Info from Aladin:
RA, Dec (J2000) 16 46 01.61 +07 18 50.8 mag 11.69
John Greaves, 2002 July 13
GSC 0396 1222 has observations for 4 nights (plus a very small number for a fifth night that don't effect the overall point but will be ignored here). On one of these nights there is a roughly 1.1 magnitude dip in V, and around +0.4 reddening in V-I. Unfortunately this latter is only from 11 observations spanning around 54 minutes and insufficient to give much indication of lightcurve behaviour, so other independent effects on that night that did not occur on the other nights could be responsible. Therefore GSC 0396 0166 lying at around 7 arcmins, which has a similar number of observations covering the same 4 nights, is used as a check star. Any anomalous weather or other behaviour on the night in question would be expected to affect both stars, not just one of them. The situation is easiest depicted by the attached graph (small gif) where x axis is JD, y axis V mag, dots are GSC 0396 1222, the suspected Algol (ie type EA), and + symbols the "check star" GSC 0396 0166. This object is not in any variability catalogues that I can see. I band data suggests that the eclipse may have been near minimum, but V band data is a bit too scattered to comment (Tom did say limiting magnitude was not as deep in Summer). To have caught it exactly at minimum is a bit coincidental though. This would be an excellent candidate for visual observers to follow up. There is no indication whatsoever with one minimum as to when any next eclipse would occur. If this star was included as part of a visual programme any future eclipse seen would be a _confirmation_ observation, as it is as yet not even certain that the detection is valid (though looking fairly likely). The observing regimes visual observers follow are the ones most likely to come across such an occurrence, and the amplitude of variation sufficient for any detected eclipse to be evident enough. A handful of eclipses are needed to be able to guesstimate a preliminary period.
John Greave's light curve from the July dataset: