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The Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation

, , , , , , , , , , , , , , , , , , , , , , and . (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/.

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The spectral evolution of the first Galaxies. III. Simulated James Webb Space Telescope spectra of reionization-epoch galaxies with Lyman continuum leakage, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1608.08217Comment: 12 pages, 7 figures, submitted to ApJ. Model grids are available from http://www.astro.uu.se/~ez/lycan/lycan.html.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.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/.The VANDELS survey: Dust attenuation in star-forming galaxies at $z=3-4$, , , , , , , , , and 7 other author(s). (2017)cite arxiv:1712.01292Comment: 15 pages, 11 figures, submitted to MNRAS.