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    This health check verifies that the ESXi hosts in the v SAN cluster have the latest version of the v SAN Health Check vib installed.This simple approach has been justified until now in view of the large uncertainties in the data, both observational and theoretical. The V and (B - V) techniques The V technique (Iben and Renzini 1983) makes use of the quantity V which is the difference in magnitude between the main sequence turnoff and the HB luminosity at the same color.It is still the basis of the ages presented in this paper, and used in the Monte Carlo simulation described in Section 5. It has the advantage of being insensitive to interstellar reddening. when it relies on theoretical models of the HB to set the HB luminosity, it provides directly a completely theoretical calibration for the globular cluster ages, given a chemical composition, which is independent of distance.The evolutionary tracks themselves are constructed using a stellar evolution code, which calculates as a function of time the evolution of a stellar model with a given mass and chemical composition.The theoretical isochrones, which are calculated in the [log T - log g] plane (the plane of stellar atmosphere parameters) for the cluster composition to the color system used for the observations (log g is the surface gravity).

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