{"created":"2021-03-01T06:11:41.621948+00:00","id":5148,"links":{},"metadata":{"_buckets":{"deposit":"a1bd9ca8-bdf7-4fc8-9171-61d0c8ac3bd9"},"_deposit":{"id":"5148","owners":[],"pid":{"revision_id":0,"type":"depid","value":"5148"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00005148","sets":["336:635:636"]},"author_link":["12873","12874"],"item_12_alternative_title_19":{"attribute_name":"その他のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"PSR B1509-58に伴うパルサーネブラからの超高エネルギーガンマ線放射の証拠","subitem_alternative_title_language":"ja"}]},"item_12_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1998-03-25","bibliographicIssueDateType":"Issued"}}]},"item_12_date_granted_64":{"attribute_name":"学位授与年月日","attribute_value_mlt":[{"subitem_dategranted":"1998-03-25"}]},"item_12_degree_grantor_62":{"attribute_name":"学位授与機関","attribute_value_mlt":[{"subitem_degreegrantor":[{"subitem_degreegrantor_language":"ja","subitem_degreegrantor_name":"名古屋大学"},{"subitem_degreegrantor_language":"en","subitem_degreegrantor_name":"Nagoya University"}],"subitem_degreegrantor_identifier":[{"subitem_degreegrantor_identifier_name":"13901","subitem_degreegrantor_identifier_scheme":"kakenhi"}]}]},"item_12_degree_name_61":{"attribute_name":"学位名","attribute_value_mlt":[{"subitem_degreename":"博士(理学)","subitem_degreename_language":"ja"}]},"item_12_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The gamma-ray pulsar PSR B1509-58 and its surrounding nebulas have been observed by using the 3.8m imaging Cerenkov telescope of the CANGAROO collaboration. The observations have been carried out during the years  1996 and 1997 in Woomera, South Australia at the gamma-ray threshold energies of 4 TeV and 1.5 TeV, respectivelly. Very high-energy gammarays-ray threshold in the 1997 data with 4.1significance. The estimated gamma-ray flrx is at energies above 1.5 Tev. On the other hand, it was possible only to set a 3 upper limit of above 4.0 TeV from the observations of 1996. No significant pulsation pulsation modulated with the pulsar ;eriod has been found in either the 1996 or the 1997 data. Our results when combined with X-ray observations lead to a value of the magnetic field strength consistent with equipartition value, in the X-ray nebula surrounding the pulsar. This field strength is much weaker than the one in the Crab nebula. This is the first evidence of VHE gamma-ray emission from a non-EGRET pulsar. It underscores the power of a new criterion for the search for VHE gamma-ray sources, i.e,. X-ray synchrotron nebulae driven by young rotation-powered pulsars.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_12_description_5":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"名古屋大学博士学位論文 学位の種類:博士(理学) (課程) 学位授与年月日:平成10年3月25日","subitem_description_language":"ja","subitem_description_type":"Other"}]},"item_12_dissertation_number_65":{"attribute_name":"学位授与番号","attribute_value_mlt":[{"subitem_dissertationnumber":"甲第3864号"}]},"item_12_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/6714"}]},"item_12_select_15":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_select_item":"publisher"}]},"item_12_text_14":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_text_value":"application/pdf"}]},"item_12_text_63":{"attribute_name":"学位授与年度","attribute_value_mlt":[{"subitem_text_value":"1997"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"open access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_abf2"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Sako, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"12873","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"﨏, 隆志","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"12874","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2018-02-19"}],"displaytype":"detail","filename":"ko3864.pdf","filesize":[{"value":"9.4 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"ko3864.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/5148/files/ko3864.pdf"},"version_id":"2249bd42-3ebc-4846-92d5-6c19285a1891"}]},"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":"doctoral thesis","resourceuri":"http://purl.org/coar/resource_type/c_db06"}]},"item_title":"Evidence of VHE Gamma-Ray Emission from the Pulsar Nebula around PSR B1509-58","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Evidence of VHE Gamma-Ray Emission from the Pulsar Nebula around PSR B1509-58","subitem_title_language":"en"}]},"item_type_id":"12","owner":"1","path":["636"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2006-07-25"},"publish_date":"2006-07-25","publish_status":"0","recid":"5148","relation_version_is_last":true,"title":["Evidence of VHE Gamma-Ray Emission from the Pulsar Nebula around PSR B1509-58"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T03:49:42.859815+00:00"}