S5 0716+714: Analysis of Color Variability for 2001-2004

Details S5 0716+714: Analysis of Color Variability for 2001-2004 S5 0716+714: Analysis of Color Variability for 2001-2004

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..360..185h&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

The results of multicolor observations of blazar S5 0716+714 carried out during 2001-2004 at the Astronomical Institute of St.Petersburg State University (AI SPbSU) are given. They have been analysed with the aim of investigating color variability. It is found that the spectral energy distribution of the variable source in the optical and near infrared bands is unchanged and may be fitted by a power law: F_ν ∝ ν^{-1.12}. Because of the high polarization often observed in the object the synchrotron nature of the variable source is undoubted.

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