Photometric Behavior of the Seyfert Galaxy Mrk 335 in the Optical Region in 1995-2004

Details Photometric Behavior of the Seyfert Galaxy Mrk 335 in the Optical Region in 1995-2004 Photometric Behavior of the Seyfert Galaxy Mrk 335 in the Optical Region in 1995-2004

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..360...49d&link_type=abstract

AGN Variability from X-Rays to Radio Waves ASP Conference Series, Vol. 360, Proceedings of the conference held 14-16 June, 2004

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results of UBVRI 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 UBVRI 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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