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
  291.0341    80.0123   0.0049    37.3609  -147.3329         6.8326550     39.734 TRIG_01162001                 
 
Foreground time interval of the image:
 -7.376  16.149 (delta_t =  23.525 [sec])
Background time interval of the image:
-239.552  -7.376 (delta_t = 232.176 [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 1.024000
 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 1.024000
 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 1.024000
 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   -7.376 sec. to   31.760 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.63337     ( -0.0700832   0.0703932 )
Norm@50keV  : 1.25712E-02    ( -0.000490979   0.00049044 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   37.16     using 59 bins.
 Reduced chi-squared = 0.65193
# Null hypothesis probability of 9.81e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 39.14 sec: 1.63266 ( -0.06768  0.06786 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.5847e-06 ( -1.87861e-07  1.884e-07 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -7.376 sec. to   31.760 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.25771     ( -0.304497   0.284774 )
Epeak [keV] : 102.879      ( -24.7679 144.102 )
Norm@50keV  : 1.91007E-02    ( -0.00508048   0.00750722 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   32.00     using 59 bins.
 Reduced chi-squared = 0.571429
# Null hypothesis probability of 9.96e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 39.14 sec: 1.59419 ( -0.07303  0.07343 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.46901e-06 ( -2.08503e-07  2.07817e-07 ) ergs/cm2
 
Band function
 
Time interval is from   -7.376 sec. to   31.760 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]    : 14.8245  (  )
R^2/D10^2   : 0.183574  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                  161.73     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 5.78e-12 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.312e-07   2.679e-08
25- 50  1.302e-06   6.576e-08
50-150  1.937e-06   1.485e-07
15-150  3.570e-06   1.624e-07
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 168.798       (-29.8321      -168.437)
Norm        : 6.62667       (-0.301363     0.325921)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   31.99     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.97e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.587e-07   4.168e-08
25- 50  1.241e-06   1.029e-07
50-150  2.567e-06   7.259e-07
15-150  4.467e-06   8.090e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.26995        (-1.23831      1.30824)
R1^2/D10^2  : 1.46574        (-0.595729      1.31703)
kT2 [keV]   : 24.8846        (-3.48806      5.43939)
R2^2/D10^2  : 2.18876E-02    (-0.011537   0.0180017)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   40.00     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.36e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.981e-07   8.161e-08
25- 50  1.267e-06   1.327e-07
50-150  2.544e-06   3.826e-07
15-150  4.409e-06   4.873e-07
Peak spectrum fit
Power-law model
 
Time interval is from    0.260 sec. to    1.260 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.25132     ( -0.105286   0.104965 )
Norm@50keV  : 7.09162E-02    ( -0.00439566   0.00439563 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   61.87     using 59 bins.
 Reduced chi-squared = 1.08544
# Null hypothesis probability of 3.06e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 8.38933 ( -0.54009  0.54079 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.09561e-07 ( -4.78932e-08  4.80565e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from    0.260 sec. to    1.260 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.912834     ( -0.457495   0.379689 )
Epeak [keV] : 178.684      ( -72.4941 -178.684 )
Norm@50keV  : 0.101884    ( -0.033   0.0618033 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   59.97     using 59 bins.
 Reduced chi-squared = 1.07089
# Null hypothesis probability of 3.34e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 8.28825 ( -0.55414  0.55472 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.78867e-07 ( -4.77769e-08  5.45487e-08 ) ergs/cm2
 
Band function
 
Time interval is from    0.260 sec. to    1.260 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]    : 18.6649  (-1.45754  1.61239)
R^2/D10^2   : 0.487448  (-0.118277   0.152967)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                  106.67     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 7.41e-05 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.359e-08   3.810e-09
25- 50  1.595e-07   1.440e-08
50-150  4.069e-07   4.425e-08
15-150  6.001e-07   4.530e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-12.5875      -200)
Norm        : 34.9723       (-2.20314     2.20314)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   84.11     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.13e-02 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.710e-08   5.815e-09
25- 50  1.676e-07   1.310e-08
50-150  3.675e-07   8.090e-08
15-150  6.222e-07   9.650e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.36058        (-2.79522      2.77126)
R1^2/D10^2  : 2.85180        (-1.39305      5.71428)
kT2 [keV]   : 34.0700        (-8.76975      26.3439)
R2^2/D10^2  : 5.11285E-02    (-0.041141   0.0972869)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   63.13     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.11e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.814e-08   1.433e-08
25- 50  1.674e-07   4.552e-08
50-150  4.758e-07   2.071e-07
15-150  7.013e-07   2.292e-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: 1.61465     ( -0.0640213   0.0642865 )
Norm@50keV  : 1.94191E-02    ( -0.000691643   0.00069108 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   34.82     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.91e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 23.52 sec: 2.50689 ( -0.0955193  0.0957799 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.26403e-06 ( -1.59555e-07  1.59863e-07 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.22706     ( -0.278016   0.261797 )
Epeak [keV] : 104.826      ( -23.5766 101.753 )
Norm@50keV  : 2.97905E-02    ( -0.00730903   0.0104127 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   28.28     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.99e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 23.52 sec: 2.44527 ( -0.10314  0.10361 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.15859e-06 ( -1.76706e-07  1.75765e-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)  = 1.21e-06
S(50-100 keV) = 1.55e-06
 T90 vs. Hardness ratio plot 
 
T90                                   = 22.336000084877 sec.
Hardness ratio (energy fluence ratio) = 1.28099
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 1.34375
Count Ratio (50-100 keV) / (15-25 keV) = 1.02144
 Mask shadow pattern 
 
IMX = -6.427102760570491E-01, IMY = 4.120911943418059E-01
 TIME vs. PHA plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
 TIME vs. DetID plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
 100 us light curve (15-350 keV)
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
 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:
-239.552000 -7.376000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5901  35.2298    6.5   9.8   44.6   0.5653   1.8    9.4	Her X-1                       
268.2034  -1.3470    0.0  46.6   10.9  -0.6351  -1.2   11.7	SW J1753.5-0127               
288.8775  10.8997    6.3  42.4  -23.0   0.9967   1.8    5.4	GRS 1915+105                  
299.5859  35.1910    0.8  32.3  -63.7   7.9539  14.8    0.7	Cyg X-1                       
308.1640  41.0248    3.5  35.8  -78.3   2.2572   3.3    5.0	Cyg X-3                       
261.8048 -10.9570    2.7  55.5   20.4   6.7834   4.3 ------	UNKNOWN                       
161.1663  83.7326    2.8  46.7 -164.7   3.0319   4.1 ------	UNKNOWN                       
286.4519  14.7063    3.0  37.9  -23.0   1.7781   3.9 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
-7.376000 16.148600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5510  35.3835    3.4   9.7   45.1  -0.3439  -3.4    5.2	Her X-1                       
268.3109  -1.5285    7.8  46.8   10.8  -0.2949  -1.5    5.7	SW J1753.5-0127               
288.6815  10.8699    5.8  42.3  -22.7   0.3796   2.0    8.2	GRS 1915+105                  
299.5900  35.2014   15.0  32.3  -63.7  -0.1523  -0.8    0.0	Cyg X-1                       
308.1891  40.9408   18.7  35.9  -78.2  -0.1790  -0.6    3.6	Cyg X-3                       
213.5794  26.1148    3.1  40.6  102.5   1.2724   3.7 ------	UNKNOWN                       
252.7378  -6.0404    2.4  50.8   31.7   1.7459   4.9 ------	UNKNOWN                       
291.0341  80.0123    0.3  37.4 -147.3   6.8323  39.8 ------	UNKNOWN                       
 58.0738  79.1616    2.3  55.7 -151.5   2.5677   4.9 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
93.148590 719.636300
720.448000 871.748600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4050  35.3875    4.4  46.8   28.7   3.9284   2.6    3.7	Her X-1                       
299.5860  35.2180    0.7  44.9  -23.0  24.8150  15.7    1.0	Cyg X-1                       
308.1542  40.9328    3.1  39.6  -33.5   5.0430   3.7    2.3	Cyg X-3                       
326.2084  38.2453    6.8  43.9  -53.8   5.1135   1.7    4.9	Cyg X-2                       
248.0804  35.4345    3.0  47.6   35.7   7.8135   3.8 ------	UNKNOWN                       
274.5848  25.2223    2.8  55.2    5.1  10.1764   4.2 ------	UNKNOWN                       
274.3015  31.4931    2.7  49.0    5.9   5.7363   4.3 ------	UNKNOWN                       
 92.8796  55.0995    2.6  44.5 -178.3   8.1283   4.4 ------	UNKNOWN                       
 76.9432  51.9051    3.0  46.7 -164.6   7.5308   3.8 ------	UNKNOWN                       
 49.0029  55.1864    2.5  40.4 -141.9   8.0099   4.6 ------	UNKNOWN                       
  8.9589  50.5768    3.5  38.4 -103.3   9.9111   3.3 ------	UNKNOWN                       
Plot creation:
Fri Jun 16 09:11:13 EDT 2023