COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2303 Konkoly Observatory Budapest 28 March 1983 HU ISSN 0374-0676 A PHOTOELECTRIC SECONDARY MINIMUM OF AR Lac The first observations from the new Dark Sky Observatory at Appalachian State University have yielded times of minima in two colors for a secondary eclipse of AR Lacertae. The observations were made with the 46 cm telescope and photoelectric photometer equipped with standard UBV filters and an uncooled 1P21 photomultiplier tube. The instrument, in fact, is the same as used by Caton et al. (1977). The amplifier output voltage is converted to a frequency and averaged by a Commodore 4016 microcomputer. The comparison star used was BD+47d3711, approximately three degrees away and almost identical in color to AR Lac. Effects of differential extinction were not removed, nor were the data converted to standard UBV. The reduced data were analyzed using the method of Kwee and Van Woerden (1956), using a computer program by Mallama (1982). The resulting times of minima for the two colors are: Color Hel. J.D. Mean Error ---------------------------------- visual 2444898.6828 + 0.0011 blue .6869 + .0023 ---------------------------------- I am grateful to the University of Florida for the loan of their photometer. D. B. CATON Department of Physics and Astronomy Appalachian State University Boone, North Carolina 28608 U.S.A. References: Caton, D.B., Fallon, F.W. and Wilson, R.E., 1977, Publ. A.S.P. 89, 530 [BIBCODE 1977PASP...89..530C ] Kwee, K.K. and Van Woerden, H., 1956, B.A.N. 12, 327 [BIBCODE 1956BAN....12..327K ] Mallama, A.D., 1982, I.A.A.P. Comm. No. 7, 14 [BIBCODE 1982IAPPP...7...14M ]