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Shown a visualizations of from Magneticum Pathfinder simulations. The left panel shows
the largest volume simulation, done with low resolution. The middle column shows a smaller
volume (the size corresponds to the dashed square in the left panel) done with much higher
resolution. The increased level of detail can be best appreciated by exploring the zoom onto
a galaxy cluster forming in the high resolution simulation (right panel). Visualized is the
gas which fills the space between the galaxies (color coded according to its temperature from
cold/brown to hot/light blue) together with the galaxies and stars forming in the simulation
(colored in white). The lower images offer an interactive zoom and panning through high resolution
versions of these visualizations. The GAUSS-Project Magneticum aims to combine for the first time such
simulations and to simulate a very large volume of the universe with very high resolution.
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Magneticum Pathfinder Publications:
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The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy Clusters
McDonald, M. et al., SPT team
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Cosmological simulations of black hole growth: AGN luminosities and downsizing
Hirschmann, M., Dolag, K., Saro, A., Borgani, S., Burkert, A.
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Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope
Saro, A. et al.
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Investigating the velocity structure and X-ray observable properties of simulated galaxy clusters with PHOX
Biffi, V., Dolag, K., Boehringer, H.
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Virial scaling of galaxies in clusters: bright to faint is cool to hot
Wu, H-Y., Hahn, O., Evrard, A.E., Wechsler, R.H., Dolag, K.
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Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
Planck Collaboration
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The Dark Halo-Spheroid Conspiracy and the Origin of Elliptical Galaxies
Remus, R-S., Burkert, A., Dolag, K., Johansson, P.H., Naab, T., Oser, L., Thomas, J.
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On the orbital and internal evolution of cluster galaxies
Iannuzzi, F., Dolag, K.
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