WEKO3
アイテム
{"_buckets": {"deposit": "7bc97dd0-05e4-4283-954d-ac89e4462b91"}, "_deposit": {"created_by": 1, "id": "5290", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "5290"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00005290", "sets": ["959", "1891"]}, "author_link": ["25560", "25559"], "item_5_biblio_info_10": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2009-02-27", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "260", "bibliographicPageStart": "256", "bibliographicVolumeNumber": "JAXA-SP-08-014E", "bibliographic_titles": [{"bibliographic_title": "宇宙航空研究開発機構特別資料"}, {"bibliographic_title": "JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop", "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": "Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008)", "subitem_description_type": "Other"}]}, "item_5_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "MAXI, Monitor of All-sky X-ray Image, is an X-ray observatory on the international space station. MAXI carries two kinds of slit scanning camera; gas slit camera (GSC) and solid-state slit camera (SSC). In the course of one station orbit, MAXI can scan almost the entire sky with a precision of 1.5 deg and with an X-ray energy range of 0.5 - 30 keV. Major purpose of MAXI is monitor of known X-ray sources and detection of new serendipitous sources such as X-ray nova whereas diffuse X-ray emission in our galaxy is also an important target especially for SSC. The good energy resolving power of SSC enables us, for the first time, to map the entire sky with various line emission from O to Fe. Based on the previous observational data, we simulate MAXI data both for SSC and GSC. Large-scale structures in our galaxy such as supernova remnants, radio loop, superbubbles are possible targets for SSC. The Galactic ridge X-ray emission is important target both for GSC and SSC.", "subitem_description_type": "Other"}]}, "item_5_description_32": {"attribute_name": "資料番号", "attribute_value_mlt": [{"subitem_description": "資料番号: AA0064306051", "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-08-014E", "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_35": {"attribute_name": "JAXAカテゴリ", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ: 特別資料"}]}, "item_5_text_40": {"attribute_name": "jaxa出版物種類", "attribute_value_mlt": [{"subitem_text_value": "jaxa出版物種類: SP"}]}, "item_5_text_43": {"attribute_name": "DSpaceコレクション番号", "attribute_value_mlt": [{"subitem_text_value": "DSpaceコレクション番号: 7"}]}, "item_5_text_6": {"attribute_name": "著者所属", "attribute_value_mlt": [{"subitem_text_value": "大阪大学理学研究科宇宙地球学専攻"}]}, "item_5_text_7": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "Department of Earth \u0026 Space Science, Graduate School of Science, Osaka University"}, {"subitem_text_language": "en", "subitem_text_value": "MAXI Team"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "宮田, 恵美"}], "nameIdentifiers": [{"nameIdentifier": "25559", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Miyata, Emi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "25560", "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": "2020-01-16"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "64306051.pdf", "filesize": [{"value": "507.3 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 507300.0, "url": {"label": "64306051.pdf", "url": "https://jaxa.repo.nii.ac.jp/record/5290/files/64306051.pdf"}, "version_id": "14341ba1-b65a-4bdf-b908-c4af90e20082"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "X-ray - all-sky survey - diffuse source - all-sky line map", "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": "Diffuse source mapping with MAXI", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Diffuse source mapping with MAXI", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["959", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/5290", "pubdate": {"attribute_name": "公開日", "attribute_value": "2015-03-26"}, "publish_date": "2015-03-26", "publish_status": "0", "recid": "5290", "relation": {}, "relation_version_is_last": true, "title": ["Diffuse source mapping with MAXI"], "weko_shared_id": -1}
Diffuse source mapping with MAXI
https://jaxa.repo.nii.ac.jp/records/5290
https://jaxa.repo.nii.ac.jp/records/52909684deee-d078-40f9-838a-d87ab0d97c95
名前 / ファイル | ライセンス | アクション |
---|---|---|
64306051.pdf (507.3 kB)
|
|
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Diffuse source mapping with MAXI | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | X-ray - all-sky survey - diffuse source - all-sky line map | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
宮田, 恵美
× 宮田, 恵美× Miyata, Emi |
|||||
著者所属 | ||||||
大阪大学理学研究科宇宙地球学専攻 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Earth & Space Science, Graduate School of Science, Osaka University | ||||||
著者所属(英) | ||||||
en | ||||||
MAXI Team | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 256-260, 発行日 2009-02-27 |
|||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | MAXI, Monitor of All-sky X-ray Image, is an X-ray observatory on the international space station. MAXI carries two kinds of slit scanning camera; gas slit camera (GSC) and solid-state slit camera (SSC). In the course of one station orbit, MAXI can scan almost the entire sky with a precision of 1.5 deg and with an X-ray energy range of 0.5 - 30 keV. Major purpose of MAXI is monitor of known X-ray sources and detection of new serendipitous sources such as X-ray nova whereas diffuse X-ray emission in our galaxy is also an important target especially for SSC. The good energy resolving power of SSC enables us, for the first time, to map the entire sky with various line emission from O to Fe. Based on the previous observational data, we simulate MAXI data both for SSC and GSC. Large-scale structures in our galaxy such as supernova remnants, radio loop, superbubbles are possible targets for SSC. The Galactic ridge X-ray emission is important target both for GSC and SSC. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064306051 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-08-014E |