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
335.4004 7.0439 0.0081 21.0832 -0.8552 1.3754527 23.616 TRIG_01404904
Foreground time interval of the image:
-8.096 15.949 (delta_t = 24.045 [sec])
Background time interval of the image:
-194.651 -8.096 (delta_t = 186.555 [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 -8.096 sec. to 125.488 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38761 ( -0.194715 0.192674 )
Norm@50keV : 9.47033E-04 ( -9.72844e-05 9.69726e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.44 using 59 bins.
Reduced chi-squared = 1.04281
# Null hypothesis probability of 3.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 133.6 sec: 0.115013 ( -0.012056 0.012083 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22585e-06 ( -1.41156e-07 1.42311e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.096 sec. to 125.488 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38524 ( -0.211711 0.179202 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 9.50391E-04 ( -9.78333e-05 9.63403e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.48 using 59 bins.
Reduced chi-squared = 1.06214
# Null hypothesis probability of 3.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 133.6 sec: 0.115002 ( -0.012068 0.012074 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23361e-06 ( -1.39583e-07 1.33891e-07 ) ergs/cm2
Band function
Time interval is from -8.096 sec. to 125.488 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] : 15.6800 (-3.04873 4.4926)
R^2/D10^2 : 1.06435E-02 (-0.00593887 0.0119287)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 108.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.79e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.260e-08 1.679e-08
25- 50 3.002e-07 5.184e-08
50-150 5.118e-07 1.070e-07
15-150 8.846e-07 1.353e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-43.1115 -200)
Norm : 0.472422 (-0.0484101 0.0484101)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.572e-07 6.498e-08
25- 50 3.024e-07 1.631e-07
50-150 6.631e-07 3.582e-07
15-150 1.123e-06 6.108e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.54959 (-1.35289 1.549)
R1^2/D10^2 : 0.111992 (-0.0547662 0.117232)
kT2 [keV] : 58.0352 (-21.6281 129.878)
R2^2/D10^2 : 1.84714E-04 (-0.000161119 0.000419056)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.36e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.553e-07 4.587e-08
25- 50 2.925e-07 9.139e-08
50-150 8.904e-07 4.518e-07
15-150 1.338e-06 5.021e-07
Peak spectrum fit
Power-law model
Time interval is from 6.420 sec. to 7.420 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20623 ( -0.198785 0.194974 )
Norm@50keV : 1.10198E-02 ( -0.00132486 0.00132482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.71 using 59 bins.
Reduced chi-squared = 1.01246
# Null hypothesis probability of 4.49e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.29465 ( -0.15932 0.15955 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11617e-07 ( -1.47446e-08 1.4845e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.420 sec. to 7.420 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.699519 ( -0.875317 0.599991 )
Epeak [keV] : 134.311 ( -56.5107 -134.311 )
Norm@50keV : 1.95867E-02 ( -0.00859104 0.0316877 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.34 using 59 bins.
Reduced chi-squared = 1.00607
# Null hypothesis probability of 4.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.27682 ( -0.16194 0.16185 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08328e-07 ( -1.59497e-08 1.57486e-08 ) ergs/cm2
Band function
Time interval is from 6.420 sec. to 7.420 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] : 17.7284 (-2.73056 3.39283)
R^2/D10^2 : 8.97345E-02 (-0.0396254 0.0678747)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.674e-09 1.457e-09
25- 50 2.594e-08 4.610e-09
50-150 5.894e-08 1.316e-08
15-150 9.056e-08 1.694e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-35.9736 -200)
Norm : 5.34859 (-0.655458 0.655458)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.26e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.332e-08 7.440e-09
25- 50 2.562e-08 1.430e-08
50-150 5.618e-08 3.131e-08
15-150 9.511e-08 5.225e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.57219 (-3.00863 3.6477)
R1^2/D10^2 : 0.451032 (-0.269014 0.528695)
kT2 [keV] : 37.0232 (-13.3352 148.282)
R2^2/D10^2 : 6.03948E-03 (-0.00590121 0.0223073)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.01e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.408e-09 5.275e-09
25- 50 2.684e-08 1.445e-08
50-150 7.393e-08 4.111e-08
15-150 1.102e-07 5.715e-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: 1.28851 ( -0.117251 0.11601 )
Norm@50keV : 3.79323E-03 ( -0.000250174 0.000250156 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 24.04 sec: 0.451599 ( -0.0309869 0.0310349 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.03668e-07 ( -6.55078e-08 6.58011e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23371 ( -0.443735 0.161121 )
Epeak [keV] : 736.271 ( -736.299 -736.299 )
Norm@50keV : 4.03418E-03 ( -0.000459014 0.00250166 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 24.04 sec: 0.450519 ( -0.031938 0.031692 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.0075e-07 ( -7.07473e-08 6.8151e-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) = 2.86e-07
S(50-100 keV) = 4.38e-07
T90 vs. Hardness ratio plot
T90 = 118 sec.
Hardness ratio (energy fluence ratio) = 1.53147
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.57119
Count Ratio (50-100 keV) / (15-25 keV) = 1.10137
Mask shadow pattern
IMX = 3.854884955338382E-01, IMY = 5.754277054750405E-03
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:
-194.651400 -8.096000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0495 38.2624 4.5 51.7 18.5 1.8690 2.5 6.8 Cyg X-2
36.4956 -29.9787 2.3 48.7 165.1 3.7759 5.0 ------ UNKNOWN
29.3082 -48.4664 3.6 52.0 -170.1 2.4263 3.2 ------ UNKNOWN
30.5484 -54.4225 2.8 56.3 -164.9 3.6422 4.1 ------ UNKNOWN
331.1285 -26.9318 2.7 25.5 -96.4 1.3322 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.096000 15.948600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
325.9349 38.3168 65.7 51.8 18.5 -0.0457 -0.2 11.2 Cyg X-2
324.2375 28.7032 2.1 44.6 9.7 0.6336 5.6 ------ UNKNOWN
25.4472 -36.2527 1.9 42.7 178.3 0.5673 6.0 ------ UNKNOWN
335.4004 7.0440 0.5 21.1 -0.9 1.3763 23.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
95.748600 962.903700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5756 35.2136 0.7 43.2 -37.8 35.5854 17.3 1.0 Cyg X-1
308.0597 40.9285 3.9 41.7 -24.9 5.7888 3.0 2.7 Cyg X-3
326.0495 38.2885 5.7 32.3 -7.3 2.4687 2.1 6.1 Cyg X-2
355.6587 -37.7789 2.1 48.7 165.1 16.4734 5.4 ------ UNKNOWN
337.5388 60.8778 3.2 53.8 7.8 10.5051 3.6 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:16:29 EST 2026