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Intensity Mapping of Fine Structure Line Emission as a Probe of Large Scale Structure and the Evolving ISM in Dusty, Star-Forming Galaxies at Moderate Redshift
https://jaxa.repo.nii.ac.jp/records/3007
https://jaxa.repo.nii.ac.jp/records/3007ea3f07d8-af1e-4cff-97a2-744b6f7619cb
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
AA1730027030.pdf (288.7 kB)
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| Item type | 会議発表論文 / Conference Paper(1) | |||||||||||
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| 公開日 | 2018-05-01 | |||||||||||
| タイトル | ||||||||||||
| タイトル | Intensity Mapping of Fine Structure Line Emission as a Probe of Large Scale Structure and the Evolving ISM in Dusty, Star-Forming Galaxies at Moderate Redshift | |||||||||||
| 言語 | en | |||||||||||
| 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 |
Uzgil, Bade D.
× Uzgil, Bade D.
× Aguirre, J. E.
× Bradford, C. M.
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| 著者所属（英） | ||||||||||||
| en | ||||||||||||
| University of Pennsylvania : National Aeronautics and Space Administration (NASA) | ||||||||||||
| 著者所属（英） | ||||||||||||
| en | ||||||||||||
| University of Pennsylvania | ||||||||||||
| 著者所属（英） | ||||||||||||
| en | ||||||||||||
| National Aeronautics and Space Administration (NASA) : California Institute of Technology | ||||||||||||
| 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. 133-135, 発行日 2018-03-09 |
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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 | 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 | We explore the possibility of studying redshifted far-IR fine-structure transitions through cosmic time using 3- dimensional power spectra obtained with an imaging spectrometer. The intensity mapping approach measures the spatio-spectral fluctuations due to line emission from all galaxies, including those well below the individual detection threshold. With assumptions about large-scale structure, the large-scale fluctuations measure the total volume emissivity in a given transition, with redshift information naturally encoded. We consider as specific examples the possibility of studying redshifted [O I] 63 μm and [Si II] 35 μm with the SAFARI instrument aboard SPICA. While envisioned SAFARI surveys will only detect the brightest galaxies individually, the fluctuation signal from the aggregate population is detected with high significance: cumulative SNR of order 100 for both the total and shot noise power spectra, and order 10 for the clustering power spectrum from surveys sketched in this proceedings article. | |||||||||||
| 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: AA1730027030 | |||||||||||
| 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 | |||||||||||
