The first pulse of the extremely bright GRB 130427a: A test lab for synchrotron shocks

R. Preece; J. Michael Burgess; A. Von Kienlin; P. N. Bhat; M. S. Briggs; D. Byrne; V. Chaplin; W. Cleveland; A. C. Collazzi; V. Connaughton; A. Diekmann; G. Fitzpatrick; S. Foley; M. Gibby; M. Giles; A. Goldstein; J. Greiner; D. Gruber; P. Jenke; R. M. Kippen; C. Kouveliotou; S. McBreen; C. Meegan; W. S. Paciesas; V. Pelassa; D. Tierney; A. J. Van Der Horst; C. Wilson-Hodge; S. Xiong; G. Younes; H. F. Yu; M. Ackermann; M. Ajello; M. Axelsson; L. Baldini; G. Barbiellini; M. G. Baring; D. Bastieri; R. Bellazzini; E. Bissaldi; E. Bonamente; J. Bregeon; M. Brigida; P. Bruel; R. Buehler; S. Buson; G. A. Caliandro; R. A. Cameron; P. A. Caraveo; C. Cecchi; E. Charles; A. Chekhtman; J. Chiang; G. Chiaro; S. Ciprini; R. Claus; J. Cohen-Tanugi; L. R. Cominsky; J. Conrad; F. D'Ammando; A. De Angelis; F. De Palma; C. D. Dermer; R. Desiante; S. W. Digel; L. Di Venere; P. S. Drell; A. Drlica-Wagner; C. Favuzzi; A. Franckowiak; Y. Fukazawa; P. Fusco; F. Gargano; N. Gehrels; S. Germani; N. Giglietto; F. Giordano; M. Giroletti; G. Godfrey; J. Granot; I. A. Grenier; S. Guiriec; D. Hadasch; Y. Hanabata; A. K. Harding; M. Hayashida; S. Iyyani; T. Jogler; G. Jóannesson; T. Kawano; J. Knödlseder; D. Kocevski; M. Kuss; J. Lande; J. Larsson; S. Larsson; L. Latronico; F. Longo; F. Loparco; M. N. Lovellette; P. Lubrano; M. Mayer; M. N. Mazziotta; P. F. Michelson; T. Mizuno; M. E. Monzani; E. Moretti; A. Morselli; S. Murgia; R. Nemmen; E. Nuss; T. Nymark; M. Ohno; T. Ohsugi; A. Okumura; N. Omodei; D. Orienti; D. Paneque; J. S. Perkins; M. Pesce-Rollins; F. Piron; G. Pivato; T. A. Porter; J. L. Racusin; S. Rainò; R. Rando; M. Razzano; S. Razzaque; A. Reimer; O. Reimer; S. Ritz; M. Roth; F. Ryde; A. Sartori; H. Scargle; A. Schulz; C. Sgrò; E. J. Siskind; G. Spandre; P. Spinelli; D. J. Suson; H. Tajima; H. Takahashi; J. G. Thayer; J. B. Thayer; L. Tibaldo; M. Tinivella; D. F. Torres; G. Tosti; E. Troja; T. L. Usher; J. Vandenbroucke; V. Vasileiou; G. Vianello; V. Vitale; M. Werner; B. L. Winer; K. S. Wood; S. Zhu

doi:10.1126/science.1242302

The first pulse of the extremely bright GRB 130427a: A test lab for synchrotron shocks

R. Preece
, J. Michael Burgess
, A. Von Kienlin
, P. N. Bhat
, M. S. Briggs
, D. Byrne
, V. Chaplin
, W. Cleveland
, A. C. Collazzi
, V. Connaughton
, A. Diekmann
, G. Fitzpatrick
, S. Foley
, M. Gibby
, M. Giles
, A. Goldstein
, J. Greiner
, D. Gruber
, P. Jenke
, R. M. Kippen

C. Kouveliotou, S. McBreen, C. Meegan, W. S. Paciesas, V. Pelassa, D. Tierney, A. J. Van Der Horst, C. Wilson-Hodge, S. Xiong, G. Younes, H. F. Yu, M. Ackermann, M. Ajello, M. Axelsson, L. Baldini, G. Barbiellini, M. G. Baring, D. Bastieri, R. Bellazzini, E. Bissaldi, E. Bonamente, J. Bregeon, M. Brigida, P. Bruel, R. Buehler, S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, C. Cecchi, E. Charles, A. Chekhtman, J. Chiang, G. Chiaro, S. Ciprini, R. Claus, J. Cohen-Tanugi, L. R. Cominsky, J. Conrad, F. D'Ammando, A. De Angelis, F. De Palma, C. D. Dermer, R. Desiante, S. W. Digel, L. Di Venere, P. S. Drell, A. Drlica-Wagner, C. Favuzzi, A. Franckowiak, Y. Fukazawa, P. Fusco, F. Gargano, N. Gehrels, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, G. Godfrey, J. Granot, I. A. Grenier, S. Guiriec, D. Hadasch, Y. Hanabata, A. K. Harding, M. Hayashida, S. Iyyani, T. Jogler, G. Jóannesson, T. Kawano, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, J. Larsson, S. Larsson, L. Latronico, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, M. Mayer, M. N. Mazziotta, P. F. Michelson, T. Mizuno, M. E. Monzani, E. Moretti, A. Morselli, S. Murgia, R. Nemmen, E. Nuss, T. Nymark, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, D. Orienti, D. Paneque, J. S. Perkins, M. Pesce-Rollins, F. Piron, G. Pivato, T. A. Porter, J. L. Racusin, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, S. Ritz, M. Roth, F. Ryde, A. Sartori, H. Scargle, A. Schulz, C. Sgrò, E. J. Siskind, G. Spandre, P. Spinelli, D. J. Suson, H. Tajima, H. Takahashi, J. G. Thayer, J. B. Thayer, L. Tibaldo, M. Tinivella, D. F. Torres, G. Tosti, E. Troja, T. L. Usher, J. Vandenbroucke, V. Vasileiou, G. Vianello, V. Vitale, M. Werner, B. L. Winer, K. S. Wood, S. Zhu

University of Alabama in Huntsville
Center for Space Plasma and Aeronomic Research
Max Planck Institut für Extraterrestrische Physik
University College Dublin
Universities Space Research Association
NASA Marshall Space Flight Center
NASA Postdoctoral Program Fellow
Jacobs Technology Inc.
MST-8, Los Alamos National Laboratory
University of Amsterdam
c/o DESY
University of California, Space Sciences Laboratory
Stockholm University
Oskar Klein Centre
KTH Royal Institute of Technology
University of Pisa
INFN Sezione di Trieste
University of Trieste
Rice University
INFN
University of Padova
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Medical University of Innsbruck
INFN Sezione di Perugia
University of Perugia
Politecnico di Bari
INFN Sezione di Bari
IEEE
Kavli Institute for Particle Astrophysics and Cosmology
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
George Mason University
Naval Research Laboratory
Science and Research Directorate
Osservatorio Astronomico di Roma
Laboratoire Univers et Particules de Montpellier
Sonoma State University
Royal Swedish Academy of Sciences
INAF Istituto di Radioastronomia
and Physics University of Udine
Hiroshima University
NASA Goddard Space Flight Center
The Open University of Israel
Université Paris-Diderot
Kyoto University
University of Iceland
IRAP/CNRS
Observatoire Midi-Pyrénées
INFN Sezione di Torino
INFN Roma Tor Vergata
ISAS/JAXA
Nagoya University
Max-Planck-Institut für Physik
Biochemical and Environmental Engineering
University of California at Santa Cruz
University of Johannesburg
University of Washington
NASA Ames Research Center
NYCB Real-Time Computing Inc.
Purdue University Northwest
Pompeu Fabra University (UPF)
University of Maryland
Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
University of Rome “Tor Vergata”
The Ohio State University

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

71 Citations (Scopus)

Résumé

Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 seconds is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of the peak energy from the onset of the pulse, consistent with models of internal synchrotron shock pulses. However, a strongly correlated power-law behavior is observed between the luminosity and the spectral peak energy that is inconsistent with curvature effects arising in the relativistic outflow. It is difficult for any of the existing models to account for all of the observed spectral and temporal behaviors simultaneously.

langue originale	Anglais
Pages (de - à)	51-54
Nombre de pages	4
journal	Science
Volume	343
Numéro de publication	6166
Les DOIs	https://doi.org/10.1126/science.1242302
état	Publié - 1 janv. 2014

Accès au document

10.1126/science.1242302

Contient cette citation

Preece, R., Burgess, J. M., Von Kienlin, A., Bhat, P. N., Briggs, M. S., Byrne, D., Chaplin, V., Cleveland, W., Collazzi, A. C., Connaughton, V., Diekmann, A., Fitzpatrick, G., Foley, S., Gibby, M., Giles, M., Goldstein, A., Greiner, J., Gruber, D., Jenke, P., ... Zhu, S. (2014). The first pulse of the extremely bright GRB 130427a: A test lab for synchrotron shocks. Science, 343(6166), 51-54. https://doi.org/10.1126/science.1242302

@article{a49c9eba88a444edb6ebd3ee3f786796,

title = "The first pulse of the extremely bright GRB 130427a: A test lab for synchrotron shocks",

abstract = "Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 seconds is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of the peak energy from the onset of the pulse, consistent with models of internal synchrotron shock pulses. However, a strongly correlated power-law behavior is observed between the luminosity and the spectral peak energy that is inconsistent with curvature effects arising in the relativistic outflow. It is difficult for any of the existing models to account for all of the observed spectral and temporal behaviors simultaneously.",

author = "R. Preece and Burgess, \{J. Michael\} and \{Von Kienlin\}, A. and Bhat, \{P. N.\} and Briggs, \{M. S.\} and D. Byrne and V. Chaplin and W. Cleveland and Collazzi, \{A. C.\} and V. Connaughton and A. Diekmann and G. Fitzpatrick and S. Foley and M. Gibby and M. Giles and A. Goldstein and J. Greiner and D. Gruber and P. Jenke and Kippen, \{R. M.\} and C. Kouveliotou and S. McBreen and C. Meegan and Paciesas, \{W. S.\} and V. Pelassa and D. Tierney and \{Van Der Horst\}, \{A. J.\} and C. Wilson-Hodge and S. Xiong and G. Younes and Yu, \{H. F.\} and M. Ackermann and M. Ajello and M. Axelsson and L. Baldini and G. Barbiellini and Baring, \{M. G.\} and D. Bastieri and R. Bellazzini and E. Bissaldi and E. Bonamente and J. Bregeon and M. Brigida and P. Bruel and R. Buehler and S. Buson and Caliandro, \{G. A.\} and Cameron, \{R. A.\} and Caraveo, \{P. A.\} and C. Cecchi and E. Charles and A. Chekhtman and J. Chiang and G. Chiaro and S. Ciprini and R. Claus and J. Cohen-Tanugi and Cominsky, \{L. R.\} and J. Conrad and F. D'Ammando and \{De Angelis\}, A. and \{De Palma\}, F. and Dermer, \{C. D.\} and R. Desiante and Digel, \{S. W.\} and \{Di Venere\}, L. and Drell, \{P. S.\} and A. Drlica-Wagner and C. Favuzzi and A. Franckowiak and Y. Fukazawa and P. Fusco and F. Gargano and N. Gehrels and S. Germani and N. Giglietto and F. Giordano and M. Giroletti and G. Godfrey and J. Granot and Grenier, \{I. A.\} and S. Guiriec and D. Hadasch and Y. Hanabata and Harding, \{A. K.\} and M. Hayashida and S. Iyyani and T. Jogler and G. J{\'o}annesson and T. Kawano and J. Kn{\"o}dlseder and D. Kocevski and M. Kuss and J. Lande and J. Larsson and S. Larsson and L. Latronico and F. Longo and F. Loparco and Lovellette, \{M. N.\} and P. Lubrano and M. Mayer and Mazziotta, \{M. N.\} and Michelson, \{P. F.\} and T. Mizuno and Monzani, \{M. E.\} and E. Moretti and A. Morselli and S. Murgia and R. Nemmen and E. Nuss and T. Nymark and M. Ohno and T. Ohsugi and A. Okumura and N. Omodei and D. Orienti and D. Paneque and Perkins, \{J. S.\} and M. Pesce-Rollins and F. Piron and G. Pivato and Porter, \{T. A.\} and Racusin, \{J. L.\} and S. Rain{\`o} and R. Rando and M. Razzano and S. Razzaque and A. Reimer and O. Reimer and S. Ritz and M. Roth and F. Ryde and A. Sartori and H. Scargle and A. Schulz and C. Sgr{\`o} and Siskind, \{E. J.\} and G. Spandre and P. Spinelli and Suson, \{D. J.\} and H. Tajima and H. Takahashi and Thayer, \{J. G.\} and Thayer, \{J. B.\} and L. Tibaldo and M. Tinivella and Torres, \{D. F.\} and G. Tosti and E. Troja and Usher, \{T. L.\} and J. Vandenbroucke and V. Vasileiou and G. Vianello and V. Vitale and M. Werner and Winer, \{B. L.\} and Wood, \{K. S.\} and S. Zhu",

year = "2014",

month = jan,

day = "1",

doi = "10.1126/science.1242302",

language = "English",

volume = "343",

pages = "51--54",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "6166",

}

Preece, R, Burgess, JM, Von Kienlin, A, Bhat, PN, Briggs, MS, Byrne, D, Chaplin, V, Cleveland, W, Collazzi, AC, Connaughton, V, Diekmann, A, Fitzpatrick, G, Foley, S, Gibby, M, Giles, M, Goldstein, A, Greiner, J, Gruber, D, Jenke, P, Kippen, RM, Kouveliotou, C, McBreen, S, Meegan, C, Paciesas, WS, Pelassa, V, Tierney, D, Van Der Horst, AJ, Wilson-Hodge, C, Xiong, S, Younes, G, Yu, HF, Ackermann, M, Ajello, M, Axelsson, M, Baldini, L, Barbiellini, G, Baring, MG, Bastieri, D, Bellazzini, R, Bissaldi, E, Bonamente, E, Bregeon, J, Brigida, M, Bruel, P, Buehler, R, Buson, S, Caliandro, GA, Cameron, RA, Caraveo, PA, Cecchi, C, Charles, E, Chekhtman, A, Chiang, J, Chiaro, G, Ciprini, S, Claus, R, Cohen-Tanugi, J, Cominsky, LR, Conrad, J, D'Ammando, F, De Angelis, A, De Palma, F, Dermer, CD, Desiante, R, Digel, SW, Di Venere, L, Drell, PS, Drlica-Wagner, A, Favuzzi, C, Franckowiak, A, Fukazawa, Y, Fusco, P, Gargano, F, Gehrels, N, Germani, S, Giglietto, N, Giordano, F, Giroletti, M, Godfrey, G, Granot, J, Grenier, IA, Guiriec, S, Hadasch, D, Hanabata, Y, Harding, AK, Hayashida, M, Iyyani, S, Jogler, T, Jóannesson, G, Kawano, T, Knödlseder, J, Kocevski, D, Kuss, M, Lande, J, Larsson, J, Larsson, S, Latronico, L, Longo, F, Loparco, F, Lovellette, MN, Lubrano, P, Mayer, M, Mazziotta, MN, Michelson, PF, Mizuno, T, Monzani, ME, Moretti, E, Morselli, A, Murgia, S, Nemmen, R, Nuss, E, Nymark, T, Ohno, M, Ohsugi, T, Okumura, A, Omodei, N, Orienti, D, Paneque, D, Perkins, JS, Pesce-Rollins, M, Piron, F, Pivato, G, Porter, TA, Racusin, JL, Rainò, S, Rando, R, Razzano, M, Razzaque, S, Reimer, A, Reimer, O, Ritz, S, Roth, M, Ryde, F, Sartori, A, Scargle, H, Schulz, A, Sgrò, C, Siskind, EJ, Spandre, G, Spinelli, P, Suson, DJ, Tajima, H, Takahashi, H, Thayer, JG, Thayer, JB, Tibaldo, L, Tinivella, M, Torres, DF, Tosti, G, Troja, E, Usher, TL, Vandenbroucke, J, Vasileiou, V, Vianello, G, Vitale, V, Werner, M, Winer, BL, Wood, KS & Zhu, S 2014, 'The first pulse of the extremely bright GRB 130427a: A test lab for synchrotron shocks', Science, VOL. 343, Numéro 6166, p. 51-54. https://doi.org/10.1126/science.1242302

TY - JOUR

T1 - The first pulse of the extremely bright GRB 130427a

T2 - A test lab for synchrotron shocks

AU - Preece, R.

AU - Burgess, J. Michael

AU - Von Kienlin, A.

AU - Bhat, P. N.

AU - Briggs, M. S.

AU - Byrne, D.

AU - Chaplin, V.

AU - Cleveland, W.

AU - Collazzi, A. C.

AU - Connaughton, V.

AU - Diekmann, A.

AU - Fitzpatrick, G.

AU - Foley, S.

AU - Gibby, M.

AU - Giles, M.

AU - Goldstein, A.

AU - Greiner, J.

AU - Gruber, D.

AU - Jenke, P.

AU - Kippen, R. M.

AU - Kouveliotou, C.

AU - McBreen, S.

AU - Meegan, C.

AU - Paciesas, W. S.

AU - Pelassa, V.

AU - Tierney, D.

AU - Van Der Horst, A. J.

AU - Wilson-Hodge, C.

AU - Xiong, S.

AU - Younes, G.

AU - Yu, H. F.

AU - Ackermann, M.

AU - Ajello, M.

AU - Axelsson, M.

AU - Baldini, L.

AU - Barbiellini, G.

AU - Baring, M. G.

AU - Bastieri, D.

AU - Bellazzini, R.

AU - Bissaldi, E.

AU - Bonamente, E.

AU - Bregeon, J.

AU - Brigida, M.

AU - Bruel, P.

AU - Buehler, R.

AU - Buson, S.

AU - Caliandro, G. A.

AU - Cameron, R. A.

AU - Caraveo, P. A.

AU - Cecchi, C.

AU - Charles, E.

AU - Chekhtman, A.

AU - Chiang, J.

AU - Chiaro, G.

AU - Ciprini, S.

AU - Claus, R.

AU - Cohen-Tanugi, J.

AU - Cominsky, L. R.

AU - Conrad, J.

AU - D'Ammando, F.

AU - De Angelis, A.

AU - De Palma, F.

AU - Dermer, C. D.

AU - Desiante, R.

AU - Digel, S. W.

AU - Di Venere, L.

AU - Drell, P. S.

AU - Drlica-Wagner, A.

AU - Favuzzi, C.

AU - Franckowiak, A.

AU - Fukazawa, Y.

AU - Fusco, P.

AU - Gargano, F.

AU - Gehrels, N.

AU - Germani, S.

AU - Giglietto, N.

AU - Giordano, F.

AU - Giroletti, M.

AU - Godfrey, G.

AU - Granot, J.

AU - Grenier, I. A.

AU - Guiriec, S.

AU - Hadasch, D.

AU - Hanabata, Y.

AU - Harding, A. K.

AU - Hayashida, M.

AU - Iyyani, S.

AU - Jogler, T.

AU - Jóannesson, G.

AU - Kawano, T.

AU - Knödlseder, J.

AU - Kocevski, D.

AU - Kuss, M.

AU - Lande, J.

AU - Larsson, J.

AU - Larsson, S.

AU - Latronico, L.

AU - Longo, F.

AU - Loparco, F.

AU - Lovellette, M. N.

AU - Lubrano, P.

AU - Mayer, M.

AU - Mazziotta, M. N.

AU - Michelson, P. F.

AU - Mizuno, T.

AU - Monzani, M. E.

AU - Moretti, E.

AU - Morselli, A.

AU - Murgia, S.

AU - Nemmen, R.

AU - Nuss, E.

AU - Nymark, T.

AU - Ohno, M.

AU - Ohsugi, T.

AU - Okumura, A.

AU - Omodei, N.

AU - Orienti, D.

AU - Paneque, D.

AU - Perkins, J. S.

AU - Pesce-Rollins, M.

AU - Piron, F.

AU - Pivato, G.

AU - Porter, T. A.

AU - Racusin, J. L.

AU - Rainò, S.

AU - Rando, R.

AU - Razzano, M.

AU - Razzaque, S.

AU - Reimer, A.

AU - Reimer, O.

AU - Ritz, S.

AU - Roth, M.

AU - Ryde, F.

AU - Sartori, A.

AU - Scargle, H.

AU - Schulz, A.

AU - Sgrò, C.

AU - Siskind, E. J.

AU - Spandre, G.

AU - Spinelli, P.

AU - Suson, D. J.

AU - Tajima, H.

AU - Takahashi, H.

AU - Thayer, J. G.

AU - Thayer, J. B.

AU - Tibaldo, L.

AU - Tinivella, M.

AU - Torres, D. F.

AU - Tosti, G.

AU - Troja, E.

AU - Usher, T. L.

AU - Vandenbroucke, J.

AU - Vasileiou, V.

AU - Vianello, G.

AU - Vitale, V.

AU - Werner, M.

AU - Winer, B. L.

AU - Wood, K. S.

AU - Zhu, S.

PY - 2014/1/1

Y1 - 2014/1/1

N2 - Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 seconds is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of the peak energy from the onset of the pulse, consistent with models of internal synchrotron shock pulses. However, a strongly correlated power-law behavior is observed between the luminosity and the spectral peak energy that is inconsistent with curvature effects arising in the relativistic outflow. It is difficult for any of the existing models to account for all of the observed spectral and temporal behaviors simultaneously.

AB - Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 seconds is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of the peak energy from the onset of the pulse, consistent with models of internal synchrotron shock pulses. However, a strongly correlated power-law behavior is observed between the luminosity and the spectral peak energy that is inconsistent with curvature effects arising in the relativistic outflow. It is difficult for any of the existing models to account for all of the observed spectral and temporal behaviors simultaneously.

U2 - 10.1126/science.1242302

DO - 10.1126/science.1242302

M3 - Article

AN - SCOPUS:84896700289

SN - 0036-8075

VL - 343

SP - 51

EP - 54

JO - Science

JF - Science

IS - 6166

ER -

The first pulse of the extremely bright GRB 130427a: A test lab for synchrotron shocks

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