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
109.0798 -23.5894 0.0079 22.8322 7.7037 1.0218882 24.224 TRIG_00671231
Foreground time interval of the image:
-0.028 11.061 (delta_t = 11.089 [sec])
Background time interval of the image:
-239.440 -0.028 (delta_t = 239.412 [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 -0.028 sec. to 14.972 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77266 ( -0.12854 0.131438 )
Norm@50keV : 4.43238E-03 ( -0.000363907 0.000360102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.64 using 59 PHA bins.
# Reduced chi-squared = 0.8183 for 57 degrees of freedom
# Null hypothesis probability = 8.345749e-01
Photon flux (15-150 keV) in 15 sec: 0.604448 ( -0.045036 0.045072 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.1286e-07 ( -5.14609e-08 5.20174e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.028 sec. to 14.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04567 ( -0.629082 0.549155 )
Epeak [keV] : 59.5825 ( -11.261 44.8546 )
Norm@50keV : 1.10122E-02 ( -0.00538645 0.0129789 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.35 using 59 PHA bins.
# Reduced chi-squared = 0.7383 for 56 degrees of freedom
# Null hypothesis probability = 9.283549e-01
Photon flux (15-150 keV) in 15 sec: 0.586432 ( -0.047017 0.047012 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.75124e-07 ( -5.71579e-08 5.85432e-08 ) ergs/cm2
Band function
Time interval is from -0.028 sec. to 14.972 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.03533 ( -0.564007 1.01834 )
beta : -2.59436 ( 2.647 0.815139 )
Epeak [keV] : 59.1680 ( -31.2242 41.224 )
Norm@50keV : 1.11611E-02 ( -0.00597402 0.946259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.29 using 59 PHA bins.
# Reduced chi-squared = 0.7506 for 55 degrees of freedom
# Null hypothesis probability = 9.147355e-01
Photon flux (15-150 keV) in 15 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] : 12.0842 (-1.02059 1.12187)
R^2/D10^2 : 0.142996 (-0.040411 0.0556908)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.39 using 59 PHA bins.
# Reduced chi-squared = 1.252 for 57 degrees of freedom
# Null hypothesis probability = 9.517257e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.629e-08 8.618e-09
25- 50 2.103e-07 1.785e-08
50-150 1.855e-07 3.204e-08
15-150 4.621e-07 4.372e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 104.521 (-25.224 39.301)
Norm : 2.65095 (-0.258457 0.302926)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.83 using 59 PHA bins.
# Reduced chi-squared = 0.7339 for 57 degrees of freedom
# Null hypothesis probability = 9.340196e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.039e-07 1.237e-08
25- 50 1.813e-07 1.523e-08
50-150 3.011e-07 1.050e-07
15-150 5.863e-07 1.154e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.93880 (-1.62225 2.0003)
R1^2/D10^2 : 1.12752 (-0.673297 2.52805)
kT2 [keV] : 18.6949 (-3.49792 7.06278)
R2^2/D10^2 : 2.16165E-02 (-0.0158548 0.0170478)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.78 using 59 PHA bins.
# Reduced chi-squared = 0.7597 for 55 degrees of freedom
# Null hypothesis probability = 9.054405e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.005e-07 4.647e-08
25- 50 1.827e-07 6.251e-08
50-150 2.794e-07 1.375e-07
15-150 5.625e-07 1.876e-07
Peak spectrum fit
Power-law model
Time interval is from 2.760 sec. to 3.760 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81961 ( -0.243769 0.258038 )
Norm@50keV : 8.46667E-03 ( -0.00146777 0.00143137 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.25 using 59 PHA bins.
# Reduced chi-squared = 0.9868 for 57 degrees of freedom
# Null hypothesis probability = 5.032577e-01
Photon flux (15-150 keV) in 1 sec: 1.17574 ( -0.17157 0.1716 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.79094e-08 ( -1.34316e-08 1.37211e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.760 sec. to 3.760 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.929266 ( -1.36922 1.00837 )
Epeak [keV] : 51.4799 ( -15.3408 -51.48 )
Norm@50keV : 2.73814E-02 ( -0.0273814 0.141013 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.16 using 59 PHA bins.
# Reduced chi-squared = 0.9672 for 56 degrees of freedom
# Null hypothesis probability = 5.446295e-01
Photon flux (15-150 keV) in 1 sec: 1.15009 ( -0.174238 0.17429 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.2124e-08 ( -1.40636e-08 1.5145e-08 ) ergs/cm2
Band function
Time interval is from 2.760 sec. to 3.760 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.929175 ( -0.829161 1.15564 )
beta : -10.00000 ( 10 3.2905e-09 )
Epeak [keV] : 51.4693 ( -14.4518 -51.4693 )
Norm@50keV : 2.73834E-02 ( -0.0163064 0.141482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.16 using 59 PHA bins.
# Reduced chi-squared = 0.9848 for 55 degrees of freedom
# Null hypothesis probability = 5.065112e-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] : 11.0591 (-1.69632 2.03683)
R^2/D10^2 : 0.396916 (-0.187253 0.341066)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.19 using 59 PHA bins.
# Reduced chi-squared = 1.073 for 57 degrees of freedom
# Null hypothesis probability = 3.281163e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.015e-08 2.919e-09
25- 50 2.891e-08 6.290e-09
50-150 2.005e-08 7.325e-09
15-150 5.912e-08 1.270e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 88.9924 (-33.1819 77.9068)
Norm : 5.42403 (-1.02255 1.3012)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.45 using 59 PHA bins.
# Reduced chi-squared = 0.9553 for 57 degrees of freedom
# Null hypothesis probability = 5.712800e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.415e-08 2.595e-09
25- 50 2.387e-08 4.485e-09
50-150 3.609e-08 2.034e-08
15-150 7.411e-08 2.219e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.93347 (-3.30243 3.95209)
R1^2/D10^2 : 2.29931 (-1.75487 3.77408)
kT2 [keV] : 17.6492 (-5.89044 44.0617)
R2^2/D10^2 : 4.96801E-02 (-0.0489202 0.238211)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.32 using 59 PHA bins.
# Reduced chi-squared = 0.9877 for 55 degrees of freedom
# Null hypothesis probability = 5.004910e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.370e-08 7.610e-09
25- 50 2.450e-08 1.287e-08
50-150 3.285e-08 1.990e-08
15-150 7.105e-08 3.761e-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: 1.71708 ( -0.12284 0.125093 )
Norm@50keV : 5.55036E-03 ( -0.000428325 0.000424701 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.47 using 59 PHA bins.
# Reduced chi-squared = 0.9556 for 57 degrees of freedom
# Null hypothesis probability = 5.707080e-01
Photon flux (15-150 keV) in 11.09 sec: 0.741603 ( -0.0533501 0.0533991 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.69182e-07 ( -4.57231e-08 4.61188e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.960362 ( -0.615732 0.539393 )
Epeak [keV] : 63.3835 ( -11.7481 44.071 )
Norm@50keV : 1.41417E-02 ( -0.0067755 0.0158264 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.48 using 59 PHA bins.
# Reduced chi-squared = 0.8658 for 56 degrees of freedom
# Null hypothesis probability = 7.520591e-01
Photon flux (15-150 keV) in 11.09 sec: 0.718035 ( -0.055866 0.055842 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.33644e-07 ( -5.11393e-08 5.21419e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.896407 ( -0.579709 2.86035 )
beta : -2.50142 ( 2.49214 0.705009 )
Epeak [keV] : 60.9592 ( -30.0404 40.8511 )
Norm@50keV : 1.54466E-02 ( -0.00686524 1.85163 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.25 using 59 PHA bins.
# Reduced chi-squared = 0.8772 for 55 degrees of freedom
# Null hypothesis probability = 7.283795e-01
Photon flux (15-150 keV) in 11.09 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) = 1.71e-07
S(50-100 keV) = 2.00e-07
T90 vs. Hardness ratio plot
T90 = 10.4999999403954 sec.
Hardness ratio (energy fluence ratio) = 1.16959
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.22756
Count Ratio (50-100 keV) / (15-25 keV) = 0.742429
Mask shadow pattern
IMX = 4.172220750241890E-01, IMY = -5.643792970956614E-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:
-239.440000 -0.028000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5164 -40.5795 1.1 24.4 -66.3 2.6207 10.4 1.6 Vela X-1
162.5867 11.7878 2.4 41.2 168.7 1.7338 4.9 ------ UNKNOWN
80.1889 -28.9283 2.7 49.2 5.5 1.9781 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.028000 11.060590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3858 -40.4804 3.8 24.3 -66.1 -0.1515 -3.0 7.9 Vela X-1
109.0798 -23.5893 0.5 22.8 7.7 1.0218 24.2 ------ UNKNOWN
161.4984 -13.4709 2.0 28.5 -152.0 0.2617 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.460610 917.060590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5243 -40.5478 1.2 27.9 -154.7 5.6172 9.9 0.5 Vela X-1
139.9915 4.2927 3.3 41.0 122.8 7.3291 3.5 ------ UNKNOWN
149.9719 -0.7768 3.6 45.7 137.7 8.3539 3.2 ------ UNKNOWN
67.1889 11.0802 3.1 53.6 17.1 9.0261 3.7 ------ UNKNOWN
123.0665 -14.4070 3.9 16.1 129.3 1.6720 2.9 ------ UNKNOWN
55.0781 -23.4851 3.3 49.2 -29.9 4.6834 3.5 ------ UNKNOWN
51.5758 -34.4127 3.7 50.8 -44.6 11.6018 3.1 ------ UNKNOWN
149.2957 -64.4272 4.9 48.5 -130.3 7.3791 2.4 ------ UNKNOWN
112.6749 -66.1815 2.9 42.7 -110.6 11.7687 4.0 ------ UNKNOWN
Plot creation:
Fri Mar 18 11:49:55 EDT 2016