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The resolution bias: low resolution feedback simulations are better at destroying galaxies

, , and . (2015)cite arxiv:1507.08283Comment: 15 pages, 12 figures, accepted for publication in MNRAS.

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The resolution bias: low resolution feedback simulations are better at destroying galaxies, , and . (2015)cite arxiv:1507.08283Comment: 15 pages, 12 figures, accepted for publication in MNRAS.Positive metallicity correlation for coreless giant planets. (Nov 19, 2014)The paradox of youth for ALMA planet candidates. (2020)cite arxiv:2001.06376Comment: Accepted to MNRAS.Dynamic Monte Carlo radiation transfer in SPH. Radiation pressure force implementation, , and . (May 2009)Quasar feedback: accelerated star formation and chaotic accretion, and . (2012)cite arxiv:1207.7200Comment: 7 pages. Submitted to MNRAS (version addressing referee's comments).