Stellar chromospheric activity database of solar-like stars based on the LAMOST Low-Resolution Spectroscopic Survey - II. The bolometric and photospheric calibration

Open Access

Fig. A.1

Distribution of T_eff,LASP values and T_eff,A2020 values for 3806 common stars, where T_eff,A2020 denotes the effective temperature in Amard et al. (2020). The dashed red line represents the case where T_eff,LASP equals T_eff,A2020. Error bars are indicated for data points that have specified uncertainty values. The lower panel displays the distribution of ΔT_eff/T_eff,LASP against T_eff,LASP, where ΔT_eff = T_eff,LASP − T_eff,A2020.

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