<?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%">Ruggeri, Rossana</style></author><author><style face="normal" font="default" size="100%">Percival, Will J.</style></author><author><style face="normal" font="default" size="100%">Gil-Marín, Héctor</style></author><author><style face="normal" font="default" size="100%">Beutler, Florian</style></author><author><style face="normal" font="default" size="100%">Mueller, Eva-Maria</style></author><author><style face="normal" font="default" size="100%">Zhu, Fangzhou</style></author><author><style face="normal" font="default" size="100%">Padmanabhan, Nikhil</style></author><author><style face="normal" font="default" size="100%">Zhao, Gong-Bo</style></author><author><style face="normal" font="default" size="100%">Zarrouk, Pauline</style></author><author><style face="normal" font="default" size="100%">Sánchez, Ariel G.</style></author><author><style face="normal" font="default" size="100%">Bautista, Julian</style></author><author><style face="normal" font="default" size="100%">Brinkmann, Jonathan</style></author><author><style face="normal" font="default" size="100%">Brownstein, Joel R.</style></author><author><style face="normal" font="default" size="100%">Baumgarten, Falk</style></author><author><style face="normal" font="default" size="100%">Chuang, Chia-Hsun</style></author><author><style face="normal" font="default" size="100%">Dawson, Kyle</style></author><author><style face="normal" font="default" size="100%">Seo, Hee-Jong</style></author><author><style face="normal" font="default" size="100%">Tojeiro, Rita</style></author><author><style face="normal" font="default" size="100%">Zhao, Cheng</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift-space distortions between redshift 0.8 and 2.2</style></title><secondary-title><style face="normal" font="default" size="100%">\mnras</style></secondary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astrophysics - Cosmology and Nongalactic Astrophysics</style></keyword><keyword><style  face="normal" font="default" size="100%">cosmology: observations</style></keyword><keyword><style  face="normal" font="default" size="100%">dark energy</style></keyword><keyword><style  face="normal" font="default" size="100%">dark matter</style></keyword><keyword><style  face="normal" font="default" size="100%">large-scale structure of universe</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2019</style></year><pub-dates><date><style  face="normal" font="default" size="100%">mar</style></date></pub-dates></dates><number><style face="normal" font="default" size="100%">3</style></number><volume><style face="normal" font="default" size="100%">483</style></volume><pages><style face="normal" font="default" size="100%">3878-3887</style></pages><language><style face="normal" font="default" size="100%">eng</style></language></record></records></xml>