paper

GRB 201015A and the nature of low-luminosity soft gamma-ray bursts

arXiv:2305.14491 · doi:10.1093/mnras/stad1703

Abstract

GRB 201015A is a peculiarly low luminosity, spectrally soft gamma-ray burst (GRB), with s (time interval of detection of 90\% of photons from the GRB), and an associated supernova (likely to be type Ic or Ic-BL). GRB 201015A has an isotropic energy erg, and photon index (15-150 keV). It follows the Amati relation, a correlation between and spectral peak energy followed by long GRBs. It appears exceptionally soft based on , the hardness ratio of HR = , and low-, so we have compared it to other GRBs sharing these properties. These events can be explained by shock breakout, poorly collimated jets, and off-axis viewing. Follow-up observations of the afterglow taken in the X-ray, optical, and radio, reveal a surprisingly late flattening in the X-ray from s to s. We fit the data to closure relations describing the synchrotron emission, finding the electron spectral index to be , and evidence of late-time energy injection with coefficient . The jet half opening angle lower limit () is inferred from the non-detection of a jet break. The launch of SVOM and Einstein Probe in 2023, should enable detection of more low luminosity events like this, providing a fuller picture of the variety of GRBs.

15 pages, 4 figures

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