SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010)

Details SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010) SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010)

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..74032063f&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/403/2063. Originally published in: 2010MNRAS.403.2063F

Physics

Surveys, X-Ray Sources, Clusters: Galaxy

Scientific paper

We present the results of a search for galaxy clusters in the Subaru-XMM Deep Field (SXDF). We reach a depth for a total cluster flux in the 0.5-2keV band of 2x10-15erg/cm2/s over one of the widest XMM-Newton contiguous raster surveys, covering an area of 1.3deg2. Cluster candidates are identified through a wavelet detection of extended X-ray emission. The red-sequence technique allows us to identify 57 cluster candidates. We report on the progress with the cluster spectroscopic follow-up and derive their properties based on the X-ray luminosity and cluster scaling relations.
(3 data files).

Affiliated with

Also associated with

No associations

Rating

SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1381323