Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
87.8870 70.1093 0.0124 35.0397 -109.5671 1.2893336 15.477 TRIG_01037828
Foreground time interval of the image:
-7.000 1.836 (delta_t = 8.836 [sec])
Background time interval of the image:
-239.728 -7.000 (delta_t = 232.728 [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 2.048000
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 2.048000
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 2.048000
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 -7.000 sec. to 1.836 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.15708 ( -0.192862 0.204151 )
Norm@50keV : 8.06551E-03 ( -0.00112619 0.00110155 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.20 using 59 bins.
Reduced chi-squared = 1.12632
# Null hypothesis probability of 2.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 8.836 sec: 1.30598 ( -0.13084 0.13086 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.66416e-07 ( -8.08237e-08 8.26248e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -7.000 sec. to 1.836 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.15433 ( -0.772193 0.208426 )
Epeak [keV] : 9999.33 ( )
Norm@50keV : 8.08362E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.20 using 59 bins.
Reduced chi-squared = 1.14643
# Null hypothesis probability of 2.11e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 8.836 sec: 1.30554 ( -0.13059 0.13064 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.47673e-07 ( -1.12313e-07 9.52706e-08 ) ergs/cm2
Band function
Time interval is from -7.000 sec. to 1.836 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] : 8.18831 (-0.918191 1.03569)
R^2/D10^2 : 1.30037 (-0.494178 0.801996)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.89e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.417e-07 2.607e-08
25- 50 2.581e-07 4.025e-08
50-150 7.311e-08 2.510e-08
15-150 4.728e-07 6.088e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 47.6277 (-11.9845 18.9141)
Norm : 7.58396 (-1.32895 1.74251)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.619e-07 2.147e-08
25- 50 2.285e-07 2.801e-08
50-150 2.118e-07 6.344e-08
15-150 6.022e-07 8.341e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.09366 (-1.18152 1.07523)
R1^2/D10^2 : 2.14786 (-0.540083 2.03469)
kT2 [keV] : 70.1978 (-47.3924 -70.673)
R2^2/D10^2 : 5.86223E-04 (-0.000507728 0.00731604)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.576e-07 3.375e-08
25- 50 2.348e-07 4.953e-08
50-150 3.006e-07 1.557e-07
15-150 6.931e-07 1.992e-07
Peak spectrum fit
Power-law model
Time interval is from -6.992 sec. to -5.992 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97529 ( -0.400599 0.455379 )
Norm@50keV : 1.16335E-02 ( -0.00343291 0.00320998 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.81 using 59 bins.
Reduced chi-squared = 1.06684
# Null hypothesis probability of 3.40e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.72562 ( -0.36442 0.36441 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07177e-07 ( -2.85612e-08 2.97377e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.992 sec. to -5.992 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.04459 ( -0.417496 1.17542 )
Epeak [keV] : 22.2293 ( -2.06256 -9999.35 )
Norm@50keV : 1.03364E-02 ( -0.00355678 0.0381089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.69 using 59 bins.
Reduced chi-squared = 1.08375
# Null hypothesis probability of 3.11e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.70572 ( -0.58403 0.38548 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -6.992 sec. to -5.992 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] : 7.25620 (-1.83554 3.17742)
R^2/D10^2 : 2.66849 (-2.00577 6.02101)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.20e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.339e-08 1.222e-08
25- 50 3.431e-08 1.560e-08
50-150 6.465e-09 4.854e-09
15-150 6.417e-08 3.211e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 71.1877 (-38.0359 -71.2391)
Norm : 8.38881 (-2.50827 4.33938)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.156e-08 7.205e-09
25- 50 3.446e-08 1.365e-08
50-150 4.481e-08 3.425e-08
15-150 1.008e-07 5.016e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.37757 (-1.51384 2.01272)
R1^2/D10^2 : 7.56460 (-5.36617 10.7059)
kT2 [keV] : 30.0524 (-14.0196 -30.0555)
R2^2/D10^2 : 1.07734E-02 (-0.0105454 0.0820437)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.49e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.592e-08 1.508e-08
25- 50 2.838e-08 1.583e-08
50-150 6.093e-08 4.024e-08
15-150 1.152e-07 6.050e-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: 2.15708 ( -0.192862 0.204151 )
Norm@50keV : 8.06551E-03 ( -0.00112619 0.00110155 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 8.836 sec: 1.30586 ( -0.130826 0.130842 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.66292e-07 ( -8.07976e-08 8.26269e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97771 ( )
Epeak [keV] : 4.69671 ( )
Norm@50keV : 1.04187E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 8.836 sec: 1.29524 ( -0.13811 0.13656 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.46591e-07 ( -1.11143e-07 9.89906e-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) = 2.09e-07
S(50-100 keV) = 1.87e-07
T90 vs. Hardness ratio plot
T90 = 8.21200001239777 sec.
Hardness ratio (energy fluence ratio) = 0.894737
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.967507
Count Ratio (50-100 keV) / (15-25 keV) = 0.38883
Mask shadow pattern
IMX = -2.348523842962926E-01, IMY = 6.607430845806622E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.728000 -7.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
230.5111 28.9278 3.2 55.9 10.8 6.2029 3.6 ------ UNKNOWN
245.9069 39.4030 3.3 57.3 -8.9 4.5404 3.5 ------ UNKNOWN
249.8232 63.7972 2.4 43.9 -35.7 2.6950 4.7 ------ UNKNOWN
253.7292 77.1714 2.8 39.2 -54.8 2.2426 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-7.000000 1.836000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
132.7744 51.9367 2.5 16.3 -159.8 0.1816 4.5 ------ UNKNOWN
87.8870 70.1093 0.7 35.0 -109.6 1.2891 15.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Fri Nov 11 22:28:10 EST 2022