@article{11190a6c79de49ec8282c5a243c30993,
title = "The 0.1 < z < 1.65 evolution of the bright end of the [O II] luminosity function",
abstract = "We present the [OII] (λλ3729,3726) luminosity function measured in the redshift range 0.1 ",
author = "Johan Comparat and Johan Richard and Kneib, {Jean Paul} and Olivier Ilbert and Violeta Gonzalez-Perez and Laurence Tresse and Julien Zoubian and Stephane Arnouts and Brownstein, {Joel R.} and Carlton Baugh and Timothee Delubac and Anne Ealet and Stephanie Escoffier and Jian Ge and Eric Jullo and Cedric Lacey and Ross, {Nicholas P.} and David Schlegel and Schneider, {Donald P.} and Oliver Steele and Lidia Tasca and Christophe Yeche and Michael Lesser and Zhaoji Jiang and Yipeng Jing and Zhou Fan and Xiaohui Fan and Jun Ma and Jundan Nie and Jiali Wang and Zhenyu Wu and Tianmeng Zhang and Xu Zhou and Zhimin Zhou and Hu Zou",
note = "Funding Information: We thank Alvaro Orsi for sending us his model predictions and for the useful discussion. We thank the referee for constructive and insightful comments on the draft. J.C. acknowledges financial support from MINECO (Spain) under project number AYA2012-31101. J.R. acknowledges support from the ERC starting grant CALENDS. J.P.K. and T.D. acknowledge support from the LIDA ERC advanced grant. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. The BOSS French Participation Group is supported by Agence Nationale de la Recherche under grant ANR-08-BLAN-0222. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1, and STFC DiRAC Operations grant ST/K003267/1 and Durham University. DiRAC is part of the National E-Infrastructure. V.G.P. acknowledges support from a European Research Council Starting Grant (DEGAS-259586) and the Science and Technology Facilities Council (grant number ST/F001166/1). Based on observations obtained with MegaPrime/Megacam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l{\textquoteright}Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. The SCUSS is funded by the Main Direction Program of Knowledge Innovation of Chinese Academy of Sciences (No. KJCX2-EW-T06). It is also an international cooperative project between National Astronomical Observatories, Chinese Academy of Sciences and Steward Observatory, University of Arizona, USA. Technical supports and observational assistances of the Bok telescope are provided by Steward Observatory. The project is managed by the National Astronomical Observatory of China and Shanghai Astronomical Observatory. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalog is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org . Publisher Copyright: {\textcopyright} ESO 2015.",
year = "2015",
month = mar,
day = "1",
doi = "10.1051/0004-6361/201424767",
language = "English (US)",
volume = "575",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",
}