During 2004, SuperWASP-North (La Palma) observed 6.7 million stars of V=8-15mag for up to 5 
months with the aim of identifying new bright transiting extra-solar planets. In the first 
year of operation, with only 5 10cm telescopes, several terabytes of data were collected. 
With such a vast amount of data, an automated but thorough approach to data reduction and 
transit detection was required. From 2006, a full complement of 16 cameras (at 
SuperWASP-North and SuperWASP-South (SAAO)) is in use, tripling the data flow. In this talk 
we will discuss the adapted BLS transit-detection algorithm and the filtering procedure we 
have developed to highlight genuine transiting exoplanets and reject both data artefacts and 
astrophysical false positives as far as possible. We will also outline the photometric and 
spectroscopic follow up procedure for the high priority candidates passing this filtering 
stage, and provide details of the latest results. Further details of the first 2 planets to 
emerge from the survey - from just 5 cameras in the opening 2004 season - WASP-1b and 
WASP-2b will be discussed following data from recent observations.

(To be given as a joint talk with Becky Enoch)