The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen

Details The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..228g&link_type=abstract

XMM-Newton Proposal ID #05062001

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 1H 0707-495, Xmm-Newton Proposal 05062001

Scientific paper

The Narrow-Line Seyfert 1 galaxy (NLS1) 1H 0707-495 exhibits a sharp spectral feature at energies around 7 keV. Both blurred ionised disc reflection and partial-covering can be used to explain the observed broad-band properties of 1H 0707-495, as both models reproduce very similar spectra in low-flux states. However, long term monitoring and a single deep observation will distinguish the correct, physically motivated AGN model, and permit us to probe the physics at work. We propose to examine 1H 0707-495 for 400 ks. A combination of monitoring (4 x 40 ks) and a deep pointing (1 x 240 ks) will be used.

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