Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
33.9038 -37.7724 0.0236 30.4678 -152.3846 0.9503037 8.141 TRIG_01037339
Foreground time interval of the image:
0.632 44.133 (delta_t = 43.501 [sec])
Background time interval of the image:
-239.368 0.632 (delta_t = 240.000 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from 0.632 sec. to 96.632 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27997 ( -0.341553 0.335135 )
Norm@50keV : 8.39768E-04 ( -0.000157072 0.000156812 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.76 using 59 bins.
Reduced chi-squared = 1.04842
# Null hypothesis probability of 3.76e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 96 sec: 9.98271E-02 ( -0.0190271 0.0191009 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.00702e-07 ( -1.67356e-07 1.70235e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.632 sec. to 96.632 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04314 ( -1.29935 1.74586 )
Epeak [keV] : 212.681 ( -293.15 -293.15 )
Norm@50keV : 1.09387E-03 ( -0.000284849 0.00299583 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.74 using 59 bins.
Reduced chi-squared = 1.06679
# Null hypothesis probability of 3.42e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 96 sec: 9.92000E-02 ( -0.0197226 0.019525 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.93051e-07 ( -1.79782e-07 1.75586e-07 ) ergs/cm2
Band function
Time interval is from 0.632 sec. to 96.632 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.0578 (-4.70362 6.43689)
R^2/D10^2 : 5.17251E-03 (-0.00314016 0.00809698)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.68e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.541e-08 1.588e-08
25- 50 1.707e-07 6.928e-08
50-150 4.559e-07 1.858e-07
15-150 6.620e-07 2.549e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-77.8895 -200)
Norm : 0.411969 (-0.0776271 0.0776271)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.15e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.852e-08 5.851e-08
25- 50 1.895e-07 1.092e-07
50-150 4.156e-07 2.379e-07
15-150 7.037e-07 4.061e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.34521 (-2.36164 4.20652)
R1^2/D10^2 : 0.135164 (-0.107953 0.678226)
kT2 [keV] : 29.4207 (-9.33487 27.7418)
R2^2/D10^2 : 1.08880E-03 (-0.000922453 0.00275372)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.65e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.923e-08 5.198e-08
25- 50 1.718e-07 9.350e-08
50-150 5.495e-07 3.166e-07
15-150 8.105e-07 4.237e-07
Peak spectrum fit
Power-law model
Time interval is from 8.132 sec. to 9.132 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67846 ( -1.39518 1.34937 )
Norm@50keV : 2.40740E-03 ( -0.00176941 0.00170942 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.90 using 59 bins.
Reduced chi-squared = 1.01579
# Null hypothesis probability of 4.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.317387 ( -0.207242 0.20798 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.23254e-08 ( -1.57058e-08 1.79463e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.132 sec. to 9.132 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.80268 ( )
Epeak [keV] : 34.7778 ( )
Norm@50keV : 5.10085E+04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.69 using 59 bins.
Reduced chi-squared = 0.95875
# Null hypothesis probability of 5.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.291972 ( -0.145799 0.178887 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5056e-08 ( -7.46987e-09 8.87936e-09 ) ergs/cm2
Band function
Time interval is from 8.132 sec. to 9.132 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.12549 (-3.05059 6.19807)
R^2/D10^2 : 0.248371 (-0.252597 0.991617)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.055e-09 2.753e-09
25- 50 8.807e-09 6.365e-09
50-150 3.504e-09 3.034e-09
15-150 1.637e-08 1.166e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 85.2524 (-85.2523 -85.2523)
Norm : 1.49078 (-1.02045 2.83908)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.47e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.882e-09 2.637e-09
25- 50 6.486e-09 4.695e-09
50-150 9.547e-09 9.345e-09
15-150 1.991e-08 1.625e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 200.000 (-200 -200)
R1^2/D10^2 : 3.73967E-05 (-3.76857e-05 -3.76857e-05)
kT2 [keV] : 8.66262 (-3.18725 5.30259)
R2^2/D10^2 : 0.280318 (-0.238175 1.28179)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42439 ( -0.301367 0.303761 )
Norm@50keV : 1.49345E-03 ( -0.000256884 0.000254452 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.5 sec: 0.182906 ( -0.0309682 0.0310419 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.24686e-07 ( -1.19078e-07 1.21356e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29314 ( -1.30443 1.84015 )
Epeak [keV] : 264.801 ( -275.714 -275.714 )
Norm@50keV : 1.73736E-03 ( -0.000492356 0.00576423 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.55e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.5 sec: 0.181821 ( -0.032345 0.031764 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.18627e-07 ( -1.30004e-07 1.25989e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.77e-07
S(50-100 keV) = 2.90e-07
T90 vs. Hardness ratio plot
T90 = 80 sec.
Hardness ratio (energy fluence ratio) = 1.63842
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.62561
Count Ratio (50-100 keV) / (15-25 keV) = 2.12381
Mask shadow pattern
IMX = -5.212699673120080E-01, IMY = 2.726921884670455E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-239.368000 0.632000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6588 22.0042 1.3 46.5 45.9 8.6095 8.8 1.5 Crab
83.0543 4.9080 2.6 36.3 66.9 3.3219 4.5 ------ UNKNOWN
31.9226 -3.5251 3.5 19.8 -67.4 1.1316 3.3 ------ UNKNOWN
13.0256 -64.8367 3.6 59.6 -161.2 8.7980 3.2 ------ UNKNOWN
11.3393 10.8393 3.4 44.6 -60.4 4.4144 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.632000 44.132600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7743 22.0153 21.9 46.6 46.0 0.2248 0.5 7.8 Crab
82.5412 1.4740 2.3 34.4 71.9 1.0867 4.9 ------ UNKNOWN
86.2932 -58.0217 2.1 54.2 158.9 2.7167 5.4 ------ UNKNOWN
66.2725 28.3881 1.9 42.4 22.4 1.0937 6.0 ------ UNKNOWN
69.3896 -5.3811 2.0 19.7 76.0 0.6730 5.9 ------ UNKNOWN
33.9038 -37.7724 1.4 30.5 -152.4 0.9504 8.1 ------ UNKNOWN
30.7655 29.0728 2.3 44.4 -23.4 0.8845 5.0 ------ UNKNOWN
25.9835 43.3478 2.0 58.8 -19.1 3.2508 5.7 ------ UNKNOWN
5.4105 -54.7449 2.1 56.1 -149.2 2.6894 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
107.132590 962.693000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
60.3509 -60.0300 2.4 27.8 112.4 5.8876 4.8 ------ UNKNOWN
48.3304 -52.7171 3.3 17.9 111.6 3.3746 3.5 ------ UNKNOWN
312.6231 -66.6092 3.0 52.4 170.4 10.3584 3.9 ------ UNKNOWN
0.7909 -21.8439 3.4 32.7 -109.5 4.8983 3.4 ------ UNKNOWN
40.9225 17.4499 2.9 55.6 -31.2 15.8921 4.0 ------ UNKNOWN
Plot creation:
Fri Nov 11 22:45:48 EST 2022