XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005)

Details XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005) XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005)

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..34440079m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/444/79. Originally published in: 2005A&A...444...79M

Physics

X-Ray Sources, Surveys, Active Gal. Nuclei

Scientific paper

This paper presents the results of a detailed X-ray spectral analysis of a sample of 123 X-ray sources detected with XMM-Newton in the Lockman Hole field. This is the deepest observation carried out with XMM-Newton with more that 600ks of good EPIC-pn data. We have spectra with good signal to noise (>500 source counts) for all objects down to 0.2-12keV fluxes of 5x10-15erg/cm2/s (flux limit of 6x10-16erg/cm2/s in the 0.5-2 and 2-10keV bands). At the time of the analysis, we had optical spectroscopic identifications for 60% of the sources, 46 being optical type-1 AGN and 28 optical type-2 AGN. Using a single power law model our sources' average spectral slope hardens at faint 0.5-2keV fluxes but not at faint 2-10keV fluxes.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005) 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 XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1733593