Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB191019970 |
|
T0 |
23:17:13 UTC |
GCN_circulars,Fermi GBM final loc |
ra |
216.3400° |
Fermi_GBM |
decl |
-40.6300° |
Fermi_GBM |
pos_error |
2.61e+00° |
Fermi_GBM |
T90 |
137.73 s |
Fermi_GBM |
T90_error |
0.572 s |
Fermi_GBM |
T90_start |
23:17:22.563 UTC |
Fermi_GBM |
fluence |
7.02e-05 erg/cm² |
Fermi_GBM |
fluence_error |
3.55e-08 erg/cm² |
Fermi_GBM |
T100 |
147.293 s |
|
GBM_located |
True |
|
mjd |
58775.970289351855 |
GCN_circulars,Fermi GBM final loc |
Fermi GBM table |
GRB_name_Fermi |
GRB191019970 |
trigger_name |
bn191019970 |
ra |
216.3400° |
decl |
-40.6300° |
pos_error |
2.61e+00° |
datum |
2019-10-19 |
t_trigger |
23:17:13.347 UTC |
T90 |
137.73 s |
T90_error |
0.572 s |
T90_start |
23:17:22.563 UTC |
fluence |
7.02e-05 erg/cm² |
fluence_error |
3.55e-08 erg/cm² |
flux_1024 |
1.36e+01 erg/cm²/s |
flux_1024_error |
3.76e-01 erg/cm²/s |
flux_1024_time |
1.25e+02 erg/cm²/s |
flux_64 |
1.65e+01 erg/cm²/s |
flux_64_error |
1.52e+00 erg/cm²/s |
GCN 26040 table |
GRB_name |
GRB191019B |
GCN_number |
26040 |
Detection_method |
Fermi GBM final loc |
t_trigger |
23:17:13 UTC |
ra |
216.3000° |
decl |
-40.6000° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 26040
SUBJECT: GRB 191019B: Fermi GBM Final Real-time Localization
DATE: 19/10/19 23:27:25 GMT
FROM: Fermi GBM Team at MSFC/Fermi-GBM
The Fermi GBM team reports the detection of a likely LONG GRB
At 23:17:13 UT on 19 Oct 2019, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 191019B (trigger 593219838.347392 / 191019970).
The on-ground calculated location, using the Fermi GBM trigger data, is RA = 216.3, Dec = -40.6 (J2000 degrees, equivalent to J2000 14h 25m, -40d 36'), with a statistical uncertainty of 1.0 degrees.
The angle from the Fermi LAT boresight is 82.0 degrees.
The skymap can be found here:
http://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2019/bn191019970/quicklook/glg_skymap_all_bn191019970.png
The HEALPix FITS file, including the estimated localization systematic, can be found here:
http://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2019/bn191019970/quicklook/glg_healpix_all_bn191019970.fit
The GBM light curve can be found here:
http://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2019/bn191019970/quicklook/glg_lc_medres34_bn191019970.gif
|
GCN 26058 table |
GRB_name |
GRB191019B |
GCN_number |
26058 |
Detection_method |
AstroSat CZTI |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 26058
SUBJECT: GRB 191019B: AstroSat CZTI detection
DATE: 19/10/22 09:32:48 GMT
FROM: Ramkrishna Gaikwad at IUCAA/AstroSat
R. Gaikwad, S. Gupta, V. Sharma and D. Bhattacharya (IUCAA), V. Bhalerao (IIT-B), A. R. Rao (TIFR) and S. Vadawale (PRL) report on behalf of the AstroSat CZTI collaboration:
Analysis of AstroSat CZTI data showed the detection of a GRB 191019B, which was also detected by Fermi GBM Final Real-time Localization (GCN #26040).
The source was clearly detected in the 40-200 keV energy range. The light curve shows multiple pulses of emission with the strongest peak at 2019-10-19 23:17:13.0 UT. The measured peak count rate associated with the burst is 265 cts/s above the background in the combined data of four quadrants, with a total of 7067 cts. The local mean background count rate was 501 cts/s. Using cumulative rates, we measure a T90 of 128.3 s.
It was also clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range.
CZTI GRB detections are reported regularly on the payload site at http://astrosat.iucaa.in/czti/?q=grb. CZTI is built by a TIFR-led consortium of institutes across India, including VSSC, ISAC, IUCAA, SAC and PRL. The Indian Space Research Organisation funded, managed and facilitated the project.
|