<?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%">Popesso, P</style></author><author><style face="normal" font="default" size="100%">Biviano, A</style></author><author><style face="normal" font="default" size="100%">Rodighiero, G</style></author><author><style face="normal" font="default" size="100%">Baronchelli, I</style></author><author><style face="normal" font="default" size="100%">Salvato, M</style></author><author><style face="normal" font="default" size="100%">Saintonge, A</style></author><author><style face="normal" font="default" size="100%">Finoguenov, A.</style></author><author><style face="normal" font="default" size="100%">Magnelli, B</style></author><author><style face="normal" font="default" size="100%">Gruppioni, C</style></author><author><style face="normal" font="default" size="100%">Pozzi, F</style></author><author><style face="normal" font="default" size="100%">others</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The evolution of the star formation activity per halo mass up to redshift\~{} 1.6 as seen by Herschel</style></title><secondary-title><style face="normal" font="default" size="100%">Astronomy &amp; Astrophysics</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2012</style></year></dates><publisher><style face="normal" font="default" size="100%">EDP sciences</style></publisher><volume><style face="normal" font="default" size="100%">537</style></volume><pages><style face="normal" font="default" size="100%">A58</style></pages><language><style face="normal" font="default" size="100%">eng</style></language></record></records></xml>