{"created":"2023-06-20T14:36:39.448544+00:00","id":3001,"links":{},"metadata":{"_buckets":{"deposit":"f9b0728b-a743-48c1-9b81-3a8627c44e27"},"_deposit":{"created_by":1,"id":"3001","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3001"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003001","sets":["1887:1891","9:789:806:807"]},"author_link":["10400","10399"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"112","bibliographicPageStart":"111","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":"I propose to search for dust-free quasars without hot-dust emission at z greater than 6. I plan to perform the deep mid-infrared photometry with Mid-infrared Camera and Spectrometer (MCS). Its high sensitive and continuous-band (5-38 μm) imaging enables us to investigate the contribution not only of the hot dust component (rest frame: 1-3 μm) but also of the warm dust component (rest frame: greater than 3 μm) of quasars at z greater than 6. When the SPICA begins the observation, several hundreds of quasars at z greater than 6 are expected to be discovered by Hyper Suprime-Cam (HSC) which is a gigantic digital still camera for 8.2m Subaru telescope. For these z greater than 6 quasars, we examine the hot-dust abundance by utilizing the spectral energy distributions of rest-frame near-infrared regime. This study is expected to provide us the clue about the origin of the dust torus.","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: AA1730027024","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":"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":"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":"鳥羽, 儀樹"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Toba, Yoshiki","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":"AA1730027024.pdf","filesize":[{"value":"319.8 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027024.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3001/files/AA1730027024.pdf"},"version_id":"0e7b69f1-f5f0-4622-be67-4986cc0a149b"}]},"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":"Search for Dust-free Quasars at z greater than 6 Using SPICA MCS Photometry","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Search for Dust-free Quasars at z greater than 6 Using SPICA MCS Photometry","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":"3001","relation_version_is_last":true,"title":["Search for Dust-free Quasars at z greater than 6 Using SPICA MCS Photometry"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:12:18.331631+00:00"}