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
Foreground time interval of the image:
-3.648 12.909 (delta_t = 16.557 [sec])
Background time interval of the image:
-172.291 -3.648 (delta_t = 168.643 [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 18.008 sec. to 369.732 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53439 ( -0.0889584 0.0896471 )
Norm@50keV : 2.96785E-03 ( -0.000142259 0.000141633 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.69 using 59 bins.
Reduced chi-squared = 1.06474
# Null hypothesis probability of 3.44e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 351.7 sec: 0.374047 ( -0.018174 0.018228 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.85013e-06 ( -5.15174e-07 5.18044e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 18.008 sec. to 369.732 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43635 ( -0.349967 0.177836 )
Epeak [keV] : 300.137 ( -299.576 -299.576 )
Norm@50keV : 3.30943E-03 ( -0.000469625 0.00151883 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.43 using 59 bins.
Reduced chi-squared = 1.07911
# Null hypothesis probability of 3.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 351.7 sec: 0.371628 ( -0.019827 0.019715 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.77469e-06 ( -5.74386e-07 5.55595e-07 ) ergs/cm2
Band function
Time interval is from 18.008 sec. to 369.732 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] : 15.8304 ( )
R^2/D10^2 : 3.38163E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 165.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.44e-12 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.177e-07 5.434e-08
25- 50 2.575e-06 1.651e-07
50-150 4.493e-06 4.150e-07
15-150 7.686e-06 4.449e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-31.7193 -200)
Norm : 1.51713 (-0.0706007 0.0706007)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.97e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.329e-06 6.788e-08
25- 50 2.557e-06 1.347e-07
50-150 5.607e-06 2.989e-07
15-150 9.493e-06 5.803e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.32846 (-0.916427 1.11857)
R1^2/D10^2 : 1.03882 (-0.545543 1.30322)
kT2 [keV] : 22.8468 (-2.45965 3.37942)
R2^2/D10^2 : 8.16043E-03 (-0.00322101 0.00424631)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.97e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.411e-06 3.689e-07
25- 50 2.339e-06 2.940e-07
50-150 5.789e-06 7.474e-07
15-150 9.538e-06 1.145e-06
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Cutoff power-law model
Band function
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.48e-06
S(50-100 keV) = 3.42e-06
T90 vs. Hardness ratio plot
T90 = 163.952000021935 sec.
Hardness ratio (energy fluence ratio) = 1.37903
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.62354
Count Ratio (50-100 keV) / (15-25 keV) = 1.75759
Mask shadow pattern
IMX = -1.623204297746111E+00, IMY = 6.593911883587135E-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:
-172.291400 -3.648000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9990 -15.6146 1.6 41.8 109.4 7.2666 7.3 1.9 Sco X-1
254.4577 35.1544 5.8 47.8 33.6 1.5581 2.0 11.3 Her X-1
251.4798 4.5471 4.4 40.7 77.1 3.1616 2.6 ------ UNKNOWN
192.4702 -45.7921 3.1 57.0 178.9 4.6617 3.7 ------ UNKNOWN
190.4072 -34.7722 3.0 47.6 -173.4 1.8783 3.9 ------ UNKNOWN
186.2093 -22.9839 2.9 39.8 -159.5 1.4628 4.0 ------ UNKNOWN
176.7253 -44.2689 2.3 61.3 -169.0 17.9352 5.0 ------ UNKNOWN
217.7764 69.4527 3.2 60.8 -13.3 10.2881 3.7 ------ UNKNOWN
163.8974 -19.1437 2.7 53.9 -137.7 8.3364 4.4 ------ UNKNOWN
171.2035 48.5257 2.4 51.7 -48.6 10.0079 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.648000 12.908600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.7869 -15.7319 0.0 41.7 109.7 0.2919 0.8 12.4 Sco X-1
254.3240 35.2569 6.8 47.7 33.4 -0.3943 -1.7 8.3 Her X-1
239.1349 -37.0244 3.0 53.0 135.4 4.0591 3.8 ------ UNKNOWN
241.4274 -24.1833 2.4 44.6 122.3 3.0642 4.8 ------ UNKNOWN
257.9979 38.8281 2.7 51.8 30.6 1.9371 4.3 ------ UNKNOWN
168.5490 -36.7342 0.7 60.3 -157.9 25.8634 17.3 ------ UNKNOWN
171.1502 -5.5525 2.2 42.0 -124.7 1.2676 5.1 ------ UNKNOWN
183.9056 66.6395 2.5 60.7 -28.0 5.1373 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.708600 361.508600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5370 -40.5560 1.5 26.0 -140.7 3.1381 7.7 0.4 Vela X-1
170.3517 -60.5766 3.7 23.9 145.9 1.3693 3.1 3.0 Cen X-3
186.6683 -62.8408 1.8 28.4 130.7 3.3216 6.6 4.2 GX 301-2
152.4683 -58.2594 2.5 24.0 169.1 1.9776 4.6 ------ UNKNOWN
168.5958 -36.7539 0.9 0.0 -176.3 4.9555 13.4 ------ UNKNOWN
97.5560 -49.8100 4.3 51.3 -160.6 2.4509 2.7 ------ UNKNOWN
82.1665 -50.8233 4.5 60.3 -165.5 8.0481 2.6 ------ UNKNOWN
181.4844 18.7822 3.6 56.8 -17.4 4.6622 3.2 ------ UNKNOWN
170.8096 7.3253 3.0 44.1 -28.9 2.6095 3.9 ------ UNKNOWN
157.6324 3.3891 3.3 41.4 -48.7 2.7167 3.5 ------ UNKNOWN
99.6412 -40.6720 3.4 52.6 -148.9 3.7052 3.4 ------ UNKNOWN
102.3049 -31.8491 2.8 53.9 -137.7 12.8419 4.1 ------ UNKNOWN
Plot creation:
Fri Nov 11 21:21:27 EST 2022