The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5

Author(s):
Ahad, S.L.; Bahé, Y.M.; Hoekstra, H. (0000-0001-7463-2893); Burg, R.F.J. van der; Muzzin, A.
Published
2021
Publication type
Article / Letter to editor
MethodsNumericalGalaxiesClustersGeneralEvolutionStellar contentAstrophysicsAstrophysics of galaxies
Date issued
2021
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2021), Vol. 504, no. 2, p. 1999-2013
hdl
1887/3250897
doi
10.1093/mnras/stab1036
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.504.1999A