{"created":"2023-05-15T14:46:51.667799+00:00","id":10536,"links":{},"metadata":{"_buckets":{"deposit":"bb8ea435-75c3-4488-8420-6ac76b6ed167"},"_deposit":{"created_by":11,"id":"10536","owners":[11],"pid":{"revision_id":0,"type":"depid","value":"10536"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:00010536","sets":["14:226:1037"]},"author_link":["22609"],"control_number":"10536","item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2020-09-30","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"124","bibliographicPageStart":"113","bibliographicVolumeNumber":"15","bibliographic_titles":[{"bibliographic_title":"京都産業大学総合学術研究所所報"}]}]},"item_10002_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"クェーサーマイクロレンズ現象は、背景クェーサーと前方銀河内の恒星の相対運動によって引き起こされる。その際、恒星の固有運動を考慮することで期待される、マイクロレンズ現象の性質の変化について数値計算を用いた評価を行った。過去行われた計算よりも高精度の計算を行った結果、固有運動はマイクロレンズ現象のタイムスケールの分布を大きく変化しないまま、増光の大きさの分布を変化させることが分かった。","subitem_description_type":"Abstract"}]},"item_10002_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"京都産業大学総合学術研究所"}]},"item_10002_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11879037","subitem_source_identifier_type":"NCID"}]},"item_10002_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1348-8465","subitem_source_identifier_type":"PISSN"}]},"item_10002_version_type_20":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"米原, 厚憲","creatorNameLang":"ja"},{"creatorName":"ヨネハラ, アツノリ","creatorNameLang":"ja-Kana"},{"creatorName":"YONEHARA, Atsunori","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":"2020-10-27"}],"displaytype":"detail","filename":"KSUSGKS_15_113.pdf","filesize":[{"value":"2.8 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KSUSGKS_15_113.pdf","url":"https://ksu.repo.nii.ac.jp/record/10536/files/KSUSGKS_15_113.pdf"},"version_id":"4dbeeffa-2043-405b-8401-25561d2980e0"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"クェーサー","subitem_subject_scheme":"Other"},{"subitem_subject":"系外惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"重力レンズ","subitem_subject_scheme":"Other"},{"subitem_subject":"固有運動","subitem_subject_scheme":"Other"},{"subitem_subject":"マイクロレンズ現象","subitem_subject_scheme":"Other"},{"subitem_subject":"quasar","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"exoplanet","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"gravitational lens","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"proper motion","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"microlens event","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":"恒星の固有運動を考慮したクェーサーマイクロレンズ現象","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"恒星の固有運動を考慮したクェーサーマイクロレンズ現象","subitem_title_language":"ja"},{"subitem_title":"Microlensing study including proper motion of stellar lens objects","subitem_title_language":"en"}]},"item_type_id":"10002","owner":"11","path":["1037"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2020-10-27"},"publish_date":"2020-10-27","publish_status":"0","recid":"10536","relation_version_is_last":true,"title":["恒星の固有運動を考慮したクェーサーマイクロレンズ現象"],"weko_creator_id":"11","weko_shared_id":-1},"updated":"2023-08-31T01:09:26.743929+00:00"}