Suzaku and XMM-Newton Observations of Type 2 ULIRGs with High [OIII] Luminosity

Details Suzaku and XMM-Newton Observations of Type 2 ULIRGs with High [OIII] Luminosity Suzaku and XMM-Newton Observations of Type 2 ULIRGs with High [OIII] Luminosity

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..445h&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Quasars, X-Ray Spectroscopy, Galactic Nuclei, Seyfert Galaxies, Brightness, Quasars, X-Ray, Galactic Nuclei, Circumnuclear Matter, And Bulges, Active And Peculiar Galaxies And Related Systems, Magnitudes And Colors, Luminosities

Scientific paper

We present results from observations of three type 2 quasar candidates with Suzaku and XMM-Newton. These are type 2 ULIRGs with quasar classification selected from the IRAS 1 Jy sample. We analyze their X-ray spectra to investigate the AGN power in these ULIRGs. The X-ray spectra are explained by a combination of unabsorbed and absorbed power-law components with Γ = 1.48-2.40. The best-fit NH for the absorbed component is in the range of (9.1-76)×1022 cm-2. The absorption-corrected L2-10 keV of AGNs are in the range for Seyferts ((4.3-24)×1042erg s-1).

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