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
254.3192 42.5675 0.0188 27.0766 11.9744 1.4358452 10.282 TRIG_01044382
Foreground time interval of the image:
-14.299 74.301 (delta_t = 88.600 [sec])
Background time interval of the image:
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 -21.304 sec. to 160.136 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47066 ( -0.18924 0.191135 )
Norm@50keV : 8.73005E-04 ( -9.80937e-05 9.75057e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.10 using 59 bins.
Reduced chi-squared = 0.84386
# Null hypothesis probability of 7.93e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 181.4 sec: 0.108151 ( -0.0119674 0.011983 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.51e-06 ( -1.8643e-07 1.88545e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -21.304 sec. to 160.136 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.963259 ( -0.923551 0.637882 )
Epeak [keV] : 101.999 ( -37.8818 -101.999 )
Norm@50keV : 1.57717E-03 ( -0.000771777 0.00274121 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.79 using 59 bins.
Reduced chi-squared = 0.835536
# Null hypothesis probability of 8.05e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 181.4 sec: 0.105752 ( -0.0124863 0.012505 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45217e-06 ( -2.05454e-07 2.0691e-07 ) ergs/cm2
Band function
Time interval is from -21.304 sec. to 160.136 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] : 15.3098 (-1.96198 2.30669)
R^2/D10^2 : 1.15560E-02 (-0.00448509 0.00712985)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.025e-07 2.198e-08
25- 50 4.150e-07 6.231e-08
50-150 6.678e-07 1.459e-07
15-150 1.185e-06 1.681e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-66.1385 -199.363)
Norm : 0.444261 (-0.0481701 0.0482581)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.09e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.007e-07 1.124e-07
25- 50 3.860e-07 2.102e-07
50-150 8.466e-07 4.647e-07
15-150 1.433e-06 5.774e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.69785 (-2.48927 3.9207)
R1^2/D10^2 : 0.189075 (-0.15027 1.99634)
kT2 [keV] : 21.2418 (-4.56296 13.2245)
R2^2/D10^2 : 3.14194E-03 (-0.00263797 0.00474574)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.66e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.852e-07 1.011e-07
25- 50 3.720e-07 1.400e-07
50-150 8.514e-07 4.698e-07
15-150 1.409e-06 6.268e-07
Peak spectrum fit
Power-law model
Time interval is from 21.020 sec. to 22.020 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.11944 ( -0.678538 0.933715 )
Norm@50keV : 3.16189E-03 ( -0.0017101 0.00150599 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.87 using 59 bins.
Reduced chi-squared = 1.08544
# Null hypothesis probability of 3.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.502319 ( -0.169728 0.169737 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.94408e-08 ( -1.26493e-08 1.36416e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 21.020 sec. to 22.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.89151 ( -3.78773 0.333503 )
Epeak [keV] : 281.185 ( )
Norm@50keV : 1.33891E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.61 using 59 bins.
Reduced chi-squared = 1.10018
# Null hypothesis probability of 2.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.384059 ( -0.207679 0.281689 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.98119e-08 ( -1.01842e-08 1.1395e-08 ) ergs/cm2
Band function
Time interval is from 21.020 sec. to 22.020 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] : 10.8085 (-3.94031 5.32045)
R^2/D10^2 : 0.170775 (-0.170665 0.770608)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.81 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 4.153e-09 2.633e-09
25- 50 1.148e-08 7.195e-09
50-150 7.472e-09 5.825e-09
15-150 2.310e-08 1.480e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 60.7770 (-60.7768 -60.7768)
Norm : 2.59401 (-1.14103 2.72221)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.91e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.533e-09 4.106e-09
25- 50 9.982e-09 6.300e-09
50-150 1.148e-08 9.855e-09
15-150 2.799e-08 1.894e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.16119 (-1.46227 2.5392)
R1^2/D10^2 : 225.817 (-370.148 -372.889)
kT2 [keV] : 13.4722 (-4.55897 9.73698)
R2^2/D10^2 : 6.47082E-02 (-0.059075 0.25641)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.11e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.502e-09 3.403e-09
25- 50 9.056e-09 5.765e-09
50-150 1.042e-08 7.120e-09
15-150 2.598e-08 1.595e-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: 1.46183 ( -0.23746 0.240388 )
Norm@50keV : 1.09724E-03 ( -0.000149722 0.000148461 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 88.6 sec: 0.135622 ( -0.0182301 0.0182668 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.28289e-07 ( -1.39751e-07 1.41627e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45908 ( -0.878258 1.61483 )
Epeak [keV] : 9989.98 ( -9987.69 -9987.69 )
Norm@50keV : 1.10081E-03 ( -0.000149489 0.00208879 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 88.6 sec: 0.135431 ( -0.018772 0.018323 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.31168e-07 ( -1.56177e-07 1.3826e-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) = 3.68e-07
S(50-100 keV) = 5.32e-07
T90 vs. Hardness ratio plot
T90 = 158.160000085831 sec.
Hardness ratio (energy fluence ratio) = 1.44565
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39196
Count Ratio (50-100 keV) / (15-25 keV) = 1.18441
Mask shadow pattern
IMX = 5.000862298625791E-01, IMY = -1.060633959254108E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-14.299400 74.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5784 35.3883 3.5 32.9 20.4 0.5732 3.3 6.5 Her X-1
299.4821 35.0340 6.7 55.8 -21.7 0.8595 1.8 11.4 Cyg X-1
254.3192 42.5675 1.1 27.1 12.0 1.4362 10.3 ------ UNKNOWN
110.4945 51.7444 2.6 55.3 -144.7 3.0987 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
124.300590 718.602900
721.000000 963.094800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4023 35.2971 7.1 7.3 41.2 0.9663 1.6 3.8 Her X-1
268.3934 -1.3997 8.4 45.7 21.7 1.6885 1.4 3.5 SW J1753.5-0127
288.8918 11.0169 11.2 43.5 -12.4 1.1408 1.0 7.0 GRS 1915+105
299.6124 35.2361 1.7 35.5 -52.1 7.0063 6.8 2.3 Cyg X-1
308.1752 40.9278 5.0 39.5 -65.0 3.9160 2.3 3.3 Cyg X-3
274.6911 -10.0521 2.9 55.8 17.1 11.4604 3.9 ------ UNKNOWN
272.8521 22.2216 3.6 25.5 -1.5 2.1259 3.2 ------ UNKNOWN
156.7287 60.9533 3.5 57.1 -173.5 8.3253 3.3 ------ UNKNOWN
306.8168 16.0796 2.8 51.8 -34.4 8.2587 4.0 ------ UNKNOWN
Plot creation:
Fri Nov 11 22:14:49 EST 2022