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
55.3401 -47.5932 0.0164 41.2340 -4.6187 0.9117218 11.708 TRIG_01107050
Foreground time interval of the image:
-8.360 7.576 (delta_t = 15.936 [sec])
Background time interval of the image:
-239.016 -8.360 (delta_t = 230.656 [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 -8.360 sec. to 7.576 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71667 ( -0.206253 0.212579 )
Norm@50keV : 3.91826E-03 ( -0.000520011 0.000512912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.68 using 59 bins.
Reduced chi-squared = 0.924211
# Null hypothesis probability of 6.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 15.94 sec: 0.523479 ( -0.065223 0.065315 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.77642e-07 ( -7.91725e-08 8.00287e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.360 sec. to 7.576 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09449 ( -1.02558 0.751972 )
Epeak [keV] : 68.2604 ( -25.1928 -68.2601 )
Norm@50keV : 8.43094E-03 ( -0.00483912 0.0209935 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.07 using 59 bins.
Reduced chi-squared = 0.911964
# Null hypothesis probability of 6.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 15.94 sec: 0.512401 ( -0.06721 0.067092 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.51999e-07 ( -8.63396e-08 8.72328e-08 ) ergs/cm2
Band function
Time interval is from -8.360 sec. to 7.576 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] : 12.6484 (-1.75492 2.06859)
R^2/D10^2 : 0.106760 (-0.0457882 0.0783081)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.63e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.774e-08 1.333e-08
25- 50 1.930e-07 3.582e-08
50-150 1.920e-07 5.032e-08
15-150 4.427e-07 7.508e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 127.781 (-48.2064 -124.677)
Norm : 2.19917 (-0.319638 0.424884)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.91e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.104e-08 1.665e-08
25- 50 1.646e-07 5.012e-08
50-150 3.028e-07 1.695e-07
15-150 5.584e-07 2.178e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.01396 (-3.25104 3.40343)
R1^2/D10^2 : 0.584394 (-0.398353 4.84576)
kT2 [keV] : 22.5752 (-7.82139 43.547)
R2^2/D10^2 : 8.99461E-03 (-0.00850116 0.0160421)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.713e-08 4.893e-08
25- 50 1.731e-07 9.221e-08
50-150 2.901e-07 1.663e-07
15-150 5.504e-07 2.911e-07
Peak spectrum fit
Power-law model
Time interval is from 0.068 sec. to 1.068 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49411 ( -0.232917 0.23645 )
Norm@50keV : 1.45653E-02 ( -0.00218456 0.00217854 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.31 using 59 bins.
Reduced chi-squared = 1.02298
# Null hypothesis probability of 4.27e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.81550 ( -0.27859 0.27928 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38325e-07 ( -2.20383e-08 2.21362e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.068 sec. to 1.068 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.731436 ( -1.13591 0.860646 )
Epeak [keV] : 87.8441 ( -26.3492 -87.8441 )
Norm@50keV : 3.44837E-02 ( -0.0210054 0.0847594 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.36 using 59 bins.
Reduced chi-squared = 1.00643
# Null hypothesis probability of 4.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.78256 ( -0.28218 0.28262 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.85869e-08 ( -3.02666e-08 2.16482e-08 ) ergs/cm2
Band function
Time interval is from 0.068 sec. to 1.068 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] : 16.0803 (-2.74487 3.2693)
R^2/D10^2 : 0.170131 (-0.0817373 0.15761)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.30e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.086e-09 2.658e-09
25- 50 3.840e-08 8.080e-09
50-150 6.953e-08 1.871e-08
15-150 1.170e-07 2.679e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-81.6224 -199.363)
Norm : 7.54834 (-1.11369 1.11543)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.63e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.880e-08 1.072e-08
25- 50 3.616e-08 2.040e-08
50-150 7.930e-08 4.419e-08
15-150 1.343e-07 7.655e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.16333 (-3.01077 4.87899)
R1^2/D10^2 : 1.53566 (-1.19795 9.28251)
kT2 [keV] : 23.9480 (-6.46001 32.7691)
R2^2/D10^2 : 3.27666E-02 (-0.0312022 0.0798103)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.43e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.630e-08 9.470e-09
25- 50 3.707e-08 1.960e-08
50-150 8.247e-08 4.702e-08
15-150 1.358e-07 7.150e-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: 1.71667 ( -0.206253 0.212579 )
Norm@50keV : 3.91826E-03 ( -0.000520011 0.000512912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 15.94 sec: 0.523456 ( -0.0652183 0.0653096 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.77554e-07 ( -7.91504e-08 8.00512e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09448 ( -1.02557 0.751974 )
Epeak [keV] : 68.2600 ( -25.1833 -68.26 )
Norm@50keV : 8.43106E-03 ( -0.00483914 0.0209934 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 15.94 sec: 0.512321 ( -0.067185 0.067074 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.52182e-07 ( -8.63852e-08 8.73034e-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) = 1.57e-07
S(50-100 keV) = 1.91e-07
T90 vs. Hardness ratio plot
T90 = 12.2879998683929 sec.
Hardness ratio (energy fluence ratio) = 1.21656
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.41965
Count Ratio (50-100 keV) / (15-25 keV) = 0.913693
Mask shadow pattern
IMX = 8.736353591956291E-01, IMY = 7.057797028375146E-02
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:
-239.016000 -8.360000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.360000 7.576000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
327.2203 -1.4556 2.1 50.3 145.3 1.3797 5.5 ------ UNKNOWN
55.3402 -47.5932 1.0 41.2 -4.6 0.9115 11.7 ------ UNKNOWN
11.6788 23.9619 2.4 46.4 -145.9 0.4924 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
109.084590 963.108800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
14.7304 -10.0755 2.9 50.7 -145.5 12.9729 4.1 ------ UNKNOWN
Plot creation:
Mon Oct 24 04:58:45 EDT 2022