Table 2
Best-fit models for the inactive stars from Table A.1 of Hintz et al. (2019) and the calculated reduced χ2 value (Col. 4) in the He I IR line.
Notes. (a) Columns 5–7 list the results of the model with the best He I IR line prediction within the subsample of the five best-fitting models for the inactive stars. For stars whose original model already resulted in an adequate description of the He I IR line, we mark the He I IR line best-fit model in gray.
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