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
132.1447 -2.7344 0.0097 32.0771 44.0417 1.5797072 19.750 TRIG_01091101
Foreground time interval of the image:
0.040 9.501 (delta_t = 9.461 [sec])
Background time interval of the image:
-239.200 0.040 (delta_t = 239.240 [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 0.256000
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 0.256000
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 0.256000
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 0.040 sec. to 127.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55074 ( -0.0505574 0.0506403 )
Norm@50keV : 6.77972E-03 ( -0.000178422 0.000178355 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.73 using 59 bins.
Reduced chi-squared = 1.04789
# Null hypothesis probability of 3.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 127 sec: 0.858482 ( -0.024497 0.024565 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.10594e-06 ( -2.27255e-07 2.27872e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.040 sec. to 127.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27927 ( -0.209456 0.199762 )
Epeak [keV] : 140.293 ( -38.9907 219.19 )
Norm@50keV : 9.10639E-03 ( -0.00173382 0.00226315 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.27 using 59 bins.
Reduced chi-squared = 0.969107
# Null hypothesis probability of 5.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 127 sec: 0.840793 ( -0.027429 0.027514 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.92855e-06 ( -2.62106e-07 2.61262e-07 ) ergs/cm2
Band function
Time interval is from 0.040 sec. to 127.064 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] : 15.6975 ( )
R^2/D10^2 : 7.86160E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 325.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.22e-39 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.108e-07 2.908e-08
25- 50 2.114e-06 7.811e-08
50-150 3.614e-06 1.905e-07
15-150 6.239e-06 1.880e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-18.5191 -200)
Norm : 3.47330 (-0.0907142 0.0907142)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.48e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.099e-06 3.258e-08
25- 50 2.114e-06 6.414e-08
50-150 4.636e-06 1.238e-07
15-150 7.848e-06 2.356e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.17670 (-0.732425 0.798398)
R1^2/D10^2 : 0.788173 (-0.234959 0.364962)
kT2 [keV] : 26.1492 (-2.40747 3.184)
R2^2/D10^2 : 1.04880E-02 (-0.00359603 0.00456695)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.004e-06 8.998e-08
25- 50 2.116e-06 1.283e-07
50-150 4.728e-06 3.581e-07
15-150 7.848e-06 4.813e-07
Peak spectrum fit
Power-law model
Time interval is from 0.064 sec. to 1.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75396 ( -0.138468 0.142615 )
Norm@50keV : 3.79135E-02 ( -0.00344709 0.00340275 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.39 using 59 bins.
Reduced chi-squared = 1.09456
# Null hypothesis probability of 2.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.13429 ( -0.41907 0.41925 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.49816e-07 ( -3.26694e-08 3.30087e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.064 sec. to 1.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26523 ( -0.64077 0.538932 )
Epeak [keV] : 69.3900 ( -18.6666 -69.39 )
Norm@50keV : 6.98654E-02 ( -0.0332736 0.0846745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.11 using 59 bins.
Reduced chi-squared = 1.07339
# Null hypothesis probability of 3.29e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.05465 ( -0.4299 0.42909 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.37023e-07 ( -3.59443e-08 3.60983e-08 ) ergs/cm2
Band function
Time interval is from 0.064 sec. to 1.064 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] : 11.9272 (-1.09572 1.22366)
R^2/D10^2 : 1.29267 (-0.39264 0.550973)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.57e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.887e-08 5.605e-09
25- 50 1.215e-07 1.270e-08
50-150 1.035e-07 1.998e-08
15-150 2.638e-07 2.590e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 114.550 (-31.6992 48.8607)
Norm : 22.0465 (-2.21328 2.7504)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.64e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.752e-08 6.570e-09
25- 50 1.021e-07 1.029e-08
50-150 1.779e-07 6.861e-08
15-150 3.375e-07 7.540e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.46680 (-2.54955 1.95039)
R1^2/D10^2 : 5.02959 (-2.52977 14.2572)
kT2 [keV] : 25.5351 (-8.64651 19.9799)
R2^2/D10^2 : 5.22734E-02 (-0.0434218 0.224373)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.32e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.379e-08 1.829e-08
25- 50 1.077e-07 3.312e-08
50-150 1.772e-07 8.688e-08
15-150 3.387e-07 1.069e-07
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: 1.68784 ( -0.130264 0.132633 )
Norm@50keV : 1.06862E-02 ( -0.000880074 0.000871025 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.23e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.461 sec: 1.41328 ( -0.105786 0.105836 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.37017e-07 ( -8.1179e-08 8.20892e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24141 ( -0.566669 0.49061 )
Epeak [keV] : 76.6042 ( -22.1774 -76.6043 )
Norm@50keV : 1.87996E-02 ( -0.00841664 0.0193069 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.72e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.461 sec: 1.38774 ( -0.10954 0.10944 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.96021e-07 ( -9.29231e-08 9.37793e-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) = 2.06e-06
S(50-100 keV) = 2.81e-06
T90 vs. Hardness ratio plot
T90 = 83.5119999647141 sec.
Hardness ratio (energy fluence ratio) = 1.36408
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.42622
Count Ratio (50-100 keV) / (15-25 keV) = 1.04436
Mask shadow pattern
IMX = 4.505223046822464E-01, IMY = -4.356992036297798E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.200000 0.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5947 -40.6202 4.7 52.9 -5.1 1.7852 2.4 5.0 Vela X-1
171.7356 27.1869 2.7 22.8 169.1 1.2022 4.2 ------ UNKNOWN
182.1063 -16.0726 2.4 29.0 -71.5 1.9264 4.8 ------ UNKNOWN
203.5042 11.7172 3.3 40.3 -132.3 1.8794 3.5 ------ UNKNOWN
202.1803 -3.1794 3.3 40.1 -109.0 3.2973 3.5 ------ UNKNOWN
207.2200 3.8552 3.8 44.0 -120.6 3.2796 3.0 ------ UNKNOWN
177.2250 -43.0603 3.4 50.6 -44.5 4.1884 3.4 ------ UNKNOWN
211.4079 9.9405 2.6 48.0 -129.2 5.6089 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.040000 9.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.7125 -40.5399 5.1 52.8 -5.1 0.2759 2.3 8.4 Vela X-1
132.1446 -2.7344 0.6 32.1 44.0 1.5797 19.7 ------ UNKNOWN
179.2322 -8.8029 2.1 21.8 -78.9 0.2914 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
62.500600 962.848000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5108 -40.5518 1.2 38.0 -43.1 13.7745 9.5 0.8 Vela X-1
82.1267 -10.4518 4.6 50.2 39.7 11.8425 2.5 ------ UNKNOWN
141.8327 38.2125 2.7 41.9 152.4 7.1857 4.3 ------ UNKNOWN
98.8663 -12.9474 3.2 34.5 31.9 3.9218 3.6 ------ UNKNOWN
148.2136 33.9681 2.9 39.7 162.1 5.3193 4.0 ------ UNKNOWN
100.6193 -24.3813 3.6 37.3 12.8 3.5490 3.2 ------ UNKNOWN
117.6347 -27.5996 3.3 28.5 -11.2 2.4751 3.5 ------ UNKNOWN
142.0859 -2.7091 3.5 9.9 -128.8 2.0712 3.3 ------ UNKNOWN
112.0431 -49.0286 2.8 49.4 -21.7 7.7356 4.2 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:11:01 EDT 2022