Fig. 16.
Predicted magnitudes in the selected NIRCAM+MIRI filters from 0.7–7.7 micron for young (< 4 Myr) proto-GCs with Mcl = 5 × 105 M⊙ and negligible SMS contribution. Solid (dotted) lines show the predictions including (excluding) nebular emission. The three curves that drop out are due to the classical photometric drop-out from the shortest wavelength filters.
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