A-ha

Think I've fixed my AAOmega w(theta) Full/COSMOS/d05 field discrepancy. All 3 w(theta) estimates now agree (obviously within the errors!) and as usual in astronomy, solving one puzzle opens the door to several others. So I ask myself, if the angular and radial masks of said fields are sound, why do I continue to get a very flat xi(s) estimation??

Been re-reading Masjedi et al. again. I really like this paper and the conclusions about the v. low LRG-LRG merger rate still has me thinking... (AAT deadline Friday 1pm...)