6533b883fe1ef96bd12dd573

RESEARCH PRODUCT

XMM-Newton survey of the ELAIS-S1 field

S. PuccettiF. FioreV. D'eliaI. PillitteriC. FeruglioA. GrazianM. BrusaP. CiliegiA. ComastriC. GruppioniM. MignoliC. VignaliG. ZamoraniF. La FrancaN. SacchiA. FranceschiniS. BertaH. ButteryJ.e. Dias

subject

Active galactic nucleigalactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysX-ray sourcesCosmologyobservational astronomyX ray sourcesNatural SciencesAstrophysics::Galaxy Astrophysics

description

The formation and evolution of cosmic structures can be probed by studying the evolution of the luminosity function of the Active Galactic Nuclei (AGNs), galaxies and clusters of galaxies and of the clustering of the X-ray active Universe, compared to the IR-UV active Universe. To this purpose, we have surveyed with XMM-Newton the central ~0.6{deg}^2^ region of the ELAIS-S1 field down to flux limits of ~5.5x10^-16^erg/cm^2^/s (0.5-2keV, soft band, S), ~2x10^-15^erg/cm^2^/s (2-10keV, hard band, H), and ~4x10^-15^erg/cm^2^/s (5-10keV, ultra hard band, HH). We present here the analysis of the XMM-Newton observations, the number counts in different energy bands and the clustering properties of the X-ray sources. Cone search capability for table J/A+A/457/501/elaisxmm (*ELAIS XMM V1.1 catalog (version of 2007-Apr-30)) Cone search capability for table J/A+A/457/501/catalog (*Multiwavelength data of XMM survey of the Elais-S1 field (version of 2007-Apr-30))

yearjournalcountryeditionlanguage
2008-01-01
10.26093/cds/vizier.34570501https://doi.org/http://doi.org/10.26093/cds/vizier.34570501