XMM-Newton Proposal 02062015

Details XMM-Newton Proposal 02062015 XMM-Newton Proposal 02062015

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..322g&link_type=abstract

XMM-Newton Proposal ID #02062015

Computer Science

Asca Lss 1, Asca Lss 2, Asca Lss 3, Asca Lss 4, Asca Lss 5, Asca Lss 6, Asca Lss 7, Asca Lss 8, Asca Lss 9, Asca Lss 10, Asca Lss 11, Asca Lss 12, Asca Lss 13, Asca Lss 14, Asca Lss 15, Xmm-Newton Proposal 02062015

Scientific paper

We propose XMM EPIC observations of the AGN sample in the ASCA Large Sky Survey, which is spectroscopically complete at a 2-10 keV limiting flux of 1E-13 erg/cm2/s and where a number of luminous and X-ray hard AGN have been found. Our observations will solve the degeneracy between spectral flatness and X-ray absorpion in these sources, which are identified as broad line objects, revealing if they are indeed obscured QSOs. Also, the column density distribution of the whole sample, compared with that expected from synthesis models, will indicate if there are variations in the average absorbing columns of high and low luminosity AGN.

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