Fig. 4
Comparison of a low-Ye (=0.1) matter case, representative for a “tidal” dynamical ejecta, with NIR JHK-band observations (https://kilonova.space/kne/GW170817/). The detailed ejecta model parameters are shown at the top of each panel. The left panel uses heating according to the FRDM nuclear mass model, for the right panel a DZ-type heating rate has been employed (see Sect. 3 in the main text for a discussion).
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