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Cited by 200

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

GRB110721A: AN EXTREME PEAK ENERGY AND SIGNATURES OF THE PHOTOSPHERE

Open access
Axelsson, M., Baldini, L., Barbiellini, G., Baring, M. G., Bellazzini, R., Bregeon, J., Brigida, M., Bruel, P., Buehler, R., Caliandro, G. A., Cameron, R. A., Caraveo, P. A., Cecchi, C., Chaves, R. C. G., Chekhtman, A., Chiang, J., Claus, R., Conrad, J., Cutini, S., D'Ammando, F., de Palma, F., Dermer, C. D., do Couto e Silva, E., Drell, P. S., Favuzzi, C., Fegan, S. J., Ferrara, E. C., Focke, W. B., Fukazawa, Y., Fusco, P., Gargano, F., Gasparrini, D., Gehrels, N., Germani, S., Giglietto, N., Giroletti, M., Godfrey, G., Guiriec, S., Hadasch, D., Hanabata, Y., Hayashida, M., Hou, X., Iyyani, S., Jackson, M. S., Kocevski, D., Kuss, M., Larsson, J., Larsson, S., Longo, F., Loparco, F., Lundman, C., Mazziotta, M. N., McEnery, J. E., Mizuno, T., Monzani, M. E., Moretti, E., Morselli, A., Murgia, S., Nuss, E., Nymark, T., Ohno, M., Omodei, N., Pesce-Rollins, M., Piron, F., Pivato, G., Racusin, J. L., Rainò, S., Razzano, M., Razzaque, S., Reimer, A., Roth, M., Ryde, F., Sanchez, D. A., Sgrò, C., Siskind, E. J., Spandre, G., Spinelli, P., Stamatikos, M., Tibaldo, L., Tinivella, M., Usher, T. L., Vandenbroucke, J., Vasileiou, V., Vianello, G., Vitale, V., Waite, A. P., Winer, B. L., Wood, K. S., Burgess, J. M., Bhat, P. N., Bissaldi, E., Briggs, M. S., Connaughton, V., Fishman, G., Fitzpatrick, G., Foley, S., Gruber, D., Kippen, R. M., Kouveliotou, C., Jenke, P., McBreen, S., McGlynn, S., Meegan, C., Paciesas, W. S., Pelassa, V., Preece, R., Tierney, D., von Kienlin, A., Wilson-Hodge, C., Xiong, S., Pe'er, A.·2012·The Astrophysical Journal

Abstract

GRB110721A was observed by the Fermi Gamma-ray Space Telescope using its two instruments, the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM). The burst consisted of one major emission episode which lasted for ∼24.5 s (in the GBM) and had a peak flux of (5.7 ± 0.2) × 10 −5 erg s −1 cm −2 . The time-resolved emission spectrum is best modeled with a combination of a Band function and a blackbody spectrum. The peak energy of the Band component was initially 15 ± 2 MeV, which is the highest value ever detected in a GRB. This measurement was made possible by combining GBM/BGO data with LAT Low Energy events to achieve continuous 10–100 MeV coverage. The peak energy later decreased as a power law in time with an index of −1.89 ± 0.10. The temperature of the blackbody component also decreased, starting from ∼80 keV, and the decay showed a significant break after ∼2 s. The spectrum provides strong constraints on the standard synchrotron model, indicating that alternative mechanisms may give rise to the emission at these energies.

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Authors
Axelsson, M., Baldini, L., Barbiellini, G., Baring, M. G., Bellazzini, R., Bregeon, J., Brigida, M., Bruel, P., Buehler, R., Caliandro, G. A., Cameron, R. A., Caraveo, P. A., Cecchi, C., Chaves, R. C. G., Chekhtman, A., Chiang, J., Claus, R., Conrad, J., Cutini, S., D'Ammando, F., de Palma, F., Dermer, C. D., do Couto e Silva, E., Drell, P. S., Favuzzi, C., Fegan, S. J., Ferrara, E. C., Focke, W. B., Fukazawa, Y., Fusco, P., Gargano, F., Gasparrini, D., Gehrels, N., Germani, S., Giglietto, N., Giroletti, M., Godfrey, G., Guiriec, S., Hadasch, D., Hanabata, Y., Hayashida, M., Hou, X., Iyyani, S., Jackson, M. S., Kocevski, D., Kuss, M., Larsson, J., Larsson, S., Longo, F., Loparco, F., Lundman, C., Mazziotta, M. N., McEnery, J. E., Mizuno, T., Monzani, M. E., Moretti, E., Morselli, A., Murgia, S., Nuss, E., Nymark, T., Ohno, M., Omodei, N., Pesce-Rollins, M., Piron, F., Pivato, G., Racusin, J. L., Rainò, S., Razzano, M., Razzaque, S., Reimer, A., Roth, M., Ryde, F., Sanchez, D. A., Sgrò, C., Siskind, E. J., Spandre, G., Spinelli, P., Stamatikos, M., Tibaldo, L., Tinivella, M., Usher, T. L., Vandenbroucke, J., Vasileiou, V., Vianello, G., Vitale, V., Waite, A. P., Winer, B. L., Wood, K. S., Burgess, J. M., Bhat, P. N., Bissaldi, E., Briggs, M. S., Connaughton, V., Fishman, G., Fitzpatrick, G., Foley, S., Gruber, D., Kippen, R. M., Kouveliotou, C., Jenke, P., McBreen, S., McGlynn, S., Meegan, C., Paciesas, W. S., Pelassa, V., Preece, R., Tierney, D., von Kienlin, A., Wilson-Hodge, C., Xiong, S., & Pe'er, A.
Venue
The Astrophysical Journal
Published
2012-09-17
Volume
757
Issue
2
Pages
L31
ISSN
  • 2041-8205 (ISSN-L)
  • 2041-8213
OpenAlex
W2143752374
Cited by
200
References
1
FWCI
11.87
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: GRB110721A: AN EXTREME PEAK ENERGY AND SIGNATURES OF THE PHOTOSPHERE. https://app.cochat.ai/papers/10.1088/2041-8205/757/2/l31
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Axelsson, M., Baldini, L., Barbiellini, G., Baring, M. G., Bellazzini, R., Bregeon, J., Brigida, M., Bruel, P., Buehler, R., Caliandro, G. A., Cameron, R. A., Caraveo, P. A., Cecchi, C., Chaves, R. C. G., Chekhtman, A., Chiang, J., Claus, R., Conrad, J., Cutini, S., . . . Pe'er, A. (2012). GRB110721A: AN EXTREME PEAK ENERGY AND SIGNATURES OF THE PHOTOSPHERE. The Astrophysical Journal. https://doi.org/10.1088/2041-8205/757/2/l31

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.