Line profiles of the He iλ10 830 and Paγ lines in HD 101412 CRIRES spectra. Rotation phases of the observations assuming the magnetic rotation period are presented close to the Paγ lines. From top to bottom, these phases correspond to observations obtained at MJD 55 662.082, 55 667.174, 55 681.023, 55 683.058, 56 361.178, 56 367.283, 55 654.085, 55 656.062, and 56 372.185 (see Table B.1). The epoch MJD 52 797.4 corresponds to phase ϕ = 0, as presented in Fig. 4 of Hubrig et al. (2011). Synthetic Paγ profiles assuming the atmospheric parameters T_eff = 8300 K and log g = 3.8 are indicated by the dotted lines.