{"created":"2024-09-04T03:13:13.273818+00:00","id":2000224,"links":{},"metadata":{"_buckets":{"deposit":"934c75c8-d07d-4273-b21b-8249c2de22fa"},"_deposit":{"created_by":11,"id":"2000224","owner":"11","owners":[11],"pid":{"revision_id":0,"type":"depid","value":"2000224"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:02000224","sets":["14:226:1725414013867"]},"author_link":["22609"],"item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2024-09-10","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"74","bibliographicPageStart":"59","bibliographicVolumeNumber":"19","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増光現象である。その増光パターンの計算の原理は単純であるが，多数の恒星の影響を同時に考慮しなければならず，その計算コストは低くない。そこで，従来行われてきた数値計算効率化のための手法をもとに，GPGPU を利用した効率的な（あるいは高速な）数値計算方法を開発し，実際に幾つかの場合について行った計算結果について紹介する。","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":"YONEHARA, Atsunori","creatorNameLang":"en"},{"creatorName":"米原, 厚憲","creatorNameLang":"ja"},{"creatorName":"ヨネハラ, アツノリ","creatorNameLang":"ja-Kana"}],"familyNames":[{"familyName":"YONEHARA","familyNameLang":"en"},{"familyName":"米原","familyNameLang":"ja"},{"familyName":"ヨネハラ","familyNameLang":"ja-Kana"}],"givenNames":[{"givenName":"Atsunori","givenNameLang":"en"},{"givenName":"厚憲","givenNameLang":"ja"},{"givenName":"アツノリ","givenNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"22609","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_access","date":[{"dateType":"Available","dateValue":"2024-09-04"}],"displaytype":"detail","filename":"KSUSGKS_19_59.pdf","filesize":[{"value":"2.7 MB"}],"format":"application/pdf","licensetype":"license_note","url":{"label":"KSUSGKS_19_59.pdf","url":"https://ksu.repo.nii.ac.jp/record/2000224/files/KSUSGKS_19_59.pdf"},"version_id":"444dbea6-2231-4d65-8843-cc5e0d3daf60"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"重力レンズ","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"マイクロレンズ現象","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"固有運動","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"光度曲線","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"数値計算","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"gravitational lens","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"microlens event","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"proper motion","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"light curve","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"numerical method","subitem_subject_language":"en","subitem_subject_scheme":"UDC"}]},"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":"クェーサーマイクロレンズ現象の効率的な数値計算方法","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"クェーサーマイクロレンズ現象の効率的な数値計算方法","subitem_title_language":"ja"},{"subitem_title":"Efficient numerical method for quasar microlensing","subitem_title_language":"en"}]},"item_type_id":"10002","owner":"11","path":["1725414013867"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2024-09-04"},"publish_date":"2024-09-04","publish_status":"0","recid":"2000224","relation_version_is_last":true,"title":["クェーサーマイクロレンズ現象の効率的な数値計算方法"],"weko_creator_id":"11","weko_shared_id":-1},"updated":"2024-09-04T03:19:58.263806+00:00"}