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Obscured AGN at z < 1.5: X-Ray to Far-infrared SEDs and Host Galaxy Morphologies in the GOODS Fields

  • Authors: William W.H. Jarvis, Connor Auge, David Sanders, Xuheng Ding, Jeana Kim-Bolt, C. Megan Urry, Eric Hooper, Alessandro Peca, Aritra Ghosh, Chuan Tian, Tonima T. Ananna, Md Mahmudunnobe

William W.H. Jarvis et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

Galaxy-only B/T ratio versus galaxy minus PS B/T ratio for 187 GOODS X-ray AGN colored by the ratio of light in the PS to the host galaxy (PS ratio). Note that the majority of fits with PS ratio > 1 show large diversions between the fit results. In some of these cases, the two-component only fit performs comparably to those with a PS subtracted, but for many sources with a large PS contribution, the B/T ratio appears to be overestimated if a PS is not subtracted. Sources above the +1σ line show, except for three galaxies, no improvement and even some evidence for overfitting if a PS is included.

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