  The increased amount of high precision seismic data for solar-like stars
calls for the existence of tools that can extract information from such data.
In the case of the study of acoustic glitches there are no publicly available
tools and most existing ones require a deep knowledge of their implementation.
In this work a tool is presented that aims to both simplify the interaction
with the user and also be capable of working automatically to determine
properties of acoustic glitches from seismic data of solar-like stars. This
tool is shown to work with both the Sun and other solar analogs but also shows
that are still severe limitations to the methods used, when considering smaller
datasets.
