WEKO3
アイテム
{"_buckets": {"deposit": "07632686-9654-4aaa-897a-9a90ec1f72ed"}, "_deposit": {"created_by": 1, "id": "2982", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "2982"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00002982", "sets": ["807", "1891"]}, "author_link": ["10238", "10237"], "item_5_biblio_info_10": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2018-03-09", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "32", "bibliographicPageStart": "29", "bibliographicVolumeNumber": "JAXA-SP-17-010E", "bibliographic_titles": [{"bibliographic_title": "宇宙航空研究開発機構特別資料"}, {"bibliographic_title": "JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA\u0027s New Window on the Cool Universe", "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": "SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA\u0027s New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan", "subitem_description_type": "Other"}]}, "item_5_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "Quasar mode AGN feedback is a popular concept in cosmological models to explain the observed galaxy mass function, but observational evidence for this idea remains controversial. We review recent results from Herschel and Spitzer that provide strong evidence that quasar mode feedback can have a profound impact on AGN host galaxies, and that much of this impact happens while the AGN is still obscured. Holistic studies of quasar mode feedback thus require observations that span a wide wavelength range; in the far-infrared early on in the feedback phase, through to the optical/UV near the end of the feedback phase. We review how SPICA can contribute to this effort, by tracking quasar mode feedback across a wide range in obscuration levels.", "subitem_description_type": "Other"}]}, "item_5_description_18": {"attribute_name": "内容記述", "attribute_value_mlt": [{"subitem_description": "形態: カラー図版あり", "subitem_description_type": "Other"}]}, "item_5_description_19": {"attribute_name": "内容記述(英)", "attribute_value_mlt": [{"subitem_description": "Physical characteristics: Original contains color illustrations", "subitem_description_type": "Other"}]}, "item_5_description_32": {"attribute_name": "資料番号", "attribute_value_mlt": [{"subitem_description": "資料番号: AA1730027005", "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-17-010E", "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(JAXA)"}]}, "item_5_publisher_9": {"attribute_name": "出版者(英)", "attribute_value_mlt": [{"subitem_publisher": "Japan Aerospace Exploration Agency (JAXA)"}]}, "item_5_source_id_22": {"attribute_name": "ISSNONLINE", "attribute_value_mlt": [{"subitem_source_identifier": "2433-2232", "subitem_source_identifier_type": "ISSN"}]}, "item_5_text_34": {"attribute_name": "メタデータ提供者", "attribute_value_mlt": [{"subitem_text_value": "メタデータ提供者: JAXA"}]}, "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_36": {"attribute_name": "JAXAカテゴリ2", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ2: IS"}]}, "item_5_text_38": {"attribute_name": "NASA分類コード", "attribute_value_mlt": [{"subitem_text_value": "NASA分類コード: 89"}]}, "item_5_text_39": {"attribute_name": "NASA分類表目標", "attribute_value_mlt": [{"subitem_text_value": "NASA分類: Astronomy"}]}, "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: 10"}]}, "item_5_text_7": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "Virginia Tech"}, {"subitem_text_language": "en", "subitem_text_value": "Virginia Tech"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Farrah, Duncan", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "10237", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Petty, Sara", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "10238", "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": "2020-01-15"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "AA1730027005.pdf", "filesize": [{"value": "443.5 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 443500.0, "url": {"label": "AA1730027005.pdf", "url": "https://jaxa.repo.nii.ac.jp/record/2982/files/AA1730027005.pdf"}, "version_id": "1ec6846e-a3ce-4a69-b923-e626bf80a4e6"}]}, "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": "Infrared Diagnostics of Quasar Mode Feedback", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Infrared Diagnostics of Quasar Mode Feedback", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["807", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/2982", "pubdate": {"attribute_name": "公開日", "attribute_value": "2018-05-01"}, "publish_date": "2018-05-01", "publish_status": "0", "recid": "2982", "relation": {}, "relation_version_is_last": true, "title": ["Infrared Diagnostics of Quasar Mode Feedback"], "weko_shared_id": -1}
Infrared Diagnostics of Quasar Mode Feedback
https://jaxa.repo.nii.ac.jp/records/2982
https://jaxa.repo.nii.ac.jp/records/29826cf89c3c-d2c2-4667-9e3f-ad784df28bb9
名前 / ファイル | ライセンス | アクション |
---|---|---|
AA1730027005.pdf (443.5 kB)
|
|
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2018-05-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Infrared Diagnostics of Quasar Mode Feedback | |||||
言語 | ||||||
言語 | eng | |||||
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 |
Farrah, Duncan
× Farrah, Duncan× Petty, Sara |
|||||
著者所属(英) | ||||||
en | ||||||
Virginia Tech | ||||||
著者所属(英) | ||||||
en | ||||||
Virginia Tech | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
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: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe 巻 JAXA-SP-17-010E, p. 29-32, 発行日 2018-03-09 |
|||||
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 | SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Quasar mode AGN feedback is a popular concept in cosmological models to explain the observed galaxy mass function, but observational evidence for this idea remains controversial. We review recent results from Herschel and Spitzer that provide strong evidence that quasar mode feedback can have a profound impact on AGN host galaxies, and that much of this impact happens while the AGN is still obscured. Holistic studies of quasar mode feedback thus require observations that span a wide wavelength range; in the far-infrared early on in the feedback phase, through to the optical/UV near the end of the feedback phase. We review how SPICA can contribute to this effort, by tracking quasar mode feedback across a wide range in obscuration levels. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1730027005 | |||||
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-17-010E |