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Ensemble Machine Learning Approach to Estimate the Asteroseismic Indices for δ Scuti Stars Observed by TESS

  • Authors: Akram Bolouki, Amir Hasanzadeh, Hossein Safari

Akram Bolouki et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

The predicted median with associated upper and lower uncertainties vs. the measured values for 60 δ Sct stars (top row), fractional errors (middle row), and distribution of fractional error (bottom row) obtained by ensemble ML for ν(Amax) (left panel), νmax (middle panel), and Δν (right panel; see supplementary electronic table hosted by Figure 1). The red dashed line (y = x) shows the ideal prediction line in the top row, whereas the black dashed line marks the zero fractional error reference in the bottom row.

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