TP-AGB stars and stellar population properties of a post-starburst galaxy at z ∼ 2 through optical and near-infrared spectroscopy with JWST

Open Access

Fig. C.1.

Paschen series indices as a function of age. The marker and the lines are the same as in Fig. 7. Predictions from M05 and M13 for Paδ are not shown because this index cannot be measured safely due to the low spectral resolution (see section 4.3 for details).

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