BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. I

Details BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. I BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. I

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap.....48..156d&link_type=abstract

Astrophysics, Volume 48, Issue 2, pp.156-178

Astronomy and Astrophysics

Astronomy

9

Extragalactic Astronomy, Agn, Comparison Stars, Photometry, Extragalactic Astronomy - Agn - Comparison Stars - Photometry

Scientific paper

Results are presented from CCD BVRI observations of comparison stars in the neighborhoods of 22 galaxies with active nuclei having right ascensions ranging from 0 to 12 hours, of which 19 are Seyfert galaxies. The observed stars have magnitudes ranging from V=11 to V=17. For stars brighter than V=14 the typical photometic error is 0.01m. The B, V, Rc, and Ic magnitudes of most of these stars were not known previously. 14′×14′ finding charts are included. These results can be used for differential photometry of the AGNs in the B, V, Rc, and Ic bands.

Affiliated with

Also associated with

No associations

Rating

BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. I does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. I, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. I will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1453947