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
2.9459 -21.8971 0.0035 16.0270 67.1769 5.3512328 55.780 TRIG_01048372
Foreground time interval of the image:
-1.084 17.077 (delta_t = 18.161 [sec])
Background time interval of the image:
-172.723 -1.084 (delta_t = 171.639 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -1.084 sec. to 75.128 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65473 ( -0.0429695 0.0430464 )
Norm@50keV : 1.04085E-02 ( -0.000225937 0.0002259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.96 using 59 bins.
Reduced chi-squared = 0.701053
# Null hypothesis probability of 9.58e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 76.21 sec: 1.36127 ( -0.03391 0.03405 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.375e-06 ( -1.65555e-07 1.6553e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.084 sec. to 75.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45056 ( -0.178123 0.171268 )
Epeak [keV] : 145.039 ( -43.3096 393.341 )
Norm@50keV : 1.29301E-02 ( -0.00209988 0.00262286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.80 using 59 bins.
Reduced chi-squared = 0.639286
# Null hypothesis probability of 9.84e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 76.21 sec: 1.33671 ( -0.03907 0.03931 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.25691e-06 ( -1.92406e-07 1.91811e-07 ) ergs/cm2
Band function
Time interval is from -1.084 sec. to 75.128 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] : 15.3324 ( )
R^2/D10^2 : 0.130055 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 453.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.50e-63 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.860e-07 2.081e-08
25- 50 1.970e-06 5.678e-08
50-150 3.182e-06 1.357e-07
15-150 5.637e-06 1.349e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.725 (-18.8729 23.2229)
Norm : 5.45639 (-0.150208 0.159116)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.055e-06 4.877e-08
25- 50 1.987e-06 1.056e-07
50-150 4.107e-06 8.768e-07
15-150 7.150e-06 9.903e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.68606 (-0.633676 0.658556)
R1^2/D10^2 : 1.05267 (-0.253577 0.366521)
kT2 [keV] : 27.7519 (-2.47645 3.19437)
R2^2/D10^2 : 1.20012E-02 (-0.00391542 0.00503876)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.11e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.460e-07 6.859e-08
25- 50 2.043e-06 8.536e-08
50-150 4.158e-06 2.568e-07
15-150 7.147e-06 3.132e-07
Peak spectrum fit
Power-law model
Time interval is from -0.520 sec. to 0.480 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17758 ( -0.0697086 0.0697294 )
Norm@50keV : 7.48113E-02 ( -0.0029893 0.0029892 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.40 using 59 bins.
Reduced chi-squared = 1.02456
# Null hypothesis probability of 4.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.321756 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.63959e-07 ( -3.45183e-08 3.46607e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.520 sec. to 0.480 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.593977 ( -0.318422 0.297214 )
Epeak [keV] : 132.808 ( -28.5789 78.0508 )
Norm@50keV : 0.139210 ( -0.0369165 0.0542434 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.48 using 59 bins.
Reduced chi-squared = 0.83
# Null hypothesis probability of 8.14e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 8.52865 ( -0.37357 0.37344 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.39009e-07 ( -3.74729e-08 3.73632e-08 ) ergs/cm2
Band function
Time interval is from -0.520 sec. to 0.480 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] : 18.9998 ( )
R^2/D10^2 : 0.487200 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 120.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.81e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.457e-08 2.640e-09
25- 50 1.663e-07 8.850e-09
50-150 4.411e-07 3.305e-08
15-150 6.420e-07 3.200e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 ( )
Norm : 35.8234 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 128.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.02e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.920e-08 3.970e-09
25- 50 1.716e-07 7.600e-09
50-150 3.763e-07 1.665e-08
15-150 6.371e-07 2.915e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.50646 (-1.67976 2.08443)
R1^2/D10^2 : 4.62495 (-2.28518 5.96786)
kT2 [keV] : 26.7947 (-3.21785 5.48501)
R2^2/D10^2 : 0.133681 (-0.0659246 0.0798166)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.13e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.081e-08 1.466e-08
25- 50 1.641e-07 2.355e-08
50-150 5.098e-07 6.185e-08
15-150 7.348e-07 9.340e-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: 1.33882 ( -0.0500131 0.0499621 )
Norm@50keV : 1.87070E-02 ( -0.000497292 0.000497286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.85e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.16 sec: 2.24854 ( -0.0643202 0.0644564 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.32639e-06 ( -9.53311e-08 9.55025e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09388 ( -0.205957 0.196733 )
Epeak [keV] : 205.327 ( -68.6588 524.014 )
Norm@50keV : 2.41725E-02 ( -0.00439264 0.00563651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.16 sec: 2.21200 ( -0.07003 0.07021 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.27479e-06 ( -1.05183e-07 1.04729e-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) = 1.96e-06
S(50-100 keV) = 2.49e-06
T90 vs. Hardness ratio plot
T90 = 70.2079999446869 sec.
Hardness ratio (energy fluence ratio) = 1.27041
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.26387
Count Ratio (50-100 keV) / (15-25 keV) = 0.841572
Mask shadow pattern
IMX = 1.114222770807317E-01, IMY = -2.647645744731804E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-172.723410 -1.084000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
330.5718 1.5041 2.3 44.6 129.6 4.1614 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.084000 17.076620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
330.4120 23.5693 2.2 54.1 156.1 2.5175 5.2 ------ UNKNOWN
2.9459 -21.8971 0.2 16.0 67.2 5.3513 55.8 ------ UNKNOWN
54.4112 -33.9403 2.7 44.2 -23.3 0.6891 4.3 ------ UNKNOWN
52.6280 -31.7791 2.7 42.0 -25.3 0.6208 4.2 ------ UNKNOWN
65.3303 -20.3327 2.9 50.5 -44.4 1.7093 4.0 ------ UNKNOWN
46.6599 15.7724 2.8 41.3 -100.7 1.4549 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
58.876600 962.208900
1353.176000 1553.226000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
318.7215 -36.1318 2.6 40.8 96.4 9.7638 4.5 ------ UNKNOWN
9.5969 -70.4527 3.0 48.7 34.0 10.5619 3.8 ------ UNKNOWN
318.6596 -1.6296 2.4 47.6 145.9 12.4764 4.9 ------ UNKNOWN
351.7683 -40.9557 3.4 21.3 60.7 2.6265 3.4 ------ UNKNOWN
335.3328 11.5328 3.9 43.0 175.1 3.9876 3.0 ------ UNKNOWN
332.1798 28.2098 3.0 58.2 -175.1 15.3857 3.8 ------ UNKNOWN
68.5810 -42.3512 2.8 57.7 -15.9 13.8911 4.1 ------ UNKNOWN
64.2148 -39.3824 4.1 54.4 -19.5 6.6626 2.8 ------ UNKNOWN
70.1557 -38.2264 2.9 59.1 -20.6 16.4411 3.9 ------ UNKNOWN
57.3986 -20.0489 2.9 50.6 -44.6 14.6406 3.9 ------ UNKNOWN
Plot creation:
Fri Nov 11 21:59:13 EST 2022