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
351.4909 54.8841 0.0033 31.2759 145.8693 16.4541058 57.649 TRIG_00887579
Foreground time interval of the image:
-6.520 9.997 (delta_t = 16.517 [sec])
Background time interval of the image:
-234.104 -6.520 (delta_t = 227.584 [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 -6.520 sec. to 54.128 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28654 ( -0.0382842 0.0381907 )
Norm@50keV : 2.07190E-02 ( -0.000419367 0.000418838 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.72 using 59 PHA bins.
# Reduced chi-squared = 0.8547 for 57 degrees of freedom
# Null hypothesis probability = 7.744700e-01
Photon flux (15-150 keV) in 60.65 sec: 2.46583 ( -0.05557 0.05573 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24604e-05 ( -2.56681e-07 2.56819e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.520 sec. to 54.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16630 ( -0.155335 0.123463 )
Epeak [keV] : 414.106 ( -197.924 -414.106 )
Norm@50keV : 2.32831E-02 ( -0.0027235 0.00368067 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.87 using 59 PHA bins.
# Reduced chi-squared = 0.8370 for 56 degrees of freedom
# Null hypothesis probability = 8.024540e-01
Photon flux (15-150 keV) in 60.65 sec: 2.44312 ( -0.06176 0.06203 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23849e-05 ( -2.73829e-07 2.73315e-07 ) ergs/cm2
Band function
Time interval is from -6.520 sec. to 54.128 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] : 20.1413 ( )
R^2/D10^2 : 0.105144 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 502.90 using 59 PHA bins.
# Reduced chi-squared = 8.8228 for 57 degrees of freedom
# Null hypothesis probability = 1.261256e-72
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.973e-07 2.208e-08
25- 50 2.489e-06 8.461e-08
50-150 7.491e-06 2.214e-07
15-150 1.048e-05 2.547e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 10.5731 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 226.87 using 59 PHA bins.
# Reduced chi-squared = 3.9803 for 57 degrees of freedom
# Null hypothesis probability = 3.989641e-22
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.597e-06 3.487e-08
25- 50 3.072e-06 6.975e-08
50-150 6.737e-06 1.456e-07
15-150 1.141e-05 2.547e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.46404 (-0.729935 0.7736)
R1^2/D10^2 : 1.13901 (-0.275531 0.396118)
kT2 [keV] : 33.3740 (-2.6306 3.3609)
R2^2/D10^2 : 1.65368E-02 (-0.00450017 0.00534468)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.11 using 59 PHA bins.
# Reduced chi-squared = 1.020 for 55 degrees of freedom
# Null hypothesis probability = 4.329504e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.094e-06 8.946e-08
25- 50 2.841e-06 1.186e-07
50-150 8.426e-06 4.458e-07
15-150 1.236e-05 4.458e-07
Peak spectrum fit
Power-law model
Time interval is from 4.864 sec. to 5.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10251 ( -0.0504505 0.0503219 )
Norm@50keV : 0.259034 ( -0.00741892 0.00741594 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.37 using 59 PHA bins.
# Reduced chi-squared = 1.112 for 57 degrees of freedom
# Null hypothesis probability = 2.619619e-01
Photon flux (15-150 keV) in 1 sec: 1.16024 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.70639e-06 ( -8.41647e-08 8.42897e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 4.864 sec. to 5.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.758025 ( -0.210817 0.201403 )
Epeak [keV] : 210.390 ( -57.869 199.937 )
Norm@50keV : 0.366799 ( -0.0659268 0.0842303 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.58 using 59 PHA bins.
# Reduced chi-squared = 0.9747 for 56 degrees of freedom
# Null hypothesis probability = 5.287088e-01
Photon flux (15-150 keV) in 1 sec: 29.5863 ( -0.9258 0.9269 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66876e-06 ( -8.83424e-08 8.80701e-08 ) ergs/cm2
Band function
Time interval is from 4.864 sec. to 5.864 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] : 21.0208 ( )
R^2/D10^2 : 1.21838 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 239.90 using 59 PHA bins.
# Reduced chi-squared = 4.2088 for 57 degrees of freedom
# Null hypothesis probability = 2.701086e-24
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.017e-07 6.170e-09
25- 50 5.229e-07 2.225e-08
50-150 1.722e-06 7.550e-08
15-150 2.347e-06 7.900e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 124.462 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 279.05 using 59 PHA bins.
# Reduced chi-squared = 4.8956 for 57 degrees of freedom
# Null hypothesis probability = 5.235570e-31
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.099e-07 9.800e-09
25- 50 5.962e-07 1.945e-08
50-150 1.307e-06 4.150e-08
15-150 2.214e-06 6.550e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.66943 (-1.1297 1.2565)
R1^2/D10^2 : 10.9107 (-3.4899 5.79171)
kT2 [keV] : 33.2577 (-3.39425 4.8335)
R2^2/D10^2 : 0.235626 (-0.0852677 0.10431)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.55 using 59 PHA bins.
# Reduced chi-squared = 0.9919 for 55 degrees of freedom
# Null hypothesis probability = 4.916736e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.946e-07 2.120e-08
25- 50 5.584e-07 4.470e-08
50-150 1.933e-06 1.685e-07
15-150 2.686e-06 2.010e-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: 1.21971 ( -0.0350456 0.0349571 )
Norm@50keV : 6.51314E-02 ( -0.00123544 0.00123411 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.25 using 59 PHA bins.
# Reduced chi-squared = 0.8114 for 57 degrees of freedom
# Null hypothesis probability = 8.449350e-01
Photon flux (15-150 keV) in 16.52 sec: 7.66698 ( -0.159452 0.159841 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08564e-05 ( -2.07531e-07 2.07584e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06057 ( -0.142904 0.138453 )
Epeak [keV] : 360.963 ( -140.387 1607.57 )
Norm@50keV : 7.57541E-02 ( -0.00812721 0.010713 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.41 using 59 PHA bins.
# Reduced chi-squared = 0.7573 for 56 degrees of freedom
# Null hypothesis probability = 9.100842e-01
Photon flux (15-150 keV) in 16.52 sec: 7.57871 ( -0.17473 0.17586 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07912e-05 ( -2.17519e-07 2.17007e-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) = 2.75e-06
S(50-100 keV) = 4.51e-06
T90 vs. Hardness ratio plot
T90 = 26.3239998817444 sec.
Hardness ratio (energy fluence ratio) = 1.64
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.54365
Count Ratio (50-100 keV) / (15-25 keV) = 1.40173
Mask shadow pattern
IMX = -5.028088987541257E-01, IMY = -3.408205251257561E-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:
-234.104000 -6.520000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4106 35.3527 3.6 41.8 16.0 1.6293 3.2 2.4 Her X-1
268.1581 -1.3831 5.7 56.0 -33.1 3.1148 2.1 13.3 SW J1753.5-0127
288.8638 10.9812 3.2 34.8 -49.4 1.4901 3.6 4.4 GRS 1915+105
299.5850 35.2042 0.4 9.1 -34.5 8.6133 31.7 0.3 Cyg X-1
308.1571 40.9966 3.6 0.5 -93.7 0.7975 3.2 3.4 Cyg X-3
326.2146 38.4649 8.8 14.2 -167.5 0.3430 1.3 8.8 Cyg X-2
14.6638 44.4317 2.5 47.5 159.0 3.5478 4.6 ------ UNKNOWN
301.0053 61.2830 2.4 20.3 86.4 1.4215 4.7 ------ UNKNOWN
248.4909 25.9489 2.7 50.9 8.2 2.9938 4.3 ------ UNKNOWN
256.9440 8.8691 3.0 55.5 -14.8 3.2303 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.520000 9.996600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3173 35.2856 5.6 41.9 16.0 -0.6687 -2.1 7.7 Her X-1
268.4692 -1.5526 9.8 56.0 -33.6 -0.8675 -1.2 8.5 SW J1753.5-0127
288.6743 10.8856 5.4 35.0 -49.2 0.5496 2.1 8.1 GRS 1915+105
299.7406 35.3449 8.8 8.9 -34.4 0.2561 1.3 11.3 Cyg X-1
308.1783 40.8873 19.4 0.6 -93.4 0.0987 0.6 5.0 Cyg X-3
326.2712 38.3710 22.8 14.3 -167.2 0.0894 0.5 5.5 Cyg X-2
351.4909 54.8841 0.2 31.3 145.9 16.4544 57.7 ------ UNKNOWN
274.9067 16.4047 2.6 37.9 -25.2 1.0653 4.5 ------ UNKNOWN
3.9349 10.7277 2.9 57.6 -158.3 4.3618 3.9 ------ UNKNOWN
313.5476 1.0216 3.0 40.8 -92.2 2.3834 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.596600 967.930200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5597 35.2211 0.5 40.4 -40.3 31.6099 24.2 1.9 Cyg X-1
307.9164 41.0173 14.3 31.7 -40.8 0.8283 0.8 9.6 Cyg X-3
326.1593 38.2916 26.1 23.8 -66.9 -0.4520 -0.4 1.9 Cyg X-2
63.2936 52.8501 3.6 40.5 118.8 10.3647 3.3 ------ UNKNOWN
54.3426 33.8826 3.7 47.6 145.9 8.0863 3.1 ------ UNKNOWN
40.8338 61.4015 1.7 26.2 112.2 7.4540 6.9 ------ UNKNOWN
40.3918 50.4065 3.0 29.4 135.0 4.3387 3.8 ------ UNKNOWN
264.4833 51.0857 2.5 49.1 0.6 6.8167 4.7 ------ UNKNOWN
258.3714 44.1072 3.0 56.9 -2.1 11.0559 3.8 ------ UNKNOWN
291.0153 48.8435 2.9 36.6 -16.9 3.9289 4.0 ------ UNKNOWN
299.5635 24.5765 2.8 48.5 -50.2 15.9047 4.1 ------ UNKNOWN
Plot creation:
Thu Mar 21 16:35:36 EDT 2019