Fig. 15
From: The THESEUS space mission: science goals, requirements and mission concept
Left panel: IR (H-band) light curves of a sample of known GRBs converted to the expected signal if they would be located at z = 8. The grey lines represent on a sample of observed afterglows. The brightest ones after 1 day from the trigger are highlighted as filled dots (colour legend in the inset). Right panel: photometric redshift as a function of the source input according to Monte-Carlo simulations of the IRT observation sequence for a sample of 113 z > 6 GRBs extracted from the sky model provided by the THESEUS consortium as part of the Mission Observation Simulator (MOS; see Section 4.3.1)