Asteroid families classification: Exploiting very large datasets

@article{Milani2014AsteroidFC,
  title={Asteroid families classification: Exploiting very large datasets},
  author={Andrea Milani and A Cellino and Zoran Kne{\vz}evi{\'c} and Bojan Novakovi{\'c} and Federica Spoto and Paolo Paolicchi},
  journal={Icarus},
  year={2014},
  volume={239},
  pages={46-73}
}
Automated Classification of Asteroids into Families at Work
TLDR
It is demonstrated how by the new approach the asteroid family classification becomes stable in general terms (converging towards a permanent list of confirmed families), and in the same time evolving in details (to account for the newly discovered asteroids) at each update.
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Previous works have identified families halos by an analysis in proper elements domains, or by using Sloan Digital Sky Survey-Moving Object Catalog data, fourth release (SDSS-MOC4) multi-band
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A sample of over 12,487 asteroid proper element triplets, computed by A. Milani and Z. Kneževic (1994, Icarus 107, 219-254), has been searched for statistically significant and robust families by
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Abstract A statistical method for the evaluation of the probable amount of interlopers included in the most recently identified asteroid families is developed. The method is based on the analysis of
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