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

We use high-resolution UV-to-optical imaging from the Hubble Space Telescope (HST) to construct spatially resolved spectral energy distributions (SEDs) for seven nearby ( z < 0.07) hard (14–195 keV) X-ray-selected broad-line active galactic nuclei (AGN) with L _bol  = 10 ^43.26 –10 ^45.34 erg s ^−1...

Täydet tiedot

Bibliografiset tiedot

Päätekijät:	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
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2026-01-01
Sarja:	The Astrophysical Journal
Aiheet:	AGN host galaxies Spectral energy distribution HST photometry X-ray active galactic nuclei Active galactic nuclei
Linkit:	https://doi.org/10.3847/1538-4357/ae581d
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