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Paper: Photometric Behavior of the Seyfert Galaxy Mrk 335 in the Optical Region in 1995-2004
Volume: 360, AGN Variability from X-Rays to Radio Waves
Page: 49
Authors: Doroshenko, V.T.; Sergeev, S.G.; Merkulova, N.I.; Sergeeva, E.A.; Golubinsky, Yu.V.
Abstract: We present results of UBV RI photometry of Mrk 335 in the period 1995–2004. Mrk 335 has a large amplitude of variability, varying by about 1.1, 0.9 and 0.7 mag in the U,B and V bands respectively and by about 0.3 mag in both R and I bands. The Structure Function (SF) has a logarithmic slope b=0.63±0.03 on time scales from 3 to 2000 days and is very similar to the SF of Mrk 6. The UBV RI spectral energy distribution is typical of Seyfert 1 galaxies. It was found that the fluxes in the V,R and I bands lag the flux in the U band by about 4, 8, and 8 days, respectively.
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