COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 816 Konkoly Observatory Budapest 1973 August 2 PHOTOELECTRIC OBSERVATIONS OF THE FLARE STAR AD Leo Continuous photoelectric monitoring of the flare star AD Leo has been carried out at the Stephanion Astronomical Station (lambda = -22d49'44", phi = +37d45'15") during the period of cooperative optical observations of this star proposed by the IAU Working Group on Flare Stars i.e. January 27-February 9, 1973 (Chugainov, 1972) using the 30-inch Cassegrain reflector of the Department of Geodetic Astronomy University of Thessaloniki. Observations have been made with a Johnson dual channel photoelectric photometer in the B colour of the international UBV system. The telescope and photometer will be described elsewhere. Here we mention only that the transformation of our instrumental UBV system to the international UBV system is given by the following equations: V = v_0 + 0.039(b-v)_0 + 1.560, (B-V) = 0.737 + 1.033(b-v)_0, (U-B) = -1.365 + 1.007(u-b)_0. The monitoring intervals in UT as well as the total monitoring time for each night are given in Table 1. Any interruption of more than one minute has been noted. TABLE 1 Date Monitoring intervals(UT) Total 1973 Monitoring time Feb. 6-7 20h56m-21h13m,2114-2121,2127-2200,2203-2225, 2228-2258,2304-2333,2335-0005,0007-0101, 0104-0133. 4h11m 7-8 2102-2130,2133-2159,2204-2234,2237-2314, 2317-2337,2343-0033,0035-0110. 3h46m Total 7h57m During the 7.95 hours of monitoring time no flare was observed. It should be noted that the standard deviation of random noise fluctuation sigma(mag) = 2.5{log(I_0 + sigma)/I_0} (Andrews et al., 1969) was equal to sigma = 0.01m during all the monitoring time. Department of Geodetic Astronomy University of Thessaloniki, Greece. G. ASTERIADIS and L.N. MAVRIDIS References: Andrews, A.D., Chugainov, P.F., Gershberg, R.E. and Oskanian, V.S. 1969, Comm. 27 IAU, IBVS No. 326. Chugainov, P.F. 1972, Comm.27 IAU, IBVS No. 744.