2012

Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7

Mandelbaum, Rachel, Slosar, Anze, Baldauf, Tobias et al.

Understand

Recent studies have shown that the cross-correlation coefficient between galaxies and dark matter is very close to unity on scales outside a few virial radii of galaxy halos, independent of the details of how galaxies populate dark matter halos.

This finding makes it possible to determine the dark matter clustering from measurements of galaxy-galaxy weak lensing and galaxy clustering.
We present new cosmological parameter constraints based on large-scale measurements of spectroscopic galaxy samples from the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7).
We generalise the approach of Baldauf et al.

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