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
47.3203 35.3228 0.0104 36.2151 -25.0657 5.3449000 18.484 TRIG_01033328
Foreground time interval of the image:
-13.476 166.725 (delta_t = 180.201 [sec])
Background time interval of the image:
-239.176 -13.476 (delta_t = 225.700 [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 -13.476 sec. to 246.584 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47483 ( -0.108997 0.10893 )
Norm@50keV : 1.71593E-03 ( -0.000111048 0.000110934 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.86 using 59 bins.
Reduced chi-squared = 0.962456
# Null hypothesis probability of 5.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 260.1 sec: 0.212803 ( -0.01424 0.014269 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.25245e-06 ( -2.95687e-07 2.97326e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -13.476 sec. to 246.584 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.815625 ( -0.507698 0.453595 )
Epeak [keV] : 91.5890 ( -20.3305 85.175 )
Norm@50keV : 3.64610E-03 ( -0.00144818 0.00276123 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.42 using 59 bins.
Reduced chi-squared = 0.864643
# Null hypothesis probability of 7.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 260.1 sec: 0.206685 ( -0.014865 0.014868 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.0695e-06 ( -3.2339e-07 3.23897e-07 ) ergs/cm2
Band function
Time interval is from -13.476 sec. to 246.584 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] : 15.5749 (-1.19076 1.31223)
R^2/D10^2 : 2.14869E-02 (-0.005383 0.00704665)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.04e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.819e-07 3.387e-08
25- 50 1.159e-06 1.009e-07
50-150 1.944e-06 2.215e-07
15-150 3.385e-06 2.601e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-35.8338 -200)
Norm : 0.876740 (-0.0562686 0.0562686)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.67e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.699e-07 4.214e-08
25- 50 1.096e-06 9.572e-08
50-150 2.404e-06 5.973e-07
15-150 4.070e-06 5.657e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.85495 (-1.88025 2.14146)
R1^2/D10^2 : 0.136171 (-0.0680157 0.186513)
kT2 [keV] : 25.5639 (-4.99106 10.6077)
R2^2/D10^2 : 2.85201E-03 (-0.00205141 0.00386542)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.41e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.729e-07 1.397e-07
25- 50 1.138e-06 3.223e-07
50-150 2.469e-06 1.106e-06
15-150 4.080e-06 1.237e-06
Peak spectrum fit
Power-law model
Time interval is from 0.092 sec. to 1.092 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13133 ( -0.378532 0.350513 )
Norm@50keV : 9.18302E-03 ( -0.00193783 0.00191446 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.94 using 59 bins.
Reduced chi-squared = 0.770877
# Null hypothesis probability of 8.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.06864 ( -0.23561 0.23714 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.50824e-08 ( -2.02861e-08 2.0332e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.092 sec. to 1.092 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.37968 ( -2.31095 4.98502 )
Epeak [keV] : 124.514 ( )
Norm@50keV : 1.21184E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.42 using 59 bins.
Reduced chi-squared = 0.775357
# Null hypothesis probability of 8.90e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.07026 ( -0.239977 0.23811 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.53059e-08 ( -2.14339e-08 1.96761e-08 ) ergs/cm2
Band function
Time interval is from 0.092 sec. to 1.092 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] : 23.3808 (-7.05667 10.5391)
R^2/D10^2 : 2.96137E-02 (-0.0201056 0.0659347)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.64e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.910e-09 1.282e-09
25- 50 1.594e-08 7.300e-09
50-150 6.502e-08 2.558e-08
15-150 8.387e-08 3.375e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-65.2059 -200)
Norm : 4.54848 (-0.962084 0.962084)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.88e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.133e-08 6.705e-09
25- 50 2.179e-08 1.306e-08
50-150 4.779e-08 2.760e-08
15-150 8.090e-08 4.674e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.59938 (-2.77372 4.16498)
R1^2/D10^2 : 0.570647 (-0.418479 1.55865)
kT2 [keV] : 47.7903 (-20.5534 -47.6795)
R2^2/D10^2 : 2.91455E-03 (-0.00269883 0.0127227)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.10e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.762e-09 5.230e-09
25- 50 2.121e-08 1.244e-08
50-150 6.810e-08 3.763e-08
15-150 9.807e-08 4.873e-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: 1.46218 ( -0.106644 0.106611 )
Norm@50keV : 2.18206E-03 ( -0.000137405 0.000137311 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.14e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 180.2 sec: 0.269731 ( -0.0176982 0.0177368 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.75439e-06 ( -2.53812e-07 2.5479e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.751762 ( -0.499647 0.448058 )
Epeak [keV] : 91.7799 ( -18.8285 65.557 )
Norm@50keV : 4.82482E-03 ( -0.00186266 0.00345228 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.56e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 180.2 sec: 0.260834 ( -0.018554 0.018565 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.59847e-06 ( -2.743e-07 2.74571e-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) = 1.04e-06
S(50-100 keV) = 1.50e-06
T90 vs. Hardness ratio plot
T90 = 215.927999973297 sec.
Hardness ratio (energy fluence ratio) = 1.44231
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.53778
Count Ratio (50-100 keV) / (15-25 keV) = 1.18856
Mask shadow pattern
IMX = 6.633276817333866E-01, IMY = 3.102406262588234E-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:
-239.176000 -13.476000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6339 22.0300 0.3 18.4 45.9 8.9454 33.5 0.9 Crab
93.8143 54.7820 2.6 50.5 26.5 3.8504 4.4 ------ UNKNOWN
101.6296 -33.6447 2.6 49.5 158.2 3.6921 4.4 ------ UNKNOWN
65.4508 31.4452 2.7 25.0 -3.3 1.0889 4.3 ------ UNKNOWN
41.8264 6.2313 2.9 30.3 -79.5 1.5687 3.9 ------ UNKNOWN
39.3328 -29.1919 3.0 48.3 -129.9 5.1198 3.9 ------ UNKNOWN
26.8267 21.5600 3.2 46.1 -56.3 4.3382 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.476000 166.724600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6648 21.8733 5.6 18.2 46.3 0.4585 2.1 8.6 Crab
75.9552 -51.4909 2.7 58.9 -172.0 5.8761 4.3 ------ UNKNOWN
47.3203 35.3228 0.6 36.2 -25.1 5.3447 18.5 ------ UNKNOWN
39.5539 -21.7940 1.9 43.3 -122.3 4.4298 6.0 ------ UNKNOWN
30.1760 8.8351 1.8 41.7 -74.2 4.8838 6.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
300.924600 962.967800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4606 35.3433 31.4 46.0 -12.3 0.3229 0.4 0.2 Her X-1
237.8488 25.4738 4.0 54.0 8.0 5.4884 2.9 ------ UNKNOWN
76.7333 42.1584 4.2 56.9 177.3 7.4258 2.8 ------ UNKNOWN
242.4721 28.3270 2.9 51.5 2.5 5.0642 4.0 ------ UNKNOWN
356.8326 55.5744 2.6 43.9 -116.5 10.7066 4.5 ------ UNKNOWN
14.2280 52.4704 3.7 48.4 -129.9 9.1380 3.2 ------ UNKNOWN
Plot creation:
Sun Nov 13 11:35:54 EST 2022