The observations reported here were obtained in the course of a program of searching for eclipsing binaries which may increase our meager knowledge of the fundamental properties of stars not on the main sequence. Of the stars discussed, three (V694 Aquilae, UU Cancri, and GG Cassiopeiae), while of considerable interest, do not appear promising from this standpoint, and observation of them is being discontinued. The other two are included because of discrepancies between published information and my observations. The stars discussed are listed in Table I.