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We have observed a sample of Delta Scuti stars discovered by the ROTSEcollaboration in 1999 with Super-LOTIS in order to characterize changes intheir pulsation periods over a time baseline of roughly three years. Achievingthese goals required the creation of an automated astrometric and photometricdata reduction pipeline for the Super-LOTIS camera. Applying this pipeline todata from a June 2002 observing campaign, we detect pulsations in 18 objects,and find that in two cases the periods have changed significantly over thethree years between the ROTSE and Super-LOTIS observations. Since theorypredicts that evolutionary period changes should be quite small, sources ofnon-evolutionary period changes due to the interactions of pulsations modes arediscussed.Comment: 9 pages, 3 figures, 2 tables. Accepted for publication in A&

A search for period changes inδScuti stars with the super-LOTIS sky patrol system