Surface Brightness Profiles of Seyfert Galaxies
A.V. Tugay, S.L. Shihov

TL;DR
This study constructs r-band surface brightness profiles for 16 Seyfert galaxies using SDSS data, aiding in more precise lightcurve analysis for these active galaxies.
Contribution
The paper presents new surface brightness profiles for Seyfert galaxies derived from SDSS data, improving lightcurve accuracy.
Findings
Profiles enable better lightcurve analysis.
Data enhances understanding of Seyfert galaxy structure.
Method improves surface brightness measurement accuracy.
Abstract
We built r-band surface brightness profiles by SDSS data for 16 Seyfert galaxies observed in Crimean Astrophysical Observatory. Obtained profiles can be used for finding more accurate lightcurves for these galaxies.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomical Observations and Instrumentation · Astronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena
