UV-X rays Spectral Energy Distributions of AGN using XMM-Newton data

Details UV-X rays Spectral Energy Distributions of AGN using XMM-Newton data UV-X rays Spectral Energy Distributions of AGN using XMM-Newton data

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009mavo.proc...59f&link_type=abstract

Multi-wavelength Astronomy and Virtual Observatory, Proceedings of the EURO-VO Workshop, held at the European Space Astronomy Ce

Astronomy and Astrophysics

Astronomy

Virtual Observatory

Scientific paper

Studies of Spectral Energy Distributions (SED) of Active Galaxies are crucial for understanding the relation among the physical components in Active Galactic Nuclei (AGN). The connection between the optical/UV and the X-ray spectra is being debated because of the lack of measurements in the spectral band joining them and because of the paucity of simultaneous measurements in these bands, which is necessary to account for the intrinsic source variability. XMM-Newton offers the opportunity to study the simultaneous X-rays and optical/UV emission by using the EPIC and Optical Monitor (OM) data. We present results of the study of 143 simultaneous observations of 111 sources.

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