Reference : XMM-LSS survey: AGN classifications (Garcet+, 2007)
Computer developments : Textual, factual or bibliographical database
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/32441
XMM-LSS survey: AGN classifications (Garcet+, 2007)
English
Garcet, O. [> > > >]
Gandhi, P. [> > > >]
Gosset, Eric mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE) >]
Sprimont, Pierre-Guillaume mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Surdej, Jean mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Borkowski, V. [> > > >]
Tajer, M. [> > > >]
Pacaud, F. [> > > >]
Pierre, M. [> > > >]
Chiappetti, L. [> > > >]
Maccagni, D. [> > > >]
Page, M. J. [> > > >]
Carrera, F. J. [> > > >]
Tedds, J. A. [> > > >]
Mateos, S. [> > > >]
Krumpe, M. [> > > >]
Contini, T. [> > > >]
Corral, A. [> > > >]
Ebrero, J. [> > > >]
Gavignaud, I. [> > > >]
Schwope, A. [> > > >]
Le Fevre, O. [> > > >]
Polletta, M. [> > > >]
Rosen, S. [> > > >]
Lonsdale, C. [> > > >]
Watson, M. [> > > >]
Borczyk, W. [> > > >]
Vaisanen, P. [> > > >]
1-Nov-2007
[en] X-ray sources ; Active gal. nuclei ; QSOs
[en] We have used the most up-to-date X-ray catalog (Pierre et al., 2007, Cat. J/MNRAS/382/279) to define a sample of 612 X-ray selected point-like sources which have both a log-likelihood of detection >20 (this roughly corresponds to >3{sigma}) in the [2-10]keV band (see Pacaud et al., 2006MNRAS.372..578P, for full details), and a total number of counts >80 in the [0.5-10]keV band. (1 data file).
Researchers ; Professionals
http://hdl.handle.net/2268/32441
http://adsabs.harvard.edu/abs/2007yCat..34740473G
http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/A+A/474/473
Optical properties and best-fit parameters from the X-ray spectral analysis (99 rows)

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