A. V. Tugay, S. L. Shihov
Published 2014-10-11Version 1
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.
Comments: 3 pages, 2 figures, reported at 18th Young Scientists Conference "Astronomy and Space Physics", May 2-7, 2011, Kyiv, Ukraine
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Probing Radio Emission in Seyfert Galaxies on Parsec- and Kiloparsec-scales
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