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
99.9457 54.9866 0.0084 17.6135 -32.7909 0.8667899 22.932 TRIG_01417793
Foreground time interval of the image:
-0.112 10.448 (delta_t = 10.560 [sec])
Background time interval of the image:
-239.408 -0.112 (delta_t = 239.296 [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 -0.112 sec. to 10.448 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76679 ( -0.116364 0.118756 )
Norm@50keV : 5.02754E-03 ( -0.000385682 0.000382614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.30 using 59 bins.
Reduced chi-squared = 1.19825
# Null hypothesis probability of 1.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.56 sec: 0.684096 ( -0.047789 0.047821 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89535e-07 ( -3.8486e-08 3.88539e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.112 sec. to 10.448 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.342717 ( -0.768243 0.645868 )
Epeak [keV] : 50.6957 ( -5.82593 9.69286 )
Norm@50keV : 3.12090E-02 ( -0.0174743 0.0530964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.34 using 59 bins.
Reduced chi-squared = 0.916786
# Null hypothesis probability of 6.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.56 sec: 0.649180 ( -0.04999 0.050081 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.32647e-07 ( -4.24684e-08 4.44355e-08 ) ergs/cm2
Band function
Time interval is from -0.112 sec. to 10.448 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] : 11.5488 (-0.817711 0.892163)
R^2/D10^2 : 0.197616 (-0.0482864 0.0627518)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.25e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.863e-08 7.096e-09
25- 50 1.762e-07 1.394e-08
50-150 1.376e-07 2.154e-08
15-150 3.725e-07 2.988e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 98.7884 (-21.2785 32.3316)
Norm : 3.06752 (-0.284683 0.320099)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.55e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.466e-08 9.889e-09
25- 50 1.460e-07 1.230e-08
50-150 2.350e-07 7.318e-08
15-150 4.657e-07 8.464e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.51182 (-1.94339 1.38856)
R1^2/D10^2 : 0.342894 (-0.115972 0.256955)
kT2 [keV] : 36.1590 (-18.4187 -37.0272)
R2^2/D10^2 : 1.40542E-03 (-0.00128169 0.0183662)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.51e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.815e-08 1.213e-08
25- 50 1.691e-07 3.311e-08
50-150 2.172e-07 9.668e-08
15-150 4.545e-07 1.328e-07
Peak spectrum fit
Power-law model
Time interval is from 0.060 sec. to 1.060 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83287 ( -0.185213 0.194372 )
Norm@50keV : 1.13122E-02 ( -0.00143425 0.00140477 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.15 using 59 bins.
Reduced chi-squared = 1.21316
# Null hypothesis probability of 1.30e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.57919 ( -0.16854 0.16859 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04061e-07 ( -1.31493e-08 1.33638e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.060 sec. to 1.060 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06589 ( -1.05918 0.826956 )
Epeak [keV] : 52.8506 ( -13.0883 -52.8496 )
Norm@50keV : 3.06514E-02 ( -0.0306542 0.0920005 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.76 using 59 bins.
Reduced chi-squared = 1.19214
# Null hypothesis probability of 1.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.53971 ( -0.17481 0.17419 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.7051e-08 ( -1.47396e-08 1.535e-08 ) ergs/cm2
Band function
Time interval is from 0.060 sec. to 1.060 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] : 11.0125 (-1.26372 1.44043)
R^2/D10^2 : 0.532930 (-0.196579 0.306231)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.10e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.351e-08 2.794e-09
25- 50 3.825e-08 5.375e-09
50-150 2.623e-08 7.155e-09
15-150 7.798e-08 1.175e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.0625 (-27.0381 50.4856)
Norm : 7.23675 (-1.04135 1.26479)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.888e-08 2.955e-09
25- 50 3.185e-08 3.780e-09
50-150 4.819e-08 2.208e-08
15-150 9.892e-08 2.329e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.77337 (-5.09691 2.75462)
R1^2/D10^2 : 1.43252 (-0.829431 74.7975)
kT2 [keV] : 24.6185 (-13.0331 -25.3068)
R2^2/D10^2 : 1.50576E-02 (-0.0131583 0.314601)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.12e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.691e-08 6.679e-09
25- 50 3.447e-08 1.471e-08
50-150 4.659e-08 2.598e-08
15-150 9.797e-08 4.528e-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: 1.76679 ( -0.116364 0.118756 )
Norm@50keV : 5.02754E-03 ( -0.000385682 0.000382614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.56 sec: 0.684063 ( -0.0477859 0.0478174 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89456e-07 ( -3.85188e-08 3.88687e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.342807 ( -0.768276 0.645835 )
Epeak [keV] : 50.6965 ( -5.82603 9.69276 )
Norm@50keV : 3.12052E-02 ( -0.0174741 0.0530966 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.56 sec: 0.649094 ( -0.049974 0.050067 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.32758e-07 ( -4.11946e-08 4.44692e-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) = 1.36e-07
S(50-100 keV) = 1.61e-07
T90 vs. Hardness ratio plot
T90 = 8.51199984550476 sec.
Hardness ratio (energy fluence ratio) = 1.18382
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.55067
Count Ratio (50-100 keV) / (15-25 keV) = 0.724398
Mask shadow pattern
IMX = 2.668885385599173E-01, IMY = 1.719381334084647E-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:
-239.408000 -0.112000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6174 22.0087 0.8 35.1 44.7 9.5341 15.0 0.9 Crab
19.4445 29.9957 2.3 43.0 143.8 5.1473 5.1 ------ UNKNOWN
88.6738 45.4538 2.3 15.9 9.0 1.5847 5.0 ------ UNKNOWN
341.6914 83.0455 2.9 34.9 -123.2 1.8239 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.112000 10.448000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5368 22.1245 13.2 35.0 44.8 0.0561 0.9 8.5 Crab
99.9457 54.9866 0.5 17.6 -32.8 0.8665 22.9 ------ UNKNOWN
308.2212 63.5035 2.5 52.6 -139.9 0.8265 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.092590 962.670300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6365 22.0215 0.9 35.1 62.7 37.2052 13.6 0.5 Crab
3.7044 55.2963 2.6 50.4 168.5 15.5335 4.4 ------ UNKNOWN
145.1374 8.3590 2.3 58.7 -19.4 22.9659 5.1 ------ UNKNOWN
180.8589 78.0122 2.7 34.9 -123.2 6.1778 4.4 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:12:51 EST 2026