Photoelectric timings are reported for 276 lunar occultation events which were observed between March 1975 and February 1976. The timings (in UTC) are based on Loran G equipment of a lunar laser-ranging group or on WWV signals. Angular diameters are determined for HR 5301, HD 176124, Chi-1-Orionis, and HR 601. Twenty cases of possible or actual double stars, including Beta Capricorni, are noted along with one probable triple system (51 Piscium). Several technical and computational difficulties encountered in this program are discussed.
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Africano et al. (1976) studied this question.
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