Modeled transit depths and emission spectra for HAT-P-26 b. with the equilibrium temperature assumed in the atmospheric model indicated in the panels showing emission. The dots and curves represent thin and thick atmospheric models (disperser used is color coded), and the error bars give the expected 1 σ uncertainties for NIRSpec transit and occultation measurements after rebinning to the indicated resolution or Aλ (photon and read noise only).