{"created":"2023-06-20T15:07:18.622348+00:00","id":36672,"links":{},"metadata":{"_buckets":{"deposit":"e7dd4531-ba1d-4371-9fe2-33d583349f14"},"_deposit":{"created_by":1,"id":"36672","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"36672"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00036672","sets":["1887:1890","1896:1898:1899:1991"]},"author_link":["424190","424188","424189"],"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2000-12","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"177","bibliographicPageStart":"171","bibliographicVolumeNumber":"14","bibliographic_titles":[{},{"bibliographic_title":"The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission","bibliographic_titleLang":"en"}]}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Following the concept presented by Takeuchi, Yoshikawa, & Yonehara (2000), weshow some concrete examples of number count of lensed galaxies in the infrared. Adopting asimple lens model of cluster of galaxies, we are able to estimate the expected number counts ofgalaxies. The result tells us that the expected number counts of galaxies around a single clusterare not so large, but in principle, we can discriminate global history of galaxy evolution efficientlyat longer waveband, i.e. FIR and/or sub-mm.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA4590679000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙科学研究所"}]},"item_9_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0288-433X","subitem_source_identifier_type":"ISSN"}]},"item_9_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA10455137","subitem_source_identifier_type":"NCID"}]},"item_9_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Astronomy, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Department of Astronomy, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Division of Particle and Astrophysical Sciences, Nagoya University"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"YONEHARA, Atsunori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"YOSIKAWA, Kohji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"TAKEUCHI, Tsutomu  T.","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":"2020-01-24"}],"displaytype":"detail","filename":"SA4590679.pdf","filesize":[{"value":"362.3 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA4590679.pdf","url":"https://jaxa.repo.nii.ac.jp/record/36672/files/SA4590679.pdf"},"version_id":"9fd727e6-4874-47d8-96ed-859ac593396d"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Gravitationally Lensed Galaxy Number Counts in the Infrared II: Concrete Examples","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Gravitationally Lensed Galaxy Number Counts in the Infrared II: Concrete Examples","subitem_title_language":"en"}]},"item_type_id":"9","owner":"1","path":["1890","1991"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"36672","relation_version_is_last":true,"title":["Gravitationally Lensed Galaxy Number Counts in the Infrared II: Concrete Examples"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T22:51:28.276593+00:00"}