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...
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| Main Authors: | , , , , , , , , , , , , , , , , , , , |
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| Format: | Artigo |
| Language: | Inglês |
| Published: |
IOP Publishing
2026-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ae581d |
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