E. Troja (NASA/GSFC/UMCP) for the Swift team
At 17:47:10 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 210422A (trigger=1044678) (Troja et al. GCN Circ. 29886). Due to an observing constraint, Swift did not slew immediately to the burst. 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.
Standard analysis products for this burst are available at https://gcn.gsfc.nasa.gov/swift_gnd_ana.html.
As reported by Barthelmy et al. (GCN Circ. 29897),
the BAT ground-calculated position is RA, Dec = 21.077, 42.100 deg which is RA(J2000) = 0
The BAT light curve (Figure 1) showed a complex structure with a duration of about ~30 s.
The time-averaged spectrum from -34.40 s to -20.56 s and -19.40s to 7.59 s is best fit by a simple power-law model.
The power law index of the time-averaged spectrum is 1.70 ± 0.22.
The fluence in the 15-150 keV band is 7.2 ± 1.1 x 1
XRT refined results are not available.
UVOT results are not available.
Figure 1. The BAT
mask-weighted light curve in the four individual and total
energy bands. The units are counts
| RA (J2000) | Dec (J2000) | Error | Note | Reference |
|---|---|---|---|---|
| 0 |
+42°05'58.2" | 2.1' | BAT-refined | Barthelmy et al. GCN Circ. 29897 |
| Band | Authors | GCN Circ. | Subject | Observatory | Notes |
|---|---|---|---|---|---|
| Optical | Lipunov et al. | 29887 | Swift GRB210422.74: Global MASTER-Net observations report |
MASTER |
April 25, 2021