Checking 206 Stardial-images from 1996 to 2000 showed
GSC 5137 507 to be a semiregular red variable star.
The period is about 110 day and the amplitude up to 0.7 mag.
Differential Photometry was done with MIRA AP 6.03 with
respect to GSC 5137-653 (=HIP94370) (V=8.06, V-I=0.63) .
The Stardial-project is one of the most fascinating aspects of the WEB,
many thanks to Peter McCullough!!