BVRI CCD-photometry of comparison stars in the neighborhoods of galaxies with active nuclei. III
Observations with a matrix photometer are reported. The stellar magnitudes in the BVRcIc bands are estimated for 80 comparison stars in the neighborhoods of 10 galaxies with active nuclei: 2 Seyfert galaxies, 4 quasars, and 4 BL Lac objects. The stellar magnitudes of the observed stars range from 11...
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Veröffentlicht in: | Astrophysics 2007-01, Vol.50 (1), p.40-53 |
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Sprache: | eng |
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Zusammenfassung: | Observations with a matrix photometer are reported. The stellar magnitudes in the BVRcIc bands are estimated for 80 comparison stars in the neighborhoods of 10 galaxies with active nuclei: 2 Seyfert galaxies, 4 quasars, and 4 BL Lac objects. The stellar magnitudes of the observed stars range from 11 to 19^sup m^.5. For stars with magnitudes of 14-15^sup m^ the typical photometric errors are 0^sup m^.011, 0^sup m^.008, 0^sup m^.006, and 0^sup m^.007 in the B, V, R, and I bands, respectively. The BVRI magnitudes for most of these stars were not known previously. 14' × 14' finding charts for these stars are included. These results can be used for differential BVRI photometry of active galactic nuclei.[PUBLICATION ABSTRACT] |
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ISSN: | 0571-7256 1573-8191 |
DOI: | 10.1007/s10511-007-0005-y |