Extended Data Table 1 Detectability of atmospheres with MIRI/LRS

From: Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3

  1. Number of occultation observations with MIRI/LRS needed to distinguish the CO2 and H2O atmospheric models from two common airless planet models These numbers were obtained using wavelength bins of constant resolution R = 3.
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