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We present non‐Local Thermodynamic Equilibrium (LTE) time‐dependent radiative‐transfer simulations of supernova (SN) IIb/Ib/Ic spectra and light curves, based on ∼1051 erg piston‐driven ejecta, with and without 56Ni, produced from single and binary Wolf–Rayet (WR) stars evolved at solar and sub‐solar metallicities. Our bolometric light curves show a 10‐d long post‐breakout plateau with a luminosity...
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