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
24.1628 -81.4020 0.0105 35.2073 2.9833 4.2250354 18.359 TRIG_01339848
Foreground time interval of the image:
-65.032 43.664 (delta_t = 108.696 [sec])
Background time interval of the image:
-158.459 -65.032 (delta_t = 93.427 [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 -65.032 sec. to 43.664 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59736 ( -0.108716 0.109539 )
Norm@50keV : 2.34590E-03 ( -0.000158238 0.000157724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.67 using 59 bins.
Reduced chi-squared = 1.08193
# Null hypothesis probability of 3.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 108.7 sec: 0.301222 ( -0.020261 0.020291 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38589e-06 ( -1.70808e-07 1.71811e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -65.032 sec. to 43.664 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.557442 ( -0.590911 0.518242 )
Epeak [keV] : 67.0693 ( -9.6924 21.1027 )
Norm@50keV : 8.08405E-03 ( -0.00366434 0.00805246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.54 using 59 bins.
Reduced chi-squared = 0.866786
# Null hypothesis probability of 7.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 108.7 sec: 0.288560 ( -0.021208 0.021214 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.2139e-06 ( -1.87856e-07 1.90346e-07 ) ergs/cm2
Band function
Time interval is from -65.032 sec. to 43.664 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] : 13.8674 (-0.977325 1.06775)
R^2/D10^2 : 4.55534E-02 (-0.0108553 0.013963)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.67e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.013e-07 2.511e-08
25- 50 7.416e-07 6.055e-08
50-150 9.345e-07 1.271e-07
15-150 1.877e-06 1.527e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 158.696 (-39.4863 -159.057)
Norm : 1.25365 (-0.0933283 0.099583)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.95e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.482e-07 2.995e-08
25- 50 6.507e-07 8.066e-08
50-150 1.314e-06 4.911e-07
15-150 2.313e-06 5.805e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.75240 (-2.87325 2.46965)
R1^2/D10^2 : 0.148054 (-0.0691858 0.286169)
kT2 [keV] : 24.5902 (-7.06119 25.9168)
R2^2/D10^2 : 3.66041E-03 (-0.00331782 0.0122182)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.01e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.786e-07 7.636e-08
25- 50 7.180e-07 1.871e-07
50-150 1.234e-06 5.639e-07
15-150 2.231e-06 7.381e-07
Peak spectrum fit
Power-law model
Time interval is from 0.464 sec. to 1.464 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36306 ( -0.201908 0.200582 )
Norm@50keV : 1.39976E-02 ( -0.00185949 0.00185824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.07 using 59 bins.
Reduced chi-squared = 0.948596
# Null hypothesis probability of 5.86e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.69097 ( -0.23072 0.23131 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3633e-07 ( -1.93666e-08 1.94853e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.464 sec. to 1.464 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.391275 ( -1.36039 1.03583 )
Epeak [keV] : 70.2187 ( -12.2693 30.0901 )
Norm@50keV : 0.101864 ( -0.101864 0.33851 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.38 using 59 bins.
Reduced chi-squared = 0.7925
# Null hypothesis probability of 8.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.61224 ( -0.23736 0.23748 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25774e-07 ( -2.00119e-08 2.05616e-08 ) ergs/cm2
Band function
Time interval is from 0.464 sec. to 1.464 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] : 16.3550 (-2.04292 2.41996)
R^2/D10^2 : 0.159503 (-0.0619867 0.0956191)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.47e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.777e-09 2.189e-09
25- 50 3.762e-08 7.115e-09
50-150 7.092e-08 1.740e-08
15-150 1.173e-07 2.126e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-56.869 -200)
Norm : 7.11872 (-0.940998 0.940998)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.17e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.773e-08 1.011e-08
25- 50 3.410e-08 1.883e-08
50-150 7.479e-08 4.130e-08
15-150 1.266e-07 6.990e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.90889 (-6.80687 -6.80687)
R1^2/D10^2 : 0.763045 (-0.792565 -0.792565)
kT2 [keV] : 18.8389 (-4.76319 -18.8057)
R2^2/D10^2 : 8.60881E-02 (-0.0869243 0.119064)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.49e-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: 1.59736 ( -0.108716 0.109539 )
Norm@50keV : 2.34590E-03 ( -0.000158238 0.000157724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 108.7 sec: 0.301212 ( -0.0202593 0.0202895 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38555e-06 ( -1.70925e-07 1.71837e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.557439 ( -0.590911 0.518243 )
Epeak [keV] : 67.0693 ( -9.6924 21.1027 )
Norm@50keV : 8.08409E-03 ( -0.00366434 0.00805246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 108.7 sec: 0.288530 ( -0.021203 0.021207 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.21466e-06 ( -1.88073e-07 1.90464e-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) = 6.17e-07
S(50-100 keV) = 8.16e-07
T90 vs. Hardness ratio plot
T90 = 84.2719999551773 sec.
Hardness ratio (energy fluence ratio) = 1.32253
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50411
Count Ratio (50-100 keV) / (15-25 keV) = 1.04988
Mask shadow pattern
IMX = 7.046558898377212E-01, IMY = -3.672382330436688E-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:
-158.459400 -65.032000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
13.7728 -16.9912 2.9 37.1 132.5 1.4678 4.0 ------ UNKNOWN
88.1499 -82.7411 2.9 38.7 -9.8 0.8563 4.0 ------ UNKNOWN
62.7951 -1.6766 2.8 48.8 -151.6 1.4586 4.1 ------ UNKNOWN
67.5209 5.3515 2.9 57.1 -149.2 3.9316 3.9 ------ UNKNOWN
76.2343 -7.6999 2.6 49.3 -132.1 3.3257 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-65.032000 43.664000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
24.1626 -81.4020 0.6 35.2 3.0 4.2241 18.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
851.440590 962.069200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6246 22.0019 1.5 48.7 -142.5 3.7852 7.7 0.9 Crab
135.6770 -40.5083 4.6 53.3 -32.8 1.8542 2.5 7.3 Vela X-1
38.9231 -40.8783 3.1 32.1 77.6 1.3484 3.8 ------ UNKNOWN
61.2859 -70.1343 1.9 45.0 30.1 2.1739 5.9 ------ UNKNOWN
58.8241 -46.3670 3.1 23.7 49.6 0.8578 3.7 ------ UNKNOWN
63.6490 -2.4040 2.9 25.0 -178.5 0.7025 3.9 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:34:30 EST 2026