Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21924809s&link_type=abstract
American Astronomical Society, AAS Meeting #219, #248.09
Astronomy and Astrophysics
Astronomy
Scientific paper
We present measurements of the triaxial dark matter halo shapes and alignment correlation functions in the Millennium and Millennium-2 N-body simulations. We largely confirm previous results on the distributions of halo axis ratios as a function of halo mass, but we show that the median angle between halo major axes at different halo radii can vary by a factor of 2 between the Millennium-1 and 2 simulations because of the different mass resolution. Thus error in the shape determinations from limited resolution is potentially degenerate with the misalignment of halo inner and outer shapes used to constrain BCG alignments in previous works. We also present fits to the 3-D halo-halo and halo-mass alignment correlation functions that are necessary ingredients to triaxial halo models for large-scale structure and models for galaxy intrinsic alignments as contaminants for cosmic shear surveys. We measure strong alignments between halos of all masses and the surrounding dark matter overdensities out to several tens of Megaparsecs, in agreement with observed shear-galaxy and cluster shape correlations. We use these measurements to forecast the contribution to the weak lensing signal around galaxy clusters from correlated mass along the line-of-sight. For prolate clusters with major axes aligned with the line-of-sight the fraction of the weak lensing signal from mass external to the cluster can be twice that predicted if the excess halo alignment correlation is assumed to be zero.
Cole Shaun
Frenk Carlos S.
Schneider Michael
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