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
13.2443 -62.0383 0.0068 28.3632 -85.6257 2.7417282 28.184 TRIG_01403191
Foreground time interval of the image:
-5.432 19.485 (delta_t = 24.917 [sec])
Background time interval of the image:
-239.816 -5.432 (delta_t = 234.384 [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 -5.432 sec. to 52.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87105 ( -0.105131 0.107265 )
Norm@50keV : 3.80536E-03 ( -0.000243168 0.000240774 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.14 using 59 bins.
Reduced chi-squared = 0.984912
# Null hypothesis probability of 5.07e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 57.5 sec: 0.539552 ( -0.031373 0.031419 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01186e-06 ( -1.27745e-07 1.28701e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.432 sec. to 52.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57086 ( -0.430069 0.363014 )
Epeak [keV] : 66.2836 ( -16.7955 -66.2836 )
Norm@50keV : 5.50408E-03 ( -0.00184434 0.00373791 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.44 using 59 bins.
Reduced chi-squared = 0.972143
# Null hypothesis probability of 5.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 57.5 sec: 0.531113 ( -0.033192 0.033199 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95928e-06 ( -1.44404e-07 1.45017e-07 ) ergs/cm2
Band function
Time interval is from -5.432 sec. to 52.064 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] : 11.6878 ( )
R^2/D10^2 : 0.136702 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 131.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.26e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.265e-07 2.228e-08
25- 50 6.908e-07 4.772e-08
50-150 5.573e-07 7.475e-08
15-150 1.475e-06 9.487e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 91.3275 (-16.9739 23.8494)
Norm : 2.41096 (-0.204795 0.230715)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.29e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.619e-07 3.637e-08
25- 50 6.140e-07 3.565e-08
50-150 9.434e-07 2.881e-07
15-150 1.919e-06 3.004e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.89067 (-1.00091 1.11117)
R1^2/D10^2 : 1.23805 (-0.573446 1.30239)
kT2 [keV] : 21.0758 (-3.31501 4.99088)
R2^2/D10^2 : 1.14383E-02 (-0.00643262 0.0113275)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.746e-07 7.731e-08
25- 50 5.900e-07 9.410e-08
50-150 9.662e-07 2.701e-07
15-150 1.931e-06 3.944e-07
Peak spectrum fit
Power-law model
Time interval is from -0.200 sec. to 0.800 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62079 ( -0.190117 0.194739 )
Norm@50keV : 1.80248E-02 ( -0.00214348 0.00211601 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.71 using 59 bins.
Reduced chi-squared = 0.819474
# Null hypothesis probability of 8.33e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.33151 ( -0.26048 0.26067 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68182e-07 ( -2.1286e-08 2.15235e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.200 sec. to 0.800 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31140 ( -0.852233 0.483552 )
Epeak [keV] : 106.915 ( -49.2176 -106.915 )
Norm@50keV : 2.62468E-02 ( -0.0101228 0.0460774 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.20 using 59 bins.
Reduced chi-squared = 0.825
# Null hypothesis probability of 8.22e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.30628 ( -0.26873 0.26714 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64305e-07 ( -2.3282e-08 2.33283e-08 ) ergs/cm2
Band function
Time interval is from -0.200 sec. to 0.800 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] : 13.6439 (-1.77495 2.08464)
R^2/D10^2 : 0.364331 (-0.146157 0.237538)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.436e-08 3.347e-09
25- 50 5.202e-08 8.575e-09
50-150 6.291e-08 1.588e-08
15-150 1.293e-07 1.870e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 160.224 (-64.4952 -162.459)
Norm : 9.58110 (-1.14756 1.36246)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.45e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.446e-08 1.345e-08
25- 50 4.577e-08 2.431e-08
50-150 9.277e-08 5.310e-08
15-150 1.630e-07 8.328e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.97270 (-1.86768 3.25162)
R1^2/D10^2 : 8.08299 (-6.61096 59.7126)
kT2 [keV] : 19.6321 (-4.12485 10.8677)
R2^2/D10^2 : 8.32499E-02 (-0.0679693 0.123473)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.68e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.546e-08 1.336e-08
25- 50 4.304e-08 1.700e-08
50-150 8.782e-08 4.108e-08
15-150 1.563e-07 5.906e-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: 1.78637 ( -0.100482 0.101981 )
Norm@50keV : 6.94361E-03 ( -0.00040568 0.000402516 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 24.92 sec: 0.951805 ( -0.0530642 0.0532001 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5938e-06 ( -9.52574e-08 9.57935e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72015 ( -0.375468 0.3674 )
Epeak [keV] : 204.339 ( -137.041 -204.338 )
Norm@50keV : 7.51512E-03 ( -0.00202486 0.00409806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.84e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 24.92 sec: 0.948164 ( -0.056094 0.055366 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58579e-06 ( -1.05947e-07 1.02379e-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) = 5.81e-07
S(50-100 keV) = 6.38e-07
T90 vs. Hardness ratio plot
T90 = 40.9919999837875 sec.
Hardness ratio (energy fluence ratio) = 1.09811
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.14148
Count Ratio (50-100 keV) / (15-25 keV) = 0.692317
Mask shadow pattern
IMX = 4.117690108531410E-02, IMY = 5.382960737307498E-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:
-239.816000 -5.432000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
69.3694 -13.7247 2.1 48.7 165.1 5.1703 5.5 ------ UNKNOWN
325.3507 -14.7167 4.6 53.0 4.6 2.5069 2.5 ------ UNKNOWN
333.2898 -36.9719 2.8 38.0 -20.9 1.7942 4.2 ------ UNKNOWN
49.5164 -49.8553 2.3 26.6 -137.2 1.8046 5.0 ------ UNKNOWN
358.4204 -65.8752 2.2 34.4 -77.0 3.0144 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.432000 19.484600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
64.2305 -2.8977 3.2 51.4 149.9 1.0837 3.6 ------ UNKNOWN
13.2443 -62.0383 0.4 28.4 -85.6 2.7417 28.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.684600 462.384600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
301.6755 -35.6507 3.0 50.6 -7.0 3.3646 3.9 ------ UNKNOWN
29.7038 -74.1727 2.8 13.5 -112.9 1.9215 4.1 ------ UNKNOWN
128.0550 -58.6468 2.8 49.3 -132.1 8.6812 4.1 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:18:43 EST 2026