Modeling the Multiwavelength Spectra and Variability of 3c 66A in 2003-2004

Details Modeling the Multiwavelength Spectra and Variability of 3c 66A in 2003-2004 Modeling the Multiwavelength Spectra and Variability of 3c 66A in 2003-2004

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007auhe.conf...25j&link_type=abstract

ASTROPHYSICS AT ULTRA-HIGH ENERGIES. Proceedings of the 15th Course of the International School of Cosmic Ray Astrophysics . Hel

Astronomy and Astrophysics

Astrophysics

Galaxies, Active, Bl Lacertae Objects, 3C 66A

Scientific paper

The BL Lac object 3C 66A was the target of an intensive multiwavelength monitoring campaign organized in 2003-2004. During the campaign, its spectral energy distribution (SED) was measured and flux measurements from radio to X-ray frequencies as well as upper limits in the very high energy (VHE) γ-ray regime were obtained. Here, we reproduce the SED and optical spectral variability pattern observed during our multiwavelength campaign using a time-dependent leptonic jet model. Our model could successfully simulate the observed SED and optical light curves and predict an intrinsic cutoff value for the VHE γ-ray emission at ~ 4 GeV.

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