... correlation of the Wilkinson Microwave Anisotropy Probe WMAP 7 year temperature map and the full sky data release of the Wide field Infrared Survey Explorer galaxy map Using careful map making and masking techniques we find a positive cross correlation signal The results are fully consistent with a LambdaCDM...
.txthttp://www.phys.uu.nl/~rutten/rrtex/bibfiles/ads/abs/kovacs.txt
[ cosmic structure formation | EBOOK DOWNLOAD :COSMIC STRUCTURE FORMATION | ] ... an attractive method for DE studies Good reasons to believe that systematics are of low amplitude Physics is well known and can be modeled today SDSS 2dFGRS measures BAO and rs DV at z 0 2 z 0 35 Constraint DV 0 35 DV 0 2 1 812 is higher than predicted by LambdaCDM WMAP SNLS DV 0 35 DV 0 2 1 67 2 4 discrepancy...
.ppthttp://www.roe.ac.uk/roe/workshop/2007/talks/Percival.ppt
[ PowerPoint ] ... matter DE 1 m Spergel et al 2003 ApJS 148 175 CMB constraints on H0 WMAP gets h 0 72 0 05 by assuming a flat LambdaCDM model with spectral index n 1 But CMB observations do not directly measure the local expansion rate of the universe Thus local Hubble constant measurements are an important test of our...
.ppthttp://www.nrao.edu/astrores/darkenergy/CondonDE2.ppt
dark 