Principal component analysis of variability fingerprints creates a stable, continuous map of young star light curves, where the main axis measures when large brightness changes begin.
AAAI Press, pp 226--231, https://www.aaai.org/Papers/KDD/1996/KDD96-037.pdf
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A survey for variable young stars with small telescopes: X -- Comparing stochastic YSO light curve
Principal component analysis of variability fingerprints creates a stable, continuous map of young star light curves, where the main axis measures when large brightness changes begin.