  The Wide Angle Search for Planets (WASP) photometrically surveys a large
number of nearby stars to uncover candidate extrasolar planet systems by virtue
of small-amplitude lightcurve dips on a < 5-day timescale typical of the
``Hot-Jupiters.'' Observations with the SuperWASP-North instrument between
April and September 2004 produced a rich photometric dataset of some 1.3
billion datapoints from 6.7 million stars. Our custom-built data acquisition
and processing system produces ~0.02 mag photometric precision at V=13.
  We present the transit-candidates in the 03h-06h RA range. Of 141,895
lightcurves with sufficient sampling to provide adequate coverage, 2688 show
statistically significant transit-like periodicities. Of these, 44 pass visual
inspection of the lightcurve, of which 24 are removed through a set of cuts on
the statistical significance of artefacts. All but 4 of the remaining 20
objects are removed when prior information at higher spatial-resolution from
existing catalogues is taken into account. Of the four candidates remaining,
one is considered a good candidate for follow-up observations with three
further second-priority targets. We provide detailed information on these
candidates, as well as a selection of the false-positives and astrophysical
false-alarms that were eliminated, and discuss briefly the impact of sampling
on our results.
