Extended Data Fig. 3: Evolution of the light curve of SN 2017iuk.
From: Signatures of a jet cocoon in early spectra of a supernova associated with a γ-ray burst
Evolution of the BVRCIC magnitude of SN 2017iuk as observed with the RBT/PST2 telescope. Coloured curves represent the interpolation functions used to estimate the peak brightness. Error bars represent 1 s.d.
