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Suzaku Observations of Local Ultraluminous Infrared Galaxies

  • Authors: Stacy H. Teng, Sylvain Veilleux, Naohisa Anabuki, Charles D. Dermer, Luigi C. Gallo, Takao Nakagawa, Christopher S. Reynolds, D. B. Sanders, Yuichi Terashima, and Andrew S. Wilson

TENG et al. 2009 The Astrophysical Journal 691 261.

  • Provider: AAS Journals

Caption: Figure 4.

Combined XIS-HXD/PIN spectrum of Mrk 273 with the best-fit scattering model. The horizontal axis is energy in the observer's frame. The directly transmitted AGN flux is ~ 5% of the intrinsic flux. The iron line at ~ 6.4 keV is detected and a MEKAL model with gas temperature ~ 0.7 keV is needed to reproduce the soft X-rays. The cross-normalization of the HXD/PIN with respect to XIS0 is assumed to be 1.13. The best-fit parameters for the full band (XIS+HXD/PIN) modeling are listed in Table 3.

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