We observed about 2200 emission line galaxy spectra on the COSMOS field with the VLT FORS2 instrument as a base to estimate the [OII] luminosity function at redshift greater than 1.
For more details on the [OII] LF
Please read the paper : The 0.1 < z < 1.65 evolution of the bright end of the [OII] luminosity function by Johan Comparat, Johan Richard, Jean-Paul Kneib, Olivier Ilbert, V. Gonzalez-Perez, Laurence Tresse, Julien Zoubian, Stephane Arnouts, Roland Bacon, Joel R. Brownstein, Carlton Baugh, Timothee Delubac, Anne Ealet, Stephanie Escoffier, Jian Ge, Eric Jullo, Cedric Lacey, Nicholas P. Ross, David Schlegel, Donald P. Schneider, Oliver Steele, Lidia Tasca, Christophe Yeche, Michael Lesser, Zhaoji Jiang, Yipeng Jing, Zhou Fan, Xiaohui Fan, Jun Ma, Jundan Nie, Jiali Wang, Zhenyu Wu, Tianmeng Zhang, Xu Zhou, Zhimin Zhou, Hu Zou.
To obtain the data:
You can browse through these folders to retrieve the observed spectra or the catalog.
The COSMOS evolution survey database contains very complementary catalogs and datasets to the one hosted here :
Canada-France-Hawaii Telescope Legacy Survey
The atomic line list.
last update, feb. 2016, by J. Comparat