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We present the results of our Johnson B and V observations of three RR Lyraecandidate stars that we identified as likely variable stars using SDSS data.The stars were selected based upon a single epoch of photometry andspectroscopy. The stars were observed at McDonald Observatory to obtain fulllight curves. We present full light curves, measured periods, and amplitudes,as well as the results of our Fourier analysis of the light curves.

Observations and Analysis of Three Field RR Lyrae Stars Selected Using Single epoch SDSS Data