| Summary table |
|---|
| Variable |
Value |
Source |
| T0 |
18:57:42 UTC |
Swift |
| ra |
276.0570° |
Swift |
| decl |
51.4610° |
Swift |
| pos_error |
2.33e-02° |
Swift |
| T90 |
0.8 s |
Swift |
| T90_start |
18:57:42 UTC |
Swift |
| fluence |
7.00e-08 erg/cm² |
Swift |
| T100 |
0.8 s |
|
| GBM_located |
False |
|
| mjd |
55891.79006944445 |
Swift |
| IPN table |
|---|
| GRB_name |
GRB111126A |
| ra |
276.1000° |
| decl |
51.4667° |
| pos_error |
5.00e-02° |
| Swift table |
|---|
| GRB_name |
GRB111126A |
| t_trigger |
18:57:42 UTC |
| ra |
276.0570° |
| decl |
51.4610° |
| pos_error |
2.33e-02° |
| T90 |
0.8 s |
| fluence |
7.00e-08 erg/cm² |
| GCN 12599 table |
|---|
| GRB_name |
GRB111126A |
| GCN_number |
12599 |
| Detection_method |
Swift-BAT Det |
| ra |
276.0570° |
| decl |
51.4610° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 12599
SUBJECT: GRB 111126A found in ground analysis of BAT data
DATE: 11/11/29 02:12:02 GMT
FROM: Jay R. Cummings at NASA/GSFC/Swift
J. R. Cummings (NASA/UMBC/CRESST), D. M. Palmer (LANL)
on behalf of the Swift-BAT team
At 18:57:42 UTC, on November 26, 2011, BAT count rates spiked during
a pre-planned slew maneuver. In a mosaic of images from slew event data,
a significant source was found at RA, Dec 276.057, +51.461, which is
RA (J2000) 18h 24m 13.6s
Dec (J2000) 51d 27' 38"
with an estimated uncertainty of 3 arcmin radius. This location is
currently about 29 degrees from the Sun. No Swift followup is anticipated.
It was a short, hard GRB with multiple peaks. T90 was 0.8 +/- 0.1 seconds.
The BAT spectrum is best fit by a simple powerlaw with a photon index of
1.1 +/- 0.3. The fluence in 0.8 seconds was 7 +/- 2 ergs/cm^2. The peak
flux was 1.2 +/- 0.4 photons/cm^2/s. The uncertainties are 90% estimated
including systematics.
|
| GCN 12603 table |
|---|
| GRB_name |
GRB111126A |
| GCN_number |
12603 |
| Detection_method |
Swift-BAT Det |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 12603
SUBJECT: GRB 111126A Circular #12599 erratum
DATE: 11/11/30 02:16:56 GMT
FROM: Jay R. Cummings at NASA/GSFC/Swift
J. R. Cummings (GSFC/UMBC/CRESST) on behalf of the Swift-BAT team
The magnitude of the fluence was omitted in the circular, it should
have been (7 +/- 2) x 10^-8 ergs/cm^2. We thank Kevin Hurley for
pointing out the error.
|