[c]abundance: High Redshift Cluster Abundance[/c][/b]
Abstract: abundance, written in Fortran, provides driver and fitting routines to compute the predicted number of clusters in a ΛCDM cosmology that agrees with CMB, SN, BAO, and H0 measurements (up to 2010) at some specified parameter confidence and the mass that would rule out that cosmology at some specified sample confidence. It also computes the expected number of such clusters in the light cone and the Eddington bias factor that must be applied to observed masses.
Credit: Mortonson, Michael; Hu, Wayne; Huterer, Dragan
Site: http://background.uchicago.edu/abundance/
http://adsabs.harvard.edu/abs/2011PhRvD..83b3015M
Bibcode: 2014ascl.soft01007M
ID: ascl:1401.007
abundance: High Redshift Cluster Abundance
abundance: High Redshift Cluster Abundance
Last edited by Ada Coda on Sun Jan 20, 2019 10:58 pm, edited 1 time in total.
Reason: Updated code entry.
Reason: Updated code entry.