  Results of a 4 year monitoring campaign of the SMC using the Rossi X-ray
timing Explorer (RXTE) are presented. This large dataset makes possible
detailed investigation of a significant sample of SMC X-ray binaries. 8 new
X-ray pulsars were discovered and a total of 20 different systems were
detected. Spectral and timing parameters were obtained for 18. In the case of
10 pulsars, repeated outbursts were observed, allowing determination of
candidate orbital periods for these systems. We also discuss the spatial and
pulse period distributions of the SMC pulsars.
