Fig. 10.
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Optical/nIR spectral energy distribution of EP250207b at 7.4 d, compared with the X-Shooter spectrum (Pian et al. 2017) and the HST spectrum (Troja et al. 2017) of AT2017gfo at a similar epoch, rescaled to match the observed photometry and redshifted to z ∼ 0.082. Data were corrected for Galactic extinction using E(B − V)≈0.05 (Schlafly & Finkbeiner 2011). The solid lines show the afterglow models.
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