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
233.3962 -18.0987 0.0073 22.0425 135.4348 1.6436622 26.412 TRIG_01308754
Foreground time interval of the image:
-0.068 15.893 (delta_t = 15.961 [sec])
Background time interval of the image:
-89.507 -0.068 (delta_t = 89.439 [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 -0.068 sec. to 234.016 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91956 ( -0.30016 0.322453 )
Norm@50keV : 4.01604E-04 ( -8.35425e-05 8.12833e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.26 using 59 bins.
Reduced chi-squared = 1.02211
# Null hypothesis probability of 4.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 234.1 sec: 5.81223E-02 ( -0.0102403 0.0102558 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.64733e-07 ( -1.72214e-07 1.76677e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.068 sec. to 234.016 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.477251 ( -1.95263 1.39599 )
Epeak [keV] : 46.3941 ( -17.1907 58.7698 )
Norm@50keV : 2.51528E-03 ( -0.002519 0.027424 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.14 using 59 bins.
Reduced chi-squared = 0.984643
# Null hypothesis probability of 5.08e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 234.1 sec: 5.50171E-02 ( -0.0106448 0.0106788 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.78184e-07 ( -1.68897e-07 1.89028e-07 ) ergs/cm2
Band function
Time interval is from -0.068 sec. to 234.016 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] : 11.4239 (-1.96376 2.37082)
R^2/D10^2 : 1.70095E-02 (-0.00874538 0.0177239)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.39e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.093e-07 3.661e-08
25- 50 3.241e-07 8.676e-08
50-150 2.458e-07 1.060e-07
15-150 6.792e-07 1.957e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 75.3157 (-29.4163 70.9313)
Norm : 0.281175 (-0.0646187 0.0867567)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.700e-07 4.538e-08
25- 50 2.758e-07 7.115e-08
50-150 3.735e-07 2.101e-07
15-150 8.193e-07 2.906e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.97662 (-3.84612 6.83494)
R1^2/D10^2 : 0.416623 (-0.396376 -0.406272)
kT2 [keV] : 13.6868 (-3.34041 25.6185)
R2^2/D10^2 : 7.56756E-03 (-0.0074611 0.0090655)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.85e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.564e-07 8.270e-08
25- 50 2.859e-07 1.556e-07
50-150 3.116e-07 1.938e-07
15-150 7.540e-07 4.009e-07
Peak spectrum fit
Power-law model
Time interval is from 0.308 sec. to 1.308 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32742 ( -0.161212 0.161027 )
Norm@50keV : 1.90791E-02 ( -0.00181046 0.00180903 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.70 using 59 bins.
Reduced chi-squared = 1.13509
# Null hypothesis probability of 2.26e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.28809 ( -0.22153 0.22197 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.87331e-07 ( -1.96476e-08 1.98071e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.308 sec. to 1.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.470378 ( -0.829721 0.373775 )
Epeak [keV] : 92.6809 ( -23.8656 152.739 )
Norm@50keV : 4.97886E-02 ( -0.0263687 0.0739297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.05 using 59 bins.
Reduced chi-squared = 1.07232
# Null hypothesis probability of 3.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.20022 ( -0.23304 0.2329 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76466e-07 ( -2.19263e-08 2.18876e-08 ) ergs/cm2
Band function
Time interval is from 0.308 sec. to 1.308 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] : 16.4754 (-1.83888 2.15032)
R^2/D10^2 : 0.197604 (-0.0677477 0.0992692)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.11e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.101e-08 1.987e-09
25- 50 4.750e-08 6.545e-09
50-150 9.110e-08 1.728e-08
15-150 1.496e-07 1.950e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-35.2792 -200)
Norm : 9.49702 (-0.900577 0.900577)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.47 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 2.365e-08 2.685e-09
25- 50 4.550e-08 1.324e-08
50-150 9.979e-08 5.394e-08
15-150 1.689e-07 8.573e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.85364 (-3.90008 1.84404)
R1^2/D10^2 : 0.680987 (-0.373316 1.92453)
kT2 [keV] : 30.0109 (-8.55654 68.7467)
R2^2/D10^2 : 1.77413E-02 (-0.0168515 0.0435939)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.590e-08 8.118e-09
25- 50 4.803e-08 2.316e-08
50-150 1.144e-07 5.836e-08
15-150 1.783e-07 8.312e-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: 1.57753 ( -0.112256 0.112913 )
Norm@50keV : 6.18217E-03 ( -0.000392161 0.000390468 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.82e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 15.96 sec: 0.789008 ( -0.0514709 0.0516157 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.25374e-07 ( -6.25618e-08 6.28797e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19138 ( -0.492013 0.426635 )
Epeak [keV] : 106.800 ( -34.3407 -106.8 )
Norm@50keV : 9.58546E-03 ( -0.00356133 0.00694554 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 15.96 sec: 0.771521 ( -0.055071 0.05518 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.99483e-07 ( -6.98713e-08 6.97532e-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) = 2.53e-07
S(50-100 keV) = 2.69e-07
T90 vs. Hardness ratio plot
T90 = 53.8359999656677 sec.
Hardness ratio (energy fluence ratio) = 1.06324
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.3042
Count Ratio (50-100 keV) / (15-25 keV) = 0.752392
Mask shadow pattern
IMX = -2.884642626841660E-01, IMY = -2.841189498997055E-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:
-89.507400 -0.068000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.0917 -60.5568 12.0 39.4 -53.9 -0.3108 -1.0 7.7 Cen X-3
186.8366 -62.9365 7.6 33.7 -63.9 0.3839 1.5 11.1 GX 301-2
244.9893 -15.6425 0.7 31.3 150.3 3.8748 16.3 0.6 Sco X-1
255.9366 -37.8598 1.7 30.9 -161.8 1.3524 6.8 2.5 4U 1700-377
256.3925 -36.4066 5.1 31.4 -164.5 0.4495 2.3 2.3 GX 349+2
262.9864 -24.7749 8.0 40.4 179.5 0.3743 1.4 2.1 GX 1+4
264.9385 -44.5025 4.2 37.1 -149.0 -0.6744 -2.7 8.9 4U 1735-44
270.1610 -25.1885 17.9 46.1 -175.9 -0.2397 -0.6 9.4 GX 5-1
270.2785 -25.7622 67.6 45.9 -175.1 0.0630 0.2 1.7 GRS 1758-258
274.0258 -14.0384 27.4 54.7 173.8 -0.2548 -0.4 1.2 GX 17+2
275.9229 -30.3639 82.3 48.7 -166.7 -0.0576 -0.1 0.2 H1820-303
285.0712 -24.7621 3.0 58.4 -168.8 -3.8635 -4.0 9.7 HT1900.1-2455
263.1587 -33.7847 3.7 37.4 -166.9 0.6720 3.1 9.0 GX 354-0
248.5424 -47.4090 2.3 26.2 -140.8 0.9121 5.0 ------ UNKNOWN
288.7144 -47.0691 2.3 53.2 -142.2 4.0970 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.068000 15.892600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3747 -60.6027 5.0 39.3 -54.0 0.2537 2.3 2.1 Cen X-3
186.4424 -62.6529 6.9 33.7 -63.3 0.1403 1.7 9.2 GX 301-2
244.8942 -15.6763 3.3 31.2 150.2 -0.2662 -3.5 5.4 Sco X-1
255.8131 -37.9006 3.7 30.8 -161.7 -0.2022 -3.1 8.9 4U 1700-377
256.5239 -36.2405 4.8 31.5 -164.8 -0.1588 -2.4 11.8 GX 349+2
263.0916 -24.5900 200.4 40.6 179.3 -0.0050 -0.1 10.4 GX 1+4
264.7270 -44.2964 17.8 37.0 -149.4 0.0518 0.7 9.2 4U 1735-44
270.2129 -25.0060 4.2 46.2 -176.1 0.2964 2.7 5.9 GX 5-1
270.2684 -25.7007 16.0 46.0 -175.2 -0.0767 -0.7 3.1 GRS 1758-258
273.8627 -14.0948 7.7 54.6 173.8 -0.3842 -1.5 9.0 GX 17+2
275.8954 -30.2530 14.9 48.7 -166.8 -0.0932 -0.8 7.0 H1820-303
285.1093 -24.9703 24.2 58.3 -168.6 -0.1508 -0.5 5.0 HT1900.1-2455
263.1909 -33.8743 9.0 37.4 -166.8 0.0915 1.3 10.3 GX 354-0
233.3962 -18.0987 0.4 22.0 135.4 1.6436 26.4 ------ UNKNOWN
269.3074 -11.9554 2.3 52.1 168.5 1.0442 5.1 ------ UNKNOWN
153.7388 -21.1033 1.9 57.0 -2.5 1.7866 6.0 ------ UNKNOWN
166.4544 -43.2015 2.5 39.8 -26.3 0.3714 4.6 ------ UNKNOWN
282.6341 -57.8329 2.2 48.0 -129.1 1.2327 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
137.092600 962.212000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.7464 -62.7924 6.0 54.9 14.5 -7.1782 -1.9 2.8 GX 301-2
244.9665 -15.6277 0.4 11.3 -110.3 30.3365 26.2 1.1 Sco X-1
254.5547 35.3837 4.6 57.1 -169.0 11.4638 2.5 5.4 Her X-1
256.0779 -37.8991 2.2 28.0 -49.8 7.8430 5.2 5.4 4U 1700-377
256.4652 -36.3206 6.1 27.3 -52.9 2.5884 1.9 6.3 GX 349+2
262.8433 -24.6200 0.0 28.1 -80.9 4.2682 2.7 11.8 GX 1+4
264.9296 -44.2782 0.0 37.2 -47.7 2.1426 1.1 13.1 4U 1735-44
268.4314 -1.4018 3.6 38.2 -121.4 -6.8177 -3.2 4.9 SW J1753.5-0127
270.4277 -25.0399 132.8 35.0 -81.4 -0.2159 -0.1 8.1 GX 5-1
270.1919 -25.8590 14.1 34.9 -80.0 1.9731 0.8 9.2 GRS 1758-258
273.9146 -13.9183 3.9 39.1 -99.5 11.8446 3.0 8.9 GX 17+2
275.9591 -30.4042 4.5 40.4 -73.5 11.2393 2.6 2.8 H1820-303
262.8145 -33.9505 4.8 30.6 -62.5 3.8058 2.4 11.1 GX 354-0
199.7414 -16.9159 3.1 32.1 77.4 9.5165 3.7 ------ UNKNOWN
217.4020 -65.3942 2.5 48.5 -0.6 9.8130 4.7 ------ UNKNOWN
238.0885 6.4514 3.2 25.0 -178.4 4.1785 3.7 ------ UNKNOWN
248.4692 -47.4274 2.5 31.8 -28.9 6.5705 4.7 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:41:53 EDT 2025