{"created":"2023-06-20T15:02:54.628021+00:00","id":31999,"links":{},"metadata":{"_buckets":{"deposit":"94bf0532-a04d-4a4d-a72e-b96d9d997e44"},"_deposit":{"created_by":1,"id":"31999","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"31999"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00031999","sets":["1887:1890","1896:1898:1899:1910"]},"author_link":["406940","406938","406939"],"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1968-03","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1_B","bibliographicPageEnd":"153","bibliographicPageStart":"145","bibliographicVolumeNumber":"4","bibliographic_titles":[{"bibliographic_title":"東京大学宇宙航空研究所報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"1MeV領域におけるγ線を気球で観測した.2個のNaIに鉛をはさんだresponseが非等方的なカウンターを用いてγ線の方向分布を測定した.その結果,観測されたγ線の(34±17)%は銀河γ線の可能性がある.更にホスヴィッチ・カウンターでγ線のエネルギー・スペクトルを測定した.方向分布の測定の結果も考慮して,銀河γ線の上限は(4.3±2.1)×10^<-3>counts/cm^2 sec ster MeVと与えられる.","subitem_description_type":"Abstract"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0125082000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"東京大学宇宙航空研究所"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0563-8100","subitem_source_identifier_type":"ISSN"}]},"item_9_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AN00161914","subitem_source_identifier_type":"NCID"}]},"item_9_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"立教大学理学部物理学教室"},{"subitem_text_value":"立教大学理学部物理学教室"},{"subitem_text_value":"立教大学理学部物理学教室"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"奥平, 清昭"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"平島, 洋"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"山上, 隆正"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-01-24"}],"displaytype":"detail","filename":"SA0125082.pdf","filesize":[{"value":"458.8 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0125082.pdf","url":"https://jaxa.repo.nii.ac.jp/record/31999/files/SA0125082.pdf"},"version_id":"bb06907e-5c83-4b42-804e-33c73560b570"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"1MeV領域の銀河γ線の上限","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"1MeV領域の銀河γ線の上限"}]},"item_type_id":"9","owner":"1","path":["1890","1910"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"31999","relation_version_is_last":true,"title":["1MeV領域の銀河γ線の上限"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:44:06.722662+00:00"}