6533b86ffe1ef96bd12cd3fb

RESEARCH PRODUCT

The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue

P. A. ShaverHans BoehringerAlastair C. EdgeDoris M. NeumannPeter SchueckerH. T. MacgillivrayChris A. CollinsR. G. CruddaceWolfgang VogesA. Ortiz-gilG. ChincariniS. De GrandiLuigi GuzzoS. Schindler

subject

Large-scale structure of Universemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSample (statistics)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAClustersX-raysROSATCluster (physics)Galaxy clusterAstrophysics::Galaxy Astrophysicsmedia_commonPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsFunction (mathematics)Galaxies:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]RedshiftCosmologyData setSpace and Planetary ScienceSkyCatalogsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Catalogs ; Surveys ; Galaxies ; Clusters ; Cosmology ; Large-scale structure of Universe ; X-rays

description

We present the catalogue of the REFLEX Cluster Survey providing information on the X-ray properties, redshifts, and some identification details of the clusters in the REFLEX sample. The catalogue describes a statistically complete X-ray flux-limited sample of 447 galaxy clusters above an X-ray flux of 3 10(-12) erg /s/cm**2 (0.1 to 2.4 keV) in an area of 4.24 ster in the southern sky. The cluster candidates were first selected by their X-ray emission in the ROSAT-All Sky Survey and subsequently spectroscopically identified in the frame of an ESO key programme. In addition to the cluster catalogue we also describe the complete selection criteria as a function of the sky position and the conversion functions used to analyse the X-ray data. These are essential for the precise statistical analysis of the large-scale cluster distribution. This data set is at present the largest, statistically complete X-ray galaxy cluster sample. Together with these data set we also provide for the first time the full three-dimensional selection function. The sample forms the basis of several cosmological studies, one of the most important applications being the assessment of the statistics of the large-scale structure of the universe and the test of cosmological models.

https://dx.doi.org/10.48550/arxiv.astro-ph/0405546