dington18-effect on convergence20 tests to fix the probability distribution of matter21 mass map of galaxies in the 2dFGRS22 bias of galaxies in the 2dFGRS23 galaxy density contrast in the galaxy redshift survey24 halo model of the galaxy power spectrum25 halo model of the matter power spectrum26 co-evolution of galaxies and dark matter27 metagalaxy (galaxy groups)28 massive dark matter haloes29 supercluster dynamics30 for field galaxies only31 the mass-clustering relation in the field32 The correlation between galaxy and mass bias33 halo bias34 local density field35 fit to the shape of the mass and galaxy correlation field36 halo bias mass scaling relation37 halo and galaxy bias scaling relation38 halo bias and the primordial non-Gaussianity39 power spectra and bispectrum40 parameter distribution41 and cosmological parameters42 local halo bias at different redshift43 well motivated cosmology44 lensing constraints on cosmology45 effect of the small scale power on cosmological inference46 lensing constraints on cosmology47 effect of the small scale power on non-linear halo bias48 cosmological constraints from photometric redshift surveys49 effect of small scale power on constraints on cosmology50 constraints on cosmology using supernova data51 parameter dependence of halo bias52 number of halo samples per redshift (for statistical inference)
Last Update: 01 April 2014.
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A special weekend that we have been waiting for is finally here. We’re leaving cold weather behind and turning our focus to autumn. We’re not sure if it’s the change of the weather or the “back to school” theme of the world, but we’re feeling like there is a sense of change.
“It’s back to school” is what we’ve been hearing for a few days. We’ve seen all the signs and props hanging in our front lawn telling us the same. We can even hear the crunching of leaves in the backyard.
“We’re going back to school” is what we’re feeling. Autumn is a time to jump back into school
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