ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY) - I. Evidence for magnetospheric accretion in the young isolated planetary-mass object 2MASS J11151597+1937266

Open Access

Fig. E.1

Results from fitting Aoyama et al. (2020, 2021) model-grid to the observed H4-H7 line profiles of 2M1115. The model-grid allows n₀ to range from 10⁹ − 10¹⁴ cm⁻³ and v₀ to range from 50 − 200 km s⁻¹. The corresponding $χ_{red}^{2}$ $\chi _{{\rm{red}}}^2$ is represented by the colour bar, with $χ_{red}^{2} = 1$ $\chi _{{\rm{red}}}^2 = 1$ indicating a good fit.

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