Latest updates on AIMS

The Asteroseismic Inference on a Massive Scale (AIMS) program is designed to estimate stellar properties and associated error bars from a set of classic and seismic constraints. It applies an MCMC algorithm while interpolating in a predetermined grid of stellar models. This poster describes some of the latest improvements of AIMS, namely the combined use of a physical age and age parameter, and the introduction of seismic indicators based on the WhoSGlAd methodology (Farnir et al. 2019)