COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1354 Konkoly Observatory Budapest 1977 October 24 PHOTOELECTRIC OBSERVATIONS OF THE FLARE STAR BD + 13d2618 IN 1973, 1974 Continuous photoelectric monitoring of the flare star BD +13deg2618 has been carried out at the Stephanion Observatory (lambda=-22d49'44", phi=+37d45'15") during the years 1973, 1974 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 ubv system to the international UBV system is given by the following equations: for the time interval from 9-4-1973 to 25-4-1973 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 for the time interval from 5-5-1973 to 6-5-1973 V = v_0 + 0.070(b-v)_0+1.865 B-V = 0.753 + 1.030(b-v)_0 U-B =-1.379 + 1.021(u-b)_0 and for the time interval from 20-4-1974 to 23-4-1974 V = v_0 -0.011(b-v)_0+2.445 B-V = 0.848 + 0.992(b-v)_0 U-B =-1.632 + 0.999(u-b)_0 The monitoring intervals in UT as well as the total monitoring time for each night are given in the Tables Ia, Ib. Any interruption of more than one minute has been noted. In the fourth column of Tables Ia, Ib the standard deviation of random noise fluctuation sigma(mag)= 2.5 log(I_0+sigma)/I_0 for different times (UT) of the corresponding monitoring interval is given. During the 10.23 hours of monitoring time no flare was observed. Table Ia Monitoring Intervals in 1973 Date Monitoring Intervals Total Monitoring sigma(U.T.) 1973 (U.T.) Time April 20h53m-21h23m,21h27m-21h58m 0.015(21h01m),0.012 9-10 22 03 -22 27, 00 19 -00 31, (21h55m),0.015(22 13), 00 33 -00 35, 00 59 -01 16. 01h56m 0.014(00 25). 20 19 48 -20 11 23 0.020(20 09). 22 20 53 -20 56, 21 00 -21 25 28 0.015(21 12) 24-25 20 36 -21 08, 21 12 -21 34, 0.015(20 57),0.014 23 12 -23 17, 23 22 -23 32, (21 24),0.020(23 54), 23 36 -23 48, 23 50 -00 04, 0.024(00 27),0.034 00 09 -00 22, 00 24 -00 30, (01 14),0.037(01 31). 00 46 -01 04, 01 07 -01 18, 01 22 -01 36. 02 45 25 20 18 -20 39 21 0.013(20 25) May 5-6 22 53 -23 01, 23 05 -23 24, 0.012(22 55),0.014 23 29 -23 50, 23 53 -00 01, (23 15),0.011(23 35), 00 10 -00 20, 00 22 -00 28 01 12 0.015(00 16) Total 07h05m Table Ib Monitoring Intervals in 1974 Date Monitoring Intervals Total Monitoring sigma(U.T.) 1974 (U.T) Time April 20 00h41m-01h23m,01h56m-01h56m 0.017(01h06m),0.018 02 00 -02 28, 01h18m (02 04) 22-23 23 59 -00 30, 00 33 -00 55, 0.012(00 12),0.015 01 02 -01 32, 01 48 -02 12 01 51 (00 38),0.013(01 05), 0.022(01 53). Total 03h09m G. KAREKLIDIS, F. MAHMOUD, L.N. MAVRIDIS, D. STAVRIDIS H.ZERVAKI - ZOEROU Department of Geodetic Astronomy University of Thessaloniki Reference: Andrews, A.D., Chugainov, P.F., Gershberg, R.E. and Oskanian, V.S. 1969, I.B.V.S. No. 326