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
323.9330 -41.8731 0.0264 39.4196 -27.6806 0.9034431 7.275 TRIG_01404126
Foreground time interval of the image:
0.392 50.845 (delta_t = 50.453 [sec])
Background time interval of the image:
-239.056 0.392 (delta_t = 239.448 [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 8.192000
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 8.192000
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 8.192000
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 0.392 sec. to 310.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68437 ( -0.363057 0.388611 )
Norm@50keV : 3.36212E-04 ( -7.5581e-05 7.24934e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.61 using 59 bins.
Reduced chi-squared = 1.18614
# Null hypothesis probability of 1.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 309.7 sec: 4.44136E-02 ( -0.0089545 0.0089721 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.65453e-07 ( -2.2315e-07 2.26863e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.392 sec. to 310.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.18060 ( -1.56972 0.0476391 )
Epeak [keV] : 69.9742 ( )
Norm@50keV : 1.84900E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.37 using 59 bins.
Reduced chi-squared = 1.20304
# Null hypothesis probability of 1.42e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 309.7 sec: 4.44137E-02 ( -0.0089647 0.0089676 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.3227e-07 ( -2.26642e-07 2.55762e-07 ) ergs/cm2
Band function
Time interval is from 0.392 sec. to 310.104 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] : 14.7049 (-3.71731 5.03074)
R^2/D10^2 : 5.08915E-03 (-0.00326737 0.00924655)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.44e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.157e-08 3.358e-08
25- 50 2.792e-07 1.187e-07
50-150 4.071e-07 1.878e-07
15-150 7.579e-07 2.786e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 155.253 (-87.7988 -155.791)
Norm : 0.180224 (-0.0389907 0.0536778)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.429e-07 8.139e-08
25- 50 2.662e-07 1.496e-07
50-150 5.329e-07 3.267e-07
15-150 9.421e-07 5.519e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.73685 (-1.58058 2.53411)
R1^2/D10^2 : 0.717661 (-0.646235 16.7571)
kT2 [keV] : 21.0673 (-5.99906 11.7084)
R2^2/D10^2 : 1.26055E-03 (-0.000980047 0.00285446)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.47e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.766e-07 9.708e-08
25- 50 2.110e-07 1.140e-07
50-150 5.575e-07 3.418e-07
15-150 9.451e-07 5.074e-07
Peak spectrum fit
Power-law model
Time interval is from 5.184 sec. to 6.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29267 ( -0.688176 0.653887 )
Norm@50keV : 4.47657E-03 ( -0.00176021 0.00175755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.82 using 59 bins.
Reduced chi-squared = 1.01439
# Null hypothesis probability of 4.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.533361 ( -0.218551 0.221679 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.4321e-08 ( -1.8212e-08 1.84675e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.184 sec. to 6.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.206018 ( -0.205968 2.10862 )
Epeak [keV] : 93.0535 ( -93.0523 -93.0523 )
Norm@50keV : 1.39508E-02 ( -0.0139515 215.795 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.35 using 59 bins.
Reduced chi-squared = 1.02411
# Null hypothesis probability of 4.25e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.512412 ( -0.283069 0.228327 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.28065e-08 ( -1.8522e-08 1.90435e-08 ) ergs/cm2
Band function
Time interval is from 5.184 sec. to 6.184 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] : 19.1479 (-6.4963 11.9574)
R^2/D10^2 : 2.91677E-02 (-0.0291677 0.0885403)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.096e-09 1.413e-09
25- 50 1.014e-08 6.420e-09
50-150 2.735e-08 1.735e-08
15-150 3.959e-08 2.533e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 2.25980 (-0.894567 0.894588)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.34e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.627e-09 3.648e-09
25- 50 1.082e-08 6.890e-09
50-150 2.374e-08 1.562e-08
15-150 4.019e-08 2.498e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.96820 (-4.96211 185.039)
R1^2/D10^2 : 1.42460 (-1.43808 -1.43808)
kT2 [keV] : 22.3884 (-22.3856 -22.3856)
R2^2/D10^2 : 1.55565E-02 (-0.0155649 0.0689987)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.14e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.808e-09 3.174e-09
25- 50 9.818e-09 5.655e-09
50-150 2.873e-08 1.846e-08
15-150 4.336e-08 2.328e-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: 1.50558 ( -0.321729 0.325488 )
Norm@50keV : 1.29974E-03 ( -0.000245162 0.000243916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.89e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 50.45 sec: 0.162503 ( -0.0314795 0.0316568 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.21483e-07 ( -1.25129e-07 1.26263e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18131 ( -1.40201 1.3243 )
Epeak [keV] : 136.594 ( -136.62 -136.62 )
Norm@50keV : 1.85516E-03 ( -0.00100504 0.00591606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.70e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 50.45 sec: 0.160230 ( -0.032697 0.032455 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.13538e-07 ( -1.28693e-07 1.29379e-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) = 2.60e-07
S(50-100 keV) = 3.22e-07
T90 vs. Hardness ratio plot
T90 = 286.975999951363 sec.
Hardness ratio (energy fluence ratio) = 1.23846
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.10946
Count Ratio (50-100 keV) / (15-25 keV) = 0.80071
Mask shadow pattern
IMX = 7.279075773863132E-01, IMY = 3.818464470884497E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.056000 0.392000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.392000 50.844600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
323.9337 -41.8732 1.6 39.4 -27.7 0.9106 7.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
138.044600 326.844600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
274.1468 -13.8746 5.5 51.2 -41.8 -2.4567 -2.1 12.7 GX 17+2
275.7447 -30.5145 7.8 39.9 -59.3 0.7529 1.5 12.9 H1820-303
285.1834 -24.8558 4.4 36.1 -44.1 -0.9504 -2.6 8.9 HT1900.1-2455
28.0161 -47.1640 2.6 44.7 150.0 3.6368 4.5 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:17:12 EST 2026