The d05 and COSMOS field

After doing a pretty basic but robust modelling of the N(z) of the data in the d05 and COSMOS field, I think I might have my first reasonable approximation of a xi(s) for the riz AAOmega data. There still seems to be (serious) issues regarding the COSMOS field (and subsequently the whole sample) but the d05 data is looking v. promising.

Among the telescope deadlines, I'm gonna to try and do a little bit of work for Croom and Sadler (both Sydney) on the radio clustering of the 2SLAQ LRGs this week.