LBL INPA
Seeing in the Dark: Cosmic Shear in SDSS
Eric Huff
250 deg^2 of SDSS WL shear measurement. Systematic errors for this measurement are probably negligible compared to the statistical errors. Omega_m and sigma8 at z=0.6 constrained.
Also use galaxy scaling relations to measure lensing magnification with many times the S/N of previous magnification results. Could be superior to shear.
LBL RPM
Quantum Electrodynamics and Ultra-High Intensities
Thomas Heinzl
Strong-field quantum electrodynamics with high-intensity
1106.5104
Modeling the tidal connection between in and around galaxy clusters
Hyunmi （賢美）Song, Jounghun Lee
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