  We present the first four years of BVRI photometry from an on-going survey to
annually monitor the photometric behavior of evolved luminous stars in M31 and
M33. Photometry was measured for 199 stars at multiple epochs, including 9
classic Luminous Blue Variables (LBVs), 22 LBV candidates, 10 post-RGB A/F type
hypergiants, and 18 B[e] supergiants. At all epochs the brightness is measured
in V and at least one other band to a precision of 0.04 -- 0.10 magnitudes down
to a limiting magnitude of 19.0 -- 19.5. Thirty three (33) stars in our survey
exhibit significant variability, including at least two classic LBVs caught in
S Doradus type outbursts. A hyper-linked version of the photometry catalog is
at: http://go.uis.edu/m31m33photcat/.
