Photometric Analysis with CONCAM Sky Monitoring Data

Details Photometric Analysis with CONCAM Sky Monitoring Data Photometric Analysis with CONCAM Sky Monitoring Data

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...19711508p&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #115.08; Bulletin of the American Astronomical Society, Vol. 32, p.1599

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Scientific paper

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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