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
356.2546 82.6281 0.0087 38.7939 149.6650 2.3323629 22.126 TRIG_01195733
Foreground time interval of the image:
-1.404 15.076 (delta_t = 16.480 [sec])
Background time interval of the image:
-133.067 -1.404 (delta_t = 131.663 [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 2.048000
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 2.048000
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 2.048000
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 -1.404 sec. to 15.076 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40462 ( -0.120272 0.119653 )
Norm@50keV : 9.45068E-03 ( -0.000652983 0.000652254 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.79 using 59 bins.
Reduced chi-squared = 1.06649
# Null hypothesis probability of 3.41e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 16.48 sec: 1.15215 ( -0.08278 0.08296 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50369e-06 ( -1.1275e-07 1.13341e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.404 sec. to 15.076 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40148 ( -0.390268 0.169476 )
Epeak [keV] : 9997.54 ( -9997.42 -9997.42 )
Norm@50keV : 9.48489E-03 ( -0.000655329 0.00591799 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.79 using 59 bins.
Reduced chi-squared = 1.08554
# Null hypothesis probability of 3.08e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 16.48 sec: 1.15150 ( -0.0849 0.08376 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50223e-06 ( -1.19312e-07 1.14645e-07 ) ergs/cm2
Band function
Time interval is from -1.404 sec. to 15.076 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] : 16.9552 ( )
R^2/D10^2 : 8.55205E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 127.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.31e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.258e-08 1.177e-08
25- 50 3.646e-07 3.650e-08
50-150 7.477e-07 9.830e-08
15-150 1.195e-06 1.087e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-24.9844 -200)
Norm : 4.78271 (-0.33046 0.33046)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.84e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.963e-07 1.516e-08
25- 50 3.775e-07 3.494e-08
50-150 8.280e-07 2.469e-07
15-150 1.402e-06 2.422e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.00133 (-1.04587 1.25576)
R1^2/D10^2 : 1.28168 (-0.562267 1.02655)
kT2 [keV] : 32.0228 (-5.73263 9.64884)
R2^2/D10^2 : 8.33662E-03 (-0.00461708 0.00769939)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.52e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.875e-07 4.272e-08
25- 50 3.618e-07 7.770e-08
50-150 9.807e-07 3.050e-07
15-150 1.530e-06 3.804e-07
Peak spectrum fit
Power-law model
Time interval is from 0.636 sec. to 1.636 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.882562 ( -0.209456 0.200901 )
Norm@50keV : 2.78518E-02 ( -0.00339965 0.00336629 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.44 using 59 bins.
Reduced chi-squared = 0.937544
# Null hypothesis probability of 6.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.19647 ( -0.38754 0.38839 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.14746e-07 ( -3.94309e-08 3.95531e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.636 sec. to 1.636 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.731923 ( -0.86841 0.521211 )
Epeak [keV] : 501.777 ( -501.784 -501.784 )
Norm@50keV : 3.23943E-02 ( -0.00713674 0.0415057 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.33 using 59 bins.
Reduced chi-squared = 0.952321
# Null hypothesis probability of 5.77e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.18370 ( -0.3927 0.39093 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.13437e-07 ( -4.05015e-08 3.9218e-08 ) ergs/cm2
Band function
Time interval is from 0.636 sec. to 1.636 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] : 24.5527 (-3.74903 4.88944)
R^2/D10^2 : 8.47311E-02 (-0.0358565 0.0567242)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.958e-09 2.396e-09
25- 50 5.035e-08 1.023e-08
50-150 2.256e-07 4.090e-08
15-150 2.849e-07 4.575e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-22.8377 -200)
Norm : 12.7107 (-1.60258 1.60258)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.58e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.164e-08 1.794e-08
25- 50 6.086e-08 3.407e-08
50-150 1.335e-07 7.350e-08
15-150 2.260e-07 1.247e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.01450 (-4.08491 4.56675)
R1^2/D10^2 : 0.954817 (-0.709722 5.7345)
kT2 [keV] : 40.0663 (-13.3695 -40.4713)
R2^2/D10^2 : 1.69752E-02 (-0.0157289 0.0413473)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.41e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.863e-08 1.086e-08
25- 50 5.618e-08 3.032e-08
50-150 2.419e-07 1.305e-07
15-150 3.167e-07 1.630e-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: 1.40462 ( -0.120272 0.119653 )
Norm@50keV : 9.45068E-03 ( -0.000652983 0.000652254 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.41e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 16.48 sec: 1.15213 ( -0.0827754 0.0829557 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50351e-06 ( -1.12875e-07 1.13495e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40148 ( -0.392622 0.166577 )
Epeak [keV] : 9997.85 ( -9997.76 -9997.76 )
Norm@50keV : 9.48489E-03 ( -0.000655328 0.00591799 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.08e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 16.48 sec: 1.15107 ( -0.04327 0.08359 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50531e-06 ( -1.2125e-07 1.11365e-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) = 3.54e-07
S(50-100 keV) = 5.36e-07
T90 vs. Hardness ratio plot
T90 = 12.0119999647141 sec.
Hardness ratio (energy fluence ratio) = 1.51412
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28462
Count Ratio (50-100 keV) / (15-25 keV) = 1.14539
Mask shadow pattern
IMX = -6.937893841732251E-01, IMY = -4.059862301839708E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-133.067410 -1.404000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
168.3586 47.9006 3.0 10.9 -16.0 0.7631 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.404000 15.076000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.2546 82.6281 0.5 38.8 149.7 2.3323 22.1 ------ UNKNOWN
270.2835 79.2854 2.4 34.5 169.5 0.3322 4.7 ------ UNKNOWN
172.3993 45.5927 2.0 13.0 -30.4 0.2989 5.9 ------ UNKNOWN
220.7717 55.7642 2.3 25.9 -134.6 0.2994 5.0 ------ UNKNOWN
262.4749 42.2995 1.8 55.1 -145.1 1.7305 6.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Tue Dec 26 22:50:44 EST 2023