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
51.4649 -29.6468 0.0074 47.6007 155.6294 5.9696474 25.946 TRIG_01351039
Foreground time interval of the image:
-0.440 14.709 (delta_t = 15.149 [sec])
Background time interval of the image:
-239.792 -0.440 (delta_t = 239.352 [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 -0.440 sec. to 40.492 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46454 ( -0.0435359 0.0434769 )
Norm@50keV : 3.44779E-02 ( -0.000847191 0.000847017 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.71 using 59 bins.
Reduced chi-squared = 1.03
# Null hypothesis probability of 4.12e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 40.93 sec: 4.26456 ( -0.1186 0.11894 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.34701e-05 ( -3.37514e-07 3.37886e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.440 sec. to 40.492 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09159 ( -0.186941 0.179777 )
Epeak [keV] : 140.023 ( -28.2787 73.9286 )
Norm@50keV : 5.04395E-02 ( -0.00826174 0.010291 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.72 using 59 bins.
Reduced chi-squared = 0.816429
# Null hypothesis probability of 8.35e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 40.93 sec: 4.16180 ( -0.12663 0.12724 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32596e-05 ( -3.55125e-07 3.54546e-07 ) ergs/cm2
Band function
Time interval is from -0.440 sec. to 40.492 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] : 17.7787 ( )
R^2/D10^2 : 0.267942 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 356.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.64e-45 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.968e-07 3.663e-08
25- 50 3.192e-06 1.181e-07
50-150 7.301e-06 2.865e-07
15-150 1.119e-05 3.131e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-5.13919 -200)
Norm : 17.8193 (-0.436551 0.436551)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.07e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.817e-06 4.727e-08
25- 50 3.495e-06 1.001e-07
50-150 7.665e-06 2.087e-07
15-150 1.298e-05 3.766e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.90276 (-0.819878 0.855546)
R1^2/D10^2 : 1.85439 (-0.450492 0.65699)
kT2 [keV] : 31.6199 (-3.13075 4.26325)
R2^2/D10^2 : 2.76827E-02 (-0.00996493 0.0129812)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.59e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.336e-06 1.140e-07
25- 50 3.514e-06 1.557e-07
50-150 8.358e-06 6.774e-07
15-150 1.321e-05 8.391e-07
Peak spectrum fit
Power-law model
Time interval is from -0.116 sec. to 0.884 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12868 ( -0.0853469 0.0846204 )
Norm@50keV : 0.145557 ( -0.00820133 0.00819495 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.02 using 59 bins.
Reduced chi-squared = 1.36877
# Null hypothesis probability of 3.37e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.461853 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50838e-06 ( -8.88323e-08 8.89697e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.116 sec. to 0.884 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59018E-02 ( -0.444355 0.404823 )
Epeak [keV] : 101.984 ( -14.5121 26.7233 )
Norm@50keV : 0.467106 ( -0.157759 0.264567 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.84 using 59 bins.
Reduced chi-squared = 0.943571
# Null hypothesis probability of 5.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 16.6533 ( -0.9891 0.9906 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48255e-06 ( -9.28214e-08 9.25568e-08 ) ergs/cm2
Band function
Time interval is from -0.116 sec. to 0.884 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] : 19.9150 (-1.21943 1.32815)
R^2/D10^2 : 0.873998 (-0.170881 0.206484)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.05e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.693e-08 7.170e-09
25- 50 3.325e-07 2.770e-08
50-150 9.769e-07 8.265e-08
15-150 1.376e-06 9.250e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 70.5504 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 136.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.62e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.757e-07 1.015e-08
25- 50 3.379e-07 2.165e-08
50-150 7.412e-07 6.330e-08
15-150 1.255e-06 8.650e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.0475 (-2.96987 1.62937)
R1^2/D10^2 : 2.53202 (-0.952109 2.10218)
kT2 [keV] : 34.2154 (-8.4348 35.0543)
R2^2/D10^2 : 9.69231E-02 (-0.084098 0.191035)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.83e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.407e-08 2.911e-08
25- 50 3.517e-07 9.610e-08
50-150 1.037e-06 3.913e-07
15-150 1.482e-06 5.413e-07
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: 1.38010 ( -0.0720534 0.0717555 )
Norm@50keV : 2.87155E-02 ( -0.00127434 0.00127424 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.52e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 15.15 sec: 3.48156 ( -0.165747 0.166078 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.22111e-06 ( -1.95515e-07 1.9572e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.558510 ( -0.350095 0.325014 )
Epeak [keV] : 96.0969 ( -13.9808 27.8978 )
Norm@50keV : 6.97322E-02 ( -0.020201 0.030991 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.87e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 15.15 sec: 3.37769 ( -0.16966 0.17011 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.09658e-06 ( -2.06676e-07 2.05252e-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) = 3.27e-06
S(50-100 keV) = 4.75e-06
T90 vs. Hardness ratio plot
T90 = 37.9959999322891 sec.
Hardness ratio (energy fluence ratio) = 1.4526
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.72966
Count Ratio (50-100 keV) / (15-25 keV) = 1.47189
Mask shadow pattern
IMX = -9.975812143972496E-01, IMY = -4.519055188255474E-01
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:
-239.792000 -0.440000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.6922 -44.5400 4.4 52.9 -13.3 2.2768 2.6 5.8 4U 1735-44
350.5143 -41.3205 2.9 33.3 77.0 3.1110 3.9 ------ UNKNOWN
351.1754 -42.3889 3.0 32.2 77.5 2.7611 3.8 ------ UNKNOWN
46.1501 -75.6693 3.4 9.3 -128.0 1.1360 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.440000 14.708570
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.8756 -44.4067 5.7 53.0 -13.0 0.2917 2.0 6.2 4U 1735-44
51.4649 -29.6467 0.4 47.6 155.6 5.9688 25.9 ------ UNKNOWN
32.8150 -44.4948 3.0 29.7 137.7 0.3455 3.8 ------ UNKNOWN
228.6682 -54.3741 2.2 50.5 -45.2 1.2559 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
109.308590 195.908600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
63.0248 0.0539 2.7 31.7 -176.7 0.7432 4.2 ------ UNKNOWN
76.8838 -20.4760 2.7 24.7 -125.1 0.6870 4.2 ------ UNKNOWN
113.8347 -73.9307 2.5 54.1 -36.8 3.9588 4.7 ------ UNKNOWN
98.1675 -28.9834 2.2 40.5 -98.1 3.3151 5.3 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:23:54 EST 2026