伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期五, 四月 17, 2009

Grindlay 2009 探测高红移伽玛暴的探测器EXIST

主要内容:
类似Swift, 但都有所扩展(没有紫外, 有光学). 可以很快地定红移

预计2017年发射

精彩摘抄:
一些参数


文章信息:

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Title:
GRB Probes of the High-z Universe with EXIST
Authors:
Grindlay, Jonathan; the EXIST Team
Publication:
eprint arXiv:0904.2210
Publication Date:
04/2009
Origin:
ARXIV
Keywords:
Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Comment:
7 pages, 5 figures, 1 table; to appear in Proc. Huntsville Gamma-ray Burst Symposium, AIPC (C. Meegan, N. Gehrels and C. Kouveliotou, eds.), in press
Bibliographic Code:
2009arXiv0904.2210G

Abstract

The Energetic X-ray Imaging Survey Telescope (EXIST) mission concept is optimized for study of high-z GRBs as probes of the early Universe. With a High Energy Telescope (HET) incorporating a 4.5m^2 5-600keV (CZT; 0.6mm pixels) detector plane for coded aperture imaging a 90deg x 70deg (>10% coding fraction) field of view with 2' resolution and <20">5 sigma sources, EXIST will perform rapid (<200sec) r =" 3000" r ="30">7, EXIST will open a new era in studies of the early Universe as well as carry out a rich program of AGN and transient-source science. An overview of the GRB science objectives and a brief discussion of the overall mission design and operations is given, and example high-z GRB IRT spectra are shown. EXIST is being proposed to the Astro2010 Decadal Survey as a 5 year Medium Class mission that could be launched as early as 2017.
Bibtex entry for this abstract Preferred format for this abstract (see Preferences)

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