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Fig. 5
Stellar S/N ratio over 1 h integration time of each M dwarf at 10 pc, binned to a resolution of 100. All NIRSpec filters and high resolution disperser are combined. Solid lines are calculated using the method described in Sect. 2.5 and dashed lines are calculated using the JWST ETC, Pandeia (Pontoppidan et al. 2016).
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