<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">J P Santos</style></author><author><style face="normal" font="default" size="100%">Chintan Shah</style></author><author><style face="normal" font="default" size="100%">José R. Crespo López-Urrutia</style></author><author><style face="normal" font="default" size="100%">Ming Feng Gu</style></author><author><style face="normal" font="default" size="100%">Thomas Pfeifer</style></author><author><style face="normal" font="default" size="100%">José Marques</style></author><author><style face="normal" font="default" size="100%">Filipe Grilo</style></author><author><style face="normal" font="default" size="100%">José Paulo Santos</style></author><author><style face="normal" font="default" size="100%">Amaro, Pedro</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s–2p and 3d–2p Line-formation Channels</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%">2019</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://doi.org/10.3847/1538-4357/ab2896</style></url></web-urls></urls><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">n/a</style></abstract><notes><style face="normal" font="default" size="100%">n/a</style></notes></record></records></xml>