Abstract:
The short-period eclipsing binary V Crateris is observed in the B and V colors of Johnson and Morgan's UBV system with attention given to the results from comparison and check stars. Magnitude differences are listed, and the standard observational error is given at 0.010 mag both for V and B filters. Observational data for V Crateris are given with the heliocentric Julian day and the magnitude difference in the standard system.
