Logged on 25/08/09 14:21:54
1) Run it through the Calico-WSRT scripts with an eye on the E-Jones options
2) Try to derive a sky model based on the apparent fluxes of the sources and use that for calibration (c.f. self-calibration)
3) Make your own differential simulation to gauge the effects of pointing errors (these are incorporated into the E-Jones by shifting the response pattern on the sky).