This section contains folded lightcurves and periodograms of all stars for which rotation periods were found. The light curves are broken up into three sections. The first section contains the highest quality light curves, those with FAP less than one percent. The second section contains those stars with FAPs of between one and five percent. The third section contains the lowest quality lightcurves -- those with FAPs of between five and 20%. The calculation of the FAPs and periodograms is discussed in Chapter 3. The fits to the light curves are 7th order polynomial fits to two cycles of the data. The standard deviation of the data to the fit, the Mean magnitude and amplitude from the mean to peak are given in each left hand panel The Order of the light curves is the same as the ordering in Tables , and respectively.