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dc.contributor.authorUlyanov , Alexei
dc.contributor.authorHanlon , Lorraine
dc.contributor.authorMcBreen , Sheila
dc.contributor.authorFoley , Suzanne
dc.date.accessioned2017-02-09T08:02:12Z
dc.date.available2017-02-09T08:02:12Z
dc.date.issued2013
dc.identifier.citationActa Polytechnica. 2013, vol. 53, no. 1.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/67018
dc.description.abstractGRIPS is a proposed gamma-ray (200 keV to 80 MeV) astronomy mission, which incorporates a pair-creation and Compton scattering telescope, along with X-ray and infrared telescopes. It will carry out a sensitive all-sky scanning survey, investigating phenomena such as gamma-ray bursts, blazars and core collapse supernovae. The main telescope is composed of a Si strip detector surroundedby a calorimeter with a fast scintillator material. We present the initial results of a study which considers the potential use of silicon photomultipliers in conjunction with the scintillator in the GRIPS calorimeter module.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/ap/article/view/1716
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectsilicon photomultiplieren
dc.subjectGRIPSen
dc.subjectgamma-rayen
dc.subjectfutureen
dc.titleStudy of Silicon Photomultipliers for the GRIPS Calorimeter Module
dc.typearticleen
dc.date.updated2017-02-09T08:02:12Z
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License