Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427A

Ackermann, M.; Ajello, M.; Asano, K.; Atwood, W.~B B.; Axelsson, M.; Baldini, L.; Ballet, J.; Barbiellini, G.; Baring, M.~G G.; Bastieri, D.; Bechtol, K.; Bellazzini, R.; Bissaldi, E.; Bonamente, E.; Bregeon, J.; Brigida, M.; Bruel, P.; Buehler, R.; Burgess, J.~M Michael; Buson, S.; Caliandro, G.~A A.; Cameron, R.~A A.; Caraveo, P.~A A.; Cecchi, C.; Chaplin, V.; Charles, E.; Chekhtman, A.; Cheung, C.~C C.; Chiang, J.; Chiaro, G.; Ciprini, S.; Claus, R.; Cleveland, W.; Cohen-Tanugi, J.; Collazzi, A.; Cominsky, L.~R R.; Connaughton, V.; Conrad, J.; Cutini, S.; D'Ammando, F.; D’Ammando, F.; de Angelis, A.; DeKlotz, M.; de Palma, F.; Dermer, C.~D D.; Desiante, R.; Diekmann, A.; Di Venere, L.; Drell, P.~S S.; Drlica-Wagner, A.; Favuzzi, C.; Fegan, S.~J J.; Ferrara, E.~C C.; Finke, J.; Fitzpatrick, G.; Focke, W.~B B.; Franckowiak, A.; Fukazawa, Y.; Funk, S.; Fusco, P.; Gargano, F.; Gehrels, N.; Germani, S.; Gibby, M.; Giglietto, N.; Giles, M.; Giordano, F.; Giroletti, M.; Godfrey, G.; Granot, J.; Grenier, I.~A A.; Grove, J.~E E.; Gruber, D.; Guiriec, S.; Hadasch, D.; Hanabata, Y.; Harding, A.~K K.; Hayashida, M.; Hays, E.; Horan, D.; Hughes, R.~E E.; Inoue, Y.; Jogler, T.; Jóhannesson, G.; Johnson, W.~N N.; Kawano, T.; Knödlseder, J.; Kocevski, D.; Kuss, M.; Lande, J.; Larsson, S.; Latronico, L.; Longo, F.; Loparco, F.; Lovellette, M.~N N.; Lubrano, P.; Mayer, M.; Mazziotta, M.~N N.; McEnery, J.~E E.; Michelson, P.~F F.; Mizuno, T.; Moiseev, A.~A A.; Monzani, M.~E E.; Moretti, E.; Morselli, A.; Moskalenko, I. V.; Murgia, S.; Nemmen, R.; Nuss, E.; Ohno, M.; Ohsugi, T.; Okumura, A.; Omodei, N.; Orienti, M.; Paneque, D.; Pelassa, V.; Perkins, J.~S S.; Pesce-Rollins, M.; Petrosian, V.; Piron, F.; Pivato, G.; Porter, T.~A A.; Racusin, J.~L L.; Rainò, S.; Rando, R.; Razzano, M.; Razzaque, S.; Reimer, A.; Reimer, O.; Ritz, S.; Roth, M.; Ryde, F.; Sartori, A.; Parkinson, P.~M.~S M. Saz; Scargle, J.~D D.; Schulz, A.; Sgrò, C.; Siskind, E.~J J.; Sonbas, E.; Spandre, G.; Spinelli, P.; Tajima, H.; Takahashi, H.; Thayer, J.~G G.; Thayer, J.~B B.; Thompson, D.~J J.; Tibaldo, L.; Tinivella, M.; Torres, D.~F F.; Tosti, G.; Troja, E.; Usher, T.~L L.; Vandenbroucke, J.; Vasileiou, V.; Vianello, G.; Vitale, V.; Winer, B.~L L.; Wood, K.~S S.; Yamazaki, R.; Younes, G.; Yu, H.-F.; Zhu, S.~J J.; Bhat, P.~N N.; Briggs, M.~S S.; Byrne, D.; Foley, S.; Goldstein, A.; Jenke, P.; Kippen, R.~M M.; Kouveliotou, C.; McBreen, S.; Meegan, C.; Paciesas, W.~S S.; Preece, R.; Rau, A.; Tierney, D.; van der Horst, A.~J J.; von Kienlin, A.; Wilson-Hodge, C.; Xiong, S.; Cusumano, G.; La Parola, V.; Parola, La; Cummings, J.~R R.

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Marco Ajello
Ackermann et al., 2013

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American Association for the Advancement of Science, Science, 6166(343), p. 42-47

DOI: 10.1126/science.1242353

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@article{Ackermann2013,
  abstract = {The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature of these unique astrophysical sources. GRB 130427A had the largest fluence, highest-energy photon (95 GeV), longest γ-ray duration (20 hours), and one of the largest isotropic energy releases ever observed from a GRB. Temporal and spectral analyses of GRB 130427A challenge the widely accepted model that the nonthermal high-energy emission in the afterglow phase of GRBs is synchrotron emission radiated by electrons accelerated at an external shock.},
  author = {Ackermann, M. and Ajello, M. and Asano, K. and Atwood, W.~B B. and Axelsson, M. and Baldini, L. and Ballet, J. and Barbiellini, G. and Baring, M.~G G. and Bastieri, D. and Bechtol, K. and Bellazzini, R. and Bissaldi, E. and Bonamente, E. and Bregeon, J. and Brigida, M. and Bruel, P. and Buehler, R. and Burgess, J.~M Michael and Buson, S. and Caliandro, G.~A A. and Cameron, R.~A A. and Caraveo, P.~A A. and Cecchi, C. and Chaplin, V. and Charles, E. and Chekhtman, A. and Cheung, C.~C C. and Chiang, J. and Chiaro, G. and Ciprini, S. and Claus, R. and Cleveland, W. and Cohen-Tanugi, J. and Collazzi, A. and Cominsky, L.~R R. and Connaughton, V. and Conrad, J. and Cutini, S. and D'Ammando, F. and D’Ammando, F. and de Angelis, A. and DeKlotz, M. and de Palma, F. and Dermer, C.~D D. and Desiante, R. and Diekmann, A. and Di Venere, L. and Drell, P.~S S. and Drlica-Wagner, A. and Favuzzi, C. and Fegan, S.~J J. and Ferrara, E.~C C. and Finke, J. and Fitzpatrick, G. and Focke, W.~B B. and Franckowiak, A. and Fukazawa, Y. and Funk, S. and Fusco, P. and Gargano, F. and Gehrels, N. and Germani, S. and Gibby, M. and Giglietto, N. and Giles, M. and Giordano, F. and Giroletti, M. and Godfrey, G. and Granot, J. and Grenier, I.~A A. and Grove, J.~E E. and Gruber, D. and Guiriec, S. and Hadasch, D. and Hanabata, Y. and Harding, A.~K K. and Hayashida, M. and Hays, E. and Horan, D. and Hughes, R.~E E. and Inoue, Y. and Jogler, T. and Jóhannesson, G. and Johnson, W.~N N. and Kawano, T. and Knödlseder, J. and Kocevski, D. and Kuss, M. and Lande, J. and Larsson, S. and Latronico, L. and Longo, F. and Loparco, F. and Lovellette, M.~N N. and Lubrano, P. and Mayer, M. and Mazziotta, M.~N N. and McEnery, J.~E E. and Michelson, P.~F F. and Mizuno, T. and Moiseev, A.~A A. and Monzani, M.~E E. and Moretti, E. and Morselli, A. and Moskalenko, I. V. and Murgia, S. and Nemmen, R. and Nuss, E. and Ohno, M. and Ohsugi, T. and Okumura, A. and Omodei, N. and Orienti, M. and Paneque, D. and Pelassa, V. and Perkins, J.~S S. and Pesce-Rollins, M. and Petrosian, V. and Piron, F. and Pivato, G. and Porter, T.~A A. and Racusin, J.~L L. and Rainò, S. and Rando, R. and Razzano, M. and Razzaque, S. and Reimer, A. and Reimer, O. and Ritz, S. and Roth, M. and Ryde, F. and Sartori, A. and Parkinson, P.~M.~S M. Saz and Scargle, J.~D D. and Schulz, A. and Sgrò, C. and Siskind, E.~J J. and Sonbas, E. and Spandre, G. and Spinelli, P. and Tajima, H. and Takahashi, H. and Thayer, J.~G G. and Thayer, J.~B B. and Thompson, D.~J J. and Tibaldo, L. and Tinivella, M. and Torres, D.~F F. and Tosti, G. and Troja, E. and Usher, T.~L L. and Vandenbroucke, J. and Vasileiou, V. and Vianello, G. and Vitale, V. and Winer, B.~L L. and Wood, K.~S S. and Yamazaki, R. and Younes, G. and Yu, H.-F. and Zhu, S.~J J. and Bhat, P.~N N. and Briggs, M.~S S. and Byrne, D. and Foley, S. and Goldstein, A. and Jenke, P. and Kippen, R.~M M. and Kouveliotou, C. and McBreen, S. and Meegan, C. and Paciesas, W.~S S. and Preece, R. and Rau, A. and Tierney, D. and van der Horst, A.~J J. and von Kienlin, A. and Wilson-Hodge, C. and Xiong, S. and Cusumano, G. and La Parola, V. and Parola, La and Cummings, J.~R R.},
  doi = {10.1126/science.1242353},
  journal = {Science},
  month = {nov},
  pages = {42-47},
  title = {Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427A},
  url = {https://oadoi.org/10.1126/science.1242353},
  volume = {343},
  year = {2013}
}

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Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427A

Journal article published in 2013 by M. Ackermann, M. Ajello

, K. Asano, W.~B B. Atwood, M. Axelsson, L. Baldini

, J. Ballet, G. Barbiellini, M.~G G. Baring, D. Bastieri

, K. Bechtol, R. Bellazzini, E. Bissaldi

, E. Bonamente, J. Bregeon and other authors. M. Ackermann, M. Ajello

, K. Asano, W.~B B. Atwood, M. Axelsson, L. Baldini

, J. Ballet, G. Barbiellini, M.~G G. Baring, D. Bastieri

, K. Bechtol, R. Bellazzini, E. Bissaldi

, E. Bonamente, J. Bregeon, M. Brigida, P. Bruel, R. Buehler, J.~M Michael Burgess

, S. Buson, G.~A A. Caliandro, R.~A A. Cameron, P.~A A. Caraveo, C. Cecchi, V. Chaplin, E. Charles, A. Chekhtman, C.~C C. Cheung, J. Chiang, G. Chiaro, S. Ciprini, R. Claus, W. Cleveland, J. Cohen-Tanugi

, A. Collazzi, L.~R R. Cominsky, V. Connaughton, J. Conrad, S. Cutini, F. D'Ammando

, F. D’Ammando, A. de Angelis, M. DeKlotz, F. de Palma, C.~D D. Dermer, R. Desiante, A. Diekmann, L. Di Venere, P.~S S. Drell, A. Drlica-Wagner, C. Favuzzi, S.~J J. Fegan, E.~C C. Ferrara, J. Finke, G. Fitzpatrick, W.~B B. Focke, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, N. Gehrels, S. Germani, M. Gibby, N. Giglietto, M. Giles, F. Giordano, M. Giroletti

, G. Godfrey, J. Granot, I.~A A. Grenier, J.~E E. Grove, D. Gruber, S. Guiriec, D. Hadasch, Y. Hanabata, A.~K K. Harding, M. Hayashida, E. Hays, D. Horan, R.~E E. Hughes, Y. Inoue, T. Jogler, G. Jóhannesson, W.~N N. Johnson, T. Kawano, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, S. Larsson, L. Latronico, F. Longo, F. Loparco, M.~N N. Lovellette, P. Lubrano, M. Mayer, M.~N N. Mazziotta, J.~E E. McEnery, P.~F F. Michelson, T. Mizuno, A.~A A. Moiseev, M.~E E. Monzani, E. Moretti, A. Morselli

, I. V. Moskalenko

, S. Murgia, R. Nemmen, E. Nuss, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei

, M. Orienti

, D. Paneque, V. Pelassa, J.~S S. Perkins, M. Pesce-Rollins, V. Petrosian, F. Piron, G. Pivato, T.~A A. Porter, J.~L L. Racusin, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, S. Ritz, M. Roth, F. Ryde, A. Sartori, P.~M.~S M. Saz Parkinson, J.~D D. Scargle, A. Schulz, C. Sgrò, E.~J J. Siskind, E. Sonbas, G. Spandre, P. Spinelli, H. Tajima, H. Takahashi, J.~G G. Thayer, J.~B B. Thayer, D.~J J. Thompson, L. Tibaldo

, M. Tinivella, D.~F F. Torres, G. Tosti, E. Troja

, T.~L L. Usher, J. Vandenbroucke, V. Vasileiou, G. Vianello, V. Vitale, B.~L L. Winer, K.~S S. Wood, R. Yamazaki, G. Younes, H.-F. Yu, S.~J J. Zhu, P.~N N. Bhat, M.~S S. Briggs, D. Byrne, S. Foley, A. Goldstein, P. Jenke, R.~M M. Kippen, C. Kouveliotou, S. McBreen, C. Meegan, W.~S S. Paciesas, R. Preece

, A. Rau, D. Tierney, A.~J J. van der Horst

, A. von Kienlin, C. Wilson-Hodge, S. Xiong, G. Cusumano, V. La Parola

, La Parola, J.~R R. Cummings

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Abstract

The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature of these unique astrophysical sources. GRB 130427A had the largest fluence, highest-energy photon (95 GeV), longest γ-ray duration (20 hours), and one of the largest isotropic energy releases ever observed from a GRB. Temporal and spectral analyses of GRB 130427A challenge the widely accepted model that the nonthermal high-energy emission in the afterglow phase of GRBs is synchrotron emission radiated by electrons accelerated at an external shock.

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Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427A

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