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:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
-12.899 73.501 (delta_t = 86.400 [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
Multiple GTIs in the spectrum
tstart tstop
100.444000 303.024300
348.000000 571.777000
573.000000 1370.288000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.06248 ( -0.0310021 0.0309938 )
Norm@50keV : 1.04242E-02 ( -0.000150152 0.000150145 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 94.84 using 59 bins.
Reduced chi-squared = 1.66386
# Null hypothesis probability of 1.23e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1224 sec: 1.61041 ( -0.03396 0.03425 ) ph/cm2/s
Energy fluence (15-150 keV) : 0.000118177 ( -1.73948e-06 1.74059e-06 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
100.444000 303.024300
348.000000 571.777000
573.000000 1370.288000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99880 ( -0.0429375 0.000997819 )
Epeak [keV] : 1.24735 ( -0.45283 1.59288 )
Norm@50keV : 1.10040E-02 ( -0.000188473 0.000368318 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 97.59 using 59 bins.
Reduced chi-squared = 1.74268
# Null hypothesis probability of 4.87e-04 with 56 degrees of freedom
Photon flux (15-150 keV) in 1224 sec: 1.63242 ( -0.03382 0.03468 ) ph/cm2/s
Energy fluence (15-150 keV) : 0.00011902 ( -5.52419e-06 1.85039e-06 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
100.444000 303.024300
348.000000 571.777000
573.000000 1370.288000
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] : 14.2465 ( )
R^2/D10^2 : 0.162337 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 1355.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.83e-246 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.504e-06 2.766e-07
25- 50 3.218e-05 6.854e-07
50-150 4.338e-05 1.095e-06
15-150 8.406e-05 1.242e-06
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 84.8561 ( )
Norm : 6.72940 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 204.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.05e-18 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.144e-05 5.753e-07
25- 50 3.579e-05 6.732e-07
50-150 5.252e-05 1.200e-06
15-150 1.098e-04 1.493e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.00634 ( )
R1^2/D10^2 : 2.04252 ( )
kT2 [keV] : 25.5755 ( )
R2^2/D10^2 : 1.30183E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 130.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.88e-08 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.152e-05 1.138e-06
25- 50 3.734e-05 9.792e-07
50-150 5.411e-05 1.512e-06
15-150 1.130e-04 2.564e-06
Peak spectrum fit
Power-law model
Time interval is from 1304.452 sec. to 1305.452 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84388 ( )
Norm@50keV : 1.71191E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 194.76 using 59 bins.
Reduced chi-squared = 3.41684
# Null hypothesis probability of 5.95e-17 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.40044 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57445e-07 ( 0 0 ) ergs/cm2
Cutoff power-law model
Time interval is from 1304.452 sec. to 1305.452 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55789 ( )
Epeak [keV] : 69.3354 ( )
Norm@50keV : 2.46755E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 194.39 using 59 bins.
Reduced chi-squared = 3.47125
# Null hypothesis probability of 3.61e-17 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.37773 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.53624e-07 ( 0 0 ) ergs/cm2
Band function
Time interval is from 1304.452 sec. to 1305.452 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] : 10.8518 ( )
R^2/D10^2 : 0.821149 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 211.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.48e-19 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.015e-08 5.070e-09
25- 50 5.598e-08 1.127e-08
50-150 3.685e-08 1.296e-08
15-150 1.130e-07 2.347e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 93.1277 ( )
Norm : 10.8017 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 194.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.15e-17 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.821e-08 5.865e-09
25- 50 4.807e-08 9.340e-09
50-150 7.472e-08 3.999e-08
15-150 1.510e-07 4.315e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.92910 ( )
R1^2/D10^2 : 5.63289 ( )
kT2 [keV] : 23.0573 ( )
R2^2/D10^2 : 3.86040E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 193.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.62e-17 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.958e-08 1.647e-08
25- 50 4.531e-08 2.321e-08
50-150 8.234e-08 4.734e-08
15-150 1.572e-07 8.183e-08
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) = 3.62e-05
S(50-100 keV) = 3.46e-05
T90 vs. Hardness ratio plot
T90 = 1104.75199997425 sec.
Hardness ratio (energy fluence ratio) = 0.955801
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.939338
Count Ratio (50-100 keV) / (15-25 keV) = 0.479208
Mask shadow pattern
IMX = 0, IMY = 0
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:
-12.899410 73.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9840 -15.6309 0.4 17.2 -78.6 15.4401 28.4 0.6 Sco X-1
254.3808 35.1978 4.7 52.7 0.9 -3.9162 -2.5 9.5 Her X-1
256.0190 -37.8347 1.3 21.7 -155.7 4.6528 8.7 1.6 4U 1700-377
256.3419 -36.3446 7.8 20.3 -155.1 -0.7626 -1.5 6.5 GX 349+2
262.8527 -24.7415 6.4 7.8 -170.4 0.9325 1.8 8.5 GX 1+4
264.7198 -44.4589 24.5 27.6 -173.3 0.2705 0.5 1.1 4U 1735-44
268.2254 -1.3258 7.2 16.5 28.9 -0.8339 -1.6 11.5 SW J1753.5-0127
270.2031 -24.9426 5.2 10.5 150.3 1.0546 2.2 9.3 GX 5-1
270.4283 -25.5642 0.0 11.1 151.6 0.8768 1.9 12.7 GRS 1758-258
273.9851 -13.9462 2.9 11.1 85.6 2.2139 4.0 5.5 GX 17+2
276.0918 -30.3853 4.1 18.1 150.1 -1.5344 -2.8 8.7 H1820-303
284.8510 -24.8641 4.3 22.0 124.4 1.7120 2.7 10.6 HT1900.1-2455
288.6644 10.9728 11.0 37.8 53.8 1.5639 1.0 8.1 GRS 1915+105
262.9698 -33.8329 105.4 16.9 -170.7 0.0532 0.1 1.0 GX 354-0
288.2548 19.8125 1.2 44.4 44.8 15.9341 9.5 ------ UNKNOWN
292.4092 -28.1307 3.3 29.4 127.2 2.9724 3.5 ------ UNKNOWN
291.1345 -71.6987 2.3 57.2 179.4 12.7798 5.1 ------ UNKNOWN
225.7715 -70.1317 2.7 57.8 -156.4 12.5074 4.3 ------ UNKNOWN
224.5977 -26.7932 2.5 36.7 -102.8 5.3748 4.6 ------ UNKNOWN
217.8282 -41.7293 1.8 45.7 -122.9 13.6909 6.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9834 -15.6310 0.4 17.2 -78.6 5.7345 26.6 0.6 Sco X-1
254.5611 35.3813 13.3 52.9 1.1 -0.5492 -0.9 5.6 Her X-1
256.0275 -37.8363 1.6 21.7 -155.7 1.5554 7.2 2.0 4U 1700-377
256.2932 -36.3462 20.2 20.3 -155.0 -0.1167 -0.6 8.3 GX 349+2
263.1672 -24.7040 20.0 7.8 -172.5 0.1180 0.6 9.0 GX 1+4
264.7221 -44.4591 13.9 27.6 -173.3 0.1890 0.8 1.0 4U 1735-44
268.2252 -1.3258 8.7 16.5 28.9 -0.2691 -1.3 11.5 SW J1753.5-0127
270.1485 -25.0085 8.8 10.6 150.7 0.2446 1.3 8.5 GX 5-1
270.4152 -25.5669 5.3 11.1 151.7 0.3894 2.2 12.2 GRS 1758-258
273.9999 -13.9397 2.9 11.1 85.6 0.8443 3.9 5.8 GX 17+2
276.0944 -30.4092 3.8 18.1 150.1 -0.6559 -3.0 9.1 H1820-303
284.8582 -24.8879 3.7 22.0 124.5 0.7791 3.1 9.9 HT1900.1-2455
288.6259 11.0196 10.8 37.8 53.7 0.6182 1.1 11.1 GRS 1915+105
262.9776 -33.8339 72.5 16.9 -170.8 0.0310 0.2 0.6 GX 354-0
288.2538 19.8095 1.3 44.4 44.8 5.9611 8.7 ------ UNKNOWN
292.3974 -28.1369 3.0 29.4 127.2 1.2819 3.9 ------ UNKNOWN
228.5273 -47.9885 2.2 41.8 -135.9 1.9709 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
158.500580 303.024300
348.000000 571.777000
573.000000 1332.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5774 35.5096 6.5 33.5 -49.8 15.8722 1.8 11.6 Her X-1
262.8279 -24.6023 62.3 50.8 -144.7 -3.8158 -0.2 13.1 GX 1+4
268.2139 -1.4075 33.8 28.9 -129.8 -2.8473 -0.3 9.6 SW J1753.5-0127
270.2538 -25.1220 9.1 48.2 -152.9 17.4898 1.3 3.1 GX 5-1
270.2831 -25.7561 6.9 48.8 -153.3 23.2298 1.7 1.3 GRS 1758-258
273.9721 -13.9847 14.0 36.6 -151.3 7.2807 0.8 3.7 GX 17+2
275.9305 -30.3669 57.4 51.5 -161.3 3.6648 0.2 0.3 H1820-303
285.0242 -24.9177 150.9 44.8 -170.8 1.0037 0.1 0.7 HT1900.1-2455
288.8062 11.0831 6.6 8.7 -178.6 -11.3227 -1.7 8.3 GRS 1915+105
299.6091 35.2013 0.7 18.4 35.8 110.5983 15.8 0.9 Cyg X-1
308.2251 40.8734 21.7 27.1 39.6 4.5133 0.5 7.1 Cyg X-3
326.3536 38.3190 7.6 37.7 57.4 32.1467 1.5 8.6 Cyg X-2
316.1950 38.5092 2.4 30.5 51.3 56.4905 4.7 ------ UNKNOWN
312.8015 2.8119 3.7 29.4 127.3 35.1769 3.2 ------ UNKNOWN
288.2647 19.7690 0.3 0.0 149.1 227.1049 33.6 ------ UNKNOWN
254.7523 -15.0946 3.4 48.0 -129.1 109.2544 3.4 ------ UNKNOWN
238.9625 32.8557 2.3 45.6 -57.9 158.5431 5.0 ------ UNKNOWN
Plot creation:
Sat Nov 4 12:09:47 EDT 2023