The planetary-mass-limit VLT/SINFONI library - Spectral extraction and atmospheric characterization via forward modeling

Open Access

Fig. 8

Best spectral fit for each target. Here, the targets are organized by their derived T_eff, from hottest at the top to coldest at the bottom. The T_eff and S/N values are shown on the right side of each spectrum. The models are color-coded to indicate the grid that provided the best match to the data, selected based on the lowest $χ_{r e d}^{2}$ $\chi _{red}^2$ value.

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