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W. E. Pereira, R. J. Nemiroff (Michigan Tech), D. Perez-Ramirez (ESA), J. B. Rafert (Michigan Tech), CONCAM Collaboration
The CONCAM Global Network of fisheye night sky camera continues to be sensitive to and set limits on bright pre-trigger and prompt optical emission from GRBs. Each of the currently deployed six CONCAMs are sensitive to about visual magnitude 6, but their wide fields and continuous operations give them a unique window for studying intrinsically transient phenomena such as GRBs. We present the latest results of ongoing searches and analyses, providing updated observational time/flux constraints on GRB afterglow behavior. The CONCAM project was made possible, in part, by grants from the National Science Foundation.
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The author(s) of this abstract have provided an email address for comments about the abstract: wpereira@mtu.edu
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.