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
77.9618 -62.3194 0.0132 29.6528 -103.8504 4.3238461 14.555 TRIG_00831816
Foreground time interval of the image:
-19.920 137.104 (delta_t = 157.024 [sec])
Background time interval of the image:
-239.200 -19.920 (delta_t = 219.280 [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 -19.920 sec. to 137.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.01391 ( -0.168211 0.175944 )
Norm@50keV : 1.46460E-03 ( -0.000167575 0.000164254 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.25 using 59 PHA bins.
# Reduced chi-squared = 0.8113 for 57 degrees of freedom
# Null hypothesis probability = 8.449724e-01
Photon flux (15-150 keV) in 157 sec: 0.221123 ( -0.020023 0.020033 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.12251e-06 ( -2.25548e-07 2.29715e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.920 sec. to 137.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57317 ( -0.86097 0.504956 )
Epeak [keV] : 39.6227 ( )
Norm@50keV : 2.65336E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.09 using 59 PHA bins.
# Reduced chi-squared = 0.8052 for 56 degrees of freedom
# Null hypothesis probability = 8.513575e-01
Photon flux (15-150 keV) in 157 sec: 0.217285 ( -0.02095 0.020906 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01981e-06 ( -2.74667e-07 2.78881e-07 ) ergs/cm2
Band function
Time interval is from -19.920 sec. to 137.104 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] : 9.05669 (-0.893313 1.02208)
R^2/D10^2 : 0.149595 (-0.0514345 0.0758044)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.78 using 59 PHA bins.
# Reduced chi-squared = 1.119 for 57 degrees of freedom
# Null hypothesis probability = 2.504768e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.763e-07 5.919e-08
25- 50 8.076e-07 9.326e-08
50-150 3.141e-07 8.337e-08
15-150 1.498e-06 1.731e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.3167 (-15.7206 24.1885)
Norm : 1.12853 (-0.166795 0.192501)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.29 using 59 PHA bins.
# Reduced chi-squared = 0.7946 for 57 degrees of freedom
# Null hypothesis probability = 8.682871e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.490e-07 6.107e-08
25- 50 6.944e-07 6.916e-08
50-150 8.256e-07 1.866e-07
15-150 1.969e-06 2.347e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.03495 (-1.05259 1.0834)
R1^2/D10^2 : 0.335401 (-0.135728 0.231528)
kT2 [keV] : 30.2749 (-10.3909 31.3203)
R2^2/D10^2 : 9.65667E-04 (-0.000835185 0.00343847)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.63 using 59 PHA bins.
# Reduced chi-squared = 0.7023 for 55 degrees of freedom
# Null hypothesis probability = 9.539920e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.424e-07 9.930e-08
25- 50 7.157e-07 2.191e-07
50-150 9.617e-07 4.995e-07
15-150 2.120e-06 6.722e-07
Peak spectrum fit
Power-law model
Time interval is from 0.964 sec. to 1.964 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66318 ( -0.345225 0.360384 )
Norm@50keV : 9.28494E-03 ( -0.00206269 0.00201206 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.68 using 59 PHA bins.
# Reduced chi-squared = 1.275 for 57 degrees of freedom
# Null hypothesis probability = 7.874071e-02
Photon flux (15-150 keV) in 1 sec: 1.21775 ( -0.249739 0.25004 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.62561e-08 ( -1.98619e-08 2.02464e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.964 sec. to 1.964 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33604 ( -1.45794 0.94639 )
Epeak [keV] : 95.4111 ( -95.4111 -95.4111 )
Norm@50keV : 1.39286E-02 ( -0.0139286 0.0703357 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.47 using 59 PHA bins.
# Reduced chi-squared = 1.294 for 56 degrees of freedom
# Null hypothesis probability = 6.853521e-02
Photon flux (15-150 keV) in 1 sec: 1.20599 ( -0.253492 0.25354 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.41395e-08 ( -2.12845e-08 2.12895e-08 ) ergs/cm2
Band function
Time interval is from 0.964 sec. to 1.964 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] : 12.5196 (-3.62021 5.14611)
R^2/D10^2 : 0.253642 (-0.177382 0.622193)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.25 using 59 PHA bins.
# Reduced chi-squared = 1.408 for 57 degrees of freedom
# Null hypothesis probability = 2.289175e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.429e-09 3.917e-09
25- 50 2.785e-08 1.064e-08
50-150 2.698e-08 1.408e-08
15-150 6.326e-08 2.219e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 153.440 (-86.5297 -150.81)
Norm : 5.01308 (-1.08857 1.61585)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.48 using 59 PHA bins.
# Reduced chi-squared = 1.272 for 57 degrees of freedom
# Null hypothesis probability = 8.111162e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.285e-08 7.350e-09
25- 50 2.390e-08 1.339e-08
50-150 4.761e-08 2.882e-08
15-150 8.436e-08 4.933e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.58206 (-2.19386 2.84055)
R1^2/D10^2 : 1.90480 (-1.37875 6.54042)
kT2 [keV] : 26.3684 (-22.0474 37.926)
R2^2/D10^2 : 1.33204E-02 (-0.0123093 0.0322005)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.66 using 59 PHA bins.
# Reduced chi-squared = 1.285 for 55 degrees of freedom
# Null hypothesis probability = 7.592168e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.394e-08 8.250e-09
25- 50 2.411e-08 1.295e-08
50-150 4.847e-08 2.713e-08
15-150 8.652e-08 4.549e-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: 2.01391 ( -0.168211 0.175944 )
Norm@50keV : 1.46460E-03 ( -0.000167575 0.000164254 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.25 using 59 PHA bins.
# Reduced chi-squared = 0.8113 for 57 degrees of freedom
# Null hypothesis probability = 8.449724e-01
Photon flux (15-150 keV) in 157 sec: 0.221107 ( -0.0200213 0.0200303 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.12214e-06 ( -2.25851e-07 2.29748e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57452 ( -0.861438 0.569123 )
Epeak [keV] : 39.6405 ( )
Norm@50keV : 2.64809E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.09 using 59 PHA bins.
# Reduced chi-squared = 0.8052 for 56 degrees of freedom
# Null hypothesis probability = 8.513575e-01
Photon flux (15-150 keV) in 157 sec: 0.217234 ( -0.020941 0.020898 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02031e-06 ( -2.74828e-07 2.79146e-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) = 6.42e-07
S(50-100 keV) = 6.36e-07
T90 vs. Hardness ratio plot
T90 = 134.016000032425 sec.
Hardness ratio (energy fluence ratio) = 0.990654
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.24403
Count Ratio (50-100 keV) / (15-25 keV) = 0.571804
Mask shadow pattern
IMX = -1.362833035213309E-01, IMY = 5.527449941697828E-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 -19.920000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5219 -40.5346 1.5 27.1 -11.7 1.7423 7.5 1.2 Vela X-1
170.2985 -60.6388 1.1 10.7 79.8 2.1104 10.5 1.1 Cen X-3
186.5890 -62.7958 2.3 15.9 107.0 1.1129 5.0 2.4 GX 301-2
243.7065 -54.9592 2.3 42.7 135.2 3.1878 5.0 ------ UNKNOWN
215.3151 -62.6933 1.1 27.0 126.3 3.0266 10.8 ------ UNKNOWN
296.8690 -66.7000 3.1 44.8 175.1 1.6668 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.920000 137.104000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5888 -40.6253 6.0 27.0 -11.6 0.3952 1.9 5.0 Vela X-1
169.9351 -60.6039 5.1 10.6 79.0 -0.3914 -2.3 11.3 Cen X-3
187.0189 -62.7230 7.8 16.1 107.1 0.2959 1.5 10.3 GX 301-2
241.0123 -54.4339 2.4 42.2 132.9 2.6371 4.8 ------ UNKNOWN
210.8343 -59.1936 2.4 27.5 117.3 1.2840 4.8 ------ UNKNOWN
77.9618 -62.3194 0.8 29.7 -103.9 4.3238 14.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Thu May 31 18:04:47 EDT 2018