CALET GBM Observations of Gamma-ray Bursts and Gravitational Wave Sources

dc.contributor.authorYamaoka, Kazutaka
dc.contributor.authorCannady, Nicholas
dc.contributor.authorCALET collaboration
dc.date.accessioned2023-10-20T12:26:53Z
dc.date.available2023-10-20T12:26:53Z
dc.date.issued2018-08-03
dc.description35th International Cosmic Ray Conference – ICRC2017; Bexco, Busan, Korea; 10-20 July, 2017en
dc.description.abstractThe CALET Gamma-ray Burst Monitor (CGBM) is secondary scientific instrument of the Calorimetric Electron Telescope (CALET) mission on the International Space Station (ISS). The primary instrument Calorimeter (CAL) is capable of detecting gamma-ray bursts (GRBs) in the GeV-TeV range, and the CGBM was attached to complement CAL gamma-ray observations in the keV-MeV range. The CGBM consists of 2 Hard X-ray Monitors (HXMs) and one Soft Gamma-ray Monitor (SGM), utilizing different scintillators LaBr3 (Ce) and BGO respectively. The CGBM covers a broadband energy range of 7 keV - 20 MeV with a wide field of view (FOV). Since the launch on August 19, 2015, the CGBM has been sucessfully operated on the ISS for about 1.5 years, and detecting about 50 GRBs (roughly 20% short GRBs among them) per year as expected from pre-launch estimation. The CALET also concluded memolandam of understanding (MOU) with LIGO/Virgo collaboration, and we are searching for hard X-ray and gamma-ray counterparts for gravitational wave (GW) sources. In this paper, we will report on CGBM in-orbit operation, performance and observations of GRBs and GW sources.en
dc.description.sponsorshipThis work is partly supported by Grant-in-Aid (24684015 KY) from the Ministry of Education, Culture, Sports, Science, and Technology (MEXT).en
dc.description.urihttps://pos.sissa.it/301/614/en
dc.format.extent8 pagesen
dc.genreconference papers and proceedingsen
dc.identifierdoi:10.13016/m28duy-vwnk
dc.identifier.citationYamaoka, Kazutaka, and on behalf of the CALET Collaboration. “CALET GBM Observations of Gamma-Ray Bursts and Gravitational Wave Sources.” In Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017), 301:614. SISSA Medialab, 2018. https://doi.org/10.22323/1.301.0614.en
dc.identifier.urihttps://doi.org/10.22323/1.301.0614
dc.identifier.urihttp://hdl.handle.net/11603/30299
dc.language.isoenen
dc.publisherProceedings of Scienceen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Physics Department
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)*
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleCALET GBM Observations of Gamma-ray Bursts and Gravitational Wave Sourcesen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955en

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