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Resolved UV–Optical HST Imaging and Spectral Energy Distribution Modeling of Nearby BAT Active Galactic Nuclei

  • Authors: Connor Auge, Michael Koss, Kriti K. Gupta, Claudio Ricci, Benny Trakhtenbrot, Franz E. Bauer, Ezequiel Treister, Alessandro Peca, Brad Cenko, Kohei Ichikawa, Arghajit Jana, Darshan Kakkad, Richard Mushotzky, Kyuseok Oh, Alejandra Rojas Lilayú, David Sanders, Roberto Serafinelli, Matilde Signorini, Alessia Tortosa, C. Megan Urry

Connor Auge et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 6.

Difference in maximum disk temperature derived from the best-fit SEDs in this work using HST UV–optical data, compared to the maximum disk temperature from G24 using Swift/UVOT data, shown as a function of the ratio of bolometric luminosities between the two datasets.

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