天基伽马射线望远镜 GAMMA-400 及其科学目标
天体物理仪器与方法
2013-06-27 v1
摘要
本文介绍了新型天基伽马射线望远镜 GAMMA-400 的设计。GAMMA-400 针对 100 GeV 能量进行了优化，具有最佳参数：角分辨率约 0.01 度，能量分辨率约 1%，质子排斥因子约，但能够测量能量范围从 100 MeV 到 10 TeV 的伽马射线和电子 + 正电子通量。GAMMA-400 旨在研究广泛的科学课题，例如寻找暗物质信号、研究银河系及河外伽马射线源、银河系及河外弥漫辐射、伽马射线暴，以及对宇宙射线电子 + 正电子和原子核谱进行高精度测量。
引用
@article{arxiv.1306.6175,
title = {The Space-Based Gamma-Ray Telescope GAMMA-400 and Its Scientific Goals},
author = {A. M. Galper and O. Adriani and R. L. Aptekar and I. V. Arkhangelskaja and A. I. Arkhangelskiy and G. A. Avanesov and L. Bergstrom and E. A. Bogomolov and M. Boezio and V. Bonvicini and K. A. Boyarchuk and V. A. Dogiel and Yu. V. Gusakov and M. I. Fradkin and Ch. Fuglesang and B. I. Hnatyk and V. A. Kachanov and V. V. Kadilin and V. A. Kaplin and M. D. Kheymits and V. Korepanov and J. Larsson and A. A. Leonov and F. Longo and P. Maestro and P. Marrocchesi and V. V. Mikhailov and E. Mocchiutti and A. A. Moiseev and N. Mori and I. Moskalenko and P. Yu. Naumov and P. Papini and M. Pearce and P. Picozza and M. F. Runtso and F. Ryde and R. Sparvoli and P. Spillantini and S. I. Suchkov and M. Tavani and N. P. Topchiev and A. Vacchi and E. Vannuccini and G. I. Vasiliev and Yu. T. Yurkin and N. Zampa and V. N. Zarikashvili and V. G. Zverev},
journal= {arXiv preprint arXiv:1306.6175},
year = {2013}
}
备注
6 pages, 3 figures, 1 table, submitted to to the Proceedings of the International Cosmic-Ray Conference 2013, Brazil, Rio de Janeiro