{"created":"2023-06-20T14:36:42.478605+00:00","id":3063,"links":{},"metadata":{"_buckets":{"deposit":"70e5ab98-b638-45ad-9a00-d8f69e82a164"},"_deposit":{"created_by":1,"id":"3063","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3063"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003063","sets":["1887:1891","9:789:806:807"]},"author_link":["10987","10989","10994","10993","10990","10991","10988","10992","10986"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"391","bibliographicPageStart":"389","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":"About 400 hours of the Herschel Space Observatory’s time has been used by the Open Time Key Programme “TNOs are Cool: A survey of the trans-Neptunian region” to obtain PACS (70, 100 and 160 μm) and SPIRE (250, 350 and 500 μm) photometry of 132 objects representing different dynamical classes (resonant, classical, scattered disk and detached TNOs as well as Centaurs), including 25 binary systems. As leftovers of the formation of the Solar System TNOs and their physical properties provide constraints to the models of formation and evolution of the various dynamical classes. SPICA is going to be a main leap forward on the way that Herschel started in the characterization of TNOs by determining size, albedo and other surface properties. SPICA is going to cover the mid- to far-IR wavelengths where TNO SEDs peaks (currently covered with Herschel/PACS and Spitzer/MIPS together). While Herschel could observe about 10% of the known TNOs, with its increased sensitivity SPICA would be able to detect most (probably all) currently known TNOs. The observing strategy we used in our key program will also be relevant for SPICA observations to beat the confusion noise.","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: AA1730027086","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_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Konkoly Observatory"},{"subitem_text_language":"en","subitem_text_value":"Max Planck Institute for Extraterrestrial Physics"},{"subitem_text_language":"en","subitem_text_value":"Max Planck Institute for Extraterrestrial Physics"},{"subitem_text_language":"en","subitem_text_value":"Konkoly Observatory"},{"subitem_text_language":"en","subitem_text_value":"Instituto de Astrofisica de Andalucia"},{"subitem_text_language":"en","subitem_text_value":"Observatorie de Paris"},{"subitem_text_language":"en","subitem_text_value":"Steward Observatory"},{"subitem_text_language":"en","subitem_text_value":"German Aerospace Center (DLR)"},{"subitem_text_language":"en","subitem_text_value":"Netherlands Institute for Space Research (SRON)"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Kiss, Cs.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Muller, Th. G.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Vilenius, E.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Pal, A.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SantosSanz, P.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Lellouch, E.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Stansberry, J.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Mommert, M.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Muller, M.","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":"AA1730027086.pdf","filesize":[{"value":"274.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027086.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3063/files/AA1730027086.pdf"},"version_id":"cba96590-6747-45c5-907a-48a5f377e69e"}]},"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 trans-Neptunian Objects after Herschel: What Could SPICA Add to the Understanding of the Kuiper Belt?","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The trans-Neptunian Objects after Herschel: What Could SPICA Add to the Understanding of the Kuiper Belt?","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["807","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2018-05-07"},"publish_date":"2018-05-07","publish_status":"0","recid":"3063","relation_version_is_last":true,"title":["The trans-Neptunian Objects after Herschel: What Could SPICA Add to the Understanding of the Kuiper Belt?"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:10:32.114442+00:00"}