Checking 211 Stardial-images from 1996 to 2000 showed
GSC 5122 790 to be a semiregular variable star.
A period analysis showed the period to be 129 days.
The amplitude in the system of Stardial ist about 0.4 mag.
Differential Photometry was done with MIRA AP 6.03 with
respect to GSC 5129-29 (V=8.72, B-V=1.2).
In fact this new variable star was one of two check
stars for GSC 5129-29, the comp star of HassfortherV45.
The Stardial-project is one of the most fascinating aspects of the WEB,
many thanks to Peter McCullough!!