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The evolution of the OII, H\beta and OIII emission-line luminosity functions

, , , , , , , , , , , , , , and . (2016)cite arxiv:1605.02875Comment: 11 pages. Submitted to MNRAS. Data available at http://projects.ift.uam-csic.es/skies-universes/ via the page emission line luminosity functions.

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The 0.1<z<1.65 evolution of the bright end of the OII luminosity function, , , , , , , , , and 26 other author(s). (2014)cite arxiv:1408.1523Comment: 20 pages, 22 Figures, submitted.Discovery of Massive, Mostly Star-formation Quenched Galaxies with Extremely Large Lyman-alpha Equivalent Widths at z ~ 3, , , , , , , , , and 14 other author(s). (2015)cite arxiv:1507.04439Comment: Accepted for publication in ApJ Letters on 15th July, 2015. 6 pages including 3 figures and 2 tables.The evolution of the OII, H\beta and OIII emission-line luminosity functions, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1605.02875Comment: 11 pages. Submitted to MNRAS. Data available at http://projects.ift.uam-csic.es/skies-universes/ via the page emission line luminosity functions.Dancing in the dark: galactic properties trace spin swings along the cosmic web, , , , , , , , , and 23 other author(s). (2014)cite arxiv:1402.1165Comment: 17 pages, 20 pages, submitted to MNRAS, comments are welcome, movies and pictures of the simulation can be found at this address http://horizon-AGN.projet-horizon.fr.Lyman-alpha Forest Tomography from Background Galaxies: The First Megaparsec-Resolution Large-Scale Structure Map at z>2, , , , , , , , , and 14 other author(s). (2014)cite arxiv:1409.5632Comment: Accepted for publication in Astrophysical Journal Letters; 8 pages and 5 figures.The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe, , , , , , , , , and 167 other author(s). (2016)cite arxiv:1606.00043Comment: 210 pages, 91 figures. Exposure draft. Appendices to the Detailed Science Case can be found at http://mse.cfht.hawaii.edu/docs/.