The BVRI catalogue of Magnier et al. (1992) contains 61,281 objects wi
thin a approximately 1 square degree region centered on the core of M3
1. We have performed deep BVI CCD photometry on approximately 0.7 squa
re degrees of the outer regions to extend the coverage to the entire d
isk of M31. Data from the two sets of observations were merged into on
e photometric system, and absolute calibration to the Johnson system w
as performed. The extended catalogue contains 485,425 objects with typ
ical completeness limits of BVRI = (20.7, 21.7, 20.2, 20.5). Photometr
ic and astrometric accuracies are approximately 4% at V = 19.5, and ap
proximately 0.8'', respectively.