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
200.2620 29.9147 0.0164 26.0034 98.9112 1.7505566 11.704 TRIG_01420873
Foreground time interval of the image:
-4.064 64.637 (delta_t = 68.701 [sec])
Background time interval of the image:
-239.064 -4.064 (delta_t = 235.000 [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 -4.064 sec. to 878.936 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 9.82727 ( -9.82727 -9.82727 )
Norm@50keV : 5.97231E-09 ( -5.97231e-09 -5.97231e-09 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.77 using 59 bins.
Reduced chi-squared = 1.01351
# Null hypothesis probability of 4.47e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 883 sec: 1.44215E-03 ( -0.00144215 0.00501693 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.11516e-07 ( 883 3.48843e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.064 sec. to 878.936 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.99983 ( 10 10 )
Epeak [keV] : 150.712 ( -150.639 -150.639 )
Norm@50keV : 8.84950E-05 ( -8.91183e-05 0.000614909 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.99 using 59 bins.
Reduced chi-squared = 1.01768
# Null hypothesis probability of 4.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 883 sec: 1.48702E-03 ( -0.00148702 0.00358956 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.3263e-09 ( 0 0 ) ergs/cm2
Band function
Time interval is from -4.064 sec. to 878.936 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] : 1.63529 (-1.87037 -1.87037)
R^2/D10^2 : 40.5906 (-40.6343 -40.6343)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.468e-08 2.287e-08
25- 50 1.122e-09 7.104e-10
50-150 1.515e-14 8.675e-15
15-150 5.580e-08 2.383e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 2.45413 (-2.43647 -2.43647)
Norm : 15.7608 (-16.886 -16.886)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.52e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.114e-08 2.763e-08
25- 50 1.303e-09 7.466e-10
50-150 1.561e-13 6.494e-14
15-150 5.244e-08 1.883e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.66656 (-1.66443 2.43848)
R1^2/D10^2 : 33.6153 (-34.389 243028)
kT2 [keV] : 199.363 (-199.363 -199.363)
R2^2/D10^2 : 1.27785E-06 (-1.35137e-06 2.5178e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.947e-08 1.581e-08
25- 50 1.276e-08 8.477e-10
50-150 2.988e-07 4.918e-08
15-150 3.610e-07 4.587e-08
Peak spectrum fit
Power-law model
Time interval is from 8.936 sec. to 9.936 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30225 ( -0.883096 0.841966 )
Norm@50keV : 4.03863E-03 ( -0.00172645 0.00172208 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.60 using 59 bins.
Reduced chi-squared = 0.905263
# Null hypothesis probability of 6.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.482024 ( -0.212981 0.214335 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.98924e-08 ( -1.86203e-08 1.90191e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.936 sec. to 9.936 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.28744 ( -1.30159 0.842968 )
Epeak [keV] : 100.171 ( -9999.36 -9999.36 )
Norm@50keV : 1.10333E-03 ( -0.00110334 0.0483544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.38 using 59 bins.
Reduced chi-squared = 0.9175
# Null hypothesis probability of 6.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.485925 ( -0.217313 0.222128 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.00396e-08 ( -1.9795e-08 1.97368e-08 ) ergs/cm2
Band function
Time interval is from 8.936 sec. to 9.936 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] : 24.0149 (-24.1047 35.2204)
R^2/D10^2 : 1.15340E-02 (-0.0113525 0.387922)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.86e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.180e-09 8.210e-10
25- 50 6.555e-09 4.336e-09
50-150 2.816e-08 1.927e-08
15-150 3.590e-08 2.473e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 1.99732 (-0.865117 0.865134)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.60e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.973e-09 3.213e-09
25- 50 9.567e-09 6.625e-09
50-150 2.098e-08 1.362e-08
15-150 3.552e-08 2.367e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.08812 (-4.32213 10.5893)
R1^2/D10^2 : 0.910843 (-0.882998 379.39)
kT2 [keV] : 36.2905 (-34.7808 -36.5914)
R2^2/D10^2 : 2.86217E-03 (-0.00278134 0.0100693)
------------------------------------------------------------
#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 5.100e-09 3.394e-09
25- 50 8.160e-09 4.113e-09
50-150 2.951e-08 1.916e-08
15-150 4.277e-08 2.381e-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: 1.61164 ( -0.226917 0.232617 )
Norm@50keV : 1.57649E-03 ( -0.000216648 0.000213043 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.28e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 68.7 sec: 0.203323 ( -0.026166 0.0261967 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01148e-06 ( -1.48345e-07 1.50412e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61830 ( -0.233722 0.228797 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.57428E-03 ( -0.00127473 0.00266484 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 68.7 sec: 0.203384 ( -0.02622 0.026071 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00823e-06 ( -1.55818e-07 1.5338e-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) = 8.21e-09
S(50-100 keV) = 7.58e-08
T90 vs. Hardness ratio plot
T90 = 125 sec.
Hardness ratio (energy fluence ratio) = 9.23264
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.520551
Count Ratio (50-100 keV) / (15-25 keV) = 0.494712
Mask shadow pattern
IMX = -7.556306271289044E-02, IMY = -4.819182467561735E-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:
-239.064000 -4.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9728 -15.6224 1.2 38.1 -104.7 8.0522 9.7 1.1 Sco X-1
254.5975 35.2724 6.9 46.0 174.8 1.1546 1.7 8.0 Her X-1
176.4810 -9.4915 2.4 41.4 14.1 2.3239 4.8 ------ UNKNOWN
258.1666 -4.8384 2.3 45.4 -127.7 5.7589 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.064000 64.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9586 -15.6633 10.9 38.1 -104.6 -0.2834 -1.1 1.8 Sco X-1
254.5165 35.2485 5.4 46.0 174.8 -0.4261 -2.1 6.3 Her X-1
200.2620 29.9147 1.0 26.0 98.9 1.7504 11.7 ------ UNKNOWN
205.3427 -5.0576 2.6 15.5 -16.3 0.4287 4.5 ------ UNKNOWN
256.9669 21.8316 2.1 43.4 -166.2 0.8595 5.5 ------ UNKNOWN
255.5288 17.9966 1.9 41.3 -160.9 0.9029 6.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
128.036590 870.036600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4180 35.1911 9.2 45.4 -151.1 -2.1675 -1.3 9.3 Her X-1
201.0640 42.3096 3.0 12.4 143.2 3.3533 3.8 ------ UNKNOWN
256.4309 56.5710 4.2 47.0 179.1 5.7789 2.8 ------ UNKNOWN
236.4674 6.2811 2.3 41.5 -102.2 19.7793 4.9 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:11:30 EST 2026