Image Details
Caption: Figure 13.
Absolute magnitude of GRB afterglows at 1 and 4 days post-burst, compared with the magnitudes of EP240414a at the same epochs. The implication is that emission like the first episode (which has spectra similar to LFBOTs) could be readily hidden, but the 4 day peak would only be straightforward to hide in a minority of bursts.
© 2025. The Author(s). Published by the American Astronomical Society.