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
55.1416 -22.4575 0.0160 23.9150 -156.5530 1.2736484 12.013 TRIG_01319125
Foreground time interval of the image:
-29.736 24.709 (delta_t = 54.445 [sec])
Background time interval of the image:
-105.891 -29.736 (delta_t = 76.155 [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 -29.736 sec. to 57.960 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33320 ( -0.218819 0.216466 )
Norm@50keV : 1.01790E-03 ( -0.000122352 0.000121976 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.68 using 59 bins.
Reduced chi-squared = 1.11719
# Null hypothesis probability of 2.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 87.7 sec: 0.122213 ( -0.015064 0.015104 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.75326e-07 ( -1.16888e-07 1.17927e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -29.736 sec. to 57.960 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31463 ( -0.651048 1.18391 )
Epeak [keV] : 9988.33 ( -9999.33 -9999.33 )
Norm@50keV : 1.03968E-03 ( -0.000789643 0.00101924 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.76 using 59 bins.
Reduced chi-squared = 1.13857
# Null hypothesis probability of 2.22e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 87.7 sec: 0.122654 ( -0.016859 0.015808 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.7878e-07 ( -1.31919e-07 1.23962e-07 ) ergs/cm2
Band function
Time interval is from -29.736 sec. to 57.960 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] : 17.8476 (-2.82206 3.55567)
R^2/D10^2 : 7.73238E-03 (-0.00352241 0.00616478)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 84.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.02e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.337e-08 1.102e-08
25- 50 1.993e-07 3.661e-08
50-150 4.597e-07 1.097e-07
15-150 7.024e-07 1.385e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-47.9393 -200)
Norm : 0.505539 (-0.0609556 0.0609556)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.104e-07 6.117e-08
25- 50 2.125e-07 1.169e-07
50-150 4.659e-07 2.554e-07
15-150 7.888e-07 4.328e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.57411 (-1.67759 2.81175)
R1^2/D10^2 : 0.275979 (-0.211098 0.810255)
kT2 [keV] : 27.3438 (-6.52773 16.0562)
R2^2/D10^2 : 1.64989E-03 (-0.00125397 0.0020637)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.071e-07 5.767e-08
25- 50 1.814e-07 6.819e-08
50-150 5.820e-07 3.028e-07
15-150 8.705e-07 3.561e-07
Peak spectrum fit
Power-law model
Time interval is from -0.276 sec. to 0.724 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24770 ( -0.328865 0.317371 )
Norm@50keV : 6.93682E-03 ( -0.0012536 0.00125305 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.19 using 59 bins.
Reduced chi-squared = 0.617368
# Null hypothesis probability of 9.90e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.820141 ( -0.152787 0.153324 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.94736e-08 ( -1.38678e-08 1.4029e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.276 sec. to 0.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24373 ( -1.12922 2.16246 )
Epeak [keV] : 9998.63 ( -9998.71 -9998.71 )
Norm@50keV : 6.96834E-03 ( -0.00125939 0.0180178 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.19 using 59 bins.
Reduced chi-squared = 0.628393
# Null hypothesis probability of 9.87e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.820788 ( -0.153732 0.152371 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.95617e-08 ( -1.48135e-08 1.42684e-08 ) ergs/cm2
Band function
Time interval is from -0.276 sec. to 0.724 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] : 18.9054 (-4.73362 6.86409)
R^2/D10^2 : 4.36957E-02 (-0.0273587 0.0710364)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.90e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.075e-09 1.247e-09
25- 50 1.474e-08 5.862e-09
50-150 3.868e-08 1.464e-08
15-150 5.649e-08 1.935e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-69.9465 -200)
Norm : 3.39974 (-0.624318 0.624318)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.466e-09 4.965e-09
25- 50 1.628e-08 9.380e-09
50-150 3.572e-08 2.060e-08
15-150 6.047e-08 3.408e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.93195 (-2.73008 4.59235)
R1^2/D10^2 : 0.839044 (-0.675102 2.56383)
kT2 [keV] : 33.1519 (-11.9491 77.705)
R2^2/D10^2 : 6.16298E-03 (-0.00570955 0.0203389)
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.405e-09 4.581e-09
25- 50 1.499e-08 8.475e-09
50-150 4.867e-08 2.783e-08
15-150 7.107e-08 3.679e-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: 1.33725 ( -0.181807 0.180187 )
Norm@50keV : 1.55614E-03 ( -0.000158552 0.000158247 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 54.44 sec: 0.186986 ( -0.0195741 0.0196239 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.29802e-07 ( -9.35666e-08 9.42977e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33373 ( -0.657401 0.287949 )
Epeak [keV] : 9982.79 ( -9930.78 -9930.78 )
Norm@50keV : 1.56238E-03 ( -0.000553683 0.00202987 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 54.44 sec: 0.187083 ( -0.02084 0.019538 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.2721e-07 ( -1.00491e-07 9.65385e-08 ) 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) = 1.98e-07
S(50-100 keV) = 3.15e-07
T90 vs. Hardness ratio plot
T90 = 65.3279999494553 sec.
Hardness ratio (energy fluence ratio) = 1.59091
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.26211
Count Ratio (50-100 keV) / (15-25 keV) = 1.11707
Mask shadow pattern
IMX = -4.068355600406741E-01, IMY = 1.764502216963156E-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:
-105.891400 -29.736000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6231 -40.5395 4.7 45.4 39.1 0.8085 2.4 4.4 Vela X-1
23.4597 -16.1027 2.5 53.7 -167.9 1.7173 4.6 ------ UNKNOWN
87.3368 4.1879 2.3 35.1 -67.6 1.1250 4.9 ------ UNKNOWN
43.2840 3.9241 2.1 49.3 -132.3 3.5531 5.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-29.736000 24.708590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5098 -40.4850 8.2 45.3 39.0 -0.4650 -1.4 4.3 Vela X-1
19.9762 -53.8840 2.9 48.8 143.3 1.9187 4.0 ------ UNKNOWN
23.8667 -44.4953 2.8 46.1 156.0 1.1490 4.1 ------ UNKNOWN
110.0226 -33.2041 2.5 25.2 24.7 0.5563 4.7 ------ UNKNOWN
36.9482 -26.8641 2.4 38.1 -175.5 0.6518 4.8 ------ UNKNOWN
55.1417 -22.4575 1.0 23.9 -156.6 1.2734 12.0 ------ UNKNOWN
31.0194 -3.2964 2.5 53.9 -149.5 1.7376 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
89.908600 902.508000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
80.1797 -51.3067 2.8 34.7 46.0 19.8914 4.1 ------ UNKNOWN
58.6682 3.0048 3.0 25.7 -98.3 13.3093 3.9 ------ UNKNOWN
71.4918 8.0273 2.5 34.4 -76.9 22.6127 4.6 ------ UNKNOWN
88.0904 9.7685 3.6 45.6 -57.8 40.4263 3.3 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:37:44 EDT 2025