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
   76.9550   -59.8161   0.0208    14.1149   -73.5724         0.6628752      9.296 TRIG_01142997                 
 
Foreground time interval of the image:
  1.064  21.096 (delta_t =  20.032 [sec])
Background time interval of the image:
-239.896   1.064 (delta_t = 240.960 [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 4.096000
 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 4.096000
 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 4.096000
 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    1.064 sec. to   21.096 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.52876     ( -0.259621   0.266231 )
Norm@50keV  : 2.18810E-03    ( -0.000359829   0.000354413 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   45.19     using 59 bins.
 Reduced chi-squared = 0.792807
# Null hypothesis probability of 8.71e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 20.03 sec: 0.275335 ( -0.042158  0.042179 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.13944e-07 ( -7.38718e-08  7.55203e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from    1.064 sec. to   21.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.842201     ( -1.3414   0.870285 )
Epeak [keV] : 77.7986      ( -28.2658 -77.7986 )
Norm@50keV  : 5.14139E-03    ( -0.00321049   0.0224365 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   43.92     using 59 bins.
 Reduced chi-squared = 0.784286
# Null hypothesis probability of 8.79e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 20.03 sec: 0.268317 ( -0.043549  0.043495 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.87268e-07 ( -8.26742e-08  8.52311e-08 ) ergs/cm2
 
Band function
 
Time interval is from    1.064 sec. to   21.096 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]    : 13.0335  (-2.30259  2.97521)
R^2/D10^2   : 5.16002E-02  (-0.0267117   0.0516283)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   50.58     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 7.13e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.724e-08   1.183e-08
25- 50  1.286e-07   3.033e-08
50-150  1.383e-07   5.095e-08
15-150  3.042e-07   7.326e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 196.446       (-103.273      -195.933)
Norm        : 1.12845       (-0.172286     0.19949)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   44.31     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.90e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.639e-08   3.195e-08
25- 50  1.083e-07   5.965e-08
50-150  2.363e-07   1.299e-07
15-150  4.010e-07   2.240e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.21480        (-3.36165      3.45239)
R1^2/D10^2  : 0.182241        (-0.117986      0.706096)
kT2 [keV]   : 28.3985        (-23.5473      -28.3926)
R2^2/D10^2  : 2.24701E-03    (-0.00221641   0.0175036)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   43.01     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.80e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.127e-08   2.848e-08
25- 50  1.185e-07   6.541e-08
50-150  2.293e-07   1.324e-07
15-150  3.991e-07   2.067e-07
Peak spectrum fit
Power-law model
 
Time interval is from    3.348 sec. to    4.348 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.47294     ( -0.475009   0.485475 )
Norm@50keV  : 5.60322E-03    ( -0.00161278   0.00157627 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   53.93     using 59 bins.
 Reduced chi-squared = 0.94614
# Null hypothesis probability of 5.91e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 0.694553 ( -0.18927  0.189495 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.34048e-08 ( -1.658e-08  1.71668e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from    3.348 sec. to    4.348 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16234     ( -3.21707   1.29805 )
Epeak [keV] : 124.353      ( -124.708 -124.708 )
Norm@50keV  : 8.27841E-03    ( -0.00471339   0.575383 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   53.86     using 59 bins.
 Reduced chi-squared = 0.961786
# Null hypothesis probability of 5.56e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 0.687093 ( -0.197114  0.194343 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.16904e-08 ( -2.01367e-08  1.8544e-08 ) ergs/cm2
 
Band function
 
Time interval is from    3.348 sec. to    4.348 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]    : 12.6668  (-3.66253  6.07085)
R^2/D10^2   : 0.143871  (-0.107702   0.341276)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   56.16     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 5.06e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.895e-09   2.961e-09
25- 50  1.639e-08   9.872e-09
50-150  1.637e-08   1.047e-08
15-150  3.765e-08   2.384e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.362       (-199.363      -199.363)
Norm        : 2.84808       (-0.769815     0.770468)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   53.89     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 5.92e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.092e-09   4.323e-09
25- 50  1.364e-08   8.250e-09
50-150  2.992e-08   1.803e-08
15-150  5.065e-08   3.034e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.18582        (-4.95977      3.67598)
R1^2/D10^2  : 0.365840        (-0.15933      1.70393)
kT2 [keV]   : 54.3673        (-116.36      -126.836)
R2^2/D10^2  : 9.14223E-04    (-0.000152797   0.0599469)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   52.57     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 5.68e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.348e-09   3.794e-09
25- 50  1.535e-08   9.305e-09
50-150  3.227e-08   1.779e-08
15-150  5.397e-08   2.526e-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: 1.52876     ( -0.259621   0.266231 )
Norm@50keV  : 2.18810E-03    ( -0.000359829   0.000354413 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   45.19     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.71e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 20.03 sec: 0.275327 ( -0.0421564  0.0421765 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.1389e-07 ( -7.38328e-08  7.5559e-08 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.842213     ( -1.3414   0.870285 )
Epeak [keV] : 77.7993      ( -28.2658 -77.7986 )
Norm@50keV  : 5.14131E-03    ( -0.00321049   0.0224365 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   43.92     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.79e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 20.03 sec: 0.268287 ( -0.04354  0.043484 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.87404e-07 ( -8.26778e-08  8.53358e-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)  = 1.04e-07
S(50-100 keV) = 1.44e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 16.8319998979568 sec.
Hardness ratio (energy fluence ratio) = 1.38462
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 1.50532
Count Ratio (50-100 keV) / (15-25 keV) = 0.980954
 Mask shadow pattern 
 
IMX = 7.111350310776945E-02, IMY = 2.411941707005720E-01
 TIME vs. PHA plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
 TIME vs. DetID plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
 100 us light curve (15-350 keV)
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
 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:
-239.896000 1.064000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5477 -40.5396    2.7  39.1 -160.4   2.6444   4.3    1.3	Vela X-1                      
 53.9413 -12.5821    2.2  40.6   53.9   4.2202   5.4 ------	UNKNOWN                       
 12.1782 -26.8815    3.6  56.9    1.5   5.0635   3.2 ------	UNKNOWN                       
 10.1126 -32.2107    3.2  55.1   -4.9   3.2858   3.6 ------	UNKNOWN                       
358.1209 -57.3477    2.9  49.5  -37.8   5.3603   3.9 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
1.064000 21.096000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.4790 -40.4093    5.2  39.1 -160.6   0.2193   2.2    9.0	Vela X-1                      
 76.9551 -59.8160    1.2  14.1  -73.6   0.6633   9.3 ------	UNKNOWN                       
150.3985 -30.0980    2.0  54.9 -163.6   1.4559   5.7 ------	UNKNOWN                       
 48.5006 -72.9672    2.5  30.9  -64.5   0.4817   4.7 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
80.804640 638.804000
640.104000 654.156000
655.104000 873.653000
875.104000 879.434300
880.104000 962.184000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5616 -40.5714    3.0  40.4 -173.7   7.1334   3.9    1.8	Vela X-1                      
170.3698 -60.6460    7.6  42.3 -128.8   3.9746   1.5    2.1	Cen X-3                       
356.4454 -35.6223    3.0  55.3   -4.8  10.0509   3.9 ------	UNKNOWN                       
Plot creation:
Wed Jun 14 13:54:47 EDT 2023