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
162.2491 -50.8025 0.0027 9.3791 -70.6202 8.7556164 71.253 TRIG_00711084
Foreground time interval of the image:
-15.200 11.701 (delta_t = 26.901 [sec])
Background time interval of the image:
-46.899 -15.200 (delta_t = 31.699 [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 1.024000
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 1.024000
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 1.024000
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 -15.200 sec. to 96.800 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.960998 ( -0.0296052 0.0294516 )
Norm@50keV : 1.26088E-02 ( -0.000209253 0.00020834 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.95 using 59 PHA bins.
# Reduced chi-squared = 0.7185 for 57 degrees of freedom
# Null hypothesis probability = 9.461659e-01
Photon flux (15-150 keV) in 112 sec: 1.44914 ( -0.02466 0.02475 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54888e-05 ( -2.3572e-07 2.36089e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.200 sec. to 96.800 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.955654 ( -0.0310547 0.0289528 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.26685E-02 ( -0.000198012 0.00119227 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.02 using 59 PHA bins.
# Reduced chi-squared = 0.7326 for 56 degrees of freedom
# Null hypothesis probability = 9.333062e-01
Photon flux (15-150 keV) in 112 sec: 1.44846 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54921e-05 ( 0 0 ) ergs/cm2
Band function
Time interval is from -15.200 sec. to 96.800 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] : 26.0169 ( )
R^2/D10^2 : 3.06380E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 699.27 using 59 PHA bins.
# Reduced chi-squared = 12.268 for 57 degrees of freedom
# Null hypothesis probability = 2.408585e-111
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.949e-07 1.249e-08
25- 50 2.285e-06 5.656e-08
50-150 1.139e-05 2.190e-07
15-150 1.407e-05 2.464e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 6.42435 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1323.70 using 59 PHA bins.
# Reduced chi-squared = 23.2227 for 57 degrees of freedom
# Null hypothesis probability = 2.475046e-239
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.792e-06 3.024e-08
25- 50 3.447e-06 5.656e-08
50-150 7.559e-06 1.282e-07
15-150 1.280e-05 1.960e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.21145 (-0.676439 0.728924)
R1^2/D10^2 : 0.425251 (-0.08884 0.117796)
kT2 [keV] : 41.0100 (-2.63959 3.284)
R2^2/D10^2 : 6.83198E-03 (-0.00138938 0.00152492)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.29 using 59 PHA bins.
# Reduced chi-squared = 0.7870 for 55 degrees of freedom
# Null hypothesis probability = 8.734923e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.590e-07 6.149e-08
25- 50 2.874e-06 9.464e-08
50-150 1.176e-05 3.640e-07
15-150 1.559e-05 3.920e-07
Peak spectrum fit
Power-law model
Time interval is from 8.300 sec. to 9.300 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.876931 ( -0.0776683 0.0768803 )
Norm@50keV : 5.43900E-02 ( -0.00231502 0.00230877 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.78 using 59 PHA bins.
# Reduced chi-squared = 1.189 for 57 degrees of freedom
# Null hypothesis probability = 1.553271e-01
Photon flux (15-150 keV) in 1 sec: 6.24220 ( -0.26496 0.26515 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.16013e-07 ( -2.92131e-08 2.93142e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.300 sec. to 9.300 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.870958 ( -0.0786195 0.0770835 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.47553E-02 ( -0.0022932 0.0181055 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.78 using 59 PHA bins.
# Reduced chi-squared = 1.210 for 56 degrees of freedom
# Null hypothesis probability = 1.344020e-01
Photon flux (15-150 keV) in 1 sec: 6.24163 ( -0.27017 0.26434 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.16042e-07 ( -2.84579e-08 2.65125e-08 ) ergs/cm2
Band function
Time interval is from 8.300 sec. to 9.300 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] : 23.6155 ( )
R^2/D10^2 : 0.182983 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 161.67 using 59 PHA bins.
# Reduced chi-squared = 2.8363 for 57 degrees of freedom
# Null hypothesis probability = 5.901151e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.826e-08 1.605e-09
25- 50 1.005e-07 6.490e-09
50-150 4.181e-07 3.110e-08
15-150 5.369e-07 2.960e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 24.2508 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 265.56 using 59 PHA bins.
# Reduced chi-squared = 4.6589 for 57 degrees of freedom
# Null hypothesis probability = 1.153077e-28
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.039e-08 3.100e-09
25- 50 1.162e-07 6.200e-09
50-150 2.548e-07 1.550e-08
15-150 4.313e-07 2.300e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.1570 (-2.25128 2.7032)
R1^2/D10^2 : 1.38090 (-0.606537 1.37401)
kT2 [keV] : 47.8105 (-11.9592 42.096)
R2^2/D10^2 : 2.01567E-02 (-0.0153414 0.0258078)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.31 using 59 PHA bins.
# Reduced chi-squared = 1.297 for 55 degrees of freedom
# Null hypothesis probability = 6.868744e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.437e-08 6.025e-09
25- 50 1.114e-07 1.547e-08
50-150 4.756e-07 1.612e-07
15-150 6.213e-07 1.602e-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: 0.896732 ( -0.0358488 0.0356385 )
Norm@50keV : 2.12020E-02 ( -0.000416942 0.000415084 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.75 using 59 PHA bins.
# Reduced chi-squared = 0.7325 for 57 degrees of freedom
# Null hypothesis probability = 9.352418e-01
Photon flux (15-150 keV) in 26.9 sec: 2.43345 ( -0.0479119 0.0480302 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.40884e-06 ( -1.22156e-07 1.22273e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.890231 ( -0.0698396 0.035418 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.13383E-02 ( -0.000395077 0.00221255 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.81 using 59 PHA bins.
# Reduced chi-squared = 0.7466 for 56 degrees of freedom
# Null hypothesis probability = 9.207095e-01
Photon flux (15-150 keV) in 26.9 sec: 2.43295 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.41038e-06 ( -1.21534e-07 1.22126e-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) = 2.80e-06
S(50-100 keV) = 5.75e-06
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 2.05357
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.82748
Count Ratio (50-100 keV) / (15-25 keV) = 1.96053
Mask shadow pattern
IMX = 5.480983421668502E-02, IMY = 1.558160213670279E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-46.899410 -15.200000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5392 -40.5670 33.0 20.8 -150.3 -0.0226 -0.3 0.9 Vela X-1
170.4790 -60.4828 10.0 9.4 -0.6 0.0698 1.2 9.7 Cen X-3
186.6487 -62.7871 0.7 17.1 7.9 1.0623 16.3 1.0 GX 301-2
277.2690 -67.1152 1.7 48.1 43.0 1.8756 6.6 ------ UNKNOWN
64.9869 -82.1133 2.4 32.2 83.3 0.6228 4.8 ------ UNKNOWN
95.5514 -41.1415 2.7 39.2 158.8 0.5058 4.3 ------ UNKNOWN
235.4117 -49.1799 2.7 46.6 5.3 0.5647 4.4 ------ UNKNOWN
162.2340 -50.8786 3.0 9.3 -70.4 0.2434 3.8 ------ UNKNOWN
123.5295 -18.8997 2.3 44.7 -152.2 0.6099 5.0 ------ UNKNOWN
155.6569 -17.1857 2.2 41.2 -107.0 1.4201 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.200000 11.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.2537 -40.5888 0.0 20.8 -150.9 0.1381 1.1 12.7 Vela X-1
170.1153 -60.4631 6.5 9.2 -0.6 0.2242 1.8 11.3 Cen X-3
186.7632 -62.9079 9.6 17.2 8.3 -0.1469 -1.2 8.8 GX 301-2
13.1172 -82.5260 2.8 37.6 76.4 1.5647 4.1 ------ UNKNOWN
190.5116 -64.4560 2.0 18.9 13.2 0.7183 5.7 ------ UNKNOWN
162.2491 -50.8025 0.2 9.4 -70.6 8.7556 71.3 ------ UNKNOWN
123.1022 -23.1578 2.4 40.9 -155.1 0.9148 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
46.100590 962.819700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.7401 -40.5579 10.3 21.0 -163.7 0.8818 1.1 9.6 Vela X-1
170.3339 -60.7723 7.6 10.9 66.2 1.1293 1.5 9.0 Cen X-3
186.6551 -62.7760 0.3 17.7 49.1 33.1988 42.3 0.3 GX 301-2
139.3256 -14.4769 3.4 40.8 -127.9 5.8790 3.5 ------ UNKNOWN
215.3497 -10.8084 3.3 58.8 -25.9 18.8528 3.6 ------ UNKNOWN
152.0162 -10.1991 3.9 41.5 -107.9 13.0771 3.0 ------ UNKNOWN
197.8678 -9.4917 3.5 50.6 -44.6 15.9415 3.3 ------ UNKNOWN
135.7342 -8.1035 3.8 48.0 -129.1 13.0201 3.0 ------ UNKNOWN
Plot creation:
Thu Oct 6 14:49:40 EDT 2016