The 2010 Very High Energy Γ-ray Flare & 10 Years of Multi-wavelength Observations of M 87

  title={The 2010 Very High Energy Γ-ray Flare & 10 Years of Multi-wavelength Observations of M 87},
  author={F. A.S. and A A.G. and G. A.Faggionia. and A. Beulah and Y. B. and J. Bandovic and B. B.T.P. and K. B. and E. B.A. and C. Bhaskar and P. Brunet and F. Bessis and T. Balamugesh and I. B and S. C.T. and M. C.H. and C P.M. and A. Coello and C R.C.G. and C A.C. and G. C.B{\"a}umlera. and J. Crawford and M. Daliri and D M.K. and D I.D. and B. Dr. and D H.J. and W. D. and D L.O’C. and G. D.V.Ablashia. and K. Dinunath and J. Deregnaucourt and K. Elango and P. Elsworth and L. F.Juarez and C. F.H.P. and S. Forestier and F. F.E. and F M.V. and A. Fazeli and G. Fiorentino and M. Ebrahimi and G Y.A. and H. GaudalupeEspitia and L. G. and D. G.KogaM. and B. Geramizaeh and G J.F. and P. G.R. and S. H.E. and H J.D. and D. H.CatherineW.SkinnerPh. and M. H.E. and G. H.U. and H J.A. and A. H.W.L. and W. H.M. and P. H.G. and A. J.HurtmannsM. and O. CraigB.ClarkD. and C. J.O. and M. Jasmineniketha and I. J and K. Ullrich M.A. and K. Kalaiselvan and U. K. and S. Karpagavalli and D. K.TomitaM. and B. KhalidM.Chraibi and W. K. and T. K. and . K and R. Kashif and H. L.G.H. and G. L.Rudolfa. and D. L.S.WondolowskiM. and T. L.S. and A. L.G. and V. Maximov and A. M.R.I. and J. M.VanniprProf.Dr. and D. M.ArakawaM. and N. M.StoffelsR. and M. Marconi and Mo Therese Hannah M.C. and R. Mukundan and E. M. and N C.L. and M.. and D. N.MiuraM. and N. Nalini and B. Nguyen and J. N. and Netravathi S.J. and {\'E}. and B. Otterbein and M. O and I. O and M. Pranali and G. P.Kesternicha. and P P.-O. and A. Q and M. R.F. and R S.M. and A. Rekha and O. R.D. and R. and F. R. and J. R.L. and B. Rajith and R C.B. and V. S and S D.A. and A. S.BordneM. and R. Sreejith and S F.M. and U. S and S. Soula and F. Souai and S J.L. and G. S.Fujisakia. and Ł. S and C. S. and K. Shahana and I. Secron and R. T.R. and M. T.S. and K. Vishnudatha and C... and G. V.Sturma. and S. Vishnukumar and M. Villemain and M. Weber and R. Winkler and A. W.H. and M. Zahariah and A. Zirnea and Z A.A. and P. Abdulla and E. Changyong and P. Chantelat and D. E.EwenCameronM. and P. M.D. and R. O and S. P.},
The giant radio galaxy M 87 with its proximity (16 Mpc), famous jet, and very massive black hole ((3 − 6) × 109M ) provides a unique opportunity to investigate the origin of very high energy (VHE; E>100 GeV) γ-ray emission generated in relativistic outflows and the surroundings of super-massive black holes. M 87 has been established as a VHE γ-ray emitter since 2006. The VHE γ-ray emission displays strong variability on timescales as short as a day. In this paper, results from a joint VHE… CONTINUE READING


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