{"created":"2023-06-20T14:38:30.016848+00:00","id":5078,"links":{},"metadata":{"_buckets":{"deposit":"0f7dde89-d70c-4922-b9ba-88e69e89ecc9"},"_deposit":{"created_by":1,"id":"5078","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5078"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005078","sets":["1887:1891","9:789:936:948"]},"author_link":["23842","23847","23848","23840","23846","23843","23845","23849","23835","23836","23838","23837","23841","23839","23844"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"381","bibliographicPageStart":"380","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 purpose of this work is to answer the question of \"how have spatial distributions of components in galaxy clusters evolved over the history of the universe?\". It is well known that galaxy clusters consist of dark matter, intergalactic hot gas, and galaxies, and that hot gas has an extended distribution and galaxy components show a morphology-density relation and the Butcher-Oemler effect. However, the origin of these cluster component distributions is still unknown. One simple interpretation is that galaxies have gradually fallen to the cluster centers, with evolution of their color and morphology. If this simple scenario is correct, the relative distributions of galaxies to hot gas should become centrally-concentrated toward lower redshifts. Our exploratory study suggests that galaxies are falling to the cluster center while hot gas is expanding with decreasing redshifts.","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: AA0064574146","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":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"},{"subitem_text_value":"理化学研究所宇宙放射線研究室"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"},{"subitem_text_language":"en","subitem_text_value":"Cosmic Radiation Laboratory, RIKEN"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"稲田, 直久"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"川原田, 円"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小波, さおり"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"三澤, 透"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"太田, 一陽"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"牧島, 一夫"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"高橋, 労太"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Inada, Naohisa","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kawaharada, Madoka","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Konami, Saori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Gandhi, Poshak","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Misawa, Toru","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ota, Kazuaki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Makishima, Kazuo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Takahashi, Rohta","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":"64574146.pdf","filesize":[{"value":"175.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574146.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5078/files/64574146.pdf"},"version_id":"3b0d5d2f-024f-43ec-8c75-984b3e8f00f6"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"galaxies: clusters: general - X-rays: galaxies: clusters","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":"Probing Evolution of Hot Gas and Galaxy Distributions in Galaxy Clusters","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Probing Evolution of Hot Gas and Galaxy Distributions in Galaxy Clusters","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":"5078","relation_version_is_last":true,"title":["Probing Evolution of Hot Gas and Galaxy Distributions in Galaxy Clusters"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:23:53.664387+00:00"}