{"created":"2023-06-20T14:38:24.256182+00:00","id":4960,"links":{},"metadata":{"_buckets":{"deposit":"6a08b829-3d8c-40e6-a14c-ac07a8d570fe"},"_deposit":{"created_by":1,"id":"4960","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"4960"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00004960","sets":["1887:1891","9:789:936:948"]},"author_link":["22883","22879","22875","22876","22869","22873","22877","22872","22881","22867","22874","22882","22870","22884","22871","22868","22878","22880"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"85","bibliographicPageStart":"82","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 present the results from long Suzaku observations of the most X-ray luminous galaxy cluster, RX J1347.5-1145 at z = 0.451. To understand the gas physics of a violent, cluster merger, we study physical properties of the hot (approximately 20 keV) gas clump in the south-east region discovered previously by Sunyaev-Zel'dovich (SZ) effect observations.　With the joint analysis of the Suzaku and Chandra data, we determine the temperature of the hot gas　in the south-east region to be 25.3(sup +6.1)(sub -4.5) (statistical; 90 % confidence level) (sup +6.9)(sub -9.5) (systematic; 90% confidence level) keV, which is in an excellent agreement with the previous joint analysis of the SZ effect in radio and the Chandra X-ray data. This is the first time that the X-ray spectroscopic observations alone have enabled a good measurement of such a high temperature gas component, because of Suzaku's unprecedented sensitivity over the wide X-ray band. These results indicate strongly that RX J1347.5-1145 has undergone a recent, violent merger. The spectral analysis shows that the SE component is consistent with being thermal. Therefore the present result confirms the presence of the hottest thermal gas in the Universe. On the other hand, no significant non-thermal hard X-ray emission is detected and we measure the 3sigma upper limit to the non-thermal flux in the 12-60 keV band, F > 8 x 10(exp -12)erg s(exp -1)cm(exp -2). Combining this limit with the synchrotron flux of a radio mini halo in this cluster, we find a lower limit to the strength of the cluster magnetic field, such that B > 0.007 micro G.","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: AA0064574028","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":"東京理科大学"},{"subitem_text_value":"埼玉大学"},{"subitem_text_value":"東邦大学"},{"subitem_text_value":"東北大学"},{"subitem_text_value":"国立天文台"},{"subitem_text_value":"国立天文台野辺山宇宙電波観測所"},{"subitem_text_value":"東京大学"},{"subitem_text_value":"筑波大学計算科学研究センター"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Tokyo University of Science"},{"subitem_text_language":"en","subitem_text_value":"Saitama University"},{"subitem_text_language":"en","subitem_text_value":"Toho University"},{"subitem_text_language":"en","subitem_text_value":"The University of Texas"},{"subitem_text_language":"en","subitem_text_value":"Tohoku University"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"Nobeyama Radio Observatory, National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"The University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Center for Computational Physics, University of Tsukuba"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"太田, 直美"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"村瀬, 弘一"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"北山, 哲"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小松, 英一郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"服部, 誠"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松尾, 宏"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"大島, 泰"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"須藤, 靖"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"吉川, 耕司"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ota, Naomi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Murase, Kouichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kitayama, Tetsu","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Komatsu, Eiichiro","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hattori, Makoto","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsuo, Hiroshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Oshima, Tai","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Suto, Yasushi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yoshikawa, Koji","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":"64574028.pdf","filesize":[{"value":"268.7 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574028.pdf","url":"https://jaxa.repo.nii.ac.jp/record/4960/files/64574028.pdf"},"version_id":"f4afb19f-0227-4c7f-93d6-448672249d6b"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"galaxies: clusters: individual: RX J1347.5-1145 - galaxies: intergalactic medium - X-rays: galaxies: clusters - cosmology: observations","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":"Extremely Hot Gas in the Most X-ray Luminous Cluster RXJ1347","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Extremely Hot Gas in the Most X-ray Luminous Cluster RXJ1347","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":"4960","relation_version_is_last":true,"title":["Extremely Hot Gas in the Most X-ray Luminous Cluster RXJ1347"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:27:44.665848+00:00"}