Fig. 10
Absolute magnitude of our models that are SN Ic progenitors (open and filled cyan circles) compared to observed upper magnitude limit for different SNe Ic (colored horizontal dashed lines followed by shortened SN label) and SN Ibc (gray horizontal dashed lines). Open (filled) symbols correspond to non-rotating (rotating) models. From top to bottom, we show the comparison between model and observations in the UBRI and HST/WFPC2 F450W, F555W, F606W, and F814W filters. Note that all models lie below the detectability limit of all SN Ic and Ibc.
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