{"created":"2023-05-15T14:40:47.461551+00:00","id":55944,"links":{},"metadata":{"_buckets":{"deposit":"90d2f1fd-8154-4ca8-a9da-9ee3f2e8b0d1"},"_deposit":{"created_by":1,"id":"55944","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"55944"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00055944","sets":["7"]},"author_link":["572479","572483","572477","572482","572481","572478","572480","572476"],"item_10004_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2014-10","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"245","bibliographicPageStart":"244","bibliographic_titles":[{"bibliographic_title":"2013 Annual Report of the Research Project with Heavy Ions at NIRS-HIMAC"}]}]},"item_10004_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We have been developing Gamma-Ray Burst (GRB) polarimeter for small tellite. The polarimeter consists of plastic scintillator and inorganic scintillator such as CsI(Tl), GSO(Ce), GYSO(Ce), or GAGG(Ce). To investigate the optimum rganic scintillator, we have compared the characteristics of the spallation for four kinds of scintillator, using 150 MeV proton beam in HIMAC. After irradiation of about 10 krad, we measured the background pulse height spectrum of each scintillator in the cave of lead for three months. As the results, we confirmed that the unting rate of the background for the GAGG scintillator is the lowest of the four after\none month of the irradiation. Then we decided to adopt the GAGG as the sorber of the GRB polarimeter","subitem_description_type":"Abstract"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Gunji, Syuichi"}],"nameIdentifiers":[{"nameIdentifier":"572476","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Nakamori, Nobuyuki"}],"nameIdentifiers":[{"nameIdentifier":"572477","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kitamura, Hisashi"}],"nameIdentifiers":[{"nameIdentifier":"572478","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kodaira, Satoshi"}],"nameIdentifiers":[{"nameIdentifier":"572479","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"郡司 修一","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"572480","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"中森 伸行","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"572481","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"北村 尚","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"572482","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"小平 聡","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"572483","nameIdentifierScheme":"WEKO"}]}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Performance Test of Gamma-ray Burst Polarimeter for Small Satellite (12H308)","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Performance Test of Gamma-ray Burst Polarimeter for Small Satellite (12H308)"}]},"item_type_id":"10004","owner":"1","path":["7"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-18"},"publish_date":"2015-03-18","publish_status":"0","recid":"55944","relation_version_is_last":true,"title":["Performance Test of Gamma-ray Burst Polarimeter for Small Satellite (12H308)"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T22:43:35.636604+00:00"}