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D. Perez-Ramirez, R. J. Nemiroff, W. E. Pereira, J. B. Rafert, C. Ftaclas (Michigan Tech)
Practical data analysis techniques useful with CONtinuous CAMera (CONCAM) data are discussed. Analysis is presented of distortion near the edges of the wide CONCAM fields and how these affect the utility of data stored at http://concam.net. Preliminary photometric analyses limiting the peak optical brightness of the optical counterparts to two gamma-ray bursts, GRB000926 and GRB001005, are presented. A preliminary photometric analysis is also given for Polaris and the variability of other bright stars. We discuss potential future scientific returns of analyzing publicly archive CONCAM data available at concam.net.
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The author(s) of this abstract have provided an email address for comments about the abstract: dperez@mtu.edu