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
38.9380 -34.6151 0.0055 24.2661 -69.1492 3.3941642 35.211 TRIG_01129775
Foreground time interval of the image:
-3.176 15.261 (delta_t = 18.437 [sec])
Background time interval of the image:
-201.539 -3.176 (delta_t = 198.363 [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 -3.176 sec. to 29.800 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28087 ( -0.0836576 0.0834755 )
Norm@50keV : 6.83597E-03 ( -0.000319943 0.000319931 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.21 using 59 bins.
Reduced chi-squared = 1.10895
# Null hypothesis probability of 2.66e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 32.98 sec: 0.812753 ( -0.039517 0.039577 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.23867e-06 ( -1.15718e-07 1.16218e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.176 sec. to 29.800 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.816820 ( -0.369794 0.340649 )
Epeak [keV] : 139.095 ( -38.8446 210.851 )
Norm@50keV : 1.12348E-02 ( -0.00335978 0.00525646 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.66 using 59 bins.
Reduced chi-squared = 1.02964
# Null hypothesis probability of 4.14e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 32.98 sec: 0.793048 ( -0.041986 0.041989 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.17456e-06 ( -1.2627e-07 1.25989e-07 ) ergs/cm2
Band function
Time interval is from -3.176 sec. to 29.800 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] : 18.2583 ( )
R^2/D10^2 : 4.94753E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 122.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.09e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.084e-07 1.029e-08
25- 50 5.067e-07 3.183e-08
50-150 1.230e-06 1.078e-07
15-150 1.846e-06 1.097e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-9.26154 -200)
Norm : 3.38371 (-0.16004 0.16004)
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.86e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.778e-07 1.550e-08
25- 50 5.345e-07 2.622e-08
50-150 1.172e-06 6.860e-08
15-150 1.985e-06 1.148e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.21581 (-1.32778 1.80536)
R1^2/D10^2 : 0.911562 (-0.520079 1.37215)
kT2 [keV] : 24.5833 (-2.68773 4.17765)
R2^2/D10^2 : 1.60348E-02 (-0.00701723 0.00834088)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.52e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.181e-07 5.950e-08
25- 50 4.894e-07 9.195e-08
50-150 1.433e-06 1.850e-07
15-150 2.141e-06 2.676e-07
Peak spectrum fit
Power-law model
Time interval is from 0.028 sec. to 1.028 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00359 ( -0.135423 0.133393 )
Norm@50keV : 2.94191E-02 ( -0.00240654 0.00240439 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.11 using 59 bins.
Reduced chi-squared = 0.896667
# Null hypothesis probability of 6.95e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.38764 ( -0.28056 0.28078 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.17753e-07 ( -2.84786e-08 2.86407e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.028 sec. to 1.028 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.332161 ( -0.64837 0.557813 )
Epeak [keV] : 140.561 ( -43.3511 351.896 )
Norm@50keV : 5.95055E-02 ( -0.0258889 0.0545339 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.78 using 59 bins.
Reduced chi-squared = 0.835357
# Null hypothesis probability of 8.05e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.32390 ( -0.28717 0.28648 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.09072e-07 ( -3.04471e-08 3.01859e-08 ) ergs/cm2
Band function
Time interval is from 0.028 sec. to 1.028 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] : 21.1580 (-2.10231 2.42993)
R^2/D10^2 : 0.141120 (-0.0410238 0.0556298)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.16e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.190e-08 1.901e-09
25- 50 6.144e-08 7.980e-09
50-150 2.051e-07 2.870e-08
15-150 2.784e-07 3.035e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-13.7085 -200)
Norm : 13.4591 (-1.15257 1.15257)
------------------------------------------------------------
#Fit statistic : Chi-Squared 91.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.49e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.351e-08 4.660e-09
25- 50 6.446e-08 1.743e-08
50-150 1.414e-07 5.689e-08
15-150 2.393e-07 8.230e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.38271 (-4.10215 6.15156)
R1^2/D10^2 : 0.826576 (-0.551155 3.70364)
kT2 [keV] : 31.4788 (-7.77951 67.3464)
R2^2/D10^2 : 3.28489E-02 (-0.0309297 0.0577613)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.65e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.940e-08 9.877e-09
25- 50 6.382e-08 2.801e-08
50-150 2.273e-07 1.151e-07
15-150 3.105e-07 1.494e-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: 1.28969 ( -0.0738128 0.0737059 )
Norm@50keV : 1.14236E-02 ( -0.000473149 0.000473134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.44 sec: 1.36030 ( -0.0586347 0.0587307 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.08689e-06 ( -9.52629e-08 9.5559e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.852482 ( -0.321105 0.299071 )
Epeak [keV] : 143.189 ( -38.7267 176.512 )
Norm@50keV : 1.82539E-02 ( -0.00489662 0.00724374 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.44 sec: 1.32957 ( -0.06205 0.06207 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03275e-06 ( -1.03946e-07 1.03375e-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) = 4.91e-07
S(50-100 keV) = 8.11e-07
T90 vs. Hardness ratio plot
T90 = 21.9839999675751 sec.
Hardness ratio (energy fluence ratio) = 1.65173
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.55011
Count Ratio (50-100 keV) / (15-25 keV) = 1.44175
Mask shadow pattern
IMX = 1.604581815327354E-01, IMY = 4.212827896937619E-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:
-201.539400 -3.176000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6459 22.0219 4.7 55.3 166.6 6.5298 2.5 0.8 Crab
341.8213 -38.0477 2.4 57.2 -16.1 7.6981 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.176000 15.260590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8063 22.0146 9.0 55.4 166.7 -0.4122 -1.3 9.6 Crab
56.2092 -11.6701 2.5 17.9 -151.3 0.2928 4.7 ------ UNKNOWN
38.9380 -34.6151 0.3 24.3 -69.1 3.3942 35.2 ------ UNKNOWN
95.6192 -1.0189 2.5 58.0 -162.5 1.9952 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
75.060600 350.060590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
357.0343 -7.2209 2.8 47.2 49.2 7.3637 4.1 468.2 UNKNOWN
321.2465 -48.6870 2.0 57.1 -16.1 11.4746 5.7 ------ UNKNOWN
Plot creation:
Fri Nov 3 18:50:20 EDT 2023