  In data from three clear nights of a WHT/UES run in 2000 Oct/Nov, and using
improved Doppler tomographic signal-analysis techniques, we have carried out a
deep search for starlight reflected from the innermost of upsilon And's three
planets. We place upper limits on the planet's radius R_p as functions of its
projected orbital velocity K_p ~ 139 sin i km/sec for various assumptions about
the wavelength-dependent geometric albedo spectrum p(\lambda) of its
atmosphere. For a grey albedo p we find R_p \sqrt{p} < 0.98 R_Jup with 0.1
percent false-alarm probability (4-sigma). For a Sudarsky et al (2000) Class V
model atmosphere, the mean albedo in our 380-676 nm bandpass is <p> ~ 0.42,
requiring R_p < 1.51 R_Jup, while an (isolated) Class IV model with <p> ~ 0.19
requires R_p < 2.23 R_Jup. The star's v sin{i} ~ 10 km/sec and estimated
rotation period P_{rot} ~ 10 d suggest a high orbital inclination i ~ 70-80
degrees. We also develop methods for assessing the false-alarm probabilities of
faint candidate detections, and for extracting information about the albedo
spectrum and other planetary parameters from faint reflected-light signals.
