<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>47</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Zahorecz, Sarolta</style></author><author><style face="normal" font="default" size="100%">Jimenez-Serra, Izaskun</style></author><author><style face="normal" font="default" size="100%">Fontani, Francesco</style></author><author><style face="normal" font="default" size="100%">Immer, Katharina</style></author><author><style face="normal" font="default" size="100%">Ke Wang</style></author><author><style face="normal" font="default" size="100%">Testi, Leonardo</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Gas Phase Vs. Dust Grain Deuterated Chemistry: HdCO and D2CO in Massive Star-Forming Regions</style></title><secondary-title><style face="normal" font="default" size="100%">Getting Ready for ALMA Band 5 - Synergy with APEX/SEPIA</style></secondary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Zenodo community band5\_2017</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2017</style></year><pub-dates><date><style  face="normal" font="default" size="100%">apr</style></date></pub-dates></dates><pages><style face="normal" font="default" size="100%">32</style></pages><language><style face="normal" font="default" size="100%">eng</style></language></record></records></xml>