The XMM-Newton Wide-Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies - Archive ouverte HAL
Article Dans Une Revue The Astrophysical Journal Année : 2007

The XMM-Newton Wide-Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies

Chris Impey
  • Fonction : Auteur
Lidia Tasca

Résumé

We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keV band of 3×10-15 ergs cm-2 s-1, having one of the widest XMM-Newton contiguous raster surveys, covering an area of 2.1 deg2. Cluster candidates are identified through a wavelet detection of extended X-ray emission. Verification of the cluster candidates is done based on a galaxy concentration analysis in redshift slices of thickness 0.1-0.2 in redshift, using the multiband photometric catalog of the COSMOS field and restricting the search to z

Dates et versions

hal-03742449 , version 1 (02-08-2022)

Identifiants

Citer

Alexis Finoguenov, L. Guzzo, G. Hasinger, Nick Scoville, Hervé Aussel, et al.. The XMM-Newton Wide-Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies. The Astrophysical Journal, 2007, 172, pp.182-195. ⟨10.1086/516577⟩. ⟨hal-03742449⟩
11 Consultations
0 Téléchargements

Altmetric

Partager

More