{"created":"2023-06-20T14:36:41.662124+00:00","id":3045,"links":{},"metadata":{"_buckets":{"deposit":"3f745994-e530-4d05-92b5-98f396d28610"},"_deposit":{"created_by":1,"id":"3045","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3045"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003045","sets":["1887:1891","9:789:806:807"]},"author_link":["10785","10786"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"320","bibliographicPageStart":"317","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 discuss significance of direct imaging observations of extrasolar planets from theoretical points of view. Statistical properties of frequency and correlations of mass, semimajor axis and eccentricity for wide separation (greater than or approximately equal to 30AU) gas giants will determine which is the dominant process for formation of gas giant planets, standard core accretion model or disk instability model. We also point out that direct imaging and spectroscopic observation for ‘habitable’ rocky planets is not completely impossible by SPICA SCI, so that it is worth challenging.","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: AA1730027068","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":"東京工業大学地球生命研究所"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Earth-Life Science Institute, Tokyo Institute of Technology"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"井田, 茂"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ida, Shigeru","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":"AA1730027068.pdf","filesize":[{"value":"411.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027068.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3045/files/AA1730027068.pdf"},"version_id":"7071f74f-f66e-4043-9e0f-64694e38c880"}]},"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":"Wide Separation Planets and Their Implications for Planet Formation Theory","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Wide Separation Planets and Their Implications for Planet Formation Theory","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":"3045","relation_version_is_last":true,"title":["Wide Separation Planets and Their Implications for Planet Formation Theory"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:11:10.333654+00:00"}