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C3 Cluster Clustering Cosmology I. New Constraints on the Cosmic Growth Rate at z ∼ 0.3 from Redshift-space Clustering Anisotropies

  • Authors: Federico Marulli, Alfonso Veropalumbo, Jorge Enrique García-Farieta, Michele Moresco, Lauro Moscardini, and Andrea Cimatti

2021 The Astrophysical Journal 920 13.

  • Provider: AAS Journals

Caption: Figure 2.

The redshift (left panel) and mass (right panel) distribution of the spectroscopic cluster sample analyzed in this work (blue solid histogram in the selected redshift range 0.1 < z < 0.42, cyan histogram at higher redshifts), compared to the redshift distributions of the WHL12 photometric and spectroscopic cluster samples (green and red histograms, respectively) and of the WHL12 sample restricted to the BOSS area (black histogram). The number of selected clusters in each catalog is reported in the label. The black solid line in the left panel shows the smoothed redshift distribution of the random catalog.

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