{"created":"2023-06-20T14:36:44.498641+00:00","id":3103,"links":{},"metadata":{"_buckets":{"deposit":"8e00e442-b633-4019-8d57-94bd3d84dbb9"},"_deposit":{"created_by":1,"id":"3103","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3103"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003103","sets":["1887:1891","9:789:806:808"]},"author_link":["11417","11424","11425","11430","11419","11428","11426","11427","11418","11415","11421","11429","11414","11413","11422","11420","11423","11416"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"184","bibliographicPageStart":"181","bibliographicVolumeNumber":"JAXA-SP-17-009E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料"},{"bibliographic_title":"JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life","bibliographic_titleLang":"en"}]}]},"item_5_description_14":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）","attribute_value_mlt":[{"subitem_description":"第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京","subitem_description_type":"Other"}]},"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 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We present the relation between stellar mass and star formation rate (SFR) of a sample of infrared (IR)-bright dust-obscured galaxies (DOGs) that are defined by (i - brackets 22 brackets)(sub AB) greater than 7.0 and flux density at 22 micrometers greater than 3.8 mJy. Combining the Sloan Digital Sky Survey (SDSS), TwoMicron All Sky Survey (TWOMASS), Wide-field Infrared Survey Explorer (WISE), Infrared Astronomical Satellite (IRAS), and AKARI catalogs, we selected 7 IR-bright DOG at Z(sub spec) is greater than 0 and less than 1. We estimated their stellar mass and SFR based on a spectral energy distribution fitting technique, and compared them with main sequence of star-forming galaxies at z is greater than 0 and less than 2 and local ULIRGs. As a result, we found that most of IR-bright DOGs lie significantly above the main sequence of star-forming galaxies at similar redshifts. We conclude that the majority of IRAS- and/or AKARI-detected IR-bright DOGs are starburst galaxies.","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: AA1730026029","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-17-009E","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":"台湾中央研究院天文及天文物理研究所 : 愛媛大学宇宙進化研究センター"},{"subitem_text_value":"愛媛大学宇宙進化研究センター"},{"subitem_text_value":"台湾中央研究院天文及天文物理研究所"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) : 総合研究大学院大学(SOKENDAI)"},{"subitem_text_value":"東北大学天文学教室"},{"subitem_text_value":"国立清華大学"},{"subitem_text_value":"国立天文台ハワイ観測所 : 総合研究大学院大学(SOKENDAI)"},{"subitem_text_value":"台湾中央研究院天文及天文物理研究所"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) : 総合研究大学院大学(SOKENDAI)"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan : Research Center for Space and Cosmic Evolution, Ehime University"},{"subitem_text_language":"en","subitem_text_value":"Research Center for Space and Cosmic Evolution, Ehime University"},{"subitem_text_language":"en","subitem_text_value":"Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) : The Graduate University for Advanced Studies (SOKENDAI)"},{"subitem_text_language":"en","subitem_text_value":"Astronomical Institute, Tohoku University"},{"subitem_text_language":"en","subitem_text_value":"National Tsing Hua University"},{"subitem_text_language":"en","subitem_text_value":"Subaru Telescope, National Astronomical Observatory of Japan : The Graduate University for Advanced Studies (SOKENDAI)"},{"subitem_text_language":"en","subitem_text_value":"Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) : The Graduate University for Advanced Studies (SOKENDAI)"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"鳥羽, 儀樹"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"長尾, 透"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Wang, Wei-Hao"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松原, 英雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"秋山, 正幸"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"後藤, 友嗣"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小山, 佑世"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"大山, 陽一"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"山村, 一誠"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Toba, Yoshiki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nagao, Toru","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Wang, Wei-Hao","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsuhara, Hideo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Akiyama, Masayuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Goto, Tomotsugu","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Koyama, Yusei","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Oyama, Yoichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yamamura, Issei","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":"AA1730026029.pdf","filesize":[{"value":"260.5 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730026029.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3103/files/AA1730026029.pdf"},"version_id":"cb1a1674-0932-4af4-ae8d-a4a139362116"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"catalogs","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"galaxies: active","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"galaxies: star formation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"infrared: galaxies","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":"Where do infrared-bright dust-obscured galaxies lie on the star formation rate-stellar mass plane?","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Where do infrared-bright dust-obscured galaxies lie on the star formation rate-stellar mass plane?","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["808","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2018-05-16"},"publish_date":"2018-05-16","publish_status":"0","recid":"3103","relation_version_is_last":true,"title":["Where do infrared-bright dust-obscured galaxies lie on the star formation rate-stellar mass plane?"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:09:35.093645+00:00"}