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
   87.8870    70.1093   0.0124    35.0397  -109.5671         1.2893336     15.477 TRIG_01037828                 
 
Foreground time interval of the image:
 -7.000   1.836 (delta_t =   8.836 [sec])
Background time interval of the image:
-239.728  -7.000 (delta_t = 232.728 [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 2.048000
 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 2.048000
 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 2.048000
 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   -7.000 sec. to    1.836 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.15708     ( -0.192862   0.204151 )
Norm@50keV  : 8.06551E-03    ( -0.00112619   0.00110155 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.20     using 59 bins.
 Reduced chi-squared = 1.12632
# Null hypothesis probability of 2.39e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 8.836 sec: 1.30598 ( -0.13084  0.13086 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.66416e-07 ( -8.08237e-08  8.26248e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -7.000 sec. to    1.836 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.15433     ( -0.772193   0.208426 )
Epeak [keV] : 9999.33      (   )
Norm@50keV  : 8.08362E-03    (     )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.20     using 59 bins.
 Reduced chi-squared = 1.14643
# Null hypothesis probability of 2.11e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 8.836 sec: 1.30554 ( -0.13059  0.13064 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.47673e-07 ( -1.12313e-07  9.52706e-08 ) ergs/cm2
 
Band function
 
Time interval is from   -7.000 sec. to    1.836 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]    : 8.18831  (-0.918191  1.03569)
R^2/D10^2   : 1.30037  (-0.494178   0.801996)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   78.92     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.89e-02 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.417e-07   2.607e-08
25- 50  2.581e-07   4.025e-08
50-150  7.311e-08   2.510e-08
15-150  4.728e-07   6.088e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 47.6277       (-11.9845      18.9141)
Norm        : 7.58396       (-1.32895     1.74251)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.80     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.23e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.619e-07   2.147e-08
25- 50  2.285e-07   2.801e-08
50-150  2.118e-07   6.344e-08
15-150  6.022e-07   8.341e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.09366        (-1.18152      1.07523)
R1^2/D10^2  : 2.14786        (-0.540083      2.03469)
kT2 [keV]   : 70.1978        (-47.3924      -70.673)
R2^2/D10^2  : 5.86223E-04    (-0.000507728   0.00731604)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   59.26     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 3.23e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.576e-07   3.375e-08
25- 50  2.348e-07   4.953e-08
50-150  3.006e-07   1.557e-07
15-150  6.931e-07   1.992e-07
Peak spectrum fit
Power-law model
 
Time interval is from   -6.992 sec. to   -5.992 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.97529     ( -0.400599   0.455379 )
Norm@50keV  : 1.16335E-02    ( -0.00343291   0.00320998 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   60.81     using 59 bins.
 Reduced chi-squared = 1.06684
# Null hypothesis probability of 3.40e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 1.72562 ( -0.36442  0.36441 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.07177e-07 ( -2.85612e-08  2.97377e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -6.992 sec. to   -5.992 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.04459     ( -0.417496   1.17542 )
Epeak [keV] : 22.2293      ( -2.06256 -9999.35 )
Norm@50keV  : 1.03364E-02    ( -0.00355678   0.0381089 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   60.69     using 59 bins.
 Reduced chi-squared = 1.08375
# Null hypothesis probability of 3.11e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 1.70572 ( -0.58403  0.38548 ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2
 
Band function
 
Time interval is from   -6.992 sec. to   -5.992 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]    : 7.25620  (-1.83554  3.17742)
R^2/D10^2   : 2.66849  (-2.00577   6.02101)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   69.73     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.20e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.339e-08   1.222e-08
25- 50  3.431e-08   1.560e-08
50-150  6.465e-09   4.854e-09
15-150  6.417e-08   3.211e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 71.1877       (-38.0359      -71.2391)
Norm        : 8.38881       (-2.50827     4.33938)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   62.31     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.93e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.156e-08   7.205e-09
25- 50  3.446e-08   1.365e-08
50-150  4.481e-08   3.425e-08
15-150  1.008e-07   5.016e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.37757        (-1.51384      2.01272)
R1^2/D10^2  : 7.56460        (-5.36617      10.7059)
kT2 [keV]   : 30.0524        (-14.0196      -30.0555)
R2^2/D10^2  : 1.07734E-02    (-0.0105454   0.0820437)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   58.47     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 3.49e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.592e-08   1.508e-08
25- 50  2.838e-08   1.583e-08
50-150  6.093e-08   4.024e-08
15-150  1.152e-07   6.050e-08
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: 2.15708     ( -0.192862   0.204151 )
Norm@50keV  : 8.06551E-03    ( -0.00112619   0.00110155 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.20     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.39e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 8.836 sec: 1.30586 ( -0.130826  0.130842 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.66292e-07 ( -8.07976e-08  8.26269e-08 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.97771     (     )
Epeak [keV] : 4.69671      (   )
Norm@50keV  : 1.04187E-02    (     )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.03     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.16e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 8.836 sec: 1.29524 ( -0.13811  0.13656 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.46591e-07 ( -1.11143e-07  9.89906e-08 ) 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)  = 2.09e-07
S(50-100 keV) = 1.87e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 8.21200001239777 sec.
Hardness ratio (energy fluence ratio) = 0.894737
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 0.967507
Count Ratio (50-100 keV) / (15-25 keV) = 0.38883
 Mask shadow pattern 
 
IMX = -2.348523842962926E-01, IMY = 6.607430845806622E-01
 TIME vs. PHA plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
 TIME vs. DetID plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
 100 us light curve (15-350 keV)
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
 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:
-239.728000 -7.000000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
230.5111  28.9278    3.2  55.9   10.8   6.2029   3.6 ------	UNKNOWN                       
245.9069  39.4030    3.3  57.3   -8.9   4.5404   3.5 ------	UNKNOWN                       
249.8232  63.7972    2.4  43.9  -35.7   2.6950   4.7 ------	UNKNOWN                       
253.7292  77.1714    2.8  39.2  -54.8   2.2426   4.2 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
-7.000000 1.836000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
132.7744  51.9367    2.5  16.3 -159.8   0.1816   4.5 ------	UNKNOWN                       
 87.8870  70.1093    0.7  35.0 -109.6   1.2891  15.5 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
 
Plot creation:
Fri Nov 11 22:28:10 EST 2022