{"created":"2023-06-20T14:36:39.760231+00:00","id":3008,"links":{},"metadata":{"_buckets":{"deposit":"790d6830-fcd1-4b49-b56e-5c6261c08f96"},"_deposit":{"created_by":1,"id":"3008","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3008"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003008","sets":["1887:1891","9:789:806:807"]},"author_link":["10467","10463","10459","10462","10469","10464","10471","10472","10457","10466","10468","10460","10458","10465","10470","10461"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"139","bibliographicPageStart":"137","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 the results of our star-forming galaxy survey of distant clusters of galaxies using Subaru (H ) and AKARI (MIR). By comparing the H and MIR data, we revealed that dust-obscured star-forming galaxies are most preferentially located in the cluster outskirts at z approximately 1. We propose to extend this H - and IR-based environmental study to higher redshifts, but a problem so far is that the existing MIR-FIR surveys always suffer from their limited depths. We can overcome this problems with the wide-field mid-infrared (MIR) camera on-board SPICA (5′FoV), which will allow us an efficient, and extremely deep MIR survey of distant clusters. In particular, the expected high sensitivity of SPICA at 20-40 μm regime promotes us to extend IR galaxy survey out to z = 2-4 (i.e. the “peak epoch” of galaxy evolution) based on their rest-frame 8 μm feature. We provide a quick overview of our recent progress with the MAHALO-Subaru collaboration, and then discuss how significantly SPICA can improve our understanding of the environmental effects on galaxy evolution in the early universe.","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: AA1730027031","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":"国立天文台"},{"subitem_text_value":"国立天文台"},{"subitem_text_value":"東京大学"},{"subitem_text_value":"国立天文台"},{"subitem_text_value":"国立天文台ハワイ観測所"},{"subitem_text_value":"総合研究大学院大学(SOKENDAI)"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)"}]},"item_5_text_7":{"attribute_name":"著者所属(英)","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"The University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"Subaru Telescope, National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"The Graduate University for Advanced Studies (SOKENDAI)"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"小山, 佑世"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"児玉, 忠恭"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"林, 将央"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"但木, 謙一"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"田中, 壱"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"嶋川, 里澄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松原, 英雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"和田, 武彦"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Koyama, Yusei","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kodama, Tadayuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hayashi, Masao","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tadaki, Kenichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tanaka, Ichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Shimakawa, Rhythm","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsuhara, Hideo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Wada, Takehiko","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":"AA1730027031.pdf","filesize":[{"value":"410.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027031.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3008/files/AA1730027031.pdf"},"version_id":"7214f3cc-5f9e-4720-ab9e-ef9514bab4df"}]},"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":"SPICA Distant Cluster Survey: Unveiling the Dust-Obscured Star Formation Triggered by Young Cluster Environments","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"SPICA Distant Cluster Survey: Unveiling the Dust-Obscured Star Formation Triggered by Young Cluster Environments","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":"3008","relation_version_is_last":true,"title":["SPICA Distant Cluster Survey: Unveiling the Dust-Obscured Star Formation Triggered by Young Cluster Environments"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:12:06.885751+00:00"}