<?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%">Zhu, Guangtun</style></author><author><style face="normal" font="default" size="100%">Blanton, Michael R.</style></author><author><style face="normal" font="default" size="100%">Burles, Scott M.</style></author><author><style face="normal" font="default" size="100%">Coil, Alison L.</style></author><author><style face="normal" font="default" size="100%">Cool, Richard J.</style></author><author><style face="normal" font="default" size="100%">Eisenstein, Daniel J.</style></author><author><style face="normal" font="default" size="100%">Moustakas, John</style></author><author><style face="normal" font="default" size="100%">Kenneth C. Wong</style></author><author><style face="normal" font="default" size="100%">Aird, James</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">PRIMUS: Obscured Star Formation on the Red Sequence</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%">2011</style></year><pub-dates><date><style  face="normal" font="default" size="100%">January 1, 2011</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://adsabs.harvard.edu/abs/2011ApJ...726..110Z</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">726</style></volume><pages><style face="normal" font="default" size="100%">110</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 quantify the fraction of galaxies at moderate redshifts (0.1 &amp;lt; z&amp;lt; 0.5) that appear red-and-dead in the optical, but in fact containobscured star formation detectable in the infrared (IR), with the PRIsmMUlti-object Survey (PRIMUS). PRIMUS has measured ~120,000 robust&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:1011.4308</style></custom3></record></records></xml>