Surface Brightness Profiles of Seyfert Galaxies
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.
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Zusammenfassung: | 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. |
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DOI: | 10.48550/arxiv.1410.2975 |