Pipeline to extract stellar clusters from GAIA data as votable. The method is using a DBSCAN-optimized clustering method in the 8-fold dimension with photometry and astrometry data. The optimization the clustering parameters is performed with an Approximate Bayesian Computation method (Weyant et al. 2013). The extraction process is currently with a stable version using the Julia language for speed constraint. An (experimental) capability is offered from version 1.7 to fit an isochrone and to extract more isolated stars in a second step ("tails", subclumps, etc). Be aware that some stellar clusters are not physically real and a final cleaning can be done with some Jupyter NB but are still experimental. A visual inspection of the final stellar cluster is still recommended. The current version is working with Gaia DR3 data.
Documentation and information can be found in the wiki pages.