Early light curve excess in Type IIb supernovae observed with ATLAS - Qualitative constraints on progenitor systems

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Fig. 8.

Correlation between ΔM₁₅, t_rise, and $M_{abs}^{peak}$ $M^{\mathrm{peak}}_{\mathrm{abs}}$ for EE (blue) and non-EE (red) SNe in the representative sample (ρ_peak ≥ 0.3 days⁻¹). Each panel reports the Pearson, Spearman, and Kendall correlation coefficients for the corresponding parameter pair.

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