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个人简介
Over the last three years I have concentrated on the GLAST reconstruction and analysis. GLAST is a gamma ray satellite mission that will expand on the success of the previous mission, EGRET, by nearly a factor of 100. It will change high-energy astrophysics from a science of exotic examples to one of statistical analysis by providing hundreds to thousands of like objects to study.
My first two years were dominated by writing and creating the track finding and track fitting algorithms presently used in the analysis. A little over year ago my attention turned to calorimetry and overall energy determinations. Finally, with a complete reconstruction in handed, this last year has been focused on the instrument’s performance: image resolution, background separation, trigger studies and the like. For example, the GLAST science requirement document requires the difficult task of increasing a separation of signal from background noise to the range of 106 to 1 with a loss in signal of less than 20%. This task has fallen to me.
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