<?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%">Eisenstein, Daniel J.</style></author><author><style face="normal" font="default" size="100%">Hu, Wayne</style></author><author><style face="normal" font="default" size="100%">Tegmark, Max</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Cosmic Complementarity: H 0 and Omega M from Combining Cosmic Microwave Background Experiments and Redshift Surveys</style></title><secondary-title><style face="normal" font="default" size="100%">The Astrophysical Journal Letters</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">1998</style></year><pub-dates><date><style  face="normal" font="default" size="100%">September 1, 199</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://adsabs.harvard.edu/abs/1998ApJ...504L..57E</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">504</style></volume><pages><style face="normal" font="default" size="100%">L57</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 show that the detection of acoustic oscillations in both upcomingcosmic microwave background (CMB) satellite experiments and&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:astro-ph/9805239</style></custom3></record></records></xml>