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
86.4423 63.5826 0.0068 21.1272 44.1789 2.6340828 28.335 TRIG_01429608
Foreground time interval of the image:
-31.264 10.037 (delta_t = 41.301 [sec])
Background time interval of the image:
-239.264 -31.264 (delta_t = 208.000 [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 -31.264 sec. to 64.736 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61246 ( -0.0560902 0.056224 )
Norm@50keV : 5.06601E-03 ( -0.000153604 0.000153487 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.90 using 59 bins.
Reduced chi-squared = 1.08596
# Null hypothesis probability of 3.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 96 sec: 0.653565 ( -0.021255 0.021312 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.54214e-06 ( -1.45095e-07 1.45572e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.264 sec. to 64.736 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27697 ( -0.236082 0.223842 )
Epeak [keV] : 111.228 ( -26.0602 111.094 )
Norm@50keV : 7.36650E-03 ( -0.00158964 0.00216509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.19 using 59 bins.
Reduced chi-squared = 0.985536
# Null hypothesis probability of 5.06e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 96 sec: 0.638655 ( -0.023237 0.023304 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.42386e-06 ( -1.65416e-07 1.64854e-07 ) ergs/cm2
Band function
Time interval is from -31.264 sec. to 64.736 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] : 14.7379 ( )
R^2/D10^2 : 7.43855E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 270.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.96e-29 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.256e-07 1.973e-08
25- 50 1.273e-06 4.896e-08
50-150 1.867e-06 1.080e-07
15-150 3.465e-06 1.238e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 178.798 (-27.6892 -178.221)
Norm : 2.64157 (-0.0911377 0.0996856)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.400e-07 3.360e-08
25- 50 1.215e-06 8.976e-08
50-150 2.566e-06 6.466e-07
15-150 4.421e-06 6.960e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.93692 (-0.804597 0.831839)
R1^2/D10^2 : 0.461100 (-0.125262 0.193474)
kT2 [keV] : 28.4542 (-3.50313 4.95238)
R2^2/D10^2 : 5.33599E-03 (-0.00230411 0.00337369)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.683e-07 5.050e-08
25- 50 1.269e-06 8.976e-08
50-150 2.576e-06 2.971e-07
15-150 4.414e-06 3.898e-07
Peak spectrum fit
Power-law model
Time interval is from 24.236 sec. to 25.236 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36517 ( -0.0874277 0.0876316 )
Norm@50keV : 3.74926E-02 ( -0.00204603 0.0020441 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.69 using 59 bins.
Reduced chi-squared = 1.08228
# Null hypothesis probability of 3.12e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.53118 ( -0.24931 0.24948 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64998e-07 ( -2.1946e-08 2.20546e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 24.236 sec. to 25.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.493040 ( -0.411308 0.375943 )
Epeak [keV] : 89.4598 ( -14.0588 29.4647 )
Norm@50keV : 0.100880 ( -0.0342149 0.0573815 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.21 using 59 bins.
Reduced chi-squared = 0.789464
# Null hypothesis probability of 8.73e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.40245 ( -0.25572 0.25566 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.47744e-07 ( -2.33969e-08 2.34748e-08 ) ergs/cm2
Band function
Time interval is from 24.236 sec. to 25.236 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] : 16.6367 (-1.05892 1.13673)
R^2/D10^2 : 0.384611 (-0.078067 0.0971975)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 87.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.28e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.180e-08 2.215e-09
25- 50 9.481e-08 6.765e-09
50-150 1.860e-07 2.000e-08
15-150 3.026e-07 2.090e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-15.6637 -200)
Norm : 18.8039 (-1.01657 1.01657)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.34e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.682e-08 2.475e-09
25- 50 9.006e-08 6.375e-09
50-150 1.975e-07 3.555e-08
15-150 3.344e-07 3.170e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.81391 (-1.37222 1.75271)
R1^2/D10^2 : 3.75398 (-1.88292 4.26332)
kT2 [keV] : 22.8917 (-2.70197 4.10219)
R2^2/D10^2 : 0.106375 (-0.0506945 0.0667659)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.20e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.733e-08 1.160e-08
25- 50 9.013e-08 1.906e-08
50-150 2.198e-07 4.510e-08
15-150 3.473e-07 6.750e-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: 1.57906 ( -0.0981325 0.0988951 )
Norm@50keV : 3.98595E-03 ( -0.000225047 0.000224194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.61e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 41.3 sec: 0.508933 ( -0.0285177 0.0285844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54362e-06 ( -9.40145e-08 9.45469e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28554 ( -0.418517 0.336485 )
Epeak [keV] : 120.373 ( -44.4038 -120.375 )
Norm@50keV : 5.62093E-03 ( -0.00176377 0.00345586 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 41.3 sec: 0.501162 ( -0.030238 0.030219 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50717e-06 ( -1.06414e-07 1.06054e-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) = 1.18e-06
S(50-100 keV) = 1.55e-06
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 1.31356
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38523
Count Ratio (50-100 keV) / (15-25 keV) = 0.921759
Mask shadow pattern
IMX = 2.771231430046500E-01, IMY = -2.692916768903330E-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:
-239.264000 -31.264000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
90.6558 50.1264 3.1 29.7 69.4 1.8128 3.8 ------ UNKNOWN
348.0515 27.6752 2.4 48.0 -129.1 6.7848 4.9 ------ UNKNOWN
300.7147 60.2297 3.5 43.8 -64.1 4.4332 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-31.264000 10.036600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
91.3923 42.0973 2.6 35.8 79.1 0.8611 4.4 ------ UNKNOWN
86.4423 63.5826 0.4 21.1 44.2 2.6340 28.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.436600 962.816000
975.736000 1065.866000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6236 21.9901 2.7 41.6 115.2 27.0996 4.2 1.6 Crab
350.5505 55.2783 2.7 44.8 -122.3 21.4372 4.3 ------ UNKNOWN
353.6636 49.7507 2.1 48.0 -129.1 30.6096 5.5 ------ UNKNOWN
255.7607 72.4438 2.7 43.8 -64.1 25.1730 4.3 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:08:51 EST 2026