{"created":"2023-06-20T14:38:30.321584+00:00","id":5085,"links":{},"metadata":{"_buckets":{"deposit":"53a1cf04-e3de-4156-9275-bb1ac657c3ce"},"_deposit":{"created_by":1,"id":"5085","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5085"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005085","sets":["1887:1891","9:789:936:948"]},"author_link":["23936","23935","23934"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"395","bibliographicPageStart":"394","bibliographicVolumeNumber":"JAXA-SP-09-008E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料:"},{"bibliographic_title":"JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H","bibliographic_titleLang":"en"}]}]},"item_5_description_15":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）（英）","attribute_value_mlt":[{"subitem_description":"The 3rd Suzaku international Conference \"Energetic Cosmos : from Suzaku to ASTRO-H\" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We report on the observations of the high energy (> 100MeV) emission from gamma-ray bursts (GRBs), including the first short GRB with GeV photons 081024B and the featureless long GRB 090217 by the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope. The high energy photons observed by the LAT from GRB 081024B is delayed with respect to the trigger time of Gamma-Ray Burst Monitor (GBM) onborad Fermi and they extend after the low energy emission of GBM as well as other LAT GRBs. Conversrsely, we found no special feature from GRB 090217: there is no delay for high energy photons, no distinct spectral component. These interesting features and differences for high energy emission observed by the LAT could help to investigate the emission mechanism of GRBs at high energy. Some of these LAT GRBs are also detected by the Suzaku Wide-band All-sky Monitor (WAM) simultaneously. The largest effective area of the WAM from 300 keV to 5000 keV could be of a good assistance for the Fermi data.","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064574153","subitem_description_type":"Other"}]},"item_5_description_33":{"attribute_name":"レポート番号","attribute_value_mlt":[{"subitem_description":"レポート番号: JAXA-SP-09-008E","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency (JAXA)"}]},"item_5_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1349-113X","subitem_source_identifier_type":"ISSN"}]},"item_5_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11984031","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)"},{"subitem_text_language":"en","subitem_text_value":"Fermi LAT/GBM collaboration"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"大野, 雅功"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ohno, Masanori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Fermi, LAT/GBM collaboration","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-01-16"}],"displaytype":"detail","filename":"64574153.pdf","filesize":[{"value":"178.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574153.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5085/files/64574153.pdf"},"version_id":"68a9dc1a-e116-4a58-8114-d6a936e08aad"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"The Energetic Cosmos, from Suzaku to Astro-H: proceedings","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"The Fermi and Suzaku/WAM Observations of GRB 081024B and GRB 090217","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The Fermi and Suzaku/WAM Observations of GRB 081024B and GRB 090217","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["948","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"5085","relation_version_is_last":true,"title":["The Fermi and Suzaku/WAM Observations of GRB 081024B and GRB 090217"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:23:41.588492+00:00"}