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
336.0867 -59.1702 0.0118 28.1929 -122.9545 1.9599230 16.275 TRIG_01443066
Foreground time interval of the image:
-6.960 20.080 (delta_t = 27.040 [sec])
Background time interval of the image:
-239.136 -6.960 (delta_t = 232.176 [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 -6.960 sec. to 20.080 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31281 ( -0.188869 0.185914 )
Norm@50keV : 4.04244E-03 ( -0.000439065 0.000437936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.93 using 59 bins.
Reduced chi-squared = 1.26193
# Null hypothesis probability of 8.79e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 27.04 sec: 0.483436 ( -0.053367 0.053428 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07695e-06 ( -1.3009e-07 1.31242e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.960 sec. to 20.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21462 ( -0.753511 0.27019 )
Epeak [keV] : 403.932 ( -403.961 -403.961 )
Norm@50keV : 4.53496E-03 ( -0.00178552 0.00610902 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.87 using 59 bins.
Reduced chi-squared = 1.28339
# Null hypothesis probability of 7.50e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 27.04 sec: 0.481745 ( -0.027386 0.05428 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0686e-06 ( -1.43019e-07 1.39089e-07 ) ergs/cm2
Band function
Time interval is from -6.960 sec. to 20.080 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] : 16.7088 (-2.3801 2.98272)
R^2/D10^2 : 3.88805E-02 (-0.0166452 0.0274262)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.49e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.005e-08 1.384e-08
25- 50 2.620e-07 4.893e-08
50-150 5.194e-07 1.096e-07
15-150 8.415e-07 1.279e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-40.2098 -200)
Norm : 2.00021 (-0.217673 0.217673)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.53e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.347e-07 7.417e-08
25- 50 2.590e-07 1.418e-07
50-150 5.681e-07 3.132e-07
15-150 9.618e-07 5.240e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.41161 (-2.05113 2.6372)
R1^2/D10^2 : 0.394530 (-0.24067 0.477796)
kT2 [keV] : 31.3574 (-8.73329 27.1356)
R2^2/D10^2 : 3.94046E-03 (-0.00326373 0.00792813)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.75e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.155e-07 6.088e-08
25- 50 2.520e-07 1.164e-07
50-150 7.134e-07 3.650e-07
15-150 1.081e-06 4.561e-07
Peak spectrum fit
Power-law model
Time interval is from 8.464 sec. to 9.464 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30144 ( -0.289663 0.282276 )
Norm@50keV : 1.34965E-02 ( -0.00235774 0.00235268 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.39 using 59 bins.
Reduced chi-squared = 0.901579
# Null hypothesis probability of 6.85e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.61061 ( -0.2874 0.28807 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33337e-07 ( -2.53653e-08 2.56348e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.464 sec. to 9.464 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.435065 ( -1.50482 0.990252 )
Epeak [keV] : 93.7374 ( -32.3033 -93.7367 )
Norm@50keV : 3.60287E-02 ( -0.0360292 0.145101 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.72 using 59 bins.
Reduced chi-squared = 0.887857
# Null hypothesis probability of 7.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.56688 ( -0.29686 0.29542 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.61721e-08 ( -1.73935e-08 9.64664e-09 ) ergs/cm2
Band function
Time interval is from 8.464 sec. to 9.464 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] : 17.3209 (-3.20128 4.29654)
R^2/D10^2 : 0.120560 (-0.0648201 0.125519)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.03e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.327e-09 2.425e-09
25- 50 3.290e-08 1.001e-08
50-150 7.089e-08 2.703e-08
15-150 1.111e-07 3.954e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-69.595 -200)
Norm : 6.71664 (-1.17738 1.17738)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.39e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.673e-08 9.580e-09
25- 50 3.218e-08 1.845e-08
50-150 7.056e-08 4.001e-08
15-150 1.195e-07 6.795e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.35065 (-5.92257 53.5106)
R1^2/D10^2 : 0.972292 (-0.856762 3271.43)
kT2 [keV] : 23.8516 (-7.52886 64.6385)
R2^2/D10^2 : 3.35227E-02 (-0.033016 0.0720676)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.79e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.225e-08 7.225e-09
25- 50 3.209e-08 1.709e-08
50-150 8.230e-08 4.835e-08
15-150 1.267e-07 6.600e-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: 1.31281 ( -0.188869 0.185914 )
Norm@50keV : 4.04244E-03 ( -0.000439065 0.000437936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.79e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 27.04 sec: 0.483430 ( -0.0533647 0.0534261 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07682e-06 ( -1.3007e-07 1.31244e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21462 ( -0.753511 0.270189 )
Epeak [keV] : 403.953 ( -403.961 -403.961 )
Norm@50keV : 4.53493E-03 ( -0.00178537 0.00610904 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.50e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 27.04 sec: 0.481697 ( -0.027348 0.027348 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.06905e-06 ( -1.43098e-07 7.0788e-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) = 2.41e-07
S(50-100 keV) = 3.89e-07
T90 vs. Hardness ratio plot
T90 = 21.6159999370575 sec.
Hardness ratio (energy fluence ratio) = 1.61411
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.33834
Count Ratio (50-100 keV) / (15-25 keV) = 1.18229
Mask shadow pattern
IMX = -2.915887081181138E-01, IMY = 4.497880771929477E-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:
-239.136000 -6.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
114.4311 -62.4506 2.9 47.7 145.5 23.0184 4.0 ------ UNKNOWN
359.5143 -10.1481 2.8 44.5 -30.4 12.4990 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.960000 20.080000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
23.9744 -9.4682 2.1 40.5 5.2 0.7392 5.4 ------ UNKNOWN
33.9577 -62.0804 2.3 13.4 162.4 0.4380 5.1 ------ UNKNOWN
20.8117 6.2190 2.1 56.3 1.2 2.4907 5.4 ------ UNKNOWN
336.0867 -59.1702 0.7 28.2 -123.0 1.9599 16.3 ------ UNKNOWN
344.4340 -33.3731 2.0 33.0 -70.4 0.9154 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
273.164600 482.924700
540.864000 962.919100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.7242 -40.6468 9.2 38.6 113.3 4.7023 1.3 10.5 Vela X-1
170.4317 -60.6127 10.2 28.7 164.4 1.8024 1.1 3.5 Cen X-3
186.9456 -62.7994 6.1 30.9 -179.9 2.8787 1.9 8.1 GX 301-2
130.2798 -39.7564 2.7 38.4 106.4 16.2017 4.3 ------ UNKNOWN
66.5068 -25.2498 2.9 52.1 28.1 14.3397 3.9 ------ UNKNOWN
182.0227 -41.4413 2.2 49.1 161.8 19.9752 5.3 ------ UNKNOWN
93.7659 -54.4409 2.6 20.6 58.5 5.7040 4.5 ------ UNKNOWN
57.6084 -42.1666 2.9 37.1 12.5 7.0019 4.0 ------ UNKNOWN
170.2561 -61.9153 1.0 27.6 165.7 16.2279 11.1 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:05:59 EST 2026