Falcone, A. D. 2009 JANUS: 一个X-ray flash探测器
主要内容:
NASA的一个小项目. 准备2013年上天.
两个望远镜: The X-Ray Flash Monitor (XRFM) and the Near-IR Telescope (NIRT). X-ray仪器的能段: 1-20keV.
sensitivity:240 mCrab.
(Note: 1 Crab unit of the 35 – 200 keV flux = 1 × 10-3 photons cm-2 s-1 keV-1.)
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文章信息:
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Title: | The JANUS X-Ray Flash Monitor | |
Authors: | Falcone, A. D.; Burrows, D. N.; Barthelmy, S.; Chang, W.; Fredley, J.; Kelly, M.; Klar, R.; Palmer, D.; Persyn, S.; Reichard, K.; Roming, P.; Seifert, E.; Smith, R. W. M.; Wood, P.; Zugger, M. | |
Publication: | eprint arXiv:0908.3005 | |
Publication Date: | 08/2009 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena | |
Comment: | submitted to Proc. SPIE, Vol. 7435 (2009), 7 pages, 8 figures | |
Bibliographic Code: | 2009arXiv0908.3005F |
Abstract
JANUS is a NASA small explorer class mission which just completed phase A and was intended for a 2013 launch date. The primary science goals of JANUS are to use high redshift (6.lt. z.lt.12).gt.6 XRFs/GRBs, which can be further studied by other instruments. XRFM would use a coded mask aperture design with hybrid CMOS Si detectors. It would be sensitive to XRFs/GRBs with flux in excess of approximately 240 mCrab. The spacecraft is designed to rapidly slew to source positions following a GRB trigger from XRFM. XRFM instrument design parameters and science goals are presented in this paper.Bibtex entry for this abstract Preferred format for this abstract (see Preferences)
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