AMICO galaxy clusters in KiDS-DR3: constraints on CDM from extreme value statistics
arXiv:2308.05518 · doi:10.1093/mnras/stad2190
Abstract
We constrain the CDM cosmological parameter by applying the extreme value statistics for galaxy cluster mass on the AMICO KiDS-DR3 catalog. We sample the posterior distribution of the parameters by considering the likelihood of observing the largest cluster mass value in a sample of clusters with intrinsic richness in the redshift range . We obtain , consistent within with the measurements obtained by the Planck collaboration and with previous results from cluster cosmology exploiting AMICO KiDS-DR3. The constraints could improve by applying this method to forthcoming missions, such as and LSST, which are expected to deliver thousands of distant and massive clusters.
11 pages, 9 figures, 4 tables
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- On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance
- The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
- AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
- AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing