{"created":"2023-05-15T14:42:36.133597+00:00","id":2937,"links":{},"metadata":{"_buckets":{"deposit":"abe64e76-89cb-4a3f-854c-eb335407d73f"},"_deposit":{"created_by":3,"id":"2937","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"2937"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:00002937","sets":["14:226:227"]},"author_link":["7890"],"control_number":"2937","item_2_biblio_info_12":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2016-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"129","bibliographicPageStart":"123","bibliographicVolumeNumber":"11","bibliographic_titles":[{"bibliographic_title":"京都産業大学総合学術研究所所報"}]}]},"item_2_description_10":{"attribute_name":"抄録(日)","attribute_value_mlt":[{"subitem_description":"本稿では，彗星の近赤外線スペクトルにおいて1μm波長帯で主な輝線を生じるCN分子を取り上げ，その発光モデルの詳細化について検討した結果を報告する。1μm波長帯はこれまでにくわしいサーベイがされておらず，京都産業大学神山天文台に設置された世界屈指の感度を誇る近赤外線高分散分光器WINEREDを用いた未同定分子のサーベイが進行中である。そうした未同定分子（CN分子の同位体を含む）は微弱な輝線を有すると考えられるため，その検出には，主な輝線を発するCN分子の同定と除去が必要となる。そこで，高精度な実験室分光データを元にした彗星CN分子輝線モデルの構築を行った。","subitem_description_type":"Other"}]},"item_2_description_11":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"In this study we discuss about emission lines caused by CN radicals in cometary coma. We have a plan to survey cometary emission lines（including unidentified lines）in 1-micron wavelength region by the high-sensitivity and high-resolution near-infrared spectrometer WINERED equipped with the 1.3m-Araki telescope in Koyama Astronomical Observatory, Kyoto-Sangyo University, Japan. In the target wavelength region（0.9 - 1.3 microns）emission lines from CN radicals are prominent and to be subtracted in order to search for weaker emission lines（isotopologues of CN and other complex molecules）. Accurate emission model for CN in cometary coma has been developed based on the recent laboratory studies and theoretical works.","subitem_description_type":"Other"}]},"item_2_description_15":{"attribute_name":"表示順","attribute_value_mlt":[{"subitem_description":"9","subitem_description_type":"Other"}]},"item_2_description_16":{"attribute_name":"アクセション番号","attribute_value_mlt":[{"subitem_description":"KJ00010262519","subitem_description_type":"Other"}]},"item_2_description_2":{"attribute_name":"ページ属性","attribute_value_mlt":[{"subitem_description":"P","subitem_description_type":"Other"}]},"item_2_description_8":{"attribute_name":"記事種別(日)","attribute_value_mlt":[{"subitem_description":"研究活動報告","subitem_description_type":"Other"}]},"item_2_description_9":{"attribute_name":"記事種別(英)","attribute_value_mlt":[{"subitem_description":"Activity Reports","subitem_description_type":"Other"}]},"item_2_source_id_1":{"attribute_name":"雑誌書誌ID","attribute_value_mlt":[{"subitem_source_identifier":"AA11879037","subitem_source_identifier_type":"NCID"}]},"item_2_source_id_19":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1348-8465","subitem_source_identifier_type":"PISSN"}]},"item_2_text_6":{"attribute_name":"著者所属(日)","attribute_value_mlt":[{"subitem_text_value":"京都産業大学理学部"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"河北, 秀世","creatorNameLang":"ja"},{"creatorName":"KAWAKITA, Hideyo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"7890","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2018-01-28"}],"displaytype":"detail","filename":"KJ00010262519.pdf","filesize":[{"value":"396.3 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00010262519.pdf","url":"https://ksu.repo.nii.ac.jp/record/2937/files/KJ00010262519.pdf"},"version_id":"b5a8e5b4-c992-4add-b971-4f09aa0d3f01"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"彗星","subitem_subject_scheme":"Other"},{"subitem_subject":"近赤外線","subitem_subject_scheme":"Other"},{"subitem_subject":"高分散分光","subitem_subject_scheme":"Other"},{"subitem_subject":"星間化学","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系起源","subitem_subject_scheme":"Other"},{"subitem_subject":"Comets","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Molecular formation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Fractionation of ^^15N","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Interstellar chemistry","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Origin of solar system","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"「近赤外線波長領域における彗星氷物質の高分散分光サーベイ」(2)研究経過報告","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"「近赤外線波長領域における彗星氷物質の高分散分光サーベイ」(2)研究経過報告","subitem_title_language":"ja"},{"subitem_title":"Research report : \"High-resolution Spectroscopic Survey of Cometary Molecules in Near-infrared Wavelength Region(2)\"","subitem_title_language":"en"}]},"item_type_id":"2","owner":"3","path":["227"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2018-01-28"},"publish_date":"2018-01-28","publish_status":"0","recid":"2937","relation_version_is_last":true,"title":["「近赤外線波長領域における彗星氷物質の高分散分光サーベイ」(2)研究経過報告"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-09-04T03:12:12.951614+00:00"}