Aleksic, J.J.AleksicAlvarez, E. A.E. A.AlvarezAntonelli, Lucio AngeloLucio AngeloAntonelliCarosi, AlessandroAlessandroCarosi2020-09-172020-09-172012-03-01https://hdl.handle.net/20.500.13025/2565Astronomy & Astrophysics, Volume 539, id.A118, <NUMPAGES>6</NUMPAGES> pp.<BR /> Aims We study the non-thermal jet emission of the BL Lac object B3 2247+381 during a high optical state. <BR /> Methods The MAGIC telescopes observed the source during 13 nights between September 30th and October 30th 2010, collecting a total of 14.2 h of good quality very high energy (VHE) gamma-ray data. Simultaneous multiwavelength data was obtained with X-ray observations by the Swift satellite and optical R-band observations at the KVA-telescope. We also use high energy gamma-ray (HE, 0.1-100 GeV) data from the Fermi satellite. <BR /> Results The BL Lac object B3 2247+381 (z = 0.119) was detected, for the first time, at VHE gamma-rays at a statistical significance of 5.6sigma. A soft VHE spectrum with a photon index of -3.2 0.6 was determined. No significant short term flux variations were found. We model the spectral energy distribution using a one-zone SSC-model, which can successfully describe our data.galaxies activeBL Lacertae objects individual B3 2247+38110.1051/0004-6361/201117967http://adsabs.harvard.edu/abs/2012A&A...539A.118A2012A&A...539A.118A