Limits on supernova-like emission from GRB111005A (arrows). The lines show the models from Levan et al. (2005), scaled to a distance of 55 Mpc. In the case of the nine-day epoch we have used a model from seven days, and extended the template from 2.2 to 4.8 μm based on a purely thermal extrapolation. We also show the observations of the type IIb SN 2011dh in M51 (Helou et al. 2013), as it would appear at 55 Mpc.