回转镜望远镜及数据采集系统

Gamma-ray Bursts: 15 Years of GRB Afterglows Pub Date : 2013-11-11 DOI:10.1051/EAS/1361087

H. Lim, S. Ahmad, P. Barrillon, S. Brandt, C. Budtz-Jørgensen, A. Castro-Tirado, Pisin Chen, Yong-Jin Choi, P. Connell, S. Dagoret-Campagne, C. Eyles, B. Grossan, M. Huang, A. Jung, S. Jeong, J. Kim, Min Bin Kim, Sug-Whan Kim, Y. W. Kim, A. S. Krasnov, J. Lee, E. Linder, T. Liu, N. Lund, K. Min, G. Na, J. Nam, M. Panasyuk, I. Park, J. Řípa, V. Reglero, J. Rodrigo, G. Smoot, J. Suh, S. Svertilov, N. Vedenkin, Minzu Wang, I. Yashin

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引用次数: 0

摘要

超快闪光天文台(UFFO)旨在探测到目前尚不为人所知的伽玛射线暴(GRB)的最早时刻，从而增强对GRB机制的理解。探路者任务被提议为UFFO的缩小版，仅包含UFFO突发警报和触发望远镜(UBAT)，测量具有宽视场的x射线/伽马射线，以及具有快速响应紫外/光学光子的旋转镜望远镜(SMT)。一旦UBAT以10角秒的定位精度检测到GRB候选者，SMT就会通过快速旋转镜将候选候选对象的UV/光学光子引导到望远镜上，并提供4角秒的早期UV/光学光子测量

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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THE SLEWING MIRROR TELESCOPE AND THE DATA-ACQUISITION SYSTEM

The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understand- ing. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst Alert & Trigger Telescope (UBAT) measuring the X-ray/gamma-ray with the wide-field of view and the Slewing Mirror Telescope (SMT) with a rapid-response for the UV/optical photons. Once the UBAT detects a GRB candidate with the position accuracy of 10 arcmin, the SMT steers the UV/optical pho- tons from the candidate to the telescope by the fast rotatable mirror and provides the early UV/optical photons measurements with 4 arcsec

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Gamma-ray Bursts: 15 Years of GRB Afterglows

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