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4 research outcomes, page 1 of 1
- publication . Article . Preprint . 2015Open Access EnglishAuthors:Andrew Pontzen; Nina Roth; Hiranya V. Peiris;Publisher: OXFORD UNIV PRESSProject: RCUK | DiRAC2: 100 Tflop/s HPC c... (ST/K000373/1), EC | COSMICDAWN (306478)
Comment: Version accepted by MNRAS; 13 pages, 6 Figures, comments still welcome
- publication . Preprint . Article . 2015Open Access EnglishAuthors:Nina Roth; Anže Slosar; Hiranya V. Peiris; Andrew Pontzen;Project: RCUK | DiRAC2: 100 Tflop/s HPC c... (ST/K000373/1), EC | COSMICDAWN (306478)
We introduce and explore "paired" cosmological simulations. A pair consists of an A and B simulation with initial conditions related by the inversion $\delta_A(x, t_{initial})=-\delta_B(x,t_{initial})$ (underdensities substituted for overdensities and vice versa). We ar...
- publication . Article . Preprint . 2017Open Access EnglishAuthors:Thomas P. Quinn; Fabio Governato; Amélie Saintonge; Hiranya V. Peiris; Michael Tremmel; Nina Roth; Marta Volonteri; Andrew Pontzen;Publisher: HAL CCSDProject: NSF | Collaborative Proposal: D... (1410012), EC | BLACK (614199), RCUK | DiRAC2: 100 Tflop/s HPC c... (ST/K000373/1), NSF | Collaborative Research: A... (1514868), EC | COSMICDAWN (306478)
We show how the interplay between active galactic nuclei (AGN) and merger history determines whether a galaxy quenches star formation at high redshift. We first simulate, in a full cosmological context, a galaxy of total dynamical mass $10^{12}\,M_{\odot}$ at $z=2$. The...
- publication . Article . Preprint . 2016Open AccessAuthors:Teresita Suarez; Julien Devriendt; Hiranya V. Peiris; Andrew Pontzen; Adrianne Slyz;Project: RCUK | DiRAC2: 100 Tflop/s HPC c... (ST/K000373/1), EC | COSMICDAWN (306478)
Comment: 8 pages, 6 figures, accepted in MNRAS
4 research outcomes, page 1 of 1