International audienceThis technical paper describes a software package that was designed to produce initial conditions for large cosmological simulations in the context of the Horizon collaboration. These tools generalize E. Bertschinger's Grafic1 software to distributed parallel architectures and offer a flexible alternative to the Grafic2 software for "zoom" initial conditions, at the price of large cumulated CPU and memory usage. The codes have been validated up to resolutions of 40963 and were used to generate the initial conditions of large hydrodynamical and dark matter simulations. They also provide means to generate constrained realizations for the purpose of generating initial conditions compatible with, for example, the local gro...
Files representing the initial conditions at z=40 for ENZO-MHD cosmological simulation of a comoving...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
International audienceThe work presented in this paper aims at restricting the input parameter value...
We describe how to define an extremely large discrete realisation of a Gaussian white noise field th...
We describe how to define an extremely large discrete realization of a Gaussian white noise field th...
We present a code to generate mock observations of 21 cm intensity mapping exper-iments. The emphasi...
We discuss a new algorithm to generate multi-scale initial conditions with multiple levels of refine...
Files representing the initial conditions of Dark Matter Particles at z=40 for ENZO-MHD cosmological...
The Dark Sky Simulations are an ongoing series of cosmological N-body simulations designed to provid...
Simulations conducted on high-performance, massively parallel mainframes have become a central tool ...
We discuss a new algorithm to generate multi-scale initial conditions with multiple levels of refine...
Large-volume cosmological hydrodynamical simulations of galaxy formation enable us to theoretically ...
Horizon Run 5 (HR5) is a cosmological hydrodynamical simulation that captures the properties of the ...
International audienceHorizon Run 5 (HR5) is a cosmological hydrodynamical simulation that captures ...
This is a preprint of a paper in the proceedings of the XSEDE12 conference, held July 16-19, 2012 in...
Files representing the initial conditions at z=40 for ENZO-MHD cosmological simulation of a comoving...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
International audienceThe work presented in this paper aims at restricting the input parameter value...
We describe how to define an extremely large discrete realisation of a Gaussian white noise field th...
We describe how to define an extremely large discrete realization of a Gaussian white noise field th...
We present a code to generate mock observations of 21 cm intensity mapping exper-iments. The emphasi...
We discuss a new algorithm to generate multi-scale initial conditions with multiple levels of refine...
Files representing the initial conditions of Dark Matter Particles at z=40 for ENZO-MHD cosmological...
The Dark Sky Simulations are an ongoing series of cosmological N-body simulations designed to provid...
Simulations conducted on high-performance, massively parallel mainframes have become a central tool ...
We discuss a new algorithm to generate multi-scale initial conditions with multiple levels of refine...
Large-volume cosmological hydrodynamical simulations of galaxy formation enable us to theoretically ...
Horizon Run 5 (HR5) is a cosmological hydrodynamical simulation that captures the properties of the ...
International audienceHorizon Run 5 (HR5) is a cosmological hydrodynamical simulation that captures ...
This is a preprint of a paper in the proceedings of the XSEDE12 conference, held July 16-19, 2012 in...
Files representing the initial conditions at z=40 for ENZO-MHD cosmological simulation of a comoving...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
International audienceThe work presented in this paper aims at restricting the input parameter value...