Observations of very high energy emission from B2 1215+30 with VERITAS
Abstract
We present results of 45 hours of data taken from January to June 2011 with VERITAS above 200 GeV in the direction of B2 1215+30. The blazar was clearly detected with a constant flux of F(E>200 GeV) = (8.0 +- 0.9) × 10-12 cm-2 s-1. The energy spectrum can be fitted using a power-law with index -3.6 +- 0.5. Simultaneous multi-wavelength data are also presented, and are used to model the spectral energy distribution with a one-zone leptonic model.
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