Sheldon previewed his job talk for UC Davis this morning; his results—which show the cross-correlation between mass and galaxy clusters—are awesome. They strongly confirm the NFW profile and what we know about intermediate-scale clustering.
Padmanabhan (Princeton) and I discussed averaging SDSS spectra, transparency, and future massive spectroscopic surveys. No real project yet, but many on the horizon and in planning.
I prepared slides for my talk at ISCAP at Columbia tomorrow. I am going to concentrate on constraining small-scale dynamics of the dark and light sectors using galaxy interactions, mergers, and accretion.
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