Abstract
We present the early radio detection and multiwavelength modeling of the short gamma-ray burst (GRB) 231117A at redshift z = 0.257. The Australia Telescope Compact Array automatically triggered a 9 hr observation of GRB 231117A at 5.5 and 9 GHz following its detection by the Neil Gehrels Swift Observatory just 1.3 hr post-burst. Splitting this observation into 1 hr time bins, the early radio afterglow exhibited flaring, scintillating and plateau phases. The scintillation allowed us to place the earliest upper limit ( 35 to Γ > 5 between ∼0.1 and 1 day. These results demonstrate the importance of rapid and sensitive radio follow-up of GRBs for exploring their central engines and outflow behaviour.
| Original language | English |
|---|---|
| Article number | 5 |
| Number of pages | 26 |
| Journal | The Astrophysical Journal |
| Volume | 994 |
| Issue number | 1 |
| Early online date | 11 Nov 2025 |
| DOIs | |
| Publication status | Published - 20 Nov 2025 |
Keywords
- X-ray transient sources
- Gamma-ray transient sources
- Transient sources
- Radio transient sources
- Gamma-ray bursts