Early-Type Galaxies And Their Sometimes Not So Old Globular Clusters

In previous papers of the series, we used a combination of optical and near-infrared colors to derive constraints on the relative age structure in globular cluster systems. Here, we present the details, strength and limitations of our method based on Monte-Carlo simulations of color-color diagrams and cumulative age distributions. The simulations are based on general informations about the globular cluster systems (e.g. color-ranges, the number ratios between sub-populations) and the different single stellar population models (SSP’s) which are used to derive relative ages. For both the modeled systems and the observed globular cluster systems we derive the cumulative age distribution and introduce two parameters to define it, the so-called 50% age and the result of the reduced χ2test of the comparison between models and observations. The method was tested successfully on several systems and allowed to reveal significant intermediate age populations in two of them.