  By analysis of Superwasp data, Srdoc and Bernhard (2012) have shown recently
that GSC 02626-00896 (18:09:30.34 + 32:45:13.52) is an RRc type variable
showing indications of Blazhko effect. A night by night reanalysis of the data
shows that in fact a 26 d secondary period is present in the 2004 observations.
However, no trace of this can be found in the 2007 and 2008 data. CCD
observations of the star on 19 nights in 2012 yielded a strictly repeating
light curve with a broad maximum similar to those derived from the second and
third SWASP data group. A slightly revised ephemeris Max.(HJD) =
2456069.3919(43) + 0.32272138(60) d x E could be derived. The CCD observations
also revealed three short period eclipsing variables in the field of GSC
02626-00896. The 15.16 R mag. GSC2.3 star N25F001920 (18:09:24.282
+32:44:51.72) shows 0.15 and 0.1 mag. shallow eclipses with the ephemeris
Max.(HJD) = 2456064.5155(13) + 0.389228(18) d x E. The 15.39 R mag. GSC 2.3
N25D013720 (18:09:41.141 +32:33:46.99) is a W UMa type star with the ephemeris
Min.(HJD) = 2456072.4354(4) + 0.393563(7) d x E and 0.45 mag. amplitude. The
16.13 R mag. GSC 2.3 N25D015132 (18:09:01.767 +32:36:53.59) is also a W UMa
type star with the ephemeris Min.(HJD) = 2456072.4909(2) + 0.287800(3) d x E
with an amplitude of 0.75 and 0.5 mag respectively.
