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
290.1988 52.4401 0.0044 35.1232 -144.9016 4.4318596 43.943 TRIG_01195887
Foreground time interval of the image:
-5.320 13.237 (delta_t = 18.557 [sec])
Background time interval of the image:
-239.064 -5.320 (delta_t = 233.744 [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 -5.320 sec. to 40.340 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57969 ( -0.0701956 0.0704107 )
Norm@50keV : 7.86962E-03 ( -0.000309696 0.000309378 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.71 using 59 bins.
Reduced chi-squared = 0.942281
# Null hypothesis probability of 5.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 45.66 sec: 1.00506 ( -0.041645 0.04174 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.3695e-06 ( -1.40667e-07 1.41134e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.320 sec. to 40.340 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18279 ( -0.301273 0.281534 )
Epeak [keV] : 106.394 ( -25.4217 123.17 )
Norm@50keV : 1.22841E-02 ( -0.00325353 0.00480189 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.77 using 59 bins.
Reduced chi-squared = 0.853036
# Null hypothesis probability of 7.75e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 45.66 sec: 0.981459 ( -0.044619 0.044701 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.26535e-06 ( -1.51786e-07 1.60173e-07 ) ergs/cm2
Band function
Time interval is from -5.320 sec. to 40.340 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] : 15.0450 ( )
R^2/D10^2 : 0.108847 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 173.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.00e-13 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.354e-07 1.833e-08
25- 50 9.379e-07 4.908e-08
50-150 1.447e-06 1.123e-07
15-150 2.620e-06 1.221e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 194.601 (-38.1614 -194.035)
Norm : 4.07417 (-0.166067 0.184362)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.99e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.639e-07 2.710e-08
25- 50 8.912e-07 5.822e-08
50-150 1.947e-06 4.564e-07
15-150 3.302e-06 5.573e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.56530 (-1.10557 1.16605)
R1^2/D10^2 : 0.790570 (-0.287573 0.546468)
kT2 [keV] : 26.3172 (-3.63927 5.48928)
R2^2/D10^2 : 1.13710E-02 (-0.00569516 0.00881807)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.42e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.180e-07 5.666e-08
25- 50 9.196e-07 9.908e-08
50-150 1.922e-06 2.956e-07
15-150 3.260e-06 3.609e-07
Peak spectrum fit
Power-law model
Time interval is from 0.068 sec. to 1.068 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55624 ( -0.169486 0.172355 )
Norm@50keV : 2.14502E-02 ( -0.00231602 0.00229796 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.85 using 59 bins.
Reduced chi-squared = 1.17281
# Null hypothesis probability of 1.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.72048 ( -0.2835 0.28371 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01786e-07 ( -2.34496e-08 2.36431e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.068 sec. to 1.068 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00867 ( -0.788987 0.619359 )
Epeak [keV] : 88.0603 ( -27.7553 -88.0605 )
Norm@50keV : 4.14900E-02 ( -0.0212228 0.0639227 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.91 using 59 bins.
Reduced chi-squared = 1.15911
# Null hypothesis probability of 1.94e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.67765 ( -0.28981 0.28905 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.94639e-07 ( -2.52676e-08 2.53141e-08 ) ergs/cm2
Band function
Time interval is from 0.068 sec. to 1.068 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] : 13.9684 (-1.65412 1.93204)
R^2/D10^2 : 0.403146 (-0.150227 0.229926)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.39e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.662e-08 3.330e-09
25- 50 6.167e-08 9.215e-09
50-150 7.914e-08 1.699e-08
15-150 1.574e-07 2.135e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 190.957 (-75.0501 -191.144)
Norm : 11.1740 (-1.16575 1.30703)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.783e-08 1.543e-08
25- 50 5.350e-08 2.882e-08
50-150 1.172e-07 6.300e-08
15-150 1.985e-07 1.081e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.22717 (-2.9374 3.25368)
R1^2/D10^2 : 2.49243 (-1.64525 12.6106)
kT2 [keV] : 24.2723 (-7.12288 24.3098)
R2^2/D10^2 : 4.20032E-02 (-0.038108 0.125021)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.53e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.596e-08 1.330e-08
25- 50 5.582e-08 2.178e-08
50-150 1.128e-07 5.864e-08
15-150 1.946e-07 9.146e-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: 1.59460 ( -0.0608819 0.0610936 )
Norm@50keV : 1.57249E-02 ( -0.000552561 0.000552124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.72e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.56 sec: 2.01737 ( -0.0747523 0.0749079 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.73127e-06 ( -1.01176e-07 1.0137e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.893384 ( -0.285975 0.268656 )
Epeak [keV] : 81.7359 ( -10.3419 19.7194 )
Norm@50keV : 3.44350E-02 ( -0.00874579 0.0126224 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.30e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.56 sec: 1.93784 ( -0.07973 0.07993 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.61148e-06 ( -1.11527e-07 1.11434e-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) = 8.68e-07
S(50-100 keV) = 1.16e-06
T90 vs. Hardness ratio plot
T90 = 34.0759998559952 sec.
Hardness ratio (energy fluence ratio) = 1.33641
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.363
Count Ratio (50-100 keV) / (15-25 keV) = 1.01973
Mask shadow pattern
IMX = -5.755117822250061E-01, IMY = 4.044529944815041E-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:
-239.064000 -5.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6142 35.1948 1.3 51.0 -159.0 8.0134 8.7 1.2 Cyg X-1
308.2034 40.9745 5.2 44.3 -167.0 1.3981 2.2 4.4 Cyg X-3
326.0531 38.3853 5.4 45.3 173.2 1.7871 2.1 6.8 Cyg X-2
341.7406 50.7953 2.6 32.1 156.9 2.4059 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.320000 13.236590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6924 35.2691 5.4 50.9 -159.1 -0.4039 -2.1 6.4 Cyg X-1
307.9560 41.0976 5.1 44.2 -166.7 0.2605 2.3 11.2 Cyg X-3
326.2554 38.1584 5.5 45.5 172.9 -0.3026 -2.1 10.6 Cyg X-2
77.6332 44.7854 2.6 44.6 50.7 1.4478 4.5 ------ UNKNOWN
0.6335 66.7972 2.3 15.8 133.2 0.3723 5.1 ------ UNKNOWN
124.3693 45.3621 2.5 49.5 6.2 0.9749 4.6 ------ UNKNOWN
290.1988 52.4401 0.3 35.1 -144.9 4.4317 43.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
87.236590 401.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4395 35.3926 5.6 30.5 -78.4 1.3850 2.1 3.1 Her X-1
288.7725 10.9959 6.8 41.5 -146.5 -1.4142 -1.7 3.4 GRS 1915+105
299.6205 35.1989 0.5 18.5 -173.4 11.5476 22.3 1.5 Cyg X-1
308.1290 40.9178 7.6 16.8 157.8 0.8168 1.5 2.3 Cyg X-3
326.1920 38.3208 192.7 28.5 136.6 0.0409 0.1 1.0 Cyg X-2
34.0694 74.1259 3.2 43.7 53.9 7.3578 3.6 ------ UNKNOWN
309.6326 34.5486 2.5 22.6 166.0 2.3332 4.6 ------ UNKNOWN
292.1352 53.2047 2.8 1.4 87.4 2.0903 4.2 ------ UNKNOWN
312.7755 -3.1664 2.1 58.8 -175.2 11.8019 5.4 ------ UNKNOWN
233.6059 33.1846 2.3 44.4 -61.2 10.9472 4.9 ------ UNKNOWN
Plot creation:
Tue Dec 26 22:40:49 EST 2023