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arXiv 0908.3005astro-ph.IMastro-ph.COastro-ph.HE
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JANUS X射线闪光监视器

The JANUS X-Ray Flash Monitor

A. D. Falcone, D. N. Burrows, S. Barthelmy, W. Chang, J. Fredley, M. Kelly, R. Klar, D. Palmer, S. Persyn, K. Reichard, P. Roming, E. Seifert, R. W. M. Smith, P. Wood, M. Zugger

摘要:

JANUS是美国宇航局的小型探索者级任务,刚刚完成A阶段,计划于2013年发射。JANUS的主要科学目标是利用高红移(6<z<12)伽马射线暴和类星体来探索早期宇宙中第一批恒星的形成历史,并研究对再电离的贡献。X射线闪光监视器(XRFM)和近红外望远镜(NIRT)是JANUS上的两个主要仪器。XRFM被设计用于探测宽视场(4球面度)上1-20 keV能量带的明亮X射线闪光(XRF)和伽马射线暴(GRB),从而便于探测z>6的XRF/GRB,这可以通过其他仪器进一步研究。XRFM将使用具有混合CMOS Si探测器的编码掩模孔径设计。它将对通量超过约240 mCrab的XRF/GRB敏感。该航天器被设计为在XRFM的GRB触发后快速旋转到源位置。本文介绍了XRFM仪器的设计参数和科学目标。

英文摘要:

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<z<12) gamma ray bursts and quasars to explore the formation history of the first stars in the early universe and to study contributions to reionization. The X-Ray Flash Monitor (XRFM) and the Near-IR Telescope (NIRT) are the two primary instruments on JANUS. XRFM has been designed to detect bright X-ray flashes (XRFs) and gamma ray bursts (GRBs) in the 1-20 keV energy band over a wide field of view (4 steradians), thus facilitating the detection of z>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.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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