The Clustering of Quasars at Redshift 2.5 from the Final SDSS-III/BOSS Sample
Measuring the mass of the dark matter halos that host quasars is a critical question in the field of galaxy evolution. Estimates of how the mean mass of the dark matter halos in which quasars are triggered evolves with time can potentially constrain scenarios in which the quasar phase is triggered in different dark-matter environments as the
Eftekharzadeh, S. et al.
Advertised on:
6
2014