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
111.7765 6.6047 0.1191 17.4904 -82.7168 1.1632581 1.620 TRIG_01403878
Foreground time interval of the image:
-0.072 796.972 (delta_t = 797.044 [sec])
Background time interval of the image:
-239.688 -0.072 (delta_t = 239.616 [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 0.512000
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 0.512000
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 0.512000
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 -0.072 sec. to 796.972 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50746 ( -0.360361 0.364857 )
Norm@50keV : 1.95713E-04 ( -4.55429e-05 4.50284e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.60 using 59 bins.
Reduced chi-squared = 0.905263
# Null hypothesis probability of 6.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 797 sec: 2.44825E-02 ( -0.0055107 0.0055208 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47818e-06 ( -3.67655e-07 3.75985e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.072 sec. to 796.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.110811 ( -2.47921 1.65426 )
Epeak [keV] : 61.2973 ( -14.3185 -61.2691 )
Norm@50keV : 1.13035E-03 ( -0.00113293 0.0241594 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.57 using 59 bins.
Reduced chi-squared = 0.885179
# Null hypothesis probability of 7.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 797 sec: 2.34535E-02 ( -0.0056394 0.0056692 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3083e-06 ( -3.77431e-07 4.25857e-07 ) ergs/cm2
Band function
Time interval is from -0.072 sec. to 796.972 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] : 13.4313 (-2.91555 3.92425)
R^2/D10^2 : 4.30508E-03 (-0.00261142 0.00605916)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.99e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.311e-07 5.666e-08
25- 50 4.676e-07 1.841e-07
50-150 5.433e-07 2.815e-07
15-150 1.142e-06 4.747e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.556 (-123.008 -198.186)
Norm : 0.101234 (-0.0225376 0.0281008)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.07e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.010e-07 1.218e-07
25- 50 3.865e-07 2.225e-07
50-150 8.465e-07 4.898e-07
15-150 1.434e-06 8.161e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.77916 (-7.86396 -7.86396)
R1^2/D10^2 : 1.54396E-02 (-0.0149229 -0.0149229)
kT2 [keV] : 20.1827 (-21.3629 -21.3629)
R2^2/D10^2 : 6.94679E-04 (-0.000503214 0.00679652)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.751e-07 1.105e-07
25- 50 4.366e-07 3.011e-07
50-150 7.088e-07 3.952e-07
15-150 1.321e-06 7.125e-07
Peak spectrum fit
Power-law model
Time interval is from -0.074 sec. to 0.926 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74201 ( -0.126958 0.130206 )
Norm@50keV : 2.08805E-02 ( -0.00178701 0.00177021 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.21 using 59 bins.
Reduced chi-squared = 0.968596
# Null hypothesis probability of 5.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.81526 ( -0.22163 0.22173 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.92792e-07 ( -1.69875e-08 1.7131e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.074 sec. to 0.926 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.799420 ( -0.667487 0.577603 )
Epeak [keV] : 58.7755 ( -9.51136 23.7728 )
Norm@50keV : 6.76749E-02 ( -0.0342666 0.0864234 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.85 using 59 bins.
Reduced chi-squared = 0.836607
# Null hypothesis probability of 8.03e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.74305 ( -0.22685 0.2265 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81147e-07 ( -1.81911e-08 1.85033e-08 ) ergs/cm2
Band function
Time interval is from -0.074 sec. to 0.926 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] : 12.4052 (-1.05386 1.15393)
R^2/D10^2 : 0.631139 (-0.177411 0.243693)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.17e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.058e-08 3.115e-09
25- 50 6.732e-08 5.935e-09
50-150 6.365e-08 1.009e-08
15-150 1.516e-07 1.455e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 113.809 (-28.7217 42.4903)
Norm : 12.1884 (-1.17788 1.41402)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.180e-08 3.795e-09
25- 50 5.637e-08 5.760e-09
50-150 9.795e-08 3.443e-08
15-150 1.861e-07 4.070e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.47788 (-2.25747 1.46993)
R1^2/D10^2 : 3.67363 (-2.23524 12.3791)
kT2 [keV] : 18.8821 (-4.03428 10.9749)
R2^2/D10^2 : 9.77449E-02 (-0.0820976 0.179151)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.42e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.955e-08 1.412e-08
25- 50 5.948e-08 2.425e-08
50-150 8.934e-08 4.587e-08
15-150 1.784e-07 6.134e-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: 1.50746 ( -0.360361 0.364857 )
Norm@50keV : 1.95713E-04 ( -4.55429e-05 4.50284e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 797 sec: 2.44819E-02 ( -0.00551046 0.00552046 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47798e-06 ( -3.67373e-07 3.76661e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.109192 ( -2.4788 1.6557 )
Epeak [keV] : 61.2681 ( -14.2242 -61.2672 )
Norm@50keV : 1.13289E-03 ( -0.00113297 0.0241509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 797 sec: 2.34515E-02 ( -0.0056386 0.0056495 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30871e-06 ( -3.77587e-07 4.27057e-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) = 3.67e-07
S(50-100 keV) = 5.16e-07
T90 vs. Hardness ratio plot
T90 = 684.683999896049 sec.
Hardness ratio (energy fluence ratio) = 1.40599
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.24651
Count Ratio (50-100 keV) / (15-25 keV) = 1.23811
Mask shadow pattern
IMX = 3.994837969108041E-02, IMY = 3.125725581834870E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.688000 -0.072000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6088 22.0164 0.4 16.5 143.0 9.2136 26.3 1.4 Crab
107.0703 14.2099 3.2 13.5 -113.1 1.2943 3.6 ------ UNKNOWN
114.3146 -17.3479 2.4 33.0 -36.5 2.1835 4.8 ------ UNKNOWN
120.0465 38.6119 3.1 37.5 -145.8 1.9424 3.7 ------ UNKNOWN
122.9397 44.8877 2.3 43.5 -150.1 3.1721 4.9 ------ UNKNOWN
135.4481 6.0713 2.8 40.9 -88.5 6.6785 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.072000 796.972000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4783 21.9434 16.7 16.5 142.5 0.4454 0.7 9.6 Crab
Post-slew image of 15-350 keV band
Time interval of the image:
957.712600 962.382400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.7366 -40.6902 0.0 11.7 117.4 -0.0367 -1.4 12.5 Vela X-1
170.2963 -60.6278 547.8 19.9 -14.3 0.0005 0.0 0.6 Cen X-3
186.8908 -62.8211 3.8 27.6 -21.1 0.0808 3.0 7.1 GX 301-2
105.4296 -24.1911 2.3 41.9 117.7 0.5159 5.0 ------ UNKNOWN
96.2284 -69.6755 2.4 36.9 42.4 0.2242 4.7 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:17:57 EST 2026