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
13.6617 -4.9528 0.0018 27.8057 -4.9107 24.9083839 107.089 TRIG_00689597
Foreground time interval of the image:
-14.548 15.485 (delta_t = 30.033 [sec])
Background time interval of the image:
-29.515 -14.548 (delta_t = 14.967 [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 -14.548 sec. to 44.080 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36873 ( -0.0233175 0.0232367 )
Norm@50keV : 3.65068E-02 ( -0.000493473 0.000492611 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.80 using 59 PHA bins.
# Reduced chi-squared = 0.7685 for 57 degrees of freedom
# Null hypothesis probability = 9.002288e-01
Photon flux (15-150 keV) in 58.63 sec: 4.41538 ( -0.07103 0.07129 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.08209e-05 ( -2.58705e-07 2.59046e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -14.548 sec. to 44.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14498 ( -0.0992864 0.097366 )
Epeak [keV] : 247.050 ( -55.4048 133.812 )
Norm@50keV : 4.45855E-02 ( -0.00364005 0.0040257 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 28.19 using 59 PHA bins.
# Reduced chi-squared = 0.5035 for 56 degrees of freedom
# Null hypothesis probability = 9.992966e-01
Photon flux (15-150 keV) in 58.63 sec: 2.62052 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.06771e-05 ( -2.65837e-07 2.65947e-07 ) ergs/cm2
Band function
Time interval is from -14.548 sec. to 44.080 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.14152 ( -0.0973749 0.0611705 )
beta : -1.60600 ( 1.61032 0.20646 )
Epeak [keV] : 241.991 ( -175.228 139.24 )
Norm@50keV : 4.47840E-02 ( -0.0039514 0.258692 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 28.15 using 59 PHA bins.
# Reduced chi-squared = 0.5119 for 55 degrees of freedom
# Null hypothesis probability = 9.990101e-01
Photon flux (15-150 keV) in 58.63 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] : 21.7166 ( )
R^2/D10^2 : 0.142412 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1161.38 using 59 PHA bins.
# Reduced chi-squared = 20.3751 for 57 degrees of freedom
# Null hypothesis probability = 1.202720e-205
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.331e-07 2.023e-08
25- 50 3.846e-06 7.886e-08
50-150 1.355e-05 2.140e-07
15-150 1.813e-05 2.492e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 19.3792 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 376.84 using 59 PHA bins.
# Reduced chi-squared = 6.6113 for 57 degrees of freedom
# Null hypothesis probability = 1.108914e-48
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.829e-06 4.280e-08
25- 50 5.442e-06 8.267e-08
50-150 1.194e-05 1.788e-07
15-150 2.021e-05 3.107e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.59750 (-0.463059 0.487069)
R1^2/D10^2 : 1.96530 (-0.33025 0.41133)
kT2 [keV] : 32.4755 (-1.38783 1.60925)
R2^2/D10^2 : 3.00596E-02 (-0.00476381 0.00514087)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.13 using 59 PHA bins.
# Reduced chi-squared = 0.7114 for 55 degrees of freedom
# Null hypothesis probability = 9.478809e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.893e-06 1.014e-07
25- 50 4.954e-06 1.126e-07
50-150 1.372e-05 2.756e-07
15-150 2.056e-05 3.694e-07
Peak spectrum fit
Power-law model
Time interval is from 11.648 sec. to 12.648 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22598 ( -0.0379953 0.0379366 )
Norm@50keV : 0.185204 ( -0.00407342 0.00407177 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.72 using 59 PHA bins.
# Reduced chi-squared = 1.171 for 57 degrees of freedom
# Null hypothesis probability = 1.774969e-01
Photon flux (15-150 keV) in 1 sec: 1.03905 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86569e-06 ( -4.28019e-08 4.28444e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 11.648 sec. to 12.648 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.686066 ( -0.17091 0.164959 )
Epeak [keV] : 143.818 ( -20.8076 36.7015 )
Norm@50keV : 0.316722 ( -0.0467146 0.0567106 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.20 using 59 PHA bins.
# Reduced chi-squared = 0.5929 for 56 degrees of freedom
# Null hypothesis probability = 9.934203e-01
Photon flux (15-150 keV) in 1 sec: 21.2201 ( -0.5366 0.5379 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.59049e-07 ( 0 0 ) ergs/cm2
Band function
Time interval is from 11.648 sec. to 12.648 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.624202 ( -0.210925 0.344033 )
beta : -1.67873 ( 1.68338 0.242973 )
Epeak [keV] : 130.954 ( -40.1951 45.0422 )
Norm@50keV : 0.341134 ( -0.0669693 0.183891 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 32.80 using 59 PHA bins.
# Reduced chi-squared = 0.5964 for 55 degrees of freedom
# Null hypothesis probability = 9.924372e-01
Photon flux (15-150 keV) in 1 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] : 20.1772 ( )
R^2/D10^2 : 0.985931 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 310.95 using 59 PHA bins.
# Reduced chi-squared = 5.4553 for 57 degrees of freedom
# Null hypothesis probability = 1.185856e-36
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.711e-08 3.365e-09
25- 50 3.863e-07 1.285e-08
50-150 1.167e-06 4.000e-08
15-150 1.631e-06 3.900e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 92.8458 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 277.34 using 59 PHA bins.
# Reduced chi-squared = 4.8656 for 57 degrees of freedom
# Null hypothesis probability = 1.042041e-30
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.312e-07 5.350e-09
25- 50 4.447e-07 9.900e-09
50-150 9.754e-07 2.255e-08
15-150 1.651e-06 3.900e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.71808 (-1.00025 1.10504)
R1^2/D10^2 : 7.88364 (-2.24816 3.52462)
kT2 [keV] : 30.1760 (-2.40363 3.29744)
R2^2/D10^2 : 0.211216 (-0.0666239 0.0761163)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.54 using 59 PHA bins.
# Reduced chi-squared = 0.7007 for 55 degrees of freedom
# Null hypothesis probability = 9.550344e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.446e-07 1.190e-08
25- 50 4.171e-07 2.150e-08
50-150 1.270e-06 7.100e-08
15-150 1.831e-06 9.300e-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: 1.28582 ( -0.0231794 0.0230941 )
Norm@50keV : 5.71952E-02 ( -0.000782055 0.000780632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.64 using 59 PHA bins.
# Reduced chi-squared = 0.9586 for 57 degrees of freedom
# Null hypothesis probability = 5.640743e-01
Photon flux (15-150 keV) in 30.03 sec: 6.80603 ( -0.107151 0.107473 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.70322e-05 ( -2.1325e-07 2.1326e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01087 ( -0.0998606 0.0979156 )
Epeak [keV] : 233.864 ( -44.4975 89.6461 )
Norm@50keV : 7.30632E-02 ( -0.00597376 0.00660653 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.10 using 59 PHA bins.
# Reduced chi-squared = 0.5554 for 56 degrees of freedom
# Null hypothesis probability = 9.971875e-01
Photon flux (15-150 keV) in 30.03 sec: 6.65368 ( -0.11727 0.11798 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69262e-05 ( -2.17507e-07 2.17417e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.01080 ( -0.0299791 0.0779549 )
beta : -10.00000 ( 10 20 )
Epeak [keV] : 233.805 ( -67.3922 89.6516 )
Norm@50keV : 7.30595E-02 ( -0.00326875 0.00661509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.10 using 59 PHA bins.
# Reduced chi-squared = 0.5655 for 55 degrees of freedom
# Null hypothesis probability = 9.961432e-01
Photon flux (15-150 keV) in 30.03 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) = 4.81e-06
S(50-100 keV) = 7.45e-06
T90 vs. Hardness ratio plot
T90 = 33.4919999837875 sec.
Hardness ratio (energy fluence ratio) = 1.54886
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.58579
Count Ratio (50-100 keV) / (15-25 keV) = 1.38861
Mask shadow pattern
IMX = 5.254311877774777E-01, IMY = 4.514434742871043E-02
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:
-29.515400 -14.548000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1617 41.0619 5.1 49.6 148.8 0.5014 2.3 7.0 Cyg X-3
325.9505 38.3473 481.1 35.7 149.9 0.0017 0.0 10.5 Cyg X-2
332.3918 69.1870 2.2 52.1 -171.2 0.5771 5.3 ------ UNKNOWN
34.9927 17.3658 2.1 31.7 -69.0 0.3402 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-14.548000 15.484600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0372 41.1359 10.4 49.7 149.0 -1.2872 -1.1 11.5 Cyg X-3
326.0181 38.2684 4.3 35.6 149.9 -1.0566 -2.7 7.9 Cyg X-2
314.4076 37.7232 2.5 44.3 145.4 3.3237 4.6 ------ UNKNOWN
13.6617 -4.9528 0.1 27.8 -4.9 24.9090 107.1 ------ UNKNOWN
24.8183 65.2217 2.5 47.5 -145.5 2.4704 4.6 ------ UNKNOWN
38.2859 63.6808 4.0 50.0 -138.2 2.5805 2.9 ------ UNKNOWN
40.3248 65.8507 2.9 52.1 -139.5 4.4838 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.684650 962.958400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
332.5155 29.9140 2.5 52.6 161.7 11.4471 4.7 ------ UNKNOWN
22.1098 5.6994 2.7 13.6 -114.0 2.1774 4.2 ------ UNKNOWN
61.8494 -33.4955 3.3 53.0 -23.5 4.8090 3.5 ------ UNKNOWN
7.7603 52.6775 6.0 57.9 -156.7 7.5050 1.9 ------ UNKNOWN
47.9443 18.6381 5.8 41.2 -98.3 6.2267 2.0 ------ UNKNOWN
36.8315 37.3061 5.6 47.5 -127.3 5.6600 2.1 ------ UNKNOWN
Plot creation:
Tue Jun 21 10:17:12 EDT 2016