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
318.1360 34.4342 0.0052 8.6178 -17.2314 6.4120871 36.706 TRIG_01167973
Foreground time interval of the image:
-32.939 11.461 (delta_t = 44.400 [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 -145.632 sec. to 56.096 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63502 ( -0.0935679 0.0945728 )
Norm@50keV : 5.57112E-03 ( -0.000279858 0.000278728 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.97 using 59 bins.
Reduced chi-squared = 1.19246
# Null hypothesis probability of 1.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 201.7 sec: 0.723927 ( -0.036862 0.037001 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04685e-05 ( -5.6099e-07 5.64018e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -145.632 sec. to 56.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63318 ( -0.260268 0.11489 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 5.58324E-03 ( -0.000281024 0.000269058 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.98 using 59 bins.
Reduced chi-squared = 1.21393
# Null hypothesis probability of 1.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 201.7 sec: 0.725923 ( -0.043466 0.038627 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04951e-05 ( -6.42588e-07 5.90695e-07 ) ergs/cm2
Band function
Time interval is from -145.632 sec. to 56.096 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] : 14.9341 ( )
R^2/D10^2 : 7.74366E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 184.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.52e-15 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.298e-07 7.160e-08
25- 50 2.888e-06 1.916e-07
50-150 4.375e-06 3.832e-07
15-150 7.993e-06 4.891e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 177.167 (-41.6861 -177.302)
Norm : 2.91254 (-0.158202 0.174754)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.19e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.484e-06 1.078e-07
25- 50 2.814e-06 3.721e-07
50-150 5.925e-06 1.898e-06
15-150 1.022e-05 2.372e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.76590 (-0.716118 0.885076)
R1^2/D10^2 : 3.55468 (-1.83691 4.01196)
kT2 [keV] : 21.5127 (-2.16201 2.8138)
R2^2/D10^2 : 1.85334E-02 (-0.00669628 0.00880646)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.37e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.757e-06 3.639e-07
25- 50 2.518e-06 2.965e-07
50-150 5.856e-06 7.655e-07
15-150 1.013e-05 1.078e-06
Peak spectrum fit
Power-law model
Time interval is from 15.884 sec. to 16.884 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33400 ( -0.104483 0.104631 )
Norm@50keV : 4.90013E-02 ( -0.00283176 0.0028252 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.48 using 59 bins.
Reduced chi-squared = 0.903158
# Null hypothesis probability of 6.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.88425 ( -0.34357 0.34401 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.80386e-07 ( -3.14132e-08 3.16258e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 15.884 sec. to 16.884 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32169 ( -0.359534 0.10621 )
Epeak [keV] : 9978.30 ( -9999.34 -9999.34 )
Norm@50keV : 4.96448E-02 ( -0.00284154 0.02284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.56 using 59 bins.
Reduced chi-squared = 0.920714
# Null hypothesis probability of 6.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.89159 ( -0.36602 0.34858 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.81271e-07 ( -3.59533e-08 3.24768e-08 ) ergs/cm2
Band function
Time interval is from 15.884 sec. to 16.884 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] : 17.2127 ( )
R^2/D10^2 : 0.420663 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 134.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.00e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.529e-08 2.890e-09
25- 50 1.130e-07 9.250e-09
50-150 2.400e-07 2.665e-08
15-150 3.784e-07 3.020e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-15.8296 -200)
Norm : 24.2022 (-1.39347 1.39347)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.06e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.028e-08 3.755e-09
25- 50 1.160e-07 7.750e-09
50-150 2.543e-07 5.830e-08
15-150 4.305e-07 6.460e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.06015 (-1.22939 1.39636)
R1^2/D10^2 : 5.58109 (-2.51497 5.41868)
kT2 [keV] : 31.0027 (-5.11438 8.36609)
R2^2/D10^2 : 5.06054E-02 (-0.0267212 0.0418981)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.40e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.254e-08 1.302e-08
25- 50 1.094e-07 1.878e-08
50-150 3.229e-07 7.400e-08
15-150 4.848e-07 7.660e-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: 1.43630 ( -0.065243 0.0652631 )
Norm@50keV : 8.69622E-03 ( -0.000299266 0.000299194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.73e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 44.4 sec: 1.06809 ( -0.0393584 0.0395052 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.7043e-06 ( -1.38079e-07 1.38447e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31787 ( -0.262263 0.155772 )
Epeak [keV] : 312.297 ( -312.297 -312.297 )
Norm@50keV : 9.87335E-03 ( -0.00140809 0.00310578 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.64e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 44.4 sec: 1.05942 ( -0.04301 0.02151 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.67523e-06 ( -1.53304e-07 1.4426e-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) = 2.76e-06
S(50-100 keV) = 3.55e-06
T90 vs. Hardness ratio plot
T90 = 178.367999911308 sec.
Hardness ratio (energy fluence ratio) = 1.28623
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.02445
Count Ratio (50-100 keV) / (15-25 keV) = 0.820044
Mask shadow pattern
IMX = 1.447515832337387E-01, IMY = 4.489497646591305E-02
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:
-32.939400 11.460600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4928 35.4718 4.3 44.0 127.5 -2.3031 -2.7 7.9 Her X-1
288.9273 11.0207 8.5 35.7 64.8 0.4793 1.4 8.8 GRS 1915+105
299.5427 35.2115 1.6 10.7 86.6 1.2347 7.3 2.4 Cyg X-1
308.2082 40.9131 6.3 2.1 114.4 0.2932 1.8 5.0 Cyg X-3
325.9936 38.2874 8.9 11.8 -56.1 -0.2132 -1.3 8.6 Cyg X-2
299.4753 15.6480 2.5 27.3 50.5 0.8664 4.5 ------ UNKNOWN
318.1361 34.4342 0.3 8.6 -17.2 6.4121 36.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
51.060600 782.430000
900.160000 934.860600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.8158 11.0724 7.3 35.5 70.3 -2.9087 -1.6 7.7 GRS 1915+105
299.5309 35.1887 1.0 15.3 112.5 11.2988 11.2 3.0 Cyg X-1
307.9130 40.9282 10.4 10.4 146.1 1.0255 1.1 9.1 Cyg X-3
325.9576 38.4126 13.0 7.4 -110.2 -0.8684 -0.9 11.5 Cyg X-2
286.5464 19.6293 2.8 31.6 84.7 6.3829 4.1 ------ UNKNOWN
308.9518 -8.9020 3.7 44.2 27.5 4.3989 3.1 ------ UNKNOWN
Plot creation:
Fri Oct 13 22:20:24 EDT 2023