Multiwavelength Variability of TeV Blazars with XMM-Newton

Details Multiwavelength Variability of TeV Blazars with XMM-Newton Multiwavelength Variability of TeV Blazars with XMM-Newton

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..251z&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Computer Science

Scientific paper

We present the simultaneous multiwavelength variability properties of the TeV blazar PKS 2155-304 obtained with the optical-UV and X-ray instruments on-board XMM-Newton. The UV variations globally follow the X-ray ones. However, compared with the X-ray light curve, the UV light curve is much less ``structured,'' and the UV variability amplitude is substantially smaller. The UV-X-ray spectra become flatter with increasing fluxes, and the UV and X-ray variations do not show detectable lags.

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