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
231.8749 6.7644 0.0129 38.9416 -141.2435 3.4962041 14.958 TRIG_01444088
Foreground time interval of the image:
-2.680 112.501 (delta_t = 115.181 [sec])
Background time interval of the image:
-239.000 -2.680 (delta_t = 236.320 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -2.680 sec. to 117.672 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75609 ( -0.145892 0.148796 )
Norm@50keV : 2.13964E-03 ( -0.000190892 0.000188845 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.28 using 59 bins.
Reduced chi-squared = 1.21544
# Null hypothesis probability of 1.28e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 120.4 sec: 0.289982 ( -0.024616 0.024666 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.37666e-06 ( -2.17492e-07 2.19232e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.680 sec. to 117.672 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65049 ( -0.563411 0.538786 )
Epeak [keV] : 159.289 ( -136.557 -159.289 )
Norm@50keV : 2.43183E-03 ( -0.00131827 0.00229119 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.16 using 59 bins.
Reduced chi-squared = 1.235
# Null hypothesis probability of 1.11e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 120.4 sec: 0.288743 ( -0.025345 0.025219 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35867e-06 ( -2.35494e-07 2.31725e-07 ) ergs/cm2
Band function
Time interval is from -2.680 sec. to 117.672 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] : 12.8650 ( )
R^2/D10^2 : 5.30914E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 115.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.80e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.244e-07 3.606e-08
25- 50 7.642e-07 8.091e-08
50-150 7.947e-07 1.375e-07
15-150 1.783e-06 1.854e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 127.535 (-38.4979 59.1984)
Norm : 1.20021 (-0.123068 0.164412)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.09e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.753e-07 4.094e-08
25- 50 6.784e-07 7.663e-08
50-150 1.247e-06 4.847e-07
15-150 2.300e-06 5.635e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.78454 (-1.20237 1.49486)
R1^2/D10^2 : 0.718292 (-0.408299 1.09838)
kT2 [keV] : 23.1930 (-4.50588 7.77564)
R2^2/D10^2 : 4.86660E-03 (-0.00316013 0.00623908)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.04e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.210e-07 1.227e-07
25- 50 6.451e-07 1.681e-07
50-150 1.272e-06 4.889e-07
15-150 2.338e-06 6.767e-07
Peak spectrum fit
Power-law model
Time interval is from 33.356 sec. to 34.356 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40987 ( -0.230749 0.230492 )
Norm@50keV : 1.74221E-02 ( -0.00239261 0.00238866 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.91 using 59 bins.
Reduced chi-squared = 1.03351
# Null hypothesis probability of 4.05e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.12653 ( -0.30112 0.30172 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68027e-07 ( -2.49664e-08 2.50987e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 33.356 sec. to 34.356 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25694 ( -0.971328 1.53999 )
Epeak [keV] : 257.452 ( -257.468 -257.468 )
Norm@50keV : 2.07093E-02 ( -0.0175995 0.0391433 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.82 using 59 bins.
Reduced chi-squared = 1.05036
# Null hypothesis probability of 3.73e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.11700 ( -0.30617 0.30535 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66905e-07 ( -2.60442e-08 2.56656e-08 ) ergs/cm2
Band function
Time interval is from 33.356 sec. to 34.356 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] : 16.7403 (-2.85377 3.58373)
R^2/D10^2 : 0.169731 (-0.0832845 0.156041)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.43e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.727e-09 2.964e-09
25- 50 4.251e-08 1.049e-08
50-150 8.463e-08 2.399e-08
15-150 1.369e-07 2.550e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-62.5848 -200)
Norm : 8.84027 (-1.21153 1.21153)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.63e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.201e-08 1.250e-08
25- 50 4.235e-08 2.366e-08
50-150 9.288e-08 5.185e-08
15-150 1.572e-07 8.825e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.41368 (-3.21544 4.15217)
R1^2/D10^2 : 1.74464 (-1.27187 12.2798)
kT2 [keV] : 29.3191 (-9.34092 54.8668)
R2^2/D10^2 : 1.99727E-02 (-0.0188999 0.0612035)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.25e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.901e-08 1.051e-08
25- 50 4.151e-08 2.150e-08
50-150 1.070e-07 5.930e-08
15-150 1.675e-07 8.645e-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: 1.77456 ( -0.147103 0.150251 )
Norm@50keV : 2.16457E-03 ( -0.000196132 0.000193856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 115.2 sec: 0.295382 ( -0.0252119 0.0252453 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.298e-06 ( -2.12764e-07 2.14249e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66936 ( -0.574765 0.522231 )
Epeak [keV] : 149.811 ( -121.961 -149.815 )
Norm@50keV : 2.46140E-03 ( -0.000963433 0.00241236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 115.2 sec: 0.294111 ( -0.025946 0.025901 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.28126e-06 ( -2.3116e-07 2.26794e-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) = 6.59e-07
S(50-100 keV) = 7.79e-07
T90 vs. Hardness ratio plot
T90 = 103.167999982834 sec.
Hardness ratio (energy fluence ratio) = 1.18209
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.05794
Count Ratio (50-100 keV) / (15-25 keV) = 0.800333
Mask shadow pattern
IMX = -6.301666798253378E-01, IMY = 5.058793776288397E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-239.000000 -2.680000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4227 -60.6569 4.8 57.3 -17.9 2.8154 2.4 3.7 Cen X-3
186.6222 -62.8171 6.0 56.7 -27.4 -3.2357 -1.9 3.0 GX 301-2
174.4687 -5.8892 2.5 20.6 58.5 1.5574 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.680000 112.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.0309 -60.5987 39.8 57.3 -17.7 -0.2130 -0.3 8.5 Cen X-3
186.5978 -62.8815 12.5 56.8 -27.4 0.8446 1.0 6.9 GX 301-2
158.4745 -26.4522 2.0 40.2 23.9 1.3437 5.8 ------ UNKNOWN
231.8749 6.7645 0.8 38.9 -141.2 3.4965 14.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
192.900600 963.165800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9648 -15.6407 0.6 25.9 -49.6 25.7273 20.9 0.8 Sco X-1
254.4477 35.5198 4.0 35.5 -167.0 3.9275 2.9 10.7 Her X-1
256.2283 -37.7226 1645.8 49.9 -44.8 -0.0309 -0.0 13.6 4U 1700-377
256.4518 -36.3761 57.7 48.9 -46.0 0.8656 0.2 2.9 GX 349+2
263.0924 -24.6605 17.6 43.7 -62.6 2.8984 0.7 6.8 GX 1+4
268.4160 -1.3548 12.9 37.4 -98.4 3.0002 0.9 6.5 SW J1753.5-0127
196.3773 -34.7935 2.7 53.3 16.9 12.5478 4.2 ------ UNKNOWN
211.6674 2.1469 3.7 20.7 58.5 3.4506 3.1 ------ UNKNOWN
243.1774 56.3115 2.1 50.4 168.5 17.3717 5.4 ------ UNKNOWN
254.6566 -12.6266 2.5 29.8 -69.1 7.3719 4.7 ------ UNKNOWN
271.2289 1.1636 2.7 39.6 -103.2 18.7404 4.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:05:02 EST 2026