J.A. Kennea (PSU) for the Swift team
Mereghetti et al. (GCN Circ. 29037) reported the GRB detection. A gamma ray burst lasting about 150 s has been detected by IBAS in the IBIS/ISGRI data at 6:18:20 UT of 14 December 2020. 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 Kennea et al. (GCN Circ. 29092). The source previously reported by Kennea et al. (GCN Circ. 29048), "Source 2", is fading with 3-sigma significance, and is therefore likely the GRB afterglow. The source is fading with α >0.6.
A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 2.7 (+0.9, -0.7). The
best-fitting absorption column is 1.9 (+2.2, -1.6) x 1
UVOT results are not available.
Figure 1. The BAT light curve is not available.
RA (J2000) | Dec (J2000) | Error | Note | Reference |
---|---|---|---|---|
1 |
+33°52'09.5" | 2.2" | XRT | Kennea et al. GCN Circ. 29092 |
Band | Authors | GCN Circ. | Subject | Observatory | Notes |
---|---|---|---|---|---|
Optical | Lipunov et al. | 29035 | Integral GRB201214.26: Global MASTER-Net observations report |
MASTER | |
Optical | Jelinek et al. | 29040 | Mates' birthday GRB optical limit from FRAM-ORM |
FRAM | upper limits |
Optical | Kumar et al. | 29091 | 1.3m DFOT, optical upper limits | Devasthal Opt.Tel. | upper limits |
Optical | Belkin et al. | 29093 | TSHAO optical upper limit | Zeiss-1000 | upper limits |
Gamma-ray | Mereghetti et al. | 29037 | A long GRB detected by INTEGRAL | INTEGRAL | Fluence=5x1 |
December 20, 2020