V. D'Elia (ASDC) for the Swift team
Bissaldi et al. (GCN Circ. 16623) reported the GRB detection. At UT 01:36:30.73 on July 23rd, 2014, Fermi-LAT detected high-energy emission from GRB 140723A, which was also detected by Fermi-GBM (trigger427772193 / 140723067). 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.
XRT results are not available.
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 |
---|---|---|---|---|---|
Optical | Guidorzi et al. | 16627 | LCO-Sutherland optical candidate | LCO | detection |
Optical | Gorbovskoy et al. | 16629 | MASTER optical observation | MASTER | |
Optical | Guidorzi et al. | 16630 | LCO-Sutherland optical candidate retraction |
LCO | retraction |
Gamma-ray | Bissaldi et al. | 16623 | Fermi-LAT detection | Fermi LAT | |
Gamma-ray | Hurley et al. | 16625 | IPN Triangulation | IPN | |
Gamma-ray | Burns | 16626 | Fermi GBM detection | Fermi GBM | Fluence=1.46±0.04x1 (8 |
Gamma-ray | Golenetskii et al. | 16628 | Konus-Wind observation | Konus-Wind | Fluence=2.3(-0.5,+0.8)x1 |
Table 3. Found no UVOT observations.
July 26, 2014