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J. R. Webb, E. S. Howard, G. Azarnia (Florida International University and the SARA Observatory), B. R. Kent (Cornell University)
We present a long-term calibrated light curve of PKS 1622-297. All of the observations were collected with the SARA telescope from 1995 to present and reduced using a recently published calibration sequence. We also discuss the optical variations in relation to the published high energy outbursts. This research is funded by NSF grant 0307537.
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.