S. Dichiara (PSU) for the Swift team
Arimoto et al. (GCN Circ. 30943) reported the GRB detection. Table 1 contains the best reported positions from Swift.
Table 2 is a summary of GCN Circulars about this GRB from observatories other than Swift.
BAT did not observe this burst.
Analysis of the initial XRT data was reported by Dichiara et al. (GCN Circ. 31010). Five uncatalogued X-ray sources have been detected, however none of them is above the RASS limit or shows definitive signs of fading.
UVOT results are not available.
Figure 1. The BAT light curve is not available.
| RA (J2000) | Dec (J2000) | Error | Note | Reference |
|---|
| Band | Authors | GCN Circ. | Subject | Observatory | Notes |
|---|---|---|---|---|---|
| Gamma-ray | Arimoto et al. | 30943 | Fermi-LAT detection | Fermi LAT | |
| Gamma-ray | Ohno et al. | 30945 | Detection by GRBAlpha | GRBAlpha | |
| Gamma-ray | Roberts and Meegan | 30947 | Fermi GBM observation | Fermi GBM |
October 27, 2021