{"created":"2023-06-20T15:07:18.026049+00:00","id":36660,"links":{},"metadata":{"_buckets":{"deposit":"7d9df53d-218c-4104-b4dc-e405f0267146"},"_deposit":{"created_by":1,"id":"36660","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"36660"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00036660","sets":["1887:1890","1896:1898:1899:1991"]},"author_link":["424156"],"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2000-12","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"81","bibliographicPageStart":"75","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":"The use of chemical tracers as timing devices to discern historical trends in theevolution of the Universe,galaxies,interstellar phenomena, and other astrophysical systems, is likely to become a dominant aim of future infrared and submillimeter astronomical missions. Thehigh sensitivities, and spatial and spectral resolving powers that will become available in the next few years will make such studies possible. Chemistry, rather than physics, will then most likely become our main tracer of the prehistory of a particular region and the influences that have shaped it.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA4586779000","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":"Cornell University"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Martin, HARWIT","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":"SA4586779.pdf","filesize":[{"value":"192.8 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA4586779.pdf","url":"https://jaxa.repo.nii.ac.jp/record/36660/files/SA4586779.pdf"},"version_id":"b14d3327-e044-470f-8c87-c8178fc2da0b"}]},"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":"Cosmochemical Evolution","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Cosmochemical Evolution","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":"36660","relation_version_is_last":true,"title":["Cosmochemical Evolution"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T22:51:49.781023+00:00"}