Using the VUDS-DR1 we kindly request that you make reference to the DR1 presentation (Tasca et al. arXiv:1602.01842), to the VUDS survey reference paper (Le Fèvre et al., 2015, A&A, 576, 79), and acknowledge the use of these data:
"Based on data obtained with the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large Program 185.A-0791, and made available by the VUDS team at the CESAM data center, Laboratoire d'Astrophysique de Marseille, France."
"The HST data matched to the VUDS-DR1 are described in Grogin et al. (2011) and Koekemoer et al. (2011) for CANDELS and include data from the ERS (Windhorst et al. 2011)."
When using data from the VVDS database in publications, please include the following acknowledgements: This research uses data from the VIMOS VLT Deep Survey, obtained from the VVDS database operated by Cesam, Laboratoire d'Astrophysique de Marseille, France.
If you are using GAMA DR2 data in a publication then please cite the DR2 paper (Liske et al. 2015) and acknowledge GAMA using the following text :
GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue 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 programmes 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/.
Any use of these data should explicitly state that they come from the Final Release of 6dFGS and cite both the 6dGS DR3 paper (Jones et al 2009) as well as the original 6dFGS survey paper (Jones et al 2004, MNRAS 355, 747).
The 2004 paper remains the most comprehensive description of the survey but the 2009 paper details many important subsequent developments and changes.