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
51.9069 74.6644 0.0135 54.7650 -165.1547 3.7336445 14.199 TRIG_01351790
Foreground time interval of the image:
-9.920 4.776 (delta_t = 14.696 [sec])
6.336 20.080 (delta_t = 13.744 [sec])
Background time interval of the image:
-239.664 -9.920 (delta_t = 229.744 [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 16.384000
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 16.384000
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 16.384000
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
Multiple GTIs in the spectrum
tstart tstop
-9.920000 4.776000
6.336000 20.080000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45772 ( -0.178222 0.175197 )
Norm@50keV : 8.76432E-03 ( -0.000933616 0.000931001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.47 using 59 bins.
Reduced chi-squared = 1.20123
# Null hypothesis probability of 1.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 28.44 sec: 1.08219 ( -0.128949 0.13004 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38215e-06 ( -2.55631e-07 2.55817e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-9.920000 4.776000
6.336000 20.080000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.956537 ( -0.805562 0.580926 )
Epeak [keV] : 120.001 ( -42.4742 -120.001 )
Norm@50keV : 1.46923E-02 ( -0.00555805 0.0175994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.93 using 59 bins.
Reduced chi-squared = 1.19518
# Null hypothesis probability of 1.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 28.44 sec: 1.05550 ( -0.134028 0.13496 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35115e-06 ( -2.619e-07 2.60772e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-9.920000 4.776000
6.336000 20.080000
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] : 18.6242 (-2.19234 2.58386)
R^2/D10^2 : 5.91151E-02 (-0.0221719 0.0337868)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.26e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.154e-07 2.591e-08
25- 50 5.474e-07 9.598e-08
50-150 1.390e-06 2.388e-07
15-150 2.052e-06 2.945e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-46.6012 -200)
Norm : 4.56553 (-0.482405 0.482405)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.36e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.235e-07 4.656e-08
25- 50 6.222e-07 1.945e-07
50-150 1.365e-06 6.609e-07
15-150 2.310e-06 8.152e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.09984 (-1.88594 3.32336)
R1^2/D10^2 : 1.63419 (-1.27714 5.91084)
kT2 [keV] : 24.6649 (-4.3658 8.84509)
R2^2/D10^2 : 1.90751E-02 (-0.0130694 0.0119457)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.50e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.929e-07 1.511e-07
25- 50 5.684e-07 2.291e-07
50-150 1.494e-06 5.485e-07
15-150 2.355e-06 8.098e-07
Peak spectrum fit
Power-law model
Time interval is from 15.780 sec. to 16.780 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33219 ( -0.520906 0.474249 )
Norm@50keV : 1.74603E-02 ( -0.00517853 0.00511703 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.27 using 59 bins.
Reduced chi-squared = 0.846842
# Null hypothesis probability of 7.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.09596 ( -0.67135 0.68997 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.71246e-07 ( -5.01193e-08 5.02827e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 15.780 sec. to 16.780 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.381522 ( -3.76132 6.45796 )
Epeak [keV] : 92.6281 ( -40.8077 -92.615 )
Norm@50keV : 4.87095E-02 ( -0.0487222 2.38673 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.66 using 59 bins.
Reduced chi-squared = 0.851071
# Null hypothesis probability of 7.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.01768 ( -0.68851 0.70979 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.63976e-07 ( -5.53985e-08 5.32641e-08 ) ergs/cm2
Band function
Time interval is from 15.780 sec. to 16.780 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] : 17.2701 (-4.72812 8.32029)
R^2/D10^2 : 0.156899 (-0.15648 0.342642)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.488e-09 6.140e-09
25- 50 4.251e-08 2.431e-08
50-150 9.097e-08 5.865e-08
15-150 1.430e-07 8.800e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-109.364 -199.363)
Norm : 9.08328 (-2.63541 2.63567)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.78e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.262e-08 1.380e-08
25- 50 4.351e-08 2.644e-08
50-150 9.542e-08 5.750e-08
15-150 1.615e-07 9.715e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.8744 (-11.7859 9.86313)
R1^2/D10^2 : 0.357437 (-0.353583 -0.353583)
kT2 [keV] : 80.8899 (-87.1356 -87.1356)
R2^2/D10^2 : 9.10228E-04 (-0.000713836 0.306655)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.45772 ( -0.178222 0.175197 )
Norm@50keV : 8.76432E-03 ( -0.000933616 0.000931001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 28.44 sec: 1.08216 ( -0.128936 0.130032 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38186e-06 ( -2.55609e-07 2.55816e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.956538 ( -0.805563 0.580925 )
Epeak [keV] : 120.001 ( -42.4743 -120.001 )
Norm@50keV : 1.46923E-02 ( -0.00555805 0.0175994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 28.44 sec: 1.05540 ( -0.133987 0.13491 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35207e-06 ( -2.62015e-07 2.60931e-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) = 5.77e-07
S(50-100 keV) = 8.39e-07
T90 vs. Hardness ratio plot
T90 = 26.7680000066757 sec.
Hardness ratio (energy fluence ratio) = 1.45407
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50586
Count Ratio (50-100 keV) / (15-25 keV) = 1.53415
Mask shadow pattern
IMX = -1.368494646823022E+00, IMY = 3.627303073479849E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
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:
-239.664000 -9.920000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6177 22.0106 0.5 20.8 -81.2 9.3093 22.2 0.9 Crab
103.1884 65.9312 2.7 53.2 -142.2 7.4510 4.2 ------ UNKNOWN
105.3052 9.1428 3.0 43.8 -64.2 6.2265 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-9.920000 4.776000
6.336000 20.080000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7804 21.8968 8.4 21.0 -80.9 -0.1165 -1.4 10.8 Crab
37.1698 -13.2572 2.2 41.0 55.3 0.9364 5.2 ------ UNKNOWN
70.8934 -26.5184 1.9 47.6 6.3 0.8133 6.1 ------ UNKNOWN
71.0991 -22.6138 2.6 43.8 4.9 0.4845 4.4 ------ UNKNOWN
47.5486 41.6037 2.9 24.5 172.3 0.2699 4.0 ------ UNKNOWN
51.9058 74.6643 0.8 54.8 -165.2 3.7600 14.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
171.436600 962.474100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6044 22.0140 1.0 55.2 2.2 28.4671 11.0 1.6 Crab
74.8765 66.6254 3.0 10.9 -16.2 3.8935 3.9 ------ UNKNOWN
280.8524 86.4792 2.6 17.9 -150.1 3.9296 4.4 ------ UNKNOWN
106.7500 35.2805 2.2 47.1 -27.2 10.0640 5.2 ------ UNKNOWN
242.5901 48.0502 3.6 57.1 -149.9 21.6618 3.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:23:10 EST 2026