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.