Parameters and abundances of stars belonging to the Br32 cluster using the GES pipeline and the OssicoNN neural network. The number of GES stars varies across quadrants since it depends on how many stars could be successfully processed through the classical pipelines for the given set of parameters. We also display the Kiel diagram and the isochrone corresponding to the age and metallicity of the cluster measured by Cantat-Gaudin et al. (2020). THe isochrone is generated using PARSEC version 1.2S (Bressan et al. (2012), Chen et al. (2014)).