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K. V. Garimella, A. L. Homewood, D. H. Hartmann (Clemson University), Clemson GRB Follow-Up Team
The Clemson GRB group utilizes a partnership with the SARA consortium to follow up bursts with the 0.9-meter telescope at Kitt Peak through prescheduled and target-of-opportunity observations. While SARA is not robotic, response times can be on the order of minutes, but typically are on the order of hours. To ensure a rapid response we have developed an automated data reduction software suite. Here we describe the details of this software and example analyses of Swift-detected bursts.
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.