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
139.3868 -30.5229 0.0085 31.4838 25.8353 4.7420407 22.817 TRIG_00796100
Foreground time interval of the image:
-70.756 36.749 (delta_t = 107.505 [sec])
Background time interval of the image:
-239.352 -70.756 (delta_t = 168.596 [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 4.096000
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 4.096000
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 4.096000
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 -70.756 sec. to 228.436 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54110 ( -0.0672311 0.0673306 )
Norm@50keV : 2.57653E-03 ( -9.18242e-05 9.16898e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.44 using 59 PHA bins.
# Reduced chi-squared = 1.025 for 57 degrees of freedom
# Null hypothesis probability = 4.221448e-01
Photon flux (15-150 keV) in 299.2 sec: 0.325349 ( -0.012267 0.01231 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.2676e-06 ( -2.78332e-07 2.79354e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -70.756 sec. to 228.436 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48523 ( -0.279627 0.102274 )
Epeak [keV] : 469.016 ( -482.532 -482.532 )
Norm@50keV : 2.74269E-03 ( -0.000434642 0.000893344 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.31 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 56 degrees of freedom
# Null hypothesis probability = 3.905639e-01
Photon flux (15-150 keV) in 299.2 sec: 0.324141 ( -0.013374 0.006715 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.23439e-06 ( -3.0218e-07 2.8741e-07 ) ergs/cm2
Band function
Time interval is from -70.756 sec. to 228.436 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] : 15.3843 ( )
R^2/D10^2 : 3.19834E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 250.47 using 59 PHA bins.
# Reduced chi-squared = 4.3942 for 57 degrees of freedom
# Null hypothesis probability = 4.429202e-26
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.721e-07 3.411e-08
25- 50 1.919e-06 9.126e-08
50-150 3.126e-06 2.322e-07
15-150 5.517e-06 2.274e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-23.4971 -200)
Norm : 1.31884 (-0.0464261 0.0464261)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.38 using 59 PHA bins.
# Reduced chi-squared = 1.077 for 57 degrees of freedom
# Null hypothesis probability = 3.218949e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.829e-07 4.084e-08
25- 50 1.891e-06 7.166e-08
50-150 4.147e-06 1.631e-07
15-150 7.020e-06 2.887e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.24367 (-0.844571 0.926078)
R1^2/D10^2 : 0.311642 (-0.103139 0.170153)
kT2 [keV] : 28.6615 (-3.67103 5.38034)
R2^2/D10^2 : 2.94017E-03 (-0.00129382 0.00184419)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.22 using 59 PHA bins.
# Reduced chi-squared = 1.113 for 55 degrees of freedom
# Null hypothesis probability = 2.625640e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.295e-07 1.082e-07
25- 50 1.892e-06 1.535e-07
50-150 4.371e-06 5.715e-07
15-150 7.193e-06 6.612e-07
Peak spectrum fit
Power-law model
Time interval is from 79.516 sec. to 80.516 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44024 ( -0.191837 0.194826 )
Norm@50keV : 1.19317E-02 ( -0.0014136 0.00140137 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.84 using 59 PHA bins.
# Reduced chi-squared = 0.8393 for 57 degrees of freedom
# Null hypothesis probability = 8.010027e-01
Photon flux (15-150 keV) in 1 sec: 1.46692 ( -0.16637 0.16643 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14401e-07 ( -1.50985e-08 1.5302e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 79.516 sec. to 80.516 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.992719 ( -0.94697 0.547402 )
Epeak [keV] : 108.198 ( -46.1001 -108.221 )
Norm@50keV : 2.05166E-02 ( -0.00968408 0.0433367 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.90 using 59 PHA bins.
# Reduced chi-squared = 0.8375 for 56 degrees of freedom
# Null hypothesis probability = 8.017112e-01
Photon flux (15-150 keV) in 1 sec: 1.44323 ( -0.17273 0.17175 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09959e-07 ( -1.73443e-08 1.71452e-08 ) ergs/cm2
Band function
Time interval is from 79.516 sec. to 80.516 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] : 14.1482 (-1.85147 2.23199)
R^2/D10^2 : 0.208385 (-0.0834432 0.131754)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.46 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 57 degrees of freedom
# Null hypothesis probability = 3.861017e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.802e-09 1.849e-09
25- 50 3.308e-08 4.900e-09
50-150 4.384e-08 1.023e-08
15-150 8.572e-08 1.306e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-65.6094 -200)
Norm : 6.01559 (-0.678178 0.678178)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.76 using 59 PHA bins.
# Reduced chi-squared = 0.8379 for 57 degrees of freedom
# Null hypothesis probability = 8.033626e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.498e-08 7.842e-09
25- 50 2.882e-08 1.592e-08
50-150 6.320e-08 3.466e-08
15-150 1.070e-07 5.930e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.0329 (-5.25083 2.8227)
R1^2/D10^2 : 0.531999 (-0.285058 3.43255)
kT2 [keV] : 45.0166 (-43.5714 -48.5267)
R2^2/D10^2 : 2.83551E-03 (-0.00212351 0.070873)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.41 using 59 PHA bins.
# Reduced chi-squared = 0.8620 for 55 degrees of freedom
# Null hypothesis probability = 7.566814e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.160e-08 4.525e-09
25- 50 3.206e-08 1.368e-08
50-150 6.688e-08 3.564e-08
15-150 1.105e-07 4.962e-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: 1.36300 ( -0.102985 0.102379 )
Norm@50keV : 2.98773E-03 ( -0.000169184 0.000169119 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.19 using 59 PHA bins.
# Reduced chi-squared = 1.477 for 57 degrees of freedom
# Null hypothesis probability = 1.109833e-02
Photon flux (15-150 keV) in 107.5 sec: 0.360911 ( -0.0214124 0.0214712 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.12787e-06 ( -1.93949e-07 1.95112e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35961 ( -0.348557 0.150769 )
Epeak [keV] : 9997.80 ( -9997.77 -9997.77 )
Norm@50keV : 2.99917E-03 ( -0.00016972 0.00160241 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.19 using 59 PHA bins.
# Reduced chi-squared = 1.503 for 56 degrees of freedom
# Null hypothesis probability = 8.769986e-03
Photon flux (15-150 keV) in 107.5 sec: 0.360691 ( -0.022334 0.021425 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.13156e-06 ( -2.15097e-07 1.90329e-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) = 1.83e-06
S(50-100 keV) = 2.52e-06
T90 vs. Hardness ratio plot
T90 = 161.647999942303 sec.
Hardness ratio (energy fluence ratio) = 1.37705
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.35089
Count Ratio (50-100 keV) / (15-25 keV) = 1.00455
Mask shadow pattern
IMX = 5.512023442474684E-01, IMY = -2.668801861278758E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.352000 -70.756000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5297 -40.7496 171.0 39.7 13.9 -0.0179 -0.1 11.7 Vela X-1
170.3707 -60.6066 6.2 48.1 -26.9 0.6900 1.9 1.9 Cen X-3
186.5721 -62.8162 2.9 52.1 -35.9 2.8176 3.9 3.6 GX 301-2
156.6379 35.7167 2.2 49.3 143.6 4.6091 5.1 ------ UNKNOWN
188.1744 1.7534 2.6 25.1 -148.2 0.8783 4.4 ------ UNKNOWN
194.7405 -1.4848 2.3 29.3 -134.9 1.1028 5.1 ------ UNKNOWN
208.3997 28.3111 2.9 56.9 -161.3 4.1173 4.0 ------ UNKNOWN
204.9182 -39.1996 2.2 42.5 -69.2 3.8853 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-70.756000 36.748590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5142 -40.4060 34.3 39.5 14.3 -0.0807 -0.3 8.9 Vela X-1
170.3076 -60.7217 10.6 48.2 -26.8 -0.3470 -1.1 5.9 Cen X-3
186.3357 -62.8258 3.9 52.1 -35.7 -1.9399 -3.0 9.4 GX 301-2
139.3868 -30.5229 0.5 31.5 25.8 4.7413 22.8 ------ UNKNOWN
189.5588 33.8823 2.2 51.0 178.9 2.3199 5.2 ------ UNKNOWN
143.9417 -56.2149 1.7 47.3 -7.4 1.8964 6.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
88.348620 482.687200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4597 -40.5459 2.3 10.5 -17.1 2.9467 5.0 3.2 Vela X-1
170.5676 -60.6211 13.6 36.5 -59.0 1.0258 0.8 7.4 Cen X-3
186.5890 -62.6561 3.0 43.9 -62.8 10.8899 3.8 7.1 GX 301-2
149.6478 20.8266 2.5 52.3 158.5 13.0599 4.7 ------ UNKNOWN
152.9892 22.7919 2.8 54.9 161.7 15.0217 4.1 ------ UNKNOWN
79.3791 -48.6969 3.3 48.3 16.3 4.7672 3.5 ------ UNKNOWN
139.3360 -30.5277 2.2 0.0 69.1 3.1310 5.3 ------ UNKNOWN
157.3476 -5.6528 2.7 30.1 -175.9 2.8282 4.3 ------ UNKNOWN
164.1295 -49.6960 3.2 26.7 -70.8 2.9952 3.5 ------ UNKNOWN
68.0953 -78.4186 2.2 56.4 -20.5 12.9734 5.2 ------ UNKNOWN
160.6256 -74.9883 2.6 45.7 -41.2 5.8428 4.5 ------ UNKNOWN
186.6108 -11.1897 3.3 47.7 -137.1 7.1134 3.5 ------ UNKNOWN
Plot creation:
Sat Jan 20 10:14:17 EST 2018