dHvA measurements have been made on the 32 Kelvin cubic superconductor
Ba0.6K0.4BiO3 (BKBO) using a new and non-destructive 50 Tesla pulsed
field magnet at the NHMFL at Los Alamos, as well as in an 18 T superco
nducting magnet at Louisiana State University. Data were taken with th
e magnetic field aligned along the [001] crystallographic direction. S
ample temperatures were varied from 1.5 to 3.9 Kelvin. The pulsed fiel
ds employed were high enough to drive the system well into the normal
state. An analysis of these results showed that the frequencies of the
observed dHvA oscillations arose from a several Fermi surface sheets.
One cross-section was nearly identical with that predicted by a new L
DA band calculation.