Johnson-Cousins magnitudes of comparison stars in the fields of ten Seyfert galaxies
B. M. Mihov, L. S. Slavcheva-Mihova

TL;DR
This paper provides calibrated UBVRcIc magnitudes for 49 comparison stars in ten Seyfert galaxy fields, including 36 stars calibrated for the first time, aiding photometric monitoring of these active galactic nuclei.
Contribution
It offers new and improved comparison star sequences in multiple Seyfert galaxy fields, including first-time calibrations and added stars closer to the galaxies for better monitoring accuracy.
Findings
36 stars calibrated for the first time
Comparison sequences improved in several fields
Additional stars included near Seyfert galaxies
Abstract
We present UBVRcIc magnitudes of 49 comparison stars in the fields of the Seyfert galaxies Mrk 335, Mrk 79, Mrk 279, Mrk 506, 3C 382, 3C 390.3, NGC 6814, Mrk 304, Ark 564, and NGC 7469 in order to facilitate the photometric monitoring of these objects; 36 of the stars have not been calibrated before. The comparison stars are situated in 5x5 arcmin fields centred on the Seyfert galaxies, their V band flux ranges from 11.7 to 18.2 mag with a median value of 16.3 mag, and their B-V colour index ranges from 0.4 to 1.6 mag with a median value of 0.8 mag. The median errors of the calibrated UBVRcIc magnitudes are 0.08, 0.04, 0.03, 0.04, and 0.06 mag, respectively. Comparison stars were calibrated for the first time in three of the fields (Mrk 506, 3C 382, and Mrk 304). The comparison sequences in the other fields were improved in various aspects. Extra stars were calibrated in four fields…
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.
