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
306.3131 48.4064 0.0160 38.1018 9.3071 2.1362971 12.031 TRIG_01342439
Foreground time interval of the image:
1.064 82.501 (delta_t = 81.437 [sec])
Background time interval of the image:
-239.000 1.064 (delta_t = 240.064 [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 1.064 sec. to 125.364 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90636 ( -0.208616 0.218888 )
Norm@50keV : 1.18855E-03 ( -0.000166036 0.000162207 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.99 using 59 bins.
Reduced chi-squared = 1.29807
# Null hypothesis probability of 6.46e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 124.3 sec: 0.171042 ( -0.020385 0.020401 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.35856e-06 ( -1.84175e-07 1.86839e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.064 sec. to 125.364 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54922 ( -1.10525 0.645515 )
Epeak [keV] : 54.6259 ( -44.6984 -54.6294 )
Norm@50keV : 1.89623E-03 ( -0.0010909 0.00624703 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.54 using 59 bins.
Reduced chi-squared = 1.31321
# Null hypothesis probability of 5.80e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 124.3 sec: 0.169005 ( -0.021121 0.021037 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.31335e-06 ( -2.16872e-07 2.14533e-07 ) ergs/cm2
Band function
Time interval is from 1.064 sec. to 125.364 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] : 10.4346 (-1.40372 1.63012)
R^2/D10^2 : 6.85947E-02 (-0.0292094 0.0505837)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 87.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.81e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.916e-07 3.915e-08
25- 50 5.052e-07 8.222e-08
50-150 2.978e-07 8.844e-08
15-150 9.946e-07 1.631e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 79.2705 (-25.4633 48.4273)
Norm : 0.806849 (-0.134506 0.175422)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.80e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.601e-07 4.319e-08
25- 50 4.272e-07 5.855e-08
50-150 5.993e-07 2.794e-07
15-150 1.287e-06 2.549e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.67755 (-2.83358 2.54503)
R1^2/D10^2 : 0.183148 (-0.105111 0.681543)
kT2 [keV] : 34.8661 (-19.9553 -34.8301)
R2^2/D10^2 : 5.05360E-04 (-0.000499053 0.0130254)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.09e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.535e-07 1.429e-07
25- 50 4.334e-07 1.792e-07
50-150 6.005e-07 3.407e-07
15-150 1.287e-06 5.840e-07
Peak spectrum fit
Power-law model
Time interval is from 10.216 sec. to 11.216 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52552 ( -0.455206 0.462471 )
Norm@50keV : 6.19998E-03 ( -0.00185487 0.0018405 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.50 using 59 bins.
Reduced chi-squared = 1.07895
# Null hypothesis probability of 3.18e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.779384 ( -0.232004 0.233206 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.85976e-08 ( -1.84e-08 1.87898e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 10.216 sec. to 11.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.429695 ( -5.49446 2.12258 )
Epeak [keV] : 56.3088 ( -18.5823 -56.0735 )
Norm@50keV : 7.16280E-02 ( -0.0741119 170.739 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.21 using 59 bins.
Reduced chi-squared = 1.05732
# Null hypothesis probability of 3.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.742180 ( -0.232402 0.23694 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.0754e-08 ( -1.93793e-08 2.11594e-08 ) ergs/cm2
Band function
Time interval is from 10.216 sec. to 11.216 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] : 12.9971 (-3.40707 5.24062)
R^2/D10^2 : 0.158359 (-0.113035 0.319307)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.674e-09 3.558e-09
25- 50 1.954e-08 1.141e-08
50-150 2.086e-08 1.405e-08
15-150 4.607e-08 2.780e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 175.763 (-114.15 -175.647)
Norm : 3.26807 (-0.96248 1.3042)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.44e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.264e-09 5.085e-09
25- 50 1.565e-08 9.385e-09
50-150 3.286e-08 1.989e-08
15-150 5.678e-08 3.344e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 30.6379 (-31.1058 -31.1058)
R1^2/D10^2 : 3.55144E-03 (-0.00306816 0.358616)
kT2 [keV] : 9.99339 (-10.0503 6.92102)
R2^2/D10^2 : 0.312307 (-0.307845 -0.307845)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.51e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.875e-09 4.619e-09
25- 50 1.883e-08 1.422e-08
50-150 2.877e-08 2.059e-08
15-150 5.448e-08 3.502e-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: 1.84313 ( -0.194253 0.201981 )
Norm@50keV : 1.67584E-03 ( -0.000212019 0.0002081 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 81.44 sec: 0.234902 ( -0.0265364 0.0265673 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25505e-06 ( -1.58012e-07 1.5992e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43982 ( -0.963261 0.664827 )
Epeak [keV] : 62.3016 ( -55.0384 -62.3091 )
Norm@50keV : 2.80133E-03 ( -0.00156413 0.00676293 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.20e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 81.44 sec: 0.231539 ( -0.027359 0.027363 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21289e-06 ( -1.80609e-07 1.80504e-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) = 3.98e-07
S(50-100 keV) = 4.24e-07
T90 vs. Hardness ratio plot
T90 = 110.108000040054 sec.
Hardness ratio (energy fluence ratio) = 1.06533
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.20009
Count Ratio (50-100 keV) / (15-25 keV) = 0.685819
Mask shadow pattern
IMX = 7.738283291555789E-01, IMY = -1.268182570105515E-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:
-239.000000 1.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9830 -15.6683 1.7 46.5 176.8 6.4630 7.0 1.7 Sco X-1
254.7038 35.4045 0.0 14.7 -77.8 0.1537 0.4 12.6 Her X-1
262.8732 -24.8436 3.9 50.5 151.7 4.5420 2.9 9.4 GX 1+4
268.3604 -1.4496 118.8 26.9 144.1 -0.0460 -0.1 0.5 SW J1753.5-0127
274.0475 -14.0370 4.4 40.1 136.3 2.8628 2.6 2.4 GX 17+2
288.8855 11.0511 3.7 25.0 87.8 1.7141 3.1 8.2 GRS 1915+105
299.6112 35.2009 0.5 29.4 29.5 12.6253 24.9 1.0 Cyg X-1
308.2024 40.9435 2.3 37.2 21.6 2.8533 4.9 4.2 Cyg X-3
326.3646 38.2955 0.0 50.9 26.8 1.2919 1.1 9.2 Cyg X-2
317.4197 40.5640 2.9 44.0 23.7 2.6263 4.0 ------ UNKNOWN
318.3027 58.5654 2.9 48.5 -0.6 2.8187 3.9 ------ UNKNOWN
217.6654 10.1567 2.0 49.3 -132.1 10.7295 5.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
1.064000 82.500590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0810 -15.6796 16.3 46.5 176.7 -0.1767 -0.7 6.3 Sco X-1
254.4515 35.3359 1455.0 14.8 -78.5 0.0010 0.0 0.5 Her X-1
263.2105 -24.7196 2.8 50.3 151.4 -2.0189 -4.0 11.1 GX 1+4
268.4220 -1.3165 4.8 26.8 144.0 0.3944 2.4 8.8 SW J1753.5-0127
274.0735 -14.1622 4.5 40.2 136.3 -0.6723 -2.5 8.5 GX 17+2
288.8487 11.0820 4.6 25.0 87.8 -0.4265 -2.5 8.7 GRS 1915+105
299.5599 34.9913 0.0 29.4 29.9 0.2190 1.4 12.7 Cyg X-1
308.0727 40.7722 7.3 37.0 21.9 0.3012 1.6 11.0 Cyg X-3
326.0838 38.4056 6.1 50.7 26.7 1.1602 1.9 6.5 Cyg X-2
306.3131 48.4064 1.0 38.1 9.3 2.1362 12.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
162.500600 963.072300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4093 35.5184 8.2 39.9 -159.7 2.4742 1.4 10.8 Her X-1
288.7936 10.8021 7.9 40.3 136.6 -4.5767 -1.5 8.6 GRS 1915+105
299.5985 35.1908 0.3 14.1 132.5 40.3210 35.8 0.8 Cyg X-1
308.0958 40.9421 2.0 7.5 99.2 6.2220 5.8 0.9 Cyg X-3
325.9997 38.1680 5.3 17.5 47.8 2.4284 2.2 12.3 Cyg X-2
4.3900 41.2177 2.6 40.8 7.0 7.5138 4.4 ------ UNKNOWN
310.5048 71.5879 3.1 23.3 -67.3 5.2527 3.7 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:31:31 EST 2026