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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 Faint-end of the UV Luminosity Function at z~6 to z~8: Combined Constraints from the Hubble Frontier Fields Clusters and Parallels, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1509.06764Comment: 13 pages, 10 figures, 4 tables, submitted to ApJ.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.Cosmological Constraints from Strong Gravitational Lensing in Clusters of Galaxies, , , , , , and . Science, 329 (5994): 924-927 (2010)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/.Warm-hot baryons comprise 5-10 per cent of filaments in the cosmic web, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1512.00454Comment: To appear in the December 3 edition of Nature.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 Origin and Evolution of Metallicity Gradients: Probing the Mode of Mass Assembly at z=2, , , and . (2012)cite arxiv:1207.4489Comment: Submitted to ApJ.Halo Mass-Concentration Relation at High-Mass End, , , , , , , , and . (2021)cite arxiv:2108.03252Comment: 12 pages, 5 figures, accepted by ApJ.