COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 4009 Konkoly Observatory Budapest 24 March 1994 HU ISSN 0374 - 0676 TIMES OF MINIMA OF NINE ECLIPSING BINARIES We report times of minima of eclipsing binaries derived from photometric observations made with the 0.4 m reflector at Droke Observatory near Fayetteville, Arkansas, and with the 0.6 m Lowell Telescope at Cerro Tololo Interamerican Observatory in Chile. Both photometers used pulse-counting techniques and the observations were corrected for system deadtime and atmospheric extinction. Heliocentric times of minimum were estimated by bisecting chords drawn across the minima. Uncertainties were estimated from differences in the timings in the two filters used - V and R at Droke Observatory and B and V at CTIO - and also differences between independent estimates of the times of each eclipse. Primary eclipses are designated as type 1 eclipses, secondary eclipses as type 2. Table 1 Star JD of Min Type Observatory Observer -2400000 SW CMa 49345.6754 +/- 0.0006 2 CTIO Lacy 49352.6453 +/- 0.0004 1 CTIO Lacy EK Cep 49248.6416 +/- 0.0007 1 Droke Fox V477 Cyg 49251.7117 +/- 0.0006 1 Droke Fox V1143 Cyg 49234.6144 +/- 0.0006 1 Droke Fox DI Her 49225.6702 +/- 0.0012 2 Droke Fox FS Mon 49343.7953 +/- 0.0005 1 CTIO Lacy GG Ori 49355.7327 +/- 0.0005 2 CTIO Lacy V530 Ori 49341.5832 +/- 0.0005 1 CTIO Lacy 49353.8048 +/- 0.0006 1 CTIO Lacy DR Vul 49228.7300 +/- 0.0007 2 Droke Fox The authors would like to thank Jorge Schwarz for his help with some of the Droke Observatory observations. CLAUD H. SANDBERG LACY GREGORY W. FOX Department of Physics University of Arkansas Fayetteville, Arkansas 72701 USA