The LPSZ-CLASH galaxy cluster sample: combining lensing and hydrostatic
  mass estimates
  Starting from the clusters included in the NIKA sample and in the NIKA2
Sunyaev-Zel'dovich Large Program (LPSZ) we have selected a sample of six common
objects with the Cluster Lensing And Supernova survey with Hubble (CLASH)
lensing data. For the LPSZ clusters we have at our disposal both high-angular
resolution observations of the thermal SZ with NIKA and NIKA2 and X-ray
observations with XMM-Newton from which hydrostatic mass estimates can be
derived. In addition, the CLASH dataset includes lensing convergence maps that
can be converted into lensing estimates of the total mass of the cluster.
One-dimensional mass profiles are used to derive integrated mass estimates
accounting for systematic effects (data processing, modeling, etc.).
Two-dimensional analysis of the maps can reveal substructures in the cluster
and, therefore, inform us about the dynamical state of each system. Moreover,
we are able to study the hydrostatic mass to lensing mass bias, across
different morphology and a range of redshift clusters to give more insight on
the hydrostatic mass bias. The analysis presented in this proceeding follows
the study discussed in Ferragamo et al. 2021.
