Radio cross-correlation and VVDS

Managed to finished off the 2SLAQ LRG-Radio Source cross-correlation for Sadler (Sydney) yesterday. Looks as if the Radio sources are more strongly clustered than the LRG autocorrelation, though, as always some more checks are needed. However, as suggested by Croom (Sydney), this can lead (via some assumptions!) to DM halo masses. V. interesting.

Also v. interesting was Meneux (INAF-IASF Milano, INAF-OA Merate) short seminar re-capping the recent results from the VIMOS VLT Deep Survey. Anyway, more about this later once I've considered the thesis implications (if any!!)