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
51.4346 -47.8814 0.0028 34.6519 -174.9311 12.0263696 69.067 TRIG_01340514
Foreground time interval of the image:
-19.496 11.757 (delta_t = 31.253 [sec])
Background time interval of the image:
-239.544 -19.496 (delta_t = 220.048 [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 1.024000
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 1.024000
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 1.024000
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 -19.496 sec. to 126.224 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27848 ( -0.0262376 0.0261389 )
Norm@50keV : 1.72575E-02 ( -0.000251223 0.000250369 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.80 using 59 bins.
Reduced chi-squared = 0.663158
# Null hypothesis probability of 9.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 145.7 sec: 2.05094 ( -0.03467 0.0348 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.49827e-05 ( -3.30891e-07 3.31186e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.496 sec. to 126.224 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27512 ( -0.0277118 0.0251451 )
Epeak [keV] : 9999.02 ( -9999.17 -9999.17 )
Norm@50keV : 1.73355E-02 ( -0.000236587 0.000459341 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.06 using 59 bins.
Reduced chi-squared = 0.679643
# Null hypothesis probability of 9.68e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 145.7 sec: 2.05003 ( -0.03465 0.01989 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.506e-05 ( -4.12083e-07 2.4872e-07 ) ergs/cm2
Band function
Time interval is from -19.496 sec. to 126.224 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] : 22.8747 ( )
R^2/D10^2 : 5.68256E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 1207.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.91e-215 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.872e-07 2.280e-08
25- 50 4.258e-06 9.835e-08
50-150 1.664e-05 2.914e-07
15-150 2.169e-05 3.133e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 9.13183 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 561.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.05e-84 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.313e-06 5.537e-08
25- 50 6.373e-06 1.071e-07
50-150 1.398e-05 2.171e-07
15-150 2.366e-05 3.715e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.53846 (-0.461572 0.482823)
R1^2/D10^2 : 0.971835 (-0.167548 0.210755)
kT2 [keV] : 36.5448 (-1.81367 2.11277)
R2^2/D10^2 : 1.05034E-02 (-0.00174427 0.00191775)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.40e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.232e-06 1.311e-07
25- 50 5.675e-06 1.537e-07
50-150 1.709e-05 3.788e-07
15-150 2.500e-05 5.172e-07
Peak spectrum fit
Power-law model
Time interval is from 33.816 sec. to 34.816 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.943855 ( -0.0522795 0.0519865 )
Norm@50keV : 0.142698 ( -0.00400704 0.00399057 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.47 using 59 bins.
Reduced chi-squared = 0.902982
# Null hypothesis probability of 6.82e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 16.3915 ( -0.4653 0.4663 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57511e-06 ( -4.69107e-08 4.69242e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 33.816 sec. to 34.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.936544 ( -0.052009 0.053351 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 0.143296 ( -0.00394265 0.0107463 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.69 using 59 bins.
Reduced chi-squared = 0.923036
# Null hypothesis probability of 6.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.00997e-07 ( -4.98812e-08 3.57857e-08 ) ergs/cm2
Band function
Time interval is from 33.816 sec. to 34.816 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] : 24.8574 ( )
R^2/D10^2 : 0.402456 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 331.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.62e-40 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.333e-08 2.570e-09
25- 50 2.451e-07 1.100e-08
50-150 1.124e-06 5.100e-08
15-150 1.412e-06 5.050e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 67.2538 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 440.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.25e-60 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.675e-07 5.100e-09
25- 50 3.222e-07 9.250e-09
50-150 7.065e-07 2.020e-08
15-150 1.196e-06 3.300e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.03666 (-0.837166 0.933721)
R1^2/D10^2 : 7.80494 (-2.33697 3.54734)
kT2 [keV] : 40.9042 (-3.92043 5.26873)
R2^2/D10^2 : 8.23994E-02 (-0.0235758 0.027894)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.56e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.090e-07 1.249e-08
25- 50 2.815e-07 2.040e-08
50-150 1.224e-06 7.950e-08
15-150 1.614e-06 8.750e-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: 1.11156 ( -0.0340794 0.033915 )
Norm@50keV : 2.59788E-02 ( -0.00049197 0.000490272 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.96e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 31.25 sec: 3.01691 ( -0.0614509 0.0614278 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.45691e-06 ( -1.53537e-07 1.53574e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10584 ( -0.0173407 0.0342386 )
Epeak [keV] : 9998.15 ( -9998.07 -9998.07 )
Norm@50keV : 2.61152E-02 ( -0.000466321 0.0034548 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 31.25 sec: 3.01517 ( -0.03486 0.06156 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.46353e-06 ( -1.49938e-07 1.50375e-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) = 5.49e-06
S(50-100 keV) = 9.06e-06
T90 vs. Hardness ratio plot
T90 = 75.7079999446869 sec.
Hardness ratio (energy fluence ratio) = 1.65027
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50506
Count Ratio (50-100 keV) / (15-25 keV) = 1.3737
Mask shadow pattern
IMX = -6.884875963893101E-01, IMY = 6.106871736789070E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.544000 -19.496000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3625 -60.6333 7.3 36.8 -54.7 0.8357 1.6 1.5 Cen X-3
186.7079 -62.8044 3.0 35.5 -41.2 1.6896 3.8 2.5 GX 301-2
264.8670 -44.3835 13.7 50.3 26.6 0.7911 0.8 6.6 4U 1735-44
324.0916 -45.7058 2.9 40.6 83.8 5.1904 3.9 ------ UNKNOWN
321.3776 -54.7395 2.8 32.2 77.5 2.4903 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.496000 11.756600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.6262 -60.6902 4.9 36.7 -54.5 -0.5686 -2.4 10.0 Cen X-3
186.7781 -62.7559 10.6 35.5 -41.2 -0.2097 -1.1 3.4 GX 301-2
264.8466 -44.3855 6.7 50.3 26.5 -1.0950 -1.7 5.9 4U 1735-44
307.7108 -47.2306 2.4 41.5 66.5 2.7614 4.8 ------ UNKNOWN
51.4346 -47.8814 0.2 34.7 -174.9 12.0260 69.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
88.956600 962.598000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
32.3469 -19.4757 2.7 32.3 158.8 6.5569 4.2 ------ UNKNOWN
114.4831 -40.6334 3.1 44.5 -61.0 19.3691 3.7 ------ UNKNOWN
76.4816 -3.5310 2.4 49.3 -132.1 24.6192 4.8 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:33:47 EST 2026