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