{"created":"2023-06-20T14:36:39.267649+00:00","id":2997,"links":{},"metadata":{"_buckets":{"deposit":"4ef3dce6-2283-4020-91f1-fbf513743552"},"_deposit":{"created_by":1,"id":"2997","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"2997"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00002997","sets":["1887:1891","9:789:806:807"]},"author_link":["10372","10376","10374","10373","10375","10377"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"97","bibliographicPageStart":"95","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":"We present a forecast for detection of high-redshift star-forming galaxies using SPICA-SAFARI and ALMA Band 10-11. We use the outputs of large cosmological simulations of galaxy formation to calculate the fluxes of infrared and far-infrared emission lines ([O III]88.3 μm, [O III] 51.8 μm, [N III]57.2 μm and [C II]158 μm). To this end, we assume empirical relations between the line fluxes and the star formation rate or far-infrared luminoisities. We consider a large survey programme with a 2′× 2′ field-of-view and the limiting flux densities of greater than 21 and greater than 32 μJy (5σ). Our models predicts that there are 604 plus or minus59 galaxies to be detected by such a survey. The number of [C II] emitters with L[C II] less than 10(exp 9)solar luminosity is expected to be 543 plus or minus 52.","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: AA1730027020","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":"東京大学国際高等研究所カブリ数物連携宇宙研究機構"},{"subitem_text_value":"国立天文台 : 総合研究大学院大学(SOKENDAI)"}]},"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":"Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan : The Graduate University for Advanced Studies (SOKENDAI)"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"早津, 夏己"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"吉田, 直紀"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松田, 有一"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hayatsu, Natsuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yoshida, Naoki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsuda, Yuichi","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":"AA1730027020.pdf","filesize":[{"value":"269.2 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027020.pdf","url":"https://jaxa.repo.nii.ac.jp/record/2997/files/AA1730027020.pdf"},"version_id":"ed47efa4-80ce-45df-aa04-58e86a01ec87"}]},"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":"Distribution of IR and Submillimeter Line Emitting Galaxies in Cosmological Simulations","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Distribution of IR and Submillimeter Line Emitting Galaxies in Cosmological Simulations","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":"2997","relation_version_is_last":true,"title":["Distribution of IR and Submillimeter Line Emitting Galaxies in Cosmological Simulations"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:12:23.876327+00:00"}