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Long term observations of B2 1215+30 with veritas
Journal article   Open access   Peer reviewed

Long term observations of B2 1215+30 with veritas

E Aliu, M Errando, S Archambault, T Arlen, T Aune, M Beilicke, J. H Buckley, V Bugaev, W Benbow, R Bird, …
The Astrophysical journal, Vol.779(2), 92
12/20/2013
DOI: 10.1088/0004-637X/779/2/92
url
https://doi.org/10.1088/0004-637X/779/2/92View
Published (Version of record) Open Access

Abstract

We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this period, the source was detected at very high energies (VHEs; E > 100 GeV) by VERITAS with a significance of 8.9σ and showed clear variability on timescales larger than months. In 2011, the source was found to be in a relatively bright state and a power-law fit to the differential photon spectrum yields a spectral index of 3.6 ± 0.4{sub stat} ± 0.3{sub syst} with an integral flux above 200 GeV of (8.0 ± 0.9{sub stat} ± 3.2{sub syst}) × 10{sup –12} cm{sup –2} s{sup –1}. No short term variability could be detected during the bright state in 2011. Multi-wavelength data were obtained contemporaneously with the VERITAS observations in 2011 and cover optical (Super-LOTIS, MDM, Swift/UVOT), X-ray (Swift/XRT), and gamma-ray (Fermi-LAT) frequencies. These were used to construct the spectral energy distribution (SED) of B2 1215+30. A one-zone leptonic model is used to model the blazar emission and the results are compared to those of MAGIC from early 2011 and other VERITAS-detected blazars. The SED can be reproduced well with model parameters typical for VHE-detected BL Lac objects.
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BL LACERTAE OBJECTS COMPARATIVE EVALUATIONS EMISSION ENERGY SPECTRA GAMMA RADIATION GEV RANGE PHOTONS WAVELENGTHS X RADIATION

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