Previous | Session 75 | Next | Author Index | Block Schedule
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.
If you would like more information about this abstract, please follow the link to http://people.clemson.edu/~kgarime/burst/index.php. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: email@example.com
Previous | Session 75 | Next
Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.