  We report the first wideband observations of pulsars C, D and J in the
globular cluster 47Tucanae (NGC 104) using the Ultra-Wideband Low (UWL)
receiver system recently installed on the Parkes 64 m radio telescope. The wide
frequency range of the UWL receiver (704-4032 MHz), along with the
well-calibrated system, allowed us to obtain flux density measurements and
polarization pulse profiles. The mean pulse profiles have significant linear
and circular polarization, allowing for determination of the Faraday rotation
measure for each pulsar. Precise measurements of the dispersion measures show a
significant deviation in the value for pulsar D compared to earlier results.
Searches for new pulsars in the cluster are on-going and we have determined
optimal bands for such searches using the Parkes UWL receiver system.
