: THE VLT OPENING SYMPOSIUM | 2000年

关键词：

D O I：

10.1007/10720961_19

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Clusters of galaxies detected in X-rays are ideal probes for the study of the large scale structure in the Universe. Based on the ROSAT All-Sky Survey we have conducted a large redshift survey as an ESO key programme to identify the X-ray brightest clusters found in the southern hemisphere. We present first results from the bright part of the survey comprising 460 identified clusters for an X-ray flux limit of 3.10(-12) erg s(-1) cm(-2). We show results for the X-ray luminosity function and discuss the assessment of the large-scale structure be means of the duster distribution power spectrum on a scale of 400h(-1) Mpc.

引用

页码：157 / 163

页数：7

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