<?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%">Zehavi, Idit</style></author><author><style face="normal" font="default" size="100%">Hogg, David W.</style></author><author><style face="normal" font="default" size="100%">Scoccimarro, Roman</style></author><author><style face="normal" font="default" size="100%">Blanton, Michael R.</style></author><author><style face="normal" font="default" size="100%">Nichol, Robert C.</style></author><author><style face="normal" font="default" size="100%">Scranton, Ryan</style></author><author><style face="normal" font="default" size="100%">Seo, Hee-Jong</style></author><author><style face="normal" font="default" size="100%">Tegmark, Max</style></author><author><style face="normal" font="default" size="100%">Zheng, Zheng</style></author><author><style face="normal" font="default" size="100%">Anderson, Scott F.</style></author><author><style face="normal" font="default" size="100%">Annis, Jim</style></author><author><style face="normal" font="default" size="100%">Bahcall, Neta</style></author><author><style face="normal" font="default" size="100%">Brinkmann, Jon</style></author><author><style face="normal" font="default" size="100%">Burles, Scott</style></author><author><style face="normal" font="default" size="100%">Castander, Francisco J.</style></author><author><style face="normal" font="default" size="100%">Connolly, Andrew</style></author><author><style face="normal" font="default" size="100%">Csabai, Istvan</style></author><author><style face="normal" font="default" size="100%">Doi, Mamoru</style></author><author><style face="normal" font="default" size="100%">Fukugita, Masataka</style></author><author><style face="normal" font="default" size="100%">Frieman, Joshua A.</style></author><author><style face="normal" font="default" size="100%">Glazebrook, Karl</style></author><author><style face="normal" font="default" size="100%">Gunn, James E.</style></author><author><style face="normal" font="default" size="100%">Hendry, John S.</style></author><author><style face="normal" font="default" size="100%">Hennessy, Gregory</style></author><author><style face="normal" font="default" size="100%">Ivezić, Zeljko</style></author><author><style face="normal" font="default" size="100%">Kent, Stephen</style></author><author><style face="normal" font="default" size="100%">Knapp, Gillian R.</style></author><author><style face="normal" font="default" size="100%">Lin, Huan</style></author><author><style face="normal" font="default" size="100%">Loh, Yeong-Shang</style></author><author><style face="normal" font="default" size="100%">Lupton, Robert H.</style></author><author><style face="normal" font="default" size="100%">Margon, Bruce</style></author><author><style face="normal" font="default" size="100%">McKay, Timothy A.</style></author><author><style face="normal" font="default" size="100%">Meiksin, Avery</style></author><author><style face="normal" font="default" size="100%">Munn, Jeffery A.</style></author><author><style face="normal" font="default" size="100%">Pope, Adrian</style></author><author><style face="normal" font="default" size="100%">Richmond, Michael W.</style></author><author><style face="normal" font="default" size="100%">Schlegel, David</style></author><author><style face="normal" font="default" size="100%">Schneider, Donald P.</style></author><author><style face="normal" font="default" size="100%">Shimasaku, Kazuhiro</style></author><author><style face="normal" font="default" size="100%">Stoughton, Christopher</style></author><author><style face="normal" font="default" size="100%">Strauss, Michael A.</style></author><author><style face="normal" font="default" size="100%">SubbaRao, Mark</style></author><author><style face="normal" font="default" size="100%">Szalay, Alexander S.</style></author><author><style face="normal" font="default" size="100%">Szapudi, István</style></author><author><style face="normal" font="default" size="100%">Tucker, Douglas L.</style></author><author><style face="normal" font="default" size="100%">Yanny, Brian</style></author><author><style face="normal" font="default" size="100%">York, Donald G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies</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%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">November 1, 2005</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://adsabs.harvard.edu/abs/2005ApJ...633..560E</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">633</style></volume><pages><style face="normal" font="default" size="100%">560-574</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 present the large-scale correlation function measured from aspectroscopic sample of 46,748 luminous red galaxies from the SloanDigital Sky Survey. The survey region covers 0.72 h&lt;sup&gt;-3&lt;/sup&gt;Gpc&lt;sup&gt;3&lt;/sup&gt; over 3816 deg&lt;sup&gt;2&lt;/sup&gt; and 0.16-1 Mpcseparation that is an excellent match to the predicted shape andlocation of the imprint of the recombination-epoch acoustic oscillationson the low-redshift clustering of matter. This detection demonstratesthe linear growth of structure by gravitational instability betweenz~1000 and the present and confirms a firm prediction of the standardcosmological theory. The acoustic peak provides a standard ruler bywhich we can measure the ratio of the distances to z=0.35 and z=1089 to&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/0501171</style></custom3></record></records></xml>