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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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Multi-wavelength consensus of large-scale linear bias, , , , , , and . (2019)cite arxiv:1909.12069Comment: 19 pages, submitted to MNRAS.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.The galaxy population in cold and warm dark matter cosmologies, , , , , , , , , and . (2016)cite arxiv:1612.04540Comment: 15 pages, 14 figures, submitted to MNRAS.The mass-metallicity relations for gas and stars in star-forming galaxies: strong outflow vs variable IMF, , , , , , and . (2017)cite arxiv:1710.11135Comment: 25 pages, 23 figures, and 5 tables. Accepted for publication to MNRAS.nIFTy Cosmology: Comparison of Galaxy Formation Models, , , , , , , , , and 26 other author(s). (2015)cite arxiv:1505.04607Comment: 35 pages, 20 figures, accepted for publication in MNRAS.