no code implementations • 27 Feb 2019 • G. W. Pratt, M. Arnaud, A. Biviano, D. Eckert, S. Ettori, D. Nagai, N. Okabe, T. H. Reiprich
On the observational side, new, sophisticated techniques are being deployed in individual mass measurements and to account for selection biases in cluster surveys.
Cosmology and Nongalactic Astrophysics