1 code implementation • 3 Dec 2017 • Boris Bolliet, Barbara Comis, Eiichiro Komatsu, Juan Francisco Macías-Pérez
Finally, by combining the tSZ power spectrum and the CMB data we find, in the $\Lambda$ Cold Dark Matter (CDM) model, the mass bias of $B=1. 71\pm 0. 17$, i. e., $1-b=0. 58\pm 0. 06$ (68% CL).
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
