I obtained the following observations good, I feel, to +-0.1 magnitude using a CCD without the benefit of on site data reduction software. I combined a calculation based on the logarithms of sky subtracted peak pixel counts with a direct visual estimate from the readout display using a 1989 AAVSO chart. (1H 1933+510 was so faint tonight that I couldn't estimate its magnitude by the above method, so I'll post those observations after they're reduced.) -- Claia Bryja CYGV503 20000728.2414 15.6V (C.Bryja) CYGV503 20000728.2544 15.7V (C.Bryja) CYGV503 20000728.2685 15.7V (C.Bryja) CYGV503 20000728.2834 15.8V (C.Bryja) CYGV503 20000728.2968 15.8V (C.Bryja) CYGV503 20000728.3117 15.7V (C.Bryja) CYGV503 20000728.3255 15.7V (C.Bryja) CYGV503 20000728.3355 15.7V (C.Bryja)