{"created":"2023-06-20T14:38:29.326440+00:00","id":5062,"links":{},"metadata":{"_buckets":{"deposit":"71fc6e72-4baa-4402-b59a-c55bd3d28fce"},"_deposit":{"created_by":1,"id":"5062","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5062"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005062","sets":["1887:1891","9:789:936:948"]},"author_link":["23711","23706","23708","23709","23715","23714","23707","23713","23710","23712"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"335","bibliographicPageStart":"334","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 results from observations of three ultraluminous infrared galaxies(ULIRGs) with Suzaku and XMM-Newton. Their optical emission lines are classified as seyfert 2 and extinction-corrected [OIII]lambda5007 line luminosities are (3.2 - 61) x 10 (sup 43) erg s(sup -1), which are in the range for quasars. Their X-ray spectra are explained by a combination of unabsorbed and absorbed power-law components. Fe Kalpha lines are not detected. The absorption-corrected 2-10 keV luminosities L(sub (2 - 10 keV)) are in the range of (3.3 - 24) x 10(sup 42) erg s(sup -1). These results indicate that these objects are Compton-thin AGNs with Seyfert class luminosity. We compare the far infrared (FIR) luminosities L(sub FIR) with the bolometric luminosities of the AGNs and find that the contribution of AGNs to L(sub FIR) is at most a few tens of percent.","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: AA0064574130","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":"愛媛大学"},{"subitem_text_value":"愛媛大学"},{"subitem_text_value":"大阪大学"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"},{"subitem_text_value":"愛媛大学"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Ehime University"},{"subitem_text_language":"en","subitem_text_value":"Ehime University"},{"subitem_text_language":"en","subitem_text_value":"Osaka University"},{"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":"Ehime University"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"平田, 義孝"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"寺島, 雄一"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"穴吹, 直久"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中川, 貴雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"粟木, 久光"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hirata, Yoshitaka","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Terashima, Yuichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Anabuki, Naohisa","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakagawa, Takao","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Awaki, Hisamitsu","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":"64574130.pdf","filesize":[{"value":"199.0 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574130.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5062/files/64574130.pdf"},"version_id":"6982fb47-e80b-4353-9bad-e4de162f3129"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"ULIRG, active galactic nuclei, starburst galaxy","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 AGN Power in Type 2 ULIRGs with a High [OIII] Luminosity Observed by Suzaku and XMM-Newton","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The AGN Power in Type 2 ULIRGs with a High [OIII] Luminosity Observed by Suzaku and XMM-Newton","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":"5062","relation_version_is_last":true,"title":["The AGN Power in Type 2 ULIRGs with a High [OIII] Luminosity Observed by Suzaku and XMM-Newton"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:24:25.209560+00:00"}