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The on-orbit calibration of the Fermi Large Area Telescope

机译:费米大面积望远镜的在轨校准

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摘要

The Large Area Telescope (LAT) on-board the Fermi Gamma-ray Space Telescope began its on-orbit operations on June 23, 2008. Calibrations, defined in a generic sense, correspond to synchronization of trigger signals, optimization of delays for latching data, determination of detector thresholds, gains and responses, evaluation of the perimeter of the South Atlantic Anomaly (SAA), measurements of live time, of absolute time, and internal and spacecraft boresight alignments. Here we describe on-orbit calibration results obtained using known astrophysical sources, galactic cosmic rays, and charge injection into the front-end electronics of each detector. Instrument response functions will be described in a separate publication. This paper demonstrates the stability of calibrations and describes minor changes observed since launch. These results have been used to calibrate the LAT datasets to be publicly released in August 2009.
机译:费米伽玛射线太空望远镜上的大面积望远镜(LAT)于2008年6月23日开始在轨运行。从一般意义上讲,校准涉及触发信号的同步,对锁存数据的延迟的优化。 ,确定探测器阈值,增益和响应,评估南大西洋异常(SAA)的周长,实时时间,绝对时间以及内部和航天器视轴对准的测量。在这里,我们描述了使用已知的天体物理学来源,银河系宇宙射线以及向每个探测器的前端电子装置注入电荷所获得的在轨校准结果。仪器响应功能将在单独的出版物中描述。本文演示了校准的稳定性,并介绍了自发射以来观察到的微小变化。这些结果已用于校准将于2009年8月公开发布的LAT数据集。

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