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
225.6007 47.4526 0.0125 42.6614 177.4083 1.0924919 15.341 TRIG_01131397
Foreground time interval of the image:
-6.544 4.192 (delta_t = 10.736 [sec])
Background time interval of the image:
-239.896 -6.544 (delta_t = 233.352 [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 -6.544 sec. to 4.192 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.36473 ( -0.190677 0.204468 )
Norm@50keV : 5.52053E-03 ( -0.000791552 0.000777669 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.35 using 59 bins.
Reduced chi-squared = 1.18158
# Null hypothesis probability of 1.64e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.74 sec: 1.00087 ( -0.098182 0.09822 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.74029e-07 ( -6.56309e-08 6.68913e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.544 sec. to 4.192 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13679 ( -1.88387 0.86577 )
Epeak [keV] : 25.1245 ( -24.1824 7.44396 )
Norm@50keV : 3.28811E-02 ( -0.0335534 0.564364 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.82 using 59 bins.
Reduced chi-squared = 1.13964
# Null hypothesis probability of 2.21e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.74 sec: 0.963126 ( -0.105214 0.104544 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -6.544 sec. to 4.192 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] : 7.52437 (-0.730496 0.817785)
R^2/D10^2 : 1.41199 (-0.492905 0.7513)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.33e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.478e-07 2.443e-08
25- 50 2.319e-07 3.147e-08
50-150 4.955e-08 1.580e-08
15-150 4.292e-07 5.268e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 36.7468 (-7.89034 10.9632)
Norm : 6.86815 (-1.27848 1.63202)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.50e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.643e-07 2.100e-08
25- 50 2.081e-07 2.411e-08
50-150 1.463e-07 4.235e-08
15-150 5.187e-07 6.320e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.67117 (-0.902382 0.894599)
R1^2/D10^2 : 2.13144 (-0.824793 1.53534)
kT2 [keV] : 33.7826 (-16.4217 -33.7827)
R2^2/D10^2 : 1.88536E-03 (-0.00184572 0.0189574)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.36e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.586e-07 3.574e-08
25- 50 2.150e-07 4.822e-08
50-150 1.918e-07 1.026e-07
15-150 5.654e-07 1.574e-07
Peak spectrum fit
Power-law model
Time interval is from -0.108 sec. to 0.892 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.17302 ( -0.175524 0.186274 )
Norm@50keV : 2.10520E-02 ( -0.00289856 0.00285131 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.45 using 59 bins.
Reduced chi-squared = 1.21842
# Null hypothesis probability of 1.25e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.43690 ( -0.37017 0.37024 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.97247e-07 ( -2.41976e-08 2.45063e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.108 sec. to 0.892 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 7.11754E-02 ( -1.45728 1.08917 )
Epeak [keV] : 34.6668 ( -5.4818 5.32156 )
Norm@50keV : 0.412678 ( -0.420179 3.20779 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.95 using 59 bins.
Reduced chi-squared = 0.999107
# Null hypothesis probability of 4.77e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.34958 ( -0.36944 0.37055 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -0.108 sec. to 0.892 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] : 8.76768 (-0.905964 1.00317)
R^2/D10^2 : 2.85018 (-1.00236 1.54242)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.206e-08 7.300e-09
25- 50 8.577e-08 1.122e-08
50-150 3.019e-08 9.655e-09
15-150 1.580e-07 2.095e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 47.6738 (-10.4338 15.0088)
Norm : 20.6622 (-3.34485 4.17642)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.81e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.995e-08 7.155e-09
25- 50 7.050e-08 9.155e-09
50-150 6.539e-08 1.857e-08
15-150 1.858e-07 2.525e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.70870 (-2.05861 1.72687)
R1^2/D10^2 : 5.95949 (-2.51882 6.66588)
kT2 [keV] : 16.0308 (-8.32239 -19.5153)
R2^2/D10^2 : 0.107865 (-0.046446 0.689869)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.40e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.687e-08 2.688e-08
25- 50 7.596e-08 4.133e-08
50-150 5.075e-08 3.152e-08
15-150 1.736e-07 9.060e-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: 2.36473 ( -0.190677 0.204468 )
Norm@50keV : 5.52053E-03 ( -0.000791552 0.000777669 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.64e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.74 sec: 1.00075 ( -0.0981671 0.0982031 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.73897e-07 ( -6.55984e-08 6.69081e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14307 ( -1.88857 0.876308 )
Epeak [keV] : 25.0821 ( -23.3818 7.46552 )
Norm@50keV : 3.25683E-02 ( -0.0334431 0.564578 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.21e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.74 sec: 0.962795 ( -0.105119 0.104515 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.08854e-07 ( -7.85191e-08 8.81367e-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) = 1.87e-07
S(50-100 keV) = 1.45e-07
T90 vs. Hardness ratio plot
T90 = 8.84800004959106 sec.
Hardness ratio (energy fluence ratio) = 0.775401
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.13114
Count Ratio (50-100 keV) / (15-25 keV) = 0.350805
Mask shadow pattern
IMX = -9.205829732229645E-01, IMY = -4.167005463225783E-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:
-239.896000 -6.544000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
156.9907 42.6781 4.6 27.2 92.3 2.1664 2.6 ------ UNKNOWN
166.2179 28.7559 3.5 13.8 66.6 2.0178 3.3 ------ UNKNOWN
177.6817 -15.9416 2.1 39.9 -42.9 5.8973 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.544000 4.192000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
225.6007 47.4526 0.7 42.7 177.4 1.0926 15.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
108.604600 962.235100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3998 35.5384 0.0 24.5 -176.1 1.5570 0.7 12.1 Her X-1
256.1016 11.6805 2.8 44.0 -150.5 19.8647 4.1 ------ UNKNOWN
Plot creation:
Wed Jun 14 13:57:48 EDT 2023