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- BL Lacertae objects: general (9)
- gamma rays: galaxies (9)
- gamma rays: general (7)
- astroparticle physics (5)
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- binaries: general (4)
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- BL Lacertae objects: individual (B2 1215+30, VER J1217+301) (2)
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- BL Lacertae objects: individual (1ES 0229+200, VER J0232+202) (1)
- BL Lacertae objects: individual (1ES 1959+650) (1)
- BL Lacertae objects: individual (1ES1218+30.4) (1)
- BL Lacertae objects: individual (PKS 1424+240)-cosmic background radiation (1)
- BL Lacertae objects: individual (VER J0521+211) (1)
- BL Lacertae objects: individual: 1ES 2344+514=VERJ2347+517 (1)
- BL Lacertae objects: individual: Markarian 501 (1)
- BL Lacertae objects: individual: Mrk 501 (1)
- BL Lacertae objects: individual: Mrk501 (1)
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- VERITAS (1)
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- galaxies: active-galaxies: individual: PMN J0948+0022 (1)
- galaxies: individual (Markarian 501) (1)
- galaxies: individual (RGB J2243+203) (1)
- galaxies: individual: 1ES 1741+196=VER J1744+195 (1)
- gamma rays : stars (1)
- gamma rays: general(HESS J0632+057, VER J0633+057) (1)
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- gamma-ray burst: individual (MGRO J1908+06, VER J1907+062) (1)
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- pulsars: individual (PSR J1907+0602) (1)
- pulsars: individual (PSR J2032+4127) (1)
- stars: individual ( KIC 8462852) (1)
- stars: individual (LS I+61 degrees 303, VER J0240+612) (1)
- supernovae : individual (CTB 87) (1)
- supernovae: individual (G0.9+0.1) (1)
- techniques: photometric (1)
Institute
B2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric Cherenkov telescopes and subsequently confirmed by the Very Energetic Radiation Imaging Telescope Array System (VERITAS) observatory with data collected between 2009 and 2012. In 2014 February 08, VERITAS detected a large-amplitude flare from B2. 1215+30 during routine monitoring observations of the blazar 1ES. 1218+304, located in the same field of view. The TeV flux reached 2.4 times the Crab Nebula flux with a variability timescale of <3.6 hr. Multiwavelength observations with Fermi-LAT, Swift, and the Tuorla Observatory revealed a correlated high GeV flux state and no significant optical counterpart to the flare, with a spectral energy distribution where the gamma-ray luminosity exceeds the synchrotron luminosity. When interpreted in the framework of a onezone leptonic model, the observed emission implies a high degree of beaming, with Doppler factor delta > 10, and an electron population with spectral index p < 2.3.