430 citations · 3.4k across the 66 of their papers we have counts for
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Analytical model for non-thermal pressure in galaxy clusters - III. Removing the hydrostatic mass bias
Xun Shi, Eiichiro Komatsu, Daisuke Nagai +1
Non-thermal pressure in galaxy clusters leads to underestimation of the mass of galaxy clusters based on hydrostatic equilibrium with thermal gas pressure. This occurs even for dyn…
Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy
Naomi Ota, Daisuke Nagai, Erwin T. Lau
Gas motions in galaxy clusters play important roles in determining the properties of the intracluster medium (ICM) and in the constraint of cosmological parameters via X-ray and Su…
nIFTy galaxy cluster simulations I: dark matter & non-radiative models
Federico Sembolini, Gustavo Yepes, Frazer R. Pearce +24
We have simulated the formation of a galaxy cluster in a CDM universe using twelve different codes modeling only gravity and non-radiative hydrodynamics (\art, \arepo, \hydra\ a…