{"created":"2023-06-20T14:36:47.039197+00:00","id":3140,"links":{},"metadata":{"_buckets":{"deposit":"1eb038fc-74ef-4600-9ecc-2892ad07ce83"},"_deposit":{"created_by":1,"id":"3140","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3140"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003140","sets":["1887:1891","9:789:806:808"]},"author_link":["11851","11852","11850","11857","11856","11855","11854","11849","11853"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"340","bibliographicPageStart":"337","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":"Star formation rate (SFR) is important to quantify for galaxies because it provides a method for reconstructing the cosmic history of star formation in the universe. H is frequently utilized in SFR studies, however, this hydrogen recombination line is strongly affected by interstellar dust extinction. For a sample of 23 galaxies, we report Br alpha/H alpha and H alpha/H beta measurements and found that for most of our sample, the traditional Balmer decrement, H alpha/H beta, unexpectedly gives higher A(sub V) than when Br alpha/H alpha is used when we adopt the Calzetti extinction law. In addition, galaxies with the highest specific star formation rate (SSFR) on average have higher A(sub V)(Br alpha/H alpha) than A(sub V)(H alpha/H beta). However, we do not find a clear trend of the line ratios against L(sub IR) or IR/UV.","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: AA1730026066","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":"Universite de Lyon : Universite Claude Bernard Lyon 1 : Ens de Lyon : The National Center for Scientific Research (CNRS) : Centre de Recherche Astrophysique de Lyon (CRAL) : Institute for Astronomy, University of Hawai'i at Manoa"},{"subitem_text_value":"Universite de Lyon : Universite Claude Bernard Lyon 1 : Ens de Lyon : The National Center for Scientific Research (CNRS) : Centre de Recherche Astrophysique de Lyon (CRAL)"},{"subitem_text_value":"University of California, Los Angeles"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)"},{"subitem_text_value":"University of California, Los Angeles"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Universite de Lyon : Universite Claude Bernard Lyon 1 : Ens de Lyon : The National Center for Scientific Research (CNRS) : Centre de Recherche Astrophysique de Lyon (CRAL) : Institute for Astronomy, University of Hawai'i at Manoa"},{"subitem_text_language":"en","subitem_text_value":"Universite de Lyon : Universite Claude Bernard Lyon 1 : Ens de Lyon : The National Center for Scientific Research (CNRS) : Centre de Recherche Astrophysique de Lyon (CRAL)"},{"subitem_text_language":"en","subitem_text_value":"University of California, Los Angeles"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)"},{"subitem_text_language":"en","subitem_text_value":"University of California, Los Angeles"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Payne, Anna V."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"稲見, 華恵"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Malkan, Matthew A."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松原, 英雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Payne, Anna V.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Inami, Hanae","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Malkan, Matthew A.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsuhara, Hideo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Sakai, Shoko","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":"AA1730026066.pdf","filesize":[{"value":"889.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730026066.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3140/files/AA1730026066.pdf"},"version_id":"7659201f-f253-4190-8204-f2670901e05b"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"interstellar dust extinction","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"star formation rate","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"luminous infrared galaxy","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":"Analyzing Hydrogen Recombination Lines in the Infrared and Optical to Determine Extinction and SFRs of Dusty Infrared Galaxies","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Analyzing Hydrogen Recombination Lines in the Infrared and Optical to Determine Extinction and SFRs of Dusty Infrared Galaxies","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["808","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2018-05-18"},"publish_date":"2018-05-18","publish_status":"0","recid":"3140","relation_version_is_last":true,"title":["Analyzing Hydrogen Recombination Lines in the Infrared and Optical to Determine Extinction and SFRs of Dusty Infrared Galaxies"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:08:40.538740+00:00"}