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Catalog Service:
Very rich Abell clusters radio analysis

Short name: J/ApJS/146/267
IVOA Identifier: ivo://CDS.VizieR/J/ApJS/146/267
DOI (Digital Object Identifier): 10.26093/cds/vizier.21460267
Publisher: CDS[+][Pub. ID]
More Info: http://cdsarc.unistra.fr/cgi-bin/cat/J/ApJS/146/267
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2003 Dec 29 21:44:03Z
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Description


Radio observations were used to detect the "active" galaxy population within rich clusters of galaxies in a nonbiased manner that is not plagued by dust extinction or the K-correction. We present wide-field radio, optical (imaging and spectroscopy), and ROSAT All-Sky Survey (RASS, Cat. <IX/10>) X-ray data for a sample of 30 very rich Abell (R>=2) cluster with z<=0.25. The VLA radio data samples the ultrafaint radio (L(1.4GHz)>=2x10^22^W/Hz) galaxy population within these extremely rich clusters for galaxies with RMAG<=-21. This is the largest sample of low-luminosity 20 cm radio galaxies within rich Abell clusters collected to date.

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under Cooperative Agreement AST0122449 with the Johns Hopkins University
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