Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
 
#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  206.4278   -44.0390   0.0070    23.6957    -0.6225         1.5616886     27.351 TRIG_01121751                 
 
Foreground time interval of the image:
 -0.200  10.213 (delta_t =  10.413 [sec])
Background time interval of the image:
-239.488  -0.200 (delta_t = 239.288 [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 0.512000
 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 0.512000
 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 0.512000
 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   -0.200 sec. to   13.008 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.43909     ( -0.0968579   0.0971864 )
Norm@50keV  : 9.17556E-03    ( -0.000488026   0.000486297 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   59.95     using 59 bins.
 Reduced chi-squared = 1.05175
# Null hypothesis probability of 3.69e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 13.21 sec: 1.12776 ( -0.06046  0.06058 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.16239e-06 ( -6.8782e-08  6.92444e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -0.200 sec. to   13.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30578     ( -0.394728   0.183188 )
Epeak [keV] : 265.724      ( -265.975 -265.975 )
Norm@50keV  : 1.06780E-02    ( -0.00192314   0.00586828 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   59.58     using 59 bins.
 Reduced chi-squared = 1.06393
# Null hypothesis probability of 3.47e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 13.21 sec: 1.11906 ( -0.06501  0.06481 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.14898e-06 ( -7.84408e-08  7.69412e-08 ) ergs/cm2
 
Band function
 
Time interval is from   -0.200 sec. to   13.008 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]    : 15.6012  (  )
R^2/D10^2   : 0.110017  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                  137.47     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.34e-08 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.353e-08   7.979e-09
25- 50  3.027e-07   2.054e-08
50-150  5.099e-07   5.522e-08
15-150  8.861e-07   6.044e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-22.0414      -200)
Norm        : 4.62565       (-0.241094     0.241094)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.14     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.41e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.522e-07   8.388e-09
25- 50  2.927e-07   1.658e-08
50-150  6.420e-07   1.347e-07
15-150  1.087e-06   1.475e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.58239        (-1.5569      1.64601)
R1^2/D10^2  : 0.844790        (-0.379633      0.961746)
kT2 [keV]   : 28.9100        (-5.65807      10.7655)
R2^2/D10^2  : 1.06215E-02    (-0.00681668   0.0125771)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   64.15     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.87e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.299e-07   2.764e-08
25- 50  2.908e-07   5.033e-08
50-150  7.208e-07   2.062e-07
15-150  1.142e-06   3.275e-07
Peak spectrum fit
Power-law model
 
Time interval is from    6.580 sec. to    7.580 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.10452     ( -0.153743   0.151309 )
Norm@50keV  : 2.25137E-02    ( -0.00194657   0.00194628 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   62.37     using 59 bins.
 Reduced chi-squared = 1.09421
# Null hypothesis probability of 2.91e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 2.61259 ( -0.23022  0.23046 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.35072e-07 ( -2.286e-08  2.30589e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from    6.580 sec. to    7.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.859342     ( -0.674033   0.320213 )
Epeak [keV] : 250.851      ( -250.868 -250.868 )
Norm@50keV  : 2.94452E-02    ( -0.00855239   0.0307103 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   61.89     using 59 bins.
 Reduced chi-squared = 1.10518
# Null hypothesis probability of 2.74e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 2.58626 ( -0.23977  0.23895 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.31143e-07 ( -2.52934e-08  2.47097e-08 ) ergs/cm2
 
Band function
 
Time interval is from    6.580 sec. to    7.580 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]    : 19.0873  (-2.12499  2.54422)
R^2/D10^2   : 0.142527  (-0.0475519   0.0673328)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   82.89     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.42e-02 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.019e-08   1.806e-09
25- 50  4.917e-08   7.015e-09
50-150  1.318e-07   2.220e-08
15-150  1.911e-07   2.240e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-18.8915      -200)
Norm        : 10.6056       (-0.946073     0.946073)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   84.54     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.04e-02 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.640e-08   7.145e-09
25- 50  5.079e-08   1.532e-08
50-150  1.114e-07   5.871e-08
15-150  1.886e-07   1.016e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 10.8578        (-4.43536      3.70693)
R1^2/D10^2  : 0.576381        (-0.310541      1.78434)
kT2 [keV]   : 45.9755        (-20.7889      -46.4595)
R2^2/D10^2  : 7.12078E-03    (-0.00670557   0.0407519)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   63.02     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.14e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.591e-08   6.221e-09
25- 50  5.178e-08   2.224e-08
50-150  1.652e-07   8.391e-08
15-150  2.329e-07   1.111e-07
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: 1.42422     ( -0.100488   0.100816 )
Norm@50keV  : 1.00308E-02    ( -0.000554228   0.000552288 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   56.41     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 4.97e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 10.41 sec: 1.22845 ( -0.0684066  0.0685397 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00412e-06 ( -6.19298e-08  6.23341e-08 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30095     ( -0.403106   0.211728 )
Epeak [keV] : 291.013      ( -291.013 -291.013 )
Norm@50keV  : 1.15348E-02    ( -0.00199145   0.00646889 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   56.10     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 4.71e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 10.41 sec: 1.21970 ( -0.0732  0.07301 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.9415e-07 ( -7.0078e-08  6.87945e-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)  = 2.79e-07
S(50-100 keV) = 4.11e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 11.1399999856949 sec.
Hardness ratio (energy fluence ratio) = 1.47312
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 1.4094
Count Ratio (50-100 keV) / (15-25 keV) = 1.09228
 Mask shadow pattern 
 
IMX = 4.388532200155590E-01, IMY = 4.767913310125819E-03
 TIME vs. PHA plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
 TIME vs. DetID plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
 100 us light curve (15-350 keV)
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
 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:
-239.488000 -0.200000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5209 -40.5818    3.4  33.3 -128.2   2.1161   3.4    1.7	Vela X-1                      
170.4556 -60.4223    0.0   4.2 -137.9   0.0233   0.1   12.7	Cen X-3                       
186.6194 -62.5880    9.1   3.9   56.1   0.5900   1.3   11.0	GX 301-2                      
 21.8140 -70.7269    3.5  47.0  133.6   7.9432   3.3 ------	UNKNOWN                       
305.0102 -81.0425    2.5  34.7  110.7   4.7993   4.6 ------	UNKNOWN                       
329.7758 -81.9303    3.1  35.9  116.8   4.5408   3.7 ------	UNKNOWN                       
228.0397 -31.5563    2.2  43.4   13.3   3.8768   5.2 ------	UNKNOWN                       
227.6188 -15.7041    2.2  57.2    3.0   8.4008   5.2 ------	UNKNOWN                       
217.8959 -18.8621    2.7  50.5   -5.9   3.3671   4.2 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
-0.200000 10.212600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.3596 -40.6710  175.5  33.3 -128.5  -0.0051  -0.1   10.4	Vela X-1                      
169.9089 -60.5536    0.0   4.4 -140.5  -0.0727  -1.4   12.7	Cen X-3                       
186.1959 -62.7523    0.0   3.7   59.4  -0.0156  -0.3   12.7	GX 301-2                      
206.4278 -44.0390    0.4  23.7   -0.6   1.5617  27.4 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
69.412600 873.112600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.4457 -40.5591    6.2  51.0 -148.1   6.9572   1.9    3.8	Vela X-1                      
170.3479 -60.4672  112.3  27.0 -176.0  -0.1564  -0.1    9.4	Cen X-3                       
187.1092 -62.7877    0.0  21.8  168.3  -0.9530  -0.7   12.5	GX 301-2                      
245.0052 -15.6413    1.2  43.2   25.5  24.1148   9.9    1.5	Sco X-1                       
255.9758 -37.8377  824.8  37.4   62.3   0.0579   0.0    0.6	4U 1700-377                   
256.5352 -36.3501    3.8  38.4   60.4  13.3408   3.0    6.5	GX 349+2                      
228.5568 -51.9521    2.3  16.7   90.3   7.6471   4.9 ------	UNKNOWN                       
119.4297 -49.8030    2.7  56.3 -164.9  21.6836   4.4 ------	UNKNOWN                       
147.6734 -29.7177    2.7  48.1 -129.1  26.2417   4.2 ------	UNKNOWN                       
Plot creation:
Wed Jun 14 14:01:36 EDT 2023