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ASTROSAT-LAXPC observations of MAXI transient sources
https://jaxa.repo.nii.ac.jp/records/5308
https://jaxa.repo.nii.ac.jp/records/530890a19dc0-daf1-4e3b-a5e8-909acdc4107e
名前 / ファイル | ライセンス | アクション |
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64306069.pdf (315.6 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | ASTROSAT-LAXPC observations of MAXI transient sources | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Stars : neutron - (Stars :) pulsars : - X-rays : stars - (Stars :) binaries : general - X-rays : binaries | |||||
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 |
Paul, Biswajit
× Paul, Biswajit |
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著者所属(英) | ||||||
en | ||||||
Raman Research Institute | ||||||
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. 362-366, 発行日 2009-02-27 |
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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 | 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 | ASTROSAT is an astronomy satellite being made for a launch in 2009. It is designed for simultaneous multi-wavelength studies with five payloads in the optical/UV and a broad X-ray energy range. One of the instruments, a set of three large area xenon proportional counters (LAXPC) will enable high time resolution X-ray measurements in the 2 - 80 keV band with moderate energy resolution. There are two imaging X-ray spectrometers, one in the soft and one in the hard X-ray band. Two telescopes will provide multi-band imaging in three optical/UV channels. An X-ray sky monitor onboard ASTROSAT, that is similar in concept to the RXTE-ASM will be used to study long term intensity variations of bright X-ray sources. This instrument will also facilitate timely X-ray observations of transient and variable sources with the LAXPC and other payloads. Here we discuss the salient features of the LAXPC and its advantage of previous large area X-ray astronomy instruments. A very large effective area for hard X-rays with good energy resolution will allow the LAXPC to probe certain properties of X-ray sources with unprecedented detail. The main science issues to be addressed with the LAXPCs are discussed here with some simulated results. We particularly mention the science topics related to variable and transient X-ray sources for which the ASTROSAT observations will benefit from the all sky monitoring with MAXI. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | B. Paul (on behalf of the LAXPC team) --As author | |||||
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: AA0064306069 | |||||
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 |