Monitoring the magnetospheric accretion of the classical T Tauri star DO Tau with SPIRou

Open Access

Fig. 1

Longitudinal magnetic field B_ℓ (red dots), and QP GPR fit to the data (full cyan line) with corresponding 68% confidence intervals (dotted cyan lines). The bottom panel zooms-in on the 2025 data. The residuals, shown in the bottom plot of each panel, have an rms of 25 G ( $χ_{r}^{2} = 1.8$ $Mathematical equation: $\chi^2_{\rm r}=1.8$$ ).

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