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Fig. 4.

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Example of convergence for the alternative model (see Table 2). All datasets (RV, TTV, VIS, CLO, T3, SYN, SED, SKY2) were taken into account, with alternative weights wrv = 100, wttv = 1000, wvis = 0.1, wclo = 0.1, wsyn = 0.1, wsky2 = 1000.0. Two of the stellar components (Ac2, Aa2) were forced to be on the main sequence, which results in tension (an increase in several χ2 contributions after 800 iteration). The nominal model does not exhibit such tension.

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