Image Details

Choose export citation format:

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 2.

Magnitude differences from three different photometric measurements for each source. Blue squares: difference in the large-aperture photometry of UVM2 and F225W; orange circles: difference in the GALFIT point-source magnitude of UVM2 and F225W; green triangles: difference in the GALFIT point-source magnitude of the F225W data and the GalSim-simulated UVM2 data. NGC7603 compares the F225W filter with UVOT/UVW1 instead of UVOT/UVM2, as no UVM2 data were available for this source in K. K. Gupta et al. (2024). For all but one source, the difference in the point-source magnitude between HST and Swift/UVOT data is larger than that in the large-aperture photometry.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse