XMM-Newton Proposal 03018901

Details XMM-Newton Proposal 03018901 XMM-Newton Proposal 03018901

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...63p&link_type=abstract

XMM-Newton Proposal ID #03018901

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Eso 113-G010, Xmm-Newton Proposal 03018901

Scientific paper

Recently a short (4ks) XMM-Newton observation of the intermediate Seyfert 1.8 galaxy ESO113-G010 (z=0.0257) has revealed a narrow emission line at 5.4keV (object rest-frame), detected at 99% confidence level. This line can be attributed to the signature of redshifted iron emission from an orbiting hotspot on the inner accretion disk surface. Performing phase-resolved X-ray spectroscopy of this object will enable us to follow the evolution of the line profile over the orbital timescale of the inner accretion disk. Measurement of the line parameters (e.g., energy shift, intensity) will give us the inclination of the disk, radial location of the hotspot and even an estimate of the black hole mass. (abridged)

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