<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Seo, Hee-Jong</style></author><author><style face="normal" font="default" size="100%">Eckel, Jonathan</style></author><author><style face="normal" font="default" size="100%">Eisenstein, Daniel J.</style></author><author><style face="normal" font="default" size="100%">Mehta, Kushal</style></author><author><style face="normal" font="default" size="100%">Metchnik, Marc</style></author><author><style face="normal" font="default" size="100%">Padmanabhan, Nikhil</style></author><author><style face="normal" font="default" size="100%">Pinto, Phillip</style></author><author><style face="normal" font="default" size="100%">Takahashi, Ryuichi</style></author><author><style face="normal" font="default" size="100%">White, Martin</style></author><author><style face="normal" font="default" size="100%">Xu, Xiaoying</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">High-precision Predictions for the Acoustic Scale in the Nonlinear Regime</style></title><secondary-title><style face="normal" font="default" size="100%">The Astrophysical Journal</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2010</style></year><pub-dates><date><style  face="normal" font="default" size="100%">September 1, 201</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://adsabs.harvard.edu/abs/2010ApJ...720.1650S</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">720</style></volume><pages><style face="normal" font="default" size="100%">1650-1667</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We measure shifts of the acoustic scale due to nonlinear growth andredshift distortions to a high precision using a very large volume ofhigh-force-resolution simulations. We compare results from various setsof simulations that differ in their force, volume, and mass resolution.We find a consistency within 1.5σ for shift values from differentsimulations and derive shift α(z) - 1 = (0.300 ± 0.015)&lt;/p&gt;
</style></abstract><notes><style face="normal" font="default" size="100%">n/a</style></notes><custom3><style face="normal" font="default" size="100%">eprintid: arXiv:0910.5005</style></custom3></record></records></xml>