{"created":"2023-06-20T14:38:40.078872+00:00","id":5256,"links":{},"metadata":{"_buckets":{"deposit":"a20aed75-b072-455f-9e7e-90583274a33b"},"_deposit":{"created_by":1,"id":"5256","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5256"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005256","sets":["1887:1891","9:789:956:959"]},"author_link":["25367","25366"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2009-02-27","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"85","bibliographicPageStart":"82","bibliographicVolumeNumber":"JAXA-SP-08-014E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料"},{"bibliographic_title":"JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop","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":"Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008)","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Thanks to its superior sensitivity, energy resolution and wide energy coverage, MAXI is expected to open a new window in the study of Galactic X-ray transients. In this paper, I selected the following eight areas in which MAXI is expected to make significant contributions to our understanding of the Galactic transient sources: (1) Detailed study of bright transients, (2) Monitor spectral variations, (3) Accretion disk spectral variation, (4) Faint transients, (5) Transient search in crowded region, (6) Supergiant fast X-ray transients, (7) Ultra-soft transients, and (8) Extragalactic stellar transients. For each area, I explain what MAXI will be able to do, in contrast to previous observations by all sky monitors.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064306017","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-08-014E","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)"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"海老沢, 研"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ebisawa, Ken","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":"64306017.pdf","filesize":[{"value":"190.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64306017.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5256/files/64306017.pdf"},"version_id":"23941eee-d047-41f9-8621-fc0de1aef474"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Galactic transients : black holes - neutron stars - white dwarfs","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":"Galactic transient sources with MAXI","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Galactic transient sources with MAXI","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["959","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"5256","relation_version_is_last":true,"title":["Galactic transient sources with MAXI"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:19:42.458434+00:00"}