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The most luminous quasars do not live in the most massive dark matter haloes at any redshift, , , , and . (2013)cite arxiv:1305.2199Comment: 11 pages, 6 figures, submitted to MNRAS (comments are welcome).The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology, , , , and . (2011)cite arxiv:1105.3731 Comment: 17 pages, 11 figures. Submitted to MNRAS.The large-scale structure of the Universe, , and . Nature, (2006)Galaxy And Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies, , , , , , , , , and 24 other author(s). (2011)cite arxiv:1107.0141Comment: 15 pages, 8 figures, accepted by MNRAS.Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations, , , , , , , , , and 2 other author(s). (2014)cite arxiv:1410.3485Comment: 19 pages, 7 figures; comments welcome.Simulations of the formation, evolution and clustering of galaxies and quasars, , , , , , , , , and 7 other author(s). Nature, (June 2005)Galaxy And Mass Assembly (GAMA): The star formation rate dependence of the stellar initial mass function, , , , , , , , , and 28 other author(s). (2011)cite arxiv:1104.2379 Comment: 18 pages, 15 figures, accepted for publication in MNRAS. Image resolution has been reduced. For the full resolution version, see http://www.gama-survey.org/pubs/papers/imf_sfr.pdf.The Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation, , , , , , , , , and 13 other author(s). (2011)cite arxiv:1112.0315Comment: 26 pages, 15 figures, submitted to MNRAS. High resolution figures and additional images can be found at http://www.aip.de/People/cscannapieco/aquila/.Principles of supernova-driven winds, , , , and . (2011)cite arxiv:1111.2529 Comment: 13 pages, 13 figures.The role of black holes in galaxy formation and evolution, , , , , , , , , and 7 other author(s). Nature, (2009)