{"created":"2023-06-20T14:38:23.930478+00:00","id":4955,"links":{},"metadata":{"_buckets":{"deposit":"0697aa66-4852-4ac3-a4d0-5d2d7ec8b75b"},"_deposit":{"created_by":1,"id":"4955","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"4955"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00004955","sets":["1887:1891","9:789:936:948"]},"author_link":["22835","22836"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"65","bibliographicPageStart":"62","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":"The X-ray Imaging Spectrometer (XIS) onboard Suzaku is characterized by three major advantages: low and stable background, good response in low energies, and superior energy resolution. Utilizing these advantages, the XIS has attacked a number of supernova remnants (SNRs). The first advantageous point allows us to detect Fe, Mn, and Cr lines from young SNRs, while the second one reveals C and N lines from evolved SNRs. The third one enables us to detect line broadening due to either the Doppler effect, the thermal Doppler effect, or the ionization-timescale variation of several plasma components. For largely extended evolved SNRs, by combining the three advantages, spatially-resolved spectral analyses show us their metal distributions in unprecedented details. I will review such a Suzaku view of thermal SNRs","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: AA0064574023","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_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Code 662, NASA Goddard Space Flight Center"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"勝田, 哲"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Katsuda, Satoru","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":"64574023.pdf","filesize":[{"value":"364.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574023.pdf","url":"https://jaxa.repo.nii.ac.jp/record/4955/files/64574023.pdf"},"version_id":"0bb38068-da34-4a27-af38-40a14fb9ee67"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"ISM: abundances - supernova remnants:","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":"Suzaku View of Thermal Supernova Remnants","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Suzaku View of Thermal Supernova Remnants","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":"4955","relation_version_is_last":true,"title":["Suzaku View of Thermal Supernova Remnants"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:27:54.535881+00:00"}