no code implementations • 19 Sep 2019 • Nick Koukoufilippas, David Alonso, Maciej Bilicki, John A. Peacock
Our measurements allow us to place constraints on the redshift dependence of the mass-observable relation for tSZ cluster count analyses in terms of the so-called 'hydrostatic mass bias' parameter $1-b_{\rm H}$.
Cosmology and Nongalactic Astrophysics
