Fig. 6
Recovered exoplanetary transmission spectra from simulated transit observations of a hot-Jupiter transiting G2 star, combing observations of 15 transits. We demonstrate the reconstruction of individual absorption lines made possible by high S/N and spectral resolution. Upper panel: spectral resolution: R = 10 000. Middle panel: spectral resolution: R = 50 000. Lower panel: spectral resolution: R = 100 000.
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