Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
344.4256 8.0869 0.0054 1.5943 -86.0699 2.4307202 35.617 TRIG_00668641
Foreground time interval of the image:
-15.560 12.741 (delta_t = 28.301 [sec])
Background time interval of the image:
-239.560 -15.560 (delta_t = 224.000 [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 -15.560 sec. to 48.440 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63856 ( -0.0726004 0.073149 )
Norm@50keV : 4.09069E-03 ( -0.000168469 0.000167933 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.70 using 59 PHA bins.
# Reduced chi-squared = 1.100 for 57 degrees of freedom
# Null hypothesis probability = 2.811764e-01
Photon flux (15-150 keV) in 64 sec: 0.532166 ( -0.021703 0.021737 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43809e-06 ( -1.07052e-07 1.07565e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.560 sec. to 48.440 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10105 ( -0.327265 0.304657 )
Epeak [keV] : 81.9709 ( -14.5737 43.0021 )
Norm@50keV : 7.65284E-03 ( -0.00224014 0.00346824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.17 using 59 PHA bins.
# Reduced chi-squared = 0.9494 for 56 degrees of freedom
# Null hypothesis probability = 5.828383e-01
Photon flux (15-150 keV) in 64 sec: 0.514680 ( -0.023643 0.023691 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32327e-06 ( -1.2374e-07 1.24383e-07 ) ergs/cm2
Band function
Time interval is from -15.560 sec. to 48.440 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.08173 ( -0.31638 0.45393 )
beta : -2.32044 ( 2.32067 0.533157 )
Epeak [keV] : 80.1930 ( -25.0952 43.0098 )
Norm@50keV : 7.84930E-03 ( -0.00239125 0.0069498 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.07 using 59 PHA bins.
# Reduced chi-squared = 0.9649 for 55 degrees of freedom
# Null hypothesis probability = 5.486459e-01
Photon flux (15-150 keV) in 64 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] : 13.9386 ( )
R^2/D10^2 : 7.44038E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 158.41 using 59 PHA bins.
# Reduced chi-squared = 2.7792 for 57 degrees of freedom
# Null hypothesis probability = 1.734319e-11
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.955e-07 1.450e-08
25- 50 7.240e-07 3.552e-08
50-150 9.240e-07 8.128e-08
15-150 1.844e-06 8.512e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 158.516 (-30.8598 36.7146)
Norm : 2.16872 (-0.0968334 0.117287)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.10 using 59 PHA bins.
# Reduced chi-squared = 0.9491 for 57 degrees of freedom
# Null hypothesis probability = 5.846491e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.547e-07 2.294e-08
25- 50 6.627e-07 5.997e-08
50-150 1.338e-06 3.837e-07
15-150 2.355e-06 4.378e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.09197 (-0.97357 1.13912)
R1^2/D10^2 : 0.831678 (-0.366662 0.761989)
kT2 [keV] : 20.7289 (-2.21689 3.18115)
R2^2/D10^2 : 1.44609E-02 (-0.00628755 0.00827655)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.03 using 59 PHA bins.
# Reduced chi-squared = 1.001 for 55 degrees of freedom
# Null hypothesis probability = 4.734631e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.437e-07 5.728e-08
25- 50 6.616e-07 7.597e-08
50-150 1.259e-06 1.744e-07
15-150 2.264e-06 2.429e-07
Peak spectrum fit
Power-law model
Time interval is from 7.940 sec. to 8.940 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64093 ( -0.21401 0.223109 )
Norm@50keV : 9.56377E-03 ( -0.00139553 0.00136925 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.87 using 59 PHA bins.
# Reduced chi-squared = 0.6819 for 57 degrees of freedom
# Null hypothesis probability = 9.683306e-01
Photon flux (15-150 keV) in 1 sec: 1.24513 ( -0.16035 0.16037 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.9041e-08 ( -1.37297e-08 1.39976e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.940 sec. to 8.940 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.807836 ( -1.21445 0.909584 )
Epeak [keV] : 63.6620 ( -17.6093 -63.6615 )
Norm@50keV : 2.78213E-02 ( -0.027822 0.104274 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.60 using 59 PHA bins.
# Reduced chi-squared = 0.6535 for 56 degrees of freedom
# Null hypothesis probability = 9.791694e-01
Photon flux (15-150 keV) in 1 sec: 1.21431 ( -0.16491 0.16435 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.241e-08 ( -1.50922e-08 1.58439e-08 ) ergs/cm2
Band function
Time interval is from 7.940 sec. to 8.940 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.701287 ( 0.643117 0.643117 )
beta : -2.32160 ( 2.32629 0.763906 )
Epeak [keV] : 59.1731 ( -57.5958 128.587 )
Norm@50keV : 3.26246E-02 ( -0.0219688 613.948 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.39 using 59 PHA bins.
# Reduced chi-squared = 0.6616 for 55 degrees of freedom
# Null hypothesis probability = 9.750864e-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] : 12.2443 (-1.66787 1.98205)
R^2/D10^2 : 0.294149 (-0.123686 0.204381)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.35 using 59 PHA bins.
# Reduced chi-squared = 0.7781 for 57 degrees of freedom
# Null hypothesis probability = 8.891423e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.341e-09 2.031e-09
25- 50 3.009e-08 5.565e-09
50-150 2.749e-08 7.990e-09
15-150 6.692e-08 1.183e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 140.869 (-59.1685 -139.19)
Norm : 5.21592 (-0.731501 0.922823)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.21 using 59 PHA bins.
# Reduced chi-squared = 0.6528 for 57 degrees of freedom
# Null hypothesis probability = 9.803696e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.346e-08 5.466e-09
25- 50 2.472e-08 1.259e-08
50-150 4.752e-08 2.786e-08
15-150 8.570e-08 4.638e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.01768 (-3.76085 5.71426)
R1^2/D10^2 : 1.90192 (-1.53755 134.552)
kT2 [keV] : 18.0958 (-5.60406 -18.2275)
R2^2/D10^2 : 5.51046E-02 (-0.0527633 0.193717)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.35 using 59 PHA bins.
# Reduced chi-squared = 0.6790 for 55 degrees of freedom
# Null hypothesis probability = 9.672317e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.280e-08 7.070e-09
25- 50 2.597e-08 1.347e-08
50-150 4.071e-08 2.358e-08
15-150 7.948e-08 4.099e-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: 1.33300 ( -0.0732835 0.0731351 )
Norm@50keV : 5.70294E-03 ( -0.000247609 0.000247508 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.46 using 59 PHA bins.
# Reduced chi-squared = 1.271 for 57 degrees of freedom
# Null hypothesis probability = 8.137328e-02
Photon flux (15-150 keV) in 28.3 sec: 0.684685 ( -0.0303508 0.0303773 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58238e-06 ( -7.60237e-08 7.6367e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.491769 ( -0.358719 0.33087 )
Epeak [keV] : 91.1128 ( -13.6077 26.9702 )
Norm@50keV : 1.48879E-02 ( -0.004583 0.00729986 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.33 using 59 PHA bins.
# Reduced chi-squared = 0.9166 for 56 degrees of freedom
# Null hypothesis probability = 6.520359e-01
Photon flux (15-150 keV) in 28.3 sec: 0.658938 ( -0.031908 0.031903 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48303e-06 ( -8.55566e-08 8.5783e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.58412E-02 ( -0.589376 3.12622 )
beta : -1.81528 ( 1.8086 0.31296 )
Epeak [keV] : 69.9600 ( -31.7946 31.2487 )
Norm@50keV : 2.59472E-02 ( -0.0147004 4.10867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.98 using 59 PHA bins.
# Reduced chi-squared = 0.8906 for 55 degrees of freedom
# Null hypothesis probability = 7.025873e-01
Photon flux (15-150 keV) in 28.3 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) = 6.40e-07
S(50-100 keV) = 8.26e-07
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 1.29062
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28033
Count Ratio (50-100 keV) / (15-25 keV) = 0.903866
Mask shadow pattern
IMX = 1.907673413937355E-03, IMY = 2.776758531718286E-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:
-239.560000 -15.560000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5689 35.2196 0.9 49.6 -15.5 6.1785 12.5 1.5 Cyg X-1
308.0290 40.9723 4.3 46.3 -4.6 1.1447 2.7 3.9 Cyg X-3
326.2129 38.4652 9.9 34.4 7.5 -0.3165 -1.2 8.8 Cyg X-2
27.5113 1.2528 3.0 42.2 133.3 2.6371 3.9 ------ UNKNOWN
333.1723 51.5352 2.3 43.9 23.9 2.3180 5.1 ------ UNKNOWN
25.4189 -34.1043 3.2 57.1 176.3 5.1717 3.6 ------ UNKNOWN
14.6873 -32.0209 2.7 49.4 -177.4 2.3405 4.2 ------ UNKNOWN
296.8932 27.0539 2.6 49.6 -26.7 2.2700 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.560000 12.740590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7021 35.2535 4.0 49.5 -15.4 0.4219 2.9 6.3 Cyg X-1
308.3450 40.9406 0.0 46.1 -4.4 -0.1433 -1.1 10.7 Cyg X-3
326.1761 38.4265 33.3 34.4 7.5 0.0317 0.3 6.3 Cyg X-2
0.0834 0.8462 2.6 16.3 154.0 0.2904 4.4 51.0 UNKNOWN
344.4255 8.0869 0.3 1.6 -86.1 2.4307 35.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
35.540600 962.496500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5942 35.2039 0.6 49.1 -21.9 29.4232 20.4 0.2 Cyg X-1
308.0681 40.9113 2.6 46.0 -10.8 5.4707 4.4 3.1 Cyg X-3
326.1816 38.3158 40.4 34.4 2.0 0.2459 0.3 0.6 Cyg X-2
22.0488 -17.7855 2.4 45.3 152.9 9.9853 4.8 ------ UNKNOWN
5.4677 -6.3874 2.5 25.5 151.8 3.6891 4.7 504.0 UNKNOWN
347.8903 16.7448 2.4 9.3 48.7 2.8883 4.8 ------ UNKNOWN
353.7632 -50.1293 4.6 58.8 -159.2 15.1374 2.5 ------ UNKNOWN
314.1496 -7.1001 3.1 33.8 -88.1 5.5049 3.8 ------ UNKNOWN
Plot creation:
Fri Mar 18 13:41:12 EDT 2016