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_US
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_US
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_US
dc.description.urihttps://pos.sissa.it/301/614/en_US
dc.format.extent8 pagesen_US
dc.genreconference papers and proceedingsen_US
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_US
dc.identifier.urihttps://doi.org/10.22323/1.301.0614
dc.identifier.urihttp://hdl.handle.net/11603/30299
dc.language.isoen_USen_US
dc.publisherProceedings of Scienceen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Physics Department
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_US
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleCALET GBM Observations of Gamma-ray Bursts and Gravitational Wave Sourcesen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955en_US

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
ICRC2017_614.pdf
Size:
370.04 KB
Format:
Adobe Portable Document Format
Description:

License bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
license.txt
Size:
2.56 KB
Format:
Item-specific license agreed upon to submission
Description: