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
284.0095 32.3300 0.0138 39.2284 138.7756 2.7561984 13.882 TRIG_01330958
Foreground time interval of the image:
-0.176 49.216 (delta_t = 49.392 [sec])
Background time interval of the image:
-239.880 -0.176 (delta_t = 239.704 [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 8.192000
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 8.192000
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 8.192000
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 -0.176 sec. to 49.216 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48184 ( -0.173015 0.172968 )
Norm@50keV : 3.54482E-03 ( -0.000382014 0.000381397 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.45 using 59 bins.
Reduced chi-squared = 0.832456
# Null hypothesis probability of 8.12e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 49.39 sec: 0.440417 ( -0.048792 0.048925 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66617e-06 ( -1.91584e-07 1.92661e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.176 sec. to 49.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.452410 ( -0.925777 0.767635 )
Epeak [keV] : 75.4628 ( -16.2145 72.4004 )
Norm@50keV : 1.17027E-02 ( -0.00679979 0.0214525 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.95 using 59 bins.
Reduced chi-squared = 0.749107
# Null hypothesis probability of 9.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 49.39 sec: 0.424573 ( -0.050385 0.050435 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56549e-06 ( -2.05829e-07 2.08128e-07 ) ergs/cm2
Band function
Time interval is from -0.176 sec. to 49.216 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] : 15.3490 (-1.75595 2.02157)
R^2/D10^2 : 4.80626E-02 (-0.0172887 0.0261935)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.166e-07 2.494e-08
25- 50 4.732e-07 7.171e-08
50-150 7.663e-07 1.558e-07
15-150 1.356e-06 1.835e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-66.1165 -199.363)
Norm : 1.82812 (-0.193933 0.194263)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.248e-07 8.023e-08
25- 50 4.325e-07 1.776e-07
50-150 9.485e-07 5.200e-07
15-150 1.606e-06 7.595e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21850 (-2.50394 4.40797)
R1^2/D10^2 : 0.330512 (-0.234735 1.01552)
kT2 [keV] : 21.7283 (-4.79725 23.6316)
R2^2/D10^2 : 1.09747E-02 (-0.0102994 0.0192509)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.18e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.885e-07 1.072e-07
25- 50 4.547e-07 2.352e-07
50-150 9.193e-07 4.640e-07
15-150 1.563e-06 8.280e-07
Peak spectrum fit
Power-law model
Time interval is from 1.932 sec. to 2.932 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.893331 ( -0.413113 0.371975 )
Norm@50keV : 1.10745E-02 ( -0.00291602 0.00284002 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.00 using 59 bins.
Reduced chi-squared = 0.894737
# Null hypothesis probability of 6.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.27098 ( -0.326776 0.33245 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24624e-07 ( -3.00983e-08 3.01186e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.932 sec. to 2.932 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.01213 ( -4.20169 1.97252 )
Epeak [keV] : 95.2528 ( -28.4737 -95.2404 )
Norm@50keV : 6.90695E-02 ( -0.0691101 2.53116 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.39 using 59 bins.
Reduced chi-squared = 0.864107
# Null hypothesis probability of 7.55e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.19899 ( -0.341417 0.34217 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17986e-07 ( -3.47406e-08 3.29004e-08 ) ergs/cm2
Band function
Time interval is from 1.932 sec. to 2.932 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] : 22.8232 (-5.29944 8.34671)
R^2/D10^2 : 4.43829E-02 (-0.027941 0.0606078)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.205e-09 2.148e-09
25- 50 2.272e-08 1.072e-08
50-150 8.841e-08 4.115e-08
15-150 1.153e-07 5.968e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-60.822 -200)
Norm : 5.38001 (-1.39689 1.39689)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.10e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.341e-08 8.325e-09
25- 50 2.580e-08 1.540e-08
50-150 5.658e-08 3.358e-08
15-150 9.578e-08 5.735e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 19.0009 (-18.3106 10.6923)
R1^2/D10^2 : 6.70899E-02 (-0.0672563 0.183841)
kT2 [keV] : 199.363 (-199.363 -199.363)
R2^2/D10^2 : 1.09211E-04 (-0.000109354 0.088183)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.53e-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: 1.48184 ( -0.173015 0.172968 )
Norm@50keV : 3.54482E-03 ( -0.000382014 0.000381397 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.12e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 49.39 sec: 0.440407 ( -0.0487898 0.0489213 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66593e-06 ( -1.91544e-07 1.92718e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.452404 ( -0.925776 0.767636 )
Epeak [keV] : 75.4625 ( -16.2145 72.4008 )
Norm@50keV : 1.17028E-02 ( -0.00679979 0.0214525 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 49.39 sec: 0.424536 ( -0.050373 0.050424 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56606e-06 ( -2.05927e-07 2.08169e-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) = 4.08e-07
S(50-100 keV) = 5.83e-07
T90 vs. Hardness ratio plot
T90 = 39.4959999322891 sec.
Hardness ratio (energy fluence ratio) = 1.42892
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.6226
Count Ratio (50-100 keV) / (15-25 keV) = 1.3626
Mask shadow pattern
IMX = -6.140466471637072E-01, IMY = -5.380198872534634E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.880000 -0.176000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5655 35.1873 0.6 27.5 127.3 8.9382 18.1 1.5 Cyg X-1
308.0058 40.8973 3.5 18.8 128.2 1.1937 3.3 5.8 Cyg X-3
326.4300 38.3791 370.5 11.8 77.8 0.0107 0.0 12.6 Cyg X-2
285.7788 23.0735 2.7 44.6 127.2 7.2993 4.4 ------ UNKNOWN
342.2208 33.1497 3.2 18.0 27.4 1.1709 3.6 ------ UNKNOWN
294.1643 65.3832 2.7 25.2 -160.5 1.6046 4.3 ------ UNKNOWN
240.5553 60.6787 2.5 49.1 -164.1 4.1685 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.176000 49.216000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5678 35.1370 11.0 27.6 127.3 0.1219 1.1 4.0 Cyg X-1
308.1626 40.9398 6.9 18.7 128.1 0.1651 1.7 2.5 Cyg X-3
325.9137 38.2636 0.0 12.0 79.5 0.1791 1.9 12.6 Cyg X-2
284.0095 32.3300 0.8 39.2 138.8 2.7561 13.9 ------ UNKNOWN
359.4403 50.5800 2.4 17.6 -47.8 0.4251 4.8 ------ UNKNOWN
38.2875 27.5440 1.7 54.4 -35.8 3.0026 6.8 ------ UNKNOWN
203.1175 74.4195 2.2 51.5 -139.2 2.0685 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
129.820610 508.320600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4244 35.3651 3.8 24.7 -162.1 1.5977 3.0 2.1 Her X-1
268.3406 -1.5642 134.4 37.0 119.3 -0.1205 -0.1 6.9 SW J1753.5-0127
288.9407 11.0988 0.0 21.7 79.4 0.8826 1.3 12.4 GRS 1915+105
299.5835 35.1896 0.5 13.3 -14.3 13.2574 24.5 0.8 Cyg X-1
308.1146 40.9929 2.2 21.1 -28.6 2.7980 5.3 2.4 Cyg X-3
326.3338 38.3998 14.7 34.7 -19.7 0.5336 0.8 9.0 Cyg X-2
298.4748 65.6134 2.5 34.5 -76.9 4.6050 4.7 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:35:58 EST 2026