Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
253.5736 -54.0371 0.0023 35.8346 15.4028 54.2269690 82.207 TRIG_00850471
Foreground time interval of the image:
-0.244 36.512 (delta_t = 36.756 [sec])
Background time interval of the image:
-239.048 -0.244 (delta_t = 238.804 [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 0.512000
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 0.512000
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 0.512000
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 -0.244 sec. to 36.512 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97205 ( -0.0256499 0.0256071 )
Norm@50keV : 8.88207E-02 ( -0.00119416 0.00119252 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.77 using 59 PHA bins.
# Reduced chi-squared = 0.7854 for 57 degrees of freedom
# Null hypothesis probability = 8.801782e-01
Photon flux (15-150 keV) in 36.76 sec: 13.1557 ( -0.2603 0.2623 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.00764e-05 ( -4.1334e-07 4.12793e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.244 sec. to 36.512 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90825 ( -0.102503 0.100381 )
Epeak [keV] : 88.3366 ( -24.6494 -88.3366 )
Norm@50keV : 9.42692E-02 ( -0.00443166 0.00919912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.61 using 59 PHA bins.
# Reduced chi-squared = 0.7787 for 56 degrees of freedom
# Null hypothesis probability = 8.861206e-01
Photon flux (15-150 keV) in 36.76 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.99361e-05 ( -4.63731e-07 4.65404e-07 ) ergs/cm2
Band function
Time interval is from -0.244 sec. to 36.512 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] : 16.8298 ( )
R^2/D10^2 : 0.737116 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1653.59 using 59 PHA bins.
# Reduced chi-squared = 29.0103 for 57 degrees of freedom
# Null hypothesis probability = 2.585130e-308
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.567e-06 4.650e-08
25- 50 6.879e-06 1.581e-07
50-150 1.387e-05 2.371e-07
15-150 2.231e-05 3.235e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 117.127 ( )
Norm : 49.0230 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 144.97 using 59 PHA bins.
# Reduced chi-squared = 2.5434 for 57 degrees of freedom
# Null hypothesis probability = 1.317447e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.698e-06 2.059e-07
25- 50 8.369e-06 2.665e-07
50-150 1.476e-05 2.709e-06
15-150 2.782e-05 2.840e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.17230 (-0.291706 0.300932)
R1^2/D10^2 : 14.7980 (-2.29254 2.79229)
kT2 [keV] : 26.2552 (-0.942663 1.0405)
R2^2/D10^2 : 0.106260 (-0.0153655 0.0170057)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.78 using 59 PHA bins.
# Reduced chi-squared = 1.032 for 55 degrees of freedom
# Null hypothesis probability = 4.083369e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.063e-06 2.757e-07
25- 50 9.258e-06 2.261e-07
50-150 1.461e-05 2.941e-07
15-150 2.893e-05 4.889e-07
Peak spectrum fit
Power-law model
Time interval is from 12.612 sec. to 13.612 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87901 ( -0.0310338 0.0310366 )
Norm@50keV : 0.925161 ( -0.0147612 0.0147553 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.73 using 59 PHA bins.
# Reduced chi-squared = 0.7496 for 57 degrees of freedom
# Null hypothesis probability = 9.199135e-01
Photon flux (15-150 keV) in 1 sec: 131.611 ( -2.854 2.872 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.50629e-06 ( -1.35624e-07 1.35625e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 12.612 sec. to 13.612 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85975 ( -0.119846 0.0478875 )
Epeak [keV] : 430.784 ( )
Norm@50keV : 0.942773 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.65 using 59 PHA bins.
# Reduced chi-squared = 0.7616 for 56 degrees of freedom
# Null hypothesis probability = 9.056243e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.07477e-06 ( -2.54171e-07 1.45231e-06 ) ergs/cm2
Band function
Time interval is from 12.612 sec. to 13.612 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] : 16.2191 ( )
R^2/D10^2 : 9.09305 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1163.64 using 59 PHA bins.
# Reduced chi-squared = 20.4147 for 57 degrees of freedom
# Null hypothesis probability = 4.102586e-206
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.930e-07 1.870e-08
25- 50 2.099e-06 5.200e-08
50-150 3.879e-06 9.200e-08
15-150 6.471e-06 1.065e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 122.262 (-10.3829 6.65436)
Norm : 517.679 (-11.6077 19.623)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 97.88 using 59 PHA bins.
# Reduced chi-squared = 1.717 for 57 degrees of freedom
# Null hypothesis probability = 6.164894e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.347e-06 6.450e-08
25- 50 2.418e-06 8.250e-08
50-150 4.355e-06 8.350e-07
15-150 8.120e-06 8.625e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.17195 (-0.353657 0.368003)
R1^2/D10^2 : 147.077 (-26.2534 33.1724)
kT2 [keV] : 27.1012 (-1.2889 1.46248)
R2^2/D10^2 : 1.04899 (-0.192405 0.220446)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.50 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 55 degrees of freedom
# Null hypothesis probability = 3.825878e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.374e-06 7.750e-08
25- 50 2.542e-06 7.000e-08
50-150 4.372e-06 1.205e-07
15-150 8.288e-06 1.890e-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: 1.97205 ( -0.0256499 0.0256071 )
Norm@50keV : 8.88207E-02 ( -0.00119416 0.00119252 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.77 using 59 PHA bins.
# Reduced chi-squared = 0.7854 for 57 degrees of freedom
# Null hypothesis probability = 8.801782e-01
Photon flux (15-150 keV) in 36.76 sec: 13.1548 ( -0.260311 0.26219 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.00707e-05 ( -4.12962e-07 4.13517e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90825 ( -0.102503 0.100381 )
Epeak [keV] : 88.3366 ( -24.6482 -88.3366 )
Norm@50keV : 9.42692E-02 ( -0.00443167 0.00919912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.61 using 59 PHA bins.
# Reduced chi-squared = 0.7787 for 56 degrees of freedom
# Null hypothesis probability = 8.861206e-01
Photon flux (15-150 keV) in 36.76 sec: 13.0280 ( -0.3197 0.2181 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.99444e-05 ( -4.63654e-07 4.13954e-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) = 8.97e-06
S(50-100 keV) = 9.15e-06
T90 vs. Hardness ratio plot
T90 = 8.6839998960495 sec.
Hardness ratio (energy fluence ratio) = 1.02007
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.09912
Count Ratio (50-100 keV) / (15-25 keV) = 0.644504
Mask shadow pattern
IMX = 6.962036737757912E-01, IMY = -1.918027696107422E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.048000 -0.244000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4255 -60.5979 4.3 38.1 -58.2 1.3658 2.7 3.6 Cen X-3
187.0866 -62.7626 5.9 35.2 -45.4 0.6663 2.0 11.8 GX 301-2
255.7995 -37.8456 27.7 51.3 23.0 -0.4271 -0.4 8.9 4U 1700-377
256.3260 -36.4822 472.7 52.5 23.8 -0.0318 -0.0 6.4 GX 349+2
264.9325 -44.5267 4.3 43.3 30.3 1.3736 2.7 9.3 4U 1735-44
242.8767 -55.0027 3.2 36.5 4.8 1.0866 3.6 ------ UNKNOWN
40.1307 -29.7518 2.4 56.6 179.4 7.6049 4.9 ------ UNKNOWN
232.7111 -52.9952 3.0 40.0 -3.7 1.3410 3.9 ------ UNKNOWN
198.4931 -57.1114 2.7 39.9 -34.8 1.5030 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.244000 36.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.5722 -60.7150 5.4 38.0 -58.1 -1.9348 -2.1 9.3 Cen X-3
186.4298 -62.8662 11.9 35.1 -46.0 0.6778 1.0 8.5 GX 301-2
255.9977 -37.9992 0.0 51.1 23.1 -4.4594 -2.3 9.3 4U 1700-377
256.4452 -36.4173 58.9 52.6 24.0 -0.4806 -0.2 0.6 GX 349+2
264.7000 -44.3878 10.3 43.5 30.1 1.1272 1.1 4.2 4U 1735-44
263.1401 -39.3924 2.4 48.6 29.9 8.1810 4.9 ------ UNKNOWN
23.2101 -29.4146 3.4 54.7 161.7 9.3500 3.3 ------ UNKNOWN
8.2038 -45.8874 2.7 36.7 148.4 3.2834 4.3 ------ UNKNOWN
26.8714 -29.5259 4.1 55.0 165.6 8.1146 2.8 ------ UNKNOWN
253.5736 -54.0371 0.1 35.8 15.4 54.2226 82.2 ------ UNKNOWN
56.9199 -65.1766 2.9 24.8 -149.4 1.7751 4.0 ------ UNKNOWN
62.5960 -33.4069 3.5 56.4 -157.2 7.9249 3.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
186.452590 459.052600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4000 -60.6089 2.4 36.3 -45.4 2.1455 4.8 2.6 Cen X-3
186.7483 -62.6312 6.3 34.4 -32.0 0.6022 1.8 8.7 GX 301-2
264.9515 -44.4220 4.4 47.1 40.2 2.7430 2.6 9.1 4U 1735-44
357.6996 -37.1702 3.0 45.8 138.8 3.9838 3.9 ------ UNKNOWN
277.4681 -56.4403 2.8 33.8 48.7 1.8010 4.1 ------ UNKNOWN
228.0206 -45.5413 2.3 49.7 5.5 2.8634 4.9 ------ UNKNOWN
21.1488 -67.5923 2.7 15.8 170.2 1.1026 4.3 ------ UNKNOWN
67.7953 -32.1733 3.0 55.0 -146.1 6.6082 3.8 ------ UNKNOWN
Plot creation:
Fri Oct 26 12:45:57 EDT 2018