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Properties of galaxy groups and clusters in the fields of lensed quasars
https://jaxa.repo.nii.ac.jp/records/5075
https://jaxa.repo.nii.ac.jp/records/50755ede9994-bec1-46b0-9d7b-a54a0d46744c
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
64574143.pdf (140.7 kB)
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| アイテムタイプ | 会議発表論文 / Conference Paper(1) | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| 公開日 | 2015-03-26 | |||||||||
| タイトル | ||||||||||
| タイトル | Properties of galaxy groups and clusters in the fields of lensed quasars | |||||||||
| 言語 | en | |||||||||
| 言語 | ||||||||||
| 言語 | eng | |||||||||
| キーワード | ||||||||||
| 言語 | en | |||||||||
| 主題Scheme | Other | |||||||||
| 主題 | galaxies: clusters - X-rays: galaxies: clusters | |||||||||
| 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 |
Grant, E. Catherine
× Grant, E. Catherine
× Bautz, Marshall
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| 著者所属（英） | ||||||||||
| en | ||||||||||
| MIT Kavli Institute for Astrophysics and Space Research | ||||||||||
| 著者所属（英） | ||||||||||
| en | ||||||||||
| MIT Kavli Institute for Astrophysics and Space Research | ||||||||||
| 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: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 374-375, 発行日 2010-02-26 |
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| 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 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||||||
| 抄録（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | Gravitationally lensed quasars can be used as a cosmological tool, however modeling of these systems requires mapping the gravitational potential along the line of sight to the quasar, including the lensing galaxy and its environment. Keeton et al. (2000) predict that at least 25% of lensing galaxies are part of a group or cluster and the growing observational evidence seems to confirm this. Finding and studying these lensing groups and clusters enhances the science that can be accomplished with lensing and provides a method for finding groups and clusters at cosmologically interesting redshifts (0.1 < z < 0.7). We have identified all observations of gravitationally lensed quasars available in the Chandra archive to search for diffuse X-ray emission from groups or clusters along the line of sight. We present a uniformly analyzed catalog of X-ray luminosities and temperatures for those fields with significant diffuse emission. These measurements are compared with optical data, where available, and with scaling relations. | |||||||||
| 内容記述（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||||||
| 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: AA0064574143 | |||||||||
| 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-09-008E | |||||||||
