Fig. 4.

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OSF reconstruction from this study (red) and by Krivova et al. (2021, blue) using ISNv2 (top) and GSN (bottom; CEA17 here and HoSc98 in Krivova et al. 2021) as input. The shaded pink area shows our upper limit estimate for the Maunder minimum, where the SNs from Carrasco et al. (2025) was used as input. Black: OSF reconstructed from the cosmogenic isotope data by Wu et al. (2018).
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