Multi-wavelength Observations of the Flaring Gamma-ray Blazar 3C 66A in 2008 October
arXiv:1011.1053 · doi:10.1088/0004-637X/726/1/43
Abstract
The BL Lacertae object 3C 66A was detected in a flaring state by the Fermi Large Area Telescope (LAT) and VERITAS in 2008 October. In addition to these gamma-ray observations, F-GAMMA, GASP-WEBT, PAIRITEL, MDM, ATOM, Swift, and Chandra provided radio to X-ray coverage. The available light curves show variability and, in particular, correlated flares are observed in the optical and Fermi-LAT gamma-ray band. The resulting spectral energy distribution can be well fit using standard leptonic models with and without an external radiation field for inverse-Compton scattering. It is found, however, that only the model with an external radiation field can accommodate the intra-night variability observed at optical wavelengths.
arXiv commentAccepted for publication in ApJ. 32 pages, 8 figures and 5 tables. Corresponding author: Luis C. Reyes ([email protected])
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