Fig. C.4.

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KNe light curves for BLh (blue lines) and APR4 (red lines) EOSs computed in the g and i filter of Rubin at inclination angle 20 deg, assuming luminosity distance dL = 100 Mpc. KNe light curves correspond to three different BNS systems. Solid lines correspond to M1=M2 = 1.33 M⊙ (the peak of the NS mass distribution); dashed lines correspond to M1 = 1.18 M⊙, M2 = 1.10 M⊙ (the BNS producing the most massive disc); dotted lines correspond to M1=M2 = 1.57 M⊙ (the BNS producing the lightest disc). KNe light curves are compared to AT2017gfo (black diamonds) (Villar 2017) placed at dL = 100 Mpc.
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