NIR photometry of X-ray luminous BCGs (Stott+, 2008)

Details NIR photometry of X-ray luminous BCGs (Stott+, 2008) NIR photometry of X-ray luminous BCGs (Stott+, 2008)

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73841502s&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/384/1502. Originally published in: 2008MNRAS.384.1502S

Physics

Clusters: Galaxy, X-Ray Sources, Galaxies: Ir, Redshifts, Photometry: Infrared

Scientific paper

To select BCGs in a homogeneous sample of massive clusters from z=0-1, we require X-ray selected clusters from a number of large surveys. A combination of the Two-Micron All-Sky Survey (2MASS) extended and point source catalogues (Skrutskie et al., 2006, Cat. VII/233) is used for the z<0.15 BCS, eBCS and XBACS BCGs.
The 0.15

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