M.G. Bernardini (INAF-OAB) for the Swift team
Arimoto et al. (GCN Circ. 17912) reported the GRB detection. The MAXI/GSC nova alert system triggered a bright uncatalogued X-ray transient source at 11:46:50 UT. 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 |
---|---|---|---|---|
0 |
-00°38'39.0" | 3.6" | XRT | Bernardini et al. GCN Circ. 17917 |
Band | Authors | GCN Circ. | Subject | Observatory | Notes |
---|---|---|---|---|---|
Optical | Saito et al. | 17920 | MITSuME Akeno optical upper limits | MITSuME Akeno | upper limits |
X-ray | Arimoto et al. | 17912 | MAXI/GSC detection | MAXI | detection |
Gamma-ray | Golenetskii et al. | 17918 | Konus-Wind observation | Konus-Wind | Fluence=2.4(-0.3,+0.3)x1 |
June 16, 2015