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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S309(10), p. 298-298, 2014

DOI: 10.1017/s1743921314009958

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Mirage simulations of the massiv sample

Journal article published in 2014 by P. Amram, V. Perret, B. Epinat, F. Bournaud, T. Contini, C. Divoy, B. Garilli ORCID, M. Kissler-Patig, O. Le Fevre, C. Lopez-Sanjuan, J. Moultaka, L. Pairo, E. Perez-Montero ORCID, J. Queyrel, L. Tasca and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

The MIRAGE sample (Merging & isolated high-redshift AMR galaxies; Perret 2014, PhD dissertation; Perret et al. 2014, AA 562, 1) has been built in order to understand the contribution of the merger processes to the mass assembly in the MASSIV (Mass Assembly Survey with SINFONI in VVDS, Contini et al. 2012, AA 539, 91) sample. It consists of a sample of idealized simulations based on the RAMSES code; the initial conditions were designed to reproduce the physical properties of the most gas-rich young galaxies. The sample is composed of 20 simulations of mergers exploring the initial parameters of mass and orientation of the disks with a spatial resolution reaching 7 parsecs.

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