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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 9.

A 2D heat map showing the agreement between HST and JWST sources. Numbers in parentheses denote the number of sources in the column. The results typically agree whether a source is disk-dominated or spheroidal, as noted by the 92% agreement on disks and 60% for spheroids. Disk-spheroids show the largest disagreement, with 4/9 HST disk-spheroids being classified as disks using JWST. This difference is likely due to the increased resolution and sensitivity of JWST, which more clearly resolved the disks from any nuclear components.

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