{"created":"2023-06-20T14:38:29.711205+00:00","id":5071,"links":{},"metadata":{"_buckets":{"deposit":"1da7b65d-fd10-4440-92ed-9f974195ef05"},"_deposit":{"created_by":1,"id":"5071","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5071"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005071","sets":["1887:1891","9:789:936:948"]},"author_link":["23780","23777","23782","23779","23778","23781","23785","23786","23784","23783"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"366","bibliographicPageStart":"364","bibliographicVolumeNumber":"JAXA-SP-09-008E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料:"},{"bibliographic_title":"JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H","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":"The 3rd Suzaku international Conference \"Energetic Cosmos : from Suzaku to ASTRO-H\" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We calibrated the peak energy-peak luminosity relation of GRBs (so called E(sub p) - L(sup p) ; Yonetoku relation) using 52 events with the redshift z < 1.755 without assuming any cosmological models. The luminosity distances to GRBs are estimated from those of large amount of Type Ia supernovae with z < 1.755. This calibrated E(sub p) - L(sup p) relation can be used as a new cosmic distance ladder toward higher redshifts. We determined the luminosity distances of 36 GRBs in 1.8 < z < 8.3 using the calibrated relation and plotted the likelihood contour in (omega(sub m), omega(sub lamda) plane. We obtained  (Omega(sub m), Omega(sub lamda) = (0.37(sup +0.14)(sub -0.11), 0.63(sup +0.11)(sub -0.14) for a flat universe. We can say that our universe in 1.8 < z < 8.3 is compatible with the cosmological model derived for z 1< 1.8. This suggests that the time variation of the dark energy may be small or zero up to z approximately 8.","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064574139","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-09-008E","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"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency (JAXA)"}]},"item_5_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1349-113X","subitem_source_identifier_type":"ISSN"}]},"item_5_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11984031","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"金沢大学理学部物理学科"},{"subitem_text_value":"金沢大学理学部物理学科"},{"subitem_text_value":"京都大学大学院理学研究科"},{"subitem_text_value":"京都大学大学院理学研究科"},{"subitem_text_value":"名古屋大学理学研究科素粒子宇宙物理学専攻"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Kanazawa University"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Kanazawa University"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics and Astrophysics, Nagoya University"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"米徳, 大輔"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"村上, 敏夫"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"筒井, 亮"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中村, 卓史"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"高橋, 慶太郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yonetoku, Daisuke","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Murakami, Toshio","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tsutsui, Ryo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakamura, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Takahashi, Keitaro","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":"2020-01-16"}],"displaytype":"detail","filename":"64574139.pdf","filesize":[{"value":"569.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574139.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5071/files/64574139.pdf"},"version_id":"d0d20325-f5fe-4f4f-9087-e8b3fbb15ddd"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Gamma-Ray: Bursts - Cosmology: Dark Energy - Distance Ladder","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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 dark energy measurement in the early universe with Gamma-Ray Bursts","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The dark energy measurement in the early universe with Gamma-Ray Bursts","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["948","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"5071","relation_version_is_last":true,"title":["The dark energy measurement in the early universe with Gamma-Ray Bursts"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:24:06.100653+00:00"}