Corrected sunspot number reconstructions SN-14C-C (panel A)) and SN-10Be-C (panel B)), after removing long-term trends (see Sect. 4.1). The black curves and the gray shading depict the mean and the 95% range (over 10⁶ ensemble members) of the reconstructions, respectively, and the green curve represents the 3 kyr reconstruction by Usoskin et al. (2014). Stars and circles denote grand maxima and minima, respectively, as in Fig. 3. Tables for this plot are available at the CDS, including the mean values and the uncertainties of the sunspot numbers reconstructed here as shown in Fig. 5.