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
251.8539 43.7419 0.0119 40.7678 172.7360 2.4382257 16.099 TRIG_00932742
Foreground time interval of the image:
-21.244 25.101 (delta_t = 46.345 [sec])
Background time interval of the image:
-239.200 -21.244 (delta_t = 217.956 [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 -21.244 sec. to 143.504 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73237 ( -0.17918 0.185004 )
Norm@50keV : 1.22423E-03 ( -0.000136717 0.000134527 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.79 using 59 PHA bins.
# Reduced chi-squared = 0.7857 for 57 degrees of freedom
# Null hypothesis probability = 8.798239e-01
Photon flux (15-150 keV) in 164.7 sec: 0.164481 ( -0.016657 0.016673 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86279e-06 ( -2.14993e-07 2.17738e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -21.244 sec. to 143.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44117 ( -0.803572 0.457351 )
Epeak [keV] : 89.6449 ( -66.0262 -89.6454 )
Norm@50keV : 1.75281E-03 ( -0.00065068 0.00290102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.29 using 59 PHA bins.
# Reduced chi-squared = 0.7910 for 56 degrees of freedom
# Null hypothesis probability = 8.707625e-01
Photon flux (15-150 keV) in 164.7 sec: 0.162433 ( -0.017417 0.017349 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81625e-06 ( -2.42577e-07 2.4331e-07 ) ergs/cm2
Band function
Time interval is from -21.244 sec. to 143.504 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] : 12.3750 (-1.53339 1.76617)
R^2/D10^2 : 3.53037E-02 (-0.0136359 0.0220737)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.30 using 59 PHA bins.
# Reduced chi-squared = 1.181 for 57 degrees of freedom
# Null hypothesis probability = 1.650517e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.887e-07 3.314e-08
25- 50 6.154e-07 8.614e-08
50-150 5.781e-07 1.323e-07
15-150 1.382e-06 1.996e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 119.841 (-43.6985 -123.567)
Norm : 0.700050 (-0.0870712 0.105439)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.41 using 59 PHA bins.
# Reduced chi-squared = 0.7791 for 57 degrees of freedom
# Null hypothesis probability = 8.878889e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.936e-07 4.010e-08
25- 50 5.298e-07 8.663e-08
50-150 9.694e-07 4.678e-07
15-150 1.793e-06 5.637e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.51269 (-2.13919 2.33851)
R1^2/D10^2 : 0.244350 (-0.152428 0.799465)
kT2 [keV] : 22.8798 (-6.3627 17.9093)
R2^2/D10^2 : 2.77543E-03 (-0.00238774 0.00737472)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.30 using 59 PHA bins.
# Reduced chi-squared = 0.8236 for 55 degrees of freedom
# Null hypothesis probability = 8.215538e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.963e-07 1.398e-07
25- 50 5.350e-07 1.961e-07
50-150 9.578e-07 5.297e-07
15-150 1.789e-06 7.942e-07
Peak spectrum fit
Power-law model
Time interval is from -0.992 sec. to 0.008 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99275 ( -0.349767 0.395529 )
Norm@50keV : 8.85271E-03 ( -0.00237402 0.00228818 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.66 using 59 PHA bins.
# Reduced chi-squared = 0.7660 for 57 degrees of freedom
# Null hypothesis probability = 9.029700e-01
Photon flux (15-150 keV) in 1 sec: 1.32359 ( -0.27144 0.27145 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.16263e-08 ( -2.00916e-08 2.09106e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.992 sec. to 0.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.101245 ( -2.83976 1.85426 )
Epeak [keV] : 41.4038 ( -12.4523 24.6396 )
Norm@50keV : 0.109894 ( -0.109885 4.71651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.66 using 59 PHA bins.
# Reduced chi-squared = 0.7261 for 56 degrees of freedom
# Null hypothesis probability = 9.385814e-01
Photon flux (15-150 keV) in 1 sec: 1.25911 ( -0.276614 0.27782 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.17034e-08 ( -1.81595e-08 2.17984e-08 ) ergs/cm2
Band function
Time interval is from -0.992 sec. to 0.008 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] : 10.5032 (-2.03519 2.4253)
R^2/D10^2 : 0.545373 (-0.298025 0.673152)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.72 using 59 PHA bins.
# Reduced chi-squared = 0.7320 for 57 degrees of freedom
# Null hypothesis probability = 9.356405e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.244e-08 5.018e-09
25- 50 3.309e-08 1.179e-08
50-150 1.987e-08 9.717e-09
15-150 6.540e-08 2.311e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.4739 (-26.9181 67.3167)
Norm : 6.88776 (-1.90467 2.64292)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.70 using 59 PHA bins.
# Reduced chi-squared = 0.7316 for 57 degrees of freedom
# Null hypothesis probability = 9.360077e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.746e-08 5.045e-09
25- 50 2.702e-08 9.500e-09
50-150 3.219e-08 2.009e-08
15-150 7.667e-08 2.925e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.96940 (-2.93603 82.0969)
R1^2/D10^2 : 35.0600 (-51.4482 -51.4482)
kT2 [keV] : 11.8220 (-2.55205 -11.6376)
R2^2/D10^2 : 0.319487 (-0.341302 0.573247)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.78 using 59 PHA bins.
# Reduced chi-squared = 0.7232 for 55 degrees of freedom
# Null hypothesis probability = 9.390716e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.558e-08 7.695e-09
25- 50 3.002e-08 1.768e-08
50-150 2.426e-08 1.552e-08
15-150 6.986e-08 3.884e-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: 1.50835 ( -0.172895 0.174121 )
Norm@50keV : 3.21079E-03 ( -0.000317871 0.000316709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.93 using 59 PHA bins.
# Reduced chi-squared = 0.8409 for 57 degrees of freedom
# Null hypothesis probability = 7.983600e-01
Photon flux (15-150 keV) in 46.34 sec: 0.401740 ( -0.0405809 0.0407205 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40957e-06 ( -1.50892e-07 1.51922e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42436 ( -0.746174 1.33809 )
Epeak [keV] : 351.292 ( -351.47 -351.47 )
Norm@50keV : 3.53607E-03 ( -0.00353586 0.00462763 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.89 using 59 PHA bins.
# Reduced chi-squared = 0.8551 for 56 degrees of freedom
# Null hypothesis probability = 7.713624e-01
Photon flux (15-150 keV) in 46.34 sec: 0.400186 ( -0.042355 0.041764 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40233e-06 ( -1.65494e-07 8.09004e-08 ) 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) = 5.11e-07
S(50-100 keV) = 6.14e-07
T90 vs. Hardness ratio plot
T90 = 142.707999944687 sec.
Hardness ratio (energy fluence ratio) = 1.20157
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.25757
Count Ratio (50-100 keV) / (15-25 keV) = 0.853862
Mask shadow pattern
IMX = -8.552778944758745E-01, IMY = -1.090181345441954E-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:
-239.200000 -21.244000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5320 35.2186 7.4 44.9 -175.8 0.6850 1.6 8.3 Her X-1
167.8192 74.8565 3.1 40.8 98.2 3.4062 3.8 ------ UNKNOWN
242.8924 59.4919 2.6 36.4 146.8 1.8334 4.5 ------ UNKNOWN
201.9792 48.3628 2.7 12.0 121.6 1.0122 4.2 ------ UNKNOWN
198.2055 14.1752 2.8 22.5 -69.7 1.2728 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-21.244000 25.100600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5285 35.3413 17.6 44.8 -176.0 0.1084 0.7 3.5 Her X-1
251.8539 43.7420 0.7 40.8 172.7 2.4377 16.1 ------ UNKNOWN
268.9665 29.0539 2.1 58.5 -174.8 3.3659 5.5 ------ UNKNOWN
168.5541 0.5492 2.3 45.4 -25.8 0.8542 5.0 ------ UNKNOWN
201.4157 -4.5852 3.0 41.3 -74.7 1.4231 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
87.900590 962.870400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3138 35.2454 14.2 8.8 -140.5 0.7103 0.8 9.1 Her X-1
268.3414 -1.2973 0.0 47.4 -149.8 2.6407 1.1 9.5 SW J1753.5-0127
288.7902 11.0141 9.3 45.7 177.3 2.3947 1.2 4.1 GRS 1915+105
299.6028 35.2001 1.2 37.3 139.5 19.1964 10.0 0.6 Cyg X-1
308.1160 40.9302 9.0 40.9 126.7 4.0269 1.3 1.4 Cyg X-3
311.9691 37.4953 2.4 45.1 129.3 21.2015 4.7 ------ UNKNOWN
Plot creation:
Wed Nov 27 16:19:38 EST 2019