Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 B2.

Results of the fits from the GALFIT analysis. Each source is grouped individually with a 3 × 3 grid showing the data, model, and residual (from left to right) for each filter. Each row shows a different filter, with F225W on the top, F435W in the middle, and F814W on the bottom. The sources are organized as follows: NGC7603 (upper left), UGC3478 (upper right), UGC524 (second left), Mrk1044 (second right), NGC985 (third left), VIIZw142 (third right), and IC 2921 (bottom left).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse