Extended Data Fig. 3: Radio luminosity of EP240414a/SN 2024g sa.
From: A fast X-ray transient from a weak relativistic jet associated with a type Ic-BL supernova
The 9 GHz radio luminosity of EP240414a/SN 2024gsa is compared to low-frequency (1–10 GHz) light curves of different classes of energetic explosions: tidal disruption events100,101, SNe102,103, relativistic Ic-BL SNe104,105, long-duration GRBs106,107,108, and fast blue optical transients109,110,111.
