CALET upper limits on GeV-energy gamma-ray burst emission

dc.contributor.authorCannady, Nicholas
dc.contributor.authorHams, Thomas
dc.contributor.authorKrizmanic, John F.
dc.contributor.authorSakai, Kenichi
dc.contributor.authorCALET Collaboration
dc.contributor.authoret al
dc.date.accessioned2019-10-23T14:52:21Z
dc.date.available2019-10-23T14:52:21Z
dc.date.issued2019-07-24
dc.descriptionCALET Collaboration Authors: O. Adriani, Y. Akaike, K. Asano, Y. Asaoka, E. Berti, G. Bigongiari, W. R. Binns, M. Bongi, P. Brogi, A. Bruno, J. H. Buckley, N. Cannady, G. Castellini, C. Checchia, M. L. Cherry, G. Collazuol, K. Ebisawa, A. W. Ficklin, H. Fuke, S. Gonzi, T. G. Guzik, T. Hams, K. Hibino, M. Ichimura, K. Ioka, W. Ishizaki, M. H. Israel, K. Kasahara, J. Kataoka, R. Kataoka, Y. Katayose, C. Kato, N. Kawanaka, Y. Kawakubo, K. Kobayashi, K. Kohri, H. S. Krawczynski, J. F. Krizmanic, P. Maestro, P. S. Marrocchesi, A. M. Messineo, J.W. Mitchell, S. Miyake, A. A. Moiseev, M. Mori, N. Mori, H. M. Motz, K. Munakata, S. Nakahira, J. Nishimura, G. A. de Nolfo, S. Okuno, J. F. Ormes, N. Ospina, S. Ozawa, L. Pacini, P. Papini, B. F. Rauch, S. B. Ricciarini, K. Sakai, T. Sakamoto, M. Sasaki, Y. Shimizu, A. Shiomi, P. Spillantini, F. Stolzi, S. Sugita, A. Sulaj, M. Takita, T. Tamura, T. Terasawa, S. Torii, Y. Tsunesada, Y. Uchihori, E. Vannuccini, J. P. Wefel, K. Yamaoka, S. Yanagita, A. Yoshida, K. Yoshida, and W. V. Zober
dc.description36th International Cosmic Ray Conference -ICRC2019- July 24th - August 1st, 2019, Madison, WI, U.S.A.en
dc.description.abstractThe CALorimetric Electron Telescope (CALET) was deployed on the International Space Station in October 2015 and has accumulated over three years of continuous data to date. The calorimeter (CAL) is sensitive to gamma rays with energies above 1 GeV, and the response has been characterized up to hundreds of GeV. In this work we investigate counterpart GeV-energy emission to gamma-ray bursts observed by the CALET Gamma-ray Burst Monitor and the Swift and FermiGBM missions. The methodologies for the event search and the setting of upper limits in the case of non-detection are presented, along with results from the first three years of CALET operations, covering over 100 GRBs.en
dc.description.urihttps://pos.sissa.it/358/557/pdfen
dc.format.extent8 pagesen
dc.genrejournal articlesen
dc.identifierdoi:10.13016/m2xoda-nkkv
dc.identifier.citation“CALET Upper Limits on GeV-energy Gamma-Ray Burst Emission,” N. Cannady for the CALET Collaboration, Proceedings of Science: 36th International Cosmic Ray Conference , (Madison, WI), 557 (2019). https://doi.org/10.22323/1.358.0557en
dc.identifier.urihttp://hdl.handle.net/11603/15960
dc.identifier.urihttps://doi.org/10.22323/1.358.0557
dc.language.isoenen
dc.publisherProceedings of Science
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/*
dc.subjectCALorimetric Electron Telescopeen
dc.subjectInternational Space Stationen
dc.subjectgamma raysen
dc.subjectGeV-energy emissionen
dc.subjectCALET Gamma-ray Burst Monitoren
dc.titleCALET upper limits on GeV-energy gamma-ray burst emissionen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955

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