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
16.1003 -12.1630 0.0039 35.4143 -171.1766 4.1439243 49.265 TRIG_01287821
Foreground time interval of the image:
-6.724 11.533 (delta_t = 18.257 [sec])
Background time interval of the image:
-239.368 -6.724 (delta_t = 232.644 [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 -6.724 sec. to 63.300 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24590 ( -0.0704296 0.0699465 )
Norm@50keV : 5.18801E-03 ( -0.000193623 0.000193268 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.36 using 59 bins.
Reduced chi-squared = 1.14667
# Null hypothesis probability of 2.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 70.02 sec: 0.613199 ( -0.024832 0.024983 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.63992e-06 ( -1.41499e-07 1.4165e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.724 sec. to 63.300 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24154 ( -0.12908 0.116867 )
Epeak [keV] : 9999.06 ( -9999.08 -9999.08 )
Norm@50keV : 5.21118E-03 ( -0.000191934 0.000750022 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.43 using 59 bins.
Reduced chi-squared = 1.16839
# Null hypothesis probability of 1.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 70.02 sec: 0.613041 ( -0.013297 0.024941 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64991e-06 ( -1.52457e-07 1.30613e-07 ) ergs/cm2
Band function
Time interval is from -6.724 sec. to 63.300 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] : 20.9543 ( )
R^2/D10^2 : 2.32140E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 243.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.52e-25 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.350e-07 1.054e-08
25- 50 6.928e-07 4.226e-08
50-150 2.267e-06 1.313e-07
15-150 3.095e-06 1.404e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 ( )
Norm : 2.61151 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 136.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.77e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.553e-07 1.856e-08
25- 50 8.759e-07 3.851e-08
50-150 1.921e-06 7.807e-08
15-150 3.252e-06 1.393e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.37950 (-0.832455 0.992015)
R1^2/D10^2 : 0.802088 (-0.333422 0.592966)
kT2 [keV] : 30.9558 (-2.96752 3.97205)
R2^2/D10^2 : 5.81512E-03 (-0.00186576 0.00228336)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.61e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.898e-07 5.665e-08
25- 50 7.489e-07 6.379e-08
50-150 2.543e-06 2.115e-07
15-150 3.682e-06 2.850e-07
Peak spectrum fit
Power-law model
Time interval is from 6.928 sec. to 7.928 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18194 ( -0.141947 0.139735 )
Norm@50keV : 2.30722E-02 ( -0.00199454 0.00199365 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.83 using 59 bins.
Reduced chi-squared = 1.08474
# Null hypothesis probability of 3.08e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.70154 ( -0.24224 0.24275 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35315e-07 ( -2.17304e-08 2.18371e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.928 sec. to 7.928 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.211964 ( -0.807836 0.672645 )
Epeak [keV] : 100.404 ( -23.4447 100.376 )
Norm@50keV : 6.58383E-02 ( -0.0334982 0.0868745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.41 using 59 bins.
Reduced chi-squared = 0.989464
# Null hypothesis probability of 4.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.61571 ( -0.25182 0.25086 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.24554e-07 ( -2.38158e-08 2.3605e-08 ) ergs/cm2
Band function
Time interval is from 6.928 sec. to 7.928 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] : 18.5200 (-1.74108 2.00633)
R^2/D10^2 : 0.167848 (-0.0495264 0.0668514)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.20e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.142e-08 1.912e-09
25- 50 5.393e-08 7.315e-09
50-150 1.352e-07 2.055e-08
15-150 2.005e-07 1.965e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-19.0267 -200)
Norm : 11.3044 (-0.996607 0.996607)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.48e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.816e-08 3.215e-09
25- 50 5.416e-08 1.307e-08
50-150 1.188e-07 5.291e-08
15-150 2.011e-07 5.765e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 14.7293 (-4.48368 2.31909)
R1^2/D10^2 : 0.304689 (-0.124713 0.360723)
kT2 [keV] : 200.000 (-173.203 -200)
R2^2/D10^2 : 2.65105E-04 (-0.000118784 8.46849e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.38e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.446e-08 4.096e-09
25- 50 5.709e-08 1.934e-08
50-150 1.517e-07 6.913e-08
15-150 2.233e-07 8.187e-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: 1.17748 ( -0.0572356 0.0568569 )
Norm@50keV : 1.51598E-02 ( -0.000476267 0.000475087 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.26 sec: 1.77402 ( -0.059814 0.060027 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.82661e-06 ( -9.09105e-08 9.10329e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08676 ( -0.237338 0.0796068 )
Epeak [keV] : 559.721 ( -738.982 -976.623 )
Norm@50keV : 1.65750E-02 ( -0.0021177 0.00386637 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.26 sec: 1.77395 ( -0.07091 0.03015 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.82124e-06 ( -9.37834e-08 9.48972e-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) = 7.84e-07
S(50-100 keV) = 1.32e-06
T90 vs. Hardness ratio plot
T90 = 41.2119998931885 sec.
Hardness ratio (energy fluence ratio) = 1.68367
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38526
Count Ratio (50-100 keV) / (15-25 keV) = 1.44234
Mask shadow pattern
IMX = -7.026230838911420E-01, IMY = 1.090655754059929E-01
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:
-239.368000 -6.724000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5609 35.2228 2.1 56.0 -26.6 8.5318 5.6 1.9 Cyg X-1
308.1134 40.9491 20.3 49.5 -19.0 0.4194 0.6 0.3 Cyg X-3
326.1068 38.2418 5.5 35.5 -17.8 0.9257 2.1 5.7 Cyg X-2
46.6431 19.4289 3.0 42.3 116.9 7.2258 3.9 ------ UNKNOWN
302.8978 47.9533 2.5 54.3 -10.9 4.1086 4.6 ------ UNKNOWN
348.3971 -12.1864 2.6 34.9 -123.2 2.3875 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.724000 11.532610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6526 35.2904 6.0 55.9 -26.5 -0.6228 -1.9 6.1 Cyg X-1
308.0891 40.9930 6.2 49.6 -18.9 0.2992 1.9 2.6 Cyg X-3
326.3053 38.3494 5.2 35.4 -17.5 -0.1945 -2.2 6.5 Cyg X-2
33.0361 57.7292 2.8 44.0 57.6 1.2802 4.1 ------ UNKNOWN
39.1593 32.9429 2.1 35.7 95.2 0.9366 5.6 ------ UNKNOWN
16.1003 -12.1630 0.2 35.4 -171.2 4.1437 49.3 ------ UNKNOWN
12.8693 -12.8790 2.1 34.9 -165.6 0.4310 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
93.932600 846.532600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
17.5755 24.9219 2.6 37.1 12.6 6.0173 4.4 ------ UNKNOWN
341.2695 -8.4135 2.4 34.5 -76.8 8.2315 4.8 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:52:04 EDT 2025