D.M. Palmer (LANL) and B. Sbarufatti (PSU) for the Swift team
At 20:59:24.168 UT on 2017-10-10, the Swift Burst Alert Telescope (BAT) triggered on GRB 171010B (trigger=778019) (Palmer and Lien GCN Circ. 21995). However, on-board analysis was truncated by a pre-planned slew to a scheduled target. 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.
BAT refined results are not available.
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
Figure 2. The XRT light curve.
Any data from a crosshatched region are not included in the fit.
RA (J2000) | Dec (J2000) | Error | Note | Reference |
---|---|---|---|---|
0 |
-54°23'28.1" | 4.4" | XRT-final | UKSSDC |
0 |
-54°23'29.2" | 5.6" | XRT | Melandri et al. GCN Circ. 22023 |
0 |
-54°24'36.7" | 1.6' | BAT-initial | Palmer and Lien GCN Circ. 21995 |
Band | Authors | GCN Circ. | Subject | Observatory | Notes |
---|---|---|---|---|---|
Gamma-ray | Poolakkil and Meegan | 21999 | Fermi GBM detection | Fermi GBM | Fluence=8.073±1.802x1 |
October 19, 2017