大孔径伽马暴观测站
高能天体物理现象
2009-06-05 v1 宇宙学与河外天体物理
天体物理仪器与方法
摘要
大孔径伽马暴观测站(LAGO)旨在利用高海拔站点(玻利维亚查卡尔塔亚，海拔5300米；委内瑞拉埃斯佩霍峰，海拔4750米；墨西哥内格拉山，海拔4650米)的水切伦科夫探测器(WCD)阵列，通过单粒子技术探测伽马射线暴的高能(约100 GeV)成分。高海拔的WCD为探测10 GeV - 1 TeV范围内的低伽马通量提供了独特可能性。本文将介绍该观测站的现状以及从2007年至今收集的数据。
引用
@article{arxiv.0906.0816,
title = {The Large Aperture GRB Observatory},
author = {D. Allard and C. Alvarez and H. Asorey and H. Barros and X. Bertou and M. Castillo and J. M. Chirinos and A. De Castro and S. Flores and J. Gonzalez and M. Gomez Berisso and J. Grajales and C. Guada and W. R. Guevara Day and J. Ishitsuka and J. A. Lopez and O. Martinez and A. Melfo and E. Meza and P. Miranda Loza and E. Moreno Barbosa and C. Murrugarra and L. A. Nunez and L. J. Otiniano Ormachea and G. Perez and Y. Perez and E. Ponce and J. Quispe and C. Quintero and H. Rivera and M. Rosales and A. C. Rovero and O. Saavedra and H. Salazar and J. C. Tello and R. Ticona Peralda and E. Varela and A. Velarde and L. Villasenor and D. Wahl and M. A. Zamalloa},
journal= {arXiv preprint arXiv:0906.0816},
year = {2009}
}
备注
4 pages, proceeding of 31st ICRC 2009