{"created":"2023-06-20T14:38:23.362903+00:00","id":4946,"links":{},"metadata":{"_buckets":{"deposit":"0157cd8b-805e-4785-929a-10f1ce52ad48"},"_deposit":{"created_by":1,"id":"4946","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"4946"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00004946","sets":["1887:1891","9:789:936:948"]},"author_link":["22707","22717","22715","22712","22709","22718","22705","22706","22708","22711","22714","22716","22710","22713"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"41","bibliographicPageStart":"40","bibliographicVolumeNumber":"JAXA-SP-09-008E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料:"},{"bibliographic_title":"JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H","bibliographic_titleLang":"en"}]}]},"item_5_description_15":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）（英）","attribute_value_mlt":[{"subitem_description":"The 3rd Suzaku international Conference \"Energetic Cosmos : from Suzaku to ASTRO-H\" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We report on the discovery of a non-thermal X-ray emission from the supernova remnant (SNR) W28. W28 is a cosmic ray accelerator from which GeV and TeV gamma-ray were detected. We analyzed the northeast part of W28, and found a power-law spectrum with a photon index of 2.4 (2.1-2.8) from an inner region which is probably non-thermal X-ray emission caused by particle acceleration. On the assumption that it is synchrotron X-ray, the cooling time of synchrotron photon is consistent with the age of W28 with a few micro-G magnetic field. On the other hand, we have no significant X-ray flux from one of the TeV gamma-ray emission region. Assuming a power-law spectrum with a photon index of 2.66, the same as in the TeV band, we obtained a 2-10 keV flux upper limit of 2.1 x 10(exp -14) ergs/s sq cm. Low brightness in X-ray and the coincidence of the molecular cloud and TeV gamma-ray emission site suggests that TeV gamma-ray is originated from accelerated protons.","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064574014","subitem_description_type":"Other"}]},"item_5_description_33":{"attribute_name":"レポート番号","attribute_value_mlt":[{"subitem_description":"レポート番号: JAXA-SP-09-008E","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency (JAXA)"}]},"item_5_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1349-113X","subitem_source_identifier_type":"ISSN"}]},"item_5_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11984031","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"},{"subitem_text_value":"広島大学理学部物理学科"},{"subitem_text_value":"国立天文台"},{"subitem_text_value":"東北大学大学院理学研究科物理学専攻"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)"},{"subitem_text_language":"en","subitem_text_value":"Department of Physical Science, Hiroshima University"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Tohoku University"},{"subitem_text_language":"en","subitem_text_value":"Institut fur Astronomie und Astrophysik"},{"subitem_text_language":"en","subitem_text_value":"Landessternwarte, Universitat Heidelberg"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"中村, 良子"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"馬場, 彩"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"石田, 学"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"山崎, 了"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"立松, 健一"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"郡, 和範"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakamura, Ryoko","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Bamba, Aya","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ishida, Manabu","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yamazaki, Ryo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tatematsu, Kenichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kohri, Kazunori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Puhlhofer, Gerd","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Wagner, Stefan J.","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":"2020-01-16"}],"displaytype":"detail","filename":"64574014.pdf","filesize":[{"value":"272.5 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574014.pdf","url":"https://jaxa.repo.nii.ac.jp/record/4946/files/64574014.pdf"},"version_id":"62458437-9411-4b9c-858b-b87c73331a3f"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"acceleration of particles -  ISM: individual (W28) - ISM: supernova remnants - X-ray: ISM","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"Discovery of a Hard X-ray Spectrum from the Mixed Morphology SNR W28 with XMM-Newton","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Discovery of a Hard X-ray Spectrum from the Mixed Morphology SNR W28 with XMM-Newton","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["948","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"4946","relation_version_is_last":true,"title":["Discovery of a Hard X-ray Spectrum from the Mixed Morphology SNR W28 with XMM-Newton"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:28:10.681780+00:00"}