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
155.9621 -5.5065 0.0137 31.2872 -78.5515 0.9828992 14.114 TRIG_01002158
Foreground time interval of the image:
-3.868 10.992 (delta_t = 14.860 [sec])
Background time interval of the image:
-239.048 -3.868 (delta_t = 235.180 [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 -3.868 sec. to 10.992 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88060 ( -0.201474 0.212196 )
Norm@50keV : 3.76237E-03 ( -0.000538809 0.000527974 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.27 using 59 bins.
Reduced chi-squared = 0.917018
# Null hypothesis probability of 6.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 14.86 sec: 0.535578 ( -0.063327 0.063341 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.14053e-07 ( -7.20163e-08 7.34748e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.868 sec. to 10.992 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.875125 ( -1.09706 0.879934 )
Epeak [keV] : 46.6420 ( -10.9493 40.2193 )
Norm@50keV : 1.44019E-02 ( -0.0144015 0.048909 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.38 using 59 bins.
Reduced chi-squared = 0.863929
# Null hypothesis probability of 7.56e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 14.86 sec: 0.520307 ( -0.064386 0.064556 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.68207e-07 ( -7.59521e-08 8.18003e-08 ) ergs/cm2
Band function
Time interval is from -3.868 sec. to 10.992 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] : 10.4783 (-1.41151 1.62878)
R^2/D10^2 : 0.216863 (-0.0910626 0.157003)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.10e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.309e-08 1.557e-08
25- 50 1.939e-07 2.757e-08
50-150 1.157e-07 3.348e-08
15-150 3.826e-07 6.174e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 77.7175 (-24.1785 44.3971)
Norm : 2.56981 (-0.41759 0.520944)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.68e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.889e-08 1.637e-08
25- 50 1.616e-07 2.020e-08
50-150 2.237e-07 1.124e-07
15-150 4.843e-07 1.055e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.02353 (-1.80461 2.27144)
R1^2/D10^2 : 1.08890 (-0.70305 2.77801)
kT2 [keV] : 17.8836 (-4.81884 12.8337)
R2^2/D10^2 : 1.96179E-02 (-0.0177571 0.0576607)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.75e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.715e-08 5.399e-08
25- 50 1.650e-07 8.611e-08
50-150 2.069e-07 1.233e-07
15-150 4.690e-07 2.431e-07
Peak spectrum fit
Power-law model
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48055 ( -0.294523 0.303568 )
Norm@50keV : 1.15405E-02 ( -0.00210845 0.00208531 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.81 using 59 bins.
Reduced chi-squared = 1.0493
# Null hypothesis probability of 3.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.43334 ( -0.25591 0.25621 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09853e-07 ( -2.1811e-08 2.20547e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.952932 ( -1.51932 0.794484 )
Epeak [keV] : 104.352 ( -45.7668 -104.348 )
Norm@50keV : 2.09376E-02 ( -0.0112409 0.0836721 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.23 using 59 bins.
Reduced chi-squared = 1.05768
# Null hypothesis probability of 3.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.40893 ( -0.26533 0.26268 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07387e-07 ( -2.25471e-08 2.27887e-08 ) ergs/cm2
Band function
Time interval is from -0.288 sec. to 0.712 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] : 16.7322 (-3.0857 3.86051)
R^2/D10^2 : 0.116261 (-0.0599143 0.118311)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.33e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.657e-09 2.599e-09
25- 50 2.908e-08 8.230e-09
50-150 5.783e-08 2.230e-08
15-150 9.357e-08 2.768e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-94.3843 -199.363)
Norm : 5.90550 (-1.03651 1.03778)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.62 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 1.470e-08 8.535e-09
25- 50 2.829e-08 1.640e-08
50-150 6.204e-08 3.602e-08
15-150 1.050e-07 5.965e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.55810 (-1.41364 2.45587)
R1^2/D10^2 : 20.5837 (-19.1953 423.445)
kT2 [keV] : 19.9539 (-4.06556 6.08935)
R2^2/D10^2 : 5.77907E-02 (-0.0353901 0.0635581)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.42e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.475e-08 7.904e-09
25- 50 2.471e-08 1.180e-08
50-150 6.517e-08 3.763e-08
15-150 1.046e-07 5.205e-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: 1.88060 ( -0.201474 0.212196 )
Norm@50keV : 3.76237E-03 ( -0.000538809 0.000527974 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 14.86 sec: 0.535545 ( -0.0633225 0.0633366 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.13972e-07 ( -7.19841e-08 7.3495e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.875146 ( -1.09707 0.879927 )
Epeak [keV] : 46.6422 ( -10.9492 40.2186 )
Norm@50keV : 1.44014E-02 ( -0.0144014 0.0489091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.56e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 14.86 sec: 0.520220 ( -0.064367 0.064535 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.683e-07 ( -7.60371e-08 8.18429e-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) = 1.49e-07
S(50-100 keV) = 1.62e-07
T90 vs. Hardness ratio plot
T90 = 11.7360000610352 sec.
Hardness ratio (energy fluence ratio) = 1.08725
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.948848
Count Ratio (50-100 keV) / (15-25 keV) = 0.606112
Mask shadow pattern
IMX = 1.206214079209319E-01, IMY = 5.956128925511488E-01
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:
-239.048000 -3.868000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5223 -40.5302 1.9 44.7 -15.3 2.5525 6.3 1.5 Vela X-1
102.5523 -4.8577 3.0 24.7 65.9 1.2455 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.868000 10.992000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4384 -40.7055 4.8 44.9 -15.1 0.1949 2.4 9.9 Vela X-1
155.9621 -5.5065 0.8 31.3 -78.6 0.9830 14.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.652590 963.102200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5255 -40.5760 2.4 39.5 12.9 4.2714 4.8 1.3 Vela X-1
170.5855 -60.5015 11.3 56.1 -20.3 -1.9397 -1.0 10.8 Cen X-3
132.9024 -26.3646 2.2 30.3 32.4 4.3082 5.3 ------ UNKNOWN
142.5132 -19.5923 3.1 19.2 30.0 1.9739 3.7 ------ UNKNOWN
168.9153 -43.6658 2.8 39.8 -26.4 3.1545 4.1 ------ UNKNOWN
196.5978 -12.9627 3.3 40.8 -88.2 10.7412 3.5 ------ UNKNOWN
199.2663 15.9631 3.2 48.0 -129.0 8.6133 3.6 ------ UNKNOWN
197.3998 -6.2002 3.9 41.2 -98.6 6.8873 3.0 ------ UNKNOWN
197.4680 -6.6439 4.6 41.3 -97.9 6.1965 2.7 ------ UNKNOWN
Plot creation:
Sun Nov 13 12:56:24 EST 2022