{"created":"2023-06-20T14:36:40.454939+00:00","id":3022,"links":{},"metadata":{"_buckets":{"deposit":"950e50f5-4106-47b6-947a-3a2249fc9f53"},"_deposit":{"created_by":1,"id":"3022","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3022"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003022","sets":["1887:1891","9:789:806:807"]},"author_link":["10580","10581","10578","10579","10582","10583"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"214","bibliographicPageStart":"211","bibliographicVolumeNumber":"JAXA-SP-17-010E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料"},{"bibliographic_title":"JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe","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":"SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Here we show the results of our ALMA cycle 0 observation toward the nearby type-1 Seyfert nucleus in NGC 1097. We observed some typical dense gas tracers such as HCN (J=4-3) and HCO+ (J=4-3). We find that the HCN (J=4- 3)/HCO+ (J=4-3) and HCN (J=4-3)/CS (J=7-6) integrated intensity ratios are enhanced in AGNs including NGC 1097 compared to nearby starburst galaxies and Galactic star forming regions. Multi-line/transition analysis of HCN and HCO+ emissions reveal that these lines are emitted from dense (10(exp 4.5) less than or equal to nH2 [cm(exp −3)] less than or equal to 10(exp 6) and hot (70 less than or equal to T(sub kin) [K] less than or equal to 550) regions, and that HCN to HCO+ abundance ratio is high (4-20). We introduce a “high-temperature chemistry” to explain the observed properties. Finally, we briefly discuss the possible future studies with ALMA and SPICA on AGN science.","subitem_description_type":"Other"}]},"item_5_description_18":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"形態: カラー図版あり","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Physical characteristics: Original contains color illustrations","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA1730027045","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-17-010E","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(JAXA)"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency (JAXA)"}]},"item_5_source_id_22":{"attribute_name":"ISSNONLINE","attribute_value_mlt":[{"subitem_source_identifier":"2433-2232","subitem_source_identifier_type":"ISSN"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学"},{"subitem_text_value":"東京大学"},{"subitem_text_value":"国立高等専門学校機構呉工業高等専門学校"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"The University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"The University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"National Institute of Technology, Kure College"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"泉, 拓磨"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"河野, 孝太郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"川勝, 望"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Izumi, Takuma","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kohno, Kotaro","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kawakatu, Nozomu","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":"2020-01-15"}],"displaytype":"detail","filename":"AA1730027045.pdf","filesize":[{"value":"653.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027045.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3022/files/AA1730027045.pdf"},"version_id":"271aec1e-d6e4-451e-b0a2-16730d01543a"}]},"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 Synergy with SPICA and ALMA: for a Robust AGN Diagnostic","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The Synergy with SPICA and ALMA: for a Robust AGN Diagnostic","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["807","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2018-05-01"},"publish_date":"2018-05-01","publish_status":"0","recid":"3022","relation_version_is_last":true,"title":["The Synergy with SPICA and ALMA: for a Robust AGN Diagnostic"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:11:48.267980+00:00"}