Many-probes multi-object spatially-resolved analyses of galaxy clusters
  in the big data era
  The thermal Sunyaev-Zeldovich (SZ) effect and the X-ray emission offer
separate and highly complementary probes of the thermodynamics of the
intracluster medium, particularly on their radial dependence. We already
released \texttt{JoXSZ}, the first publicly available code designed to jointly
fit SZ and X-ray data coming from various instruments to derive the
thermodynamic radial profiles of galaxy clusters, including mass.
\texttt{JoXSZ;} follows a fully Bayesian forward-modelling approach, adopts
flexible parametrization for the thermodynamic profiles and includes many
useful options that users can customize according to their needs. We are
including shear measurement in our joint analysis, and moving from
single-cluster to multi-cluster analyses, allowing to quantify the
heterogeneity of thermodynamic properties within the cluster population. At the
same time, we are creating a suitable framework that efficiently stores and
optimally processes huge volumes of data being released by the current and new
generation surveys.
