Fig. 21
Predicted apparent fluxes of GJ 504b in the near- and mid-infrared corresponding to the best-fitting synthetic spectra found in Sect. 5 with the G statistics and some knowledge of the object radius. The transmission of some key filters of JWST instruments are overlaid. We report the L-band photometry (Subaru/IRCS, LBTI/LMIRcam) of GJ 504b (black).
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