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
2.0541 -61.6687 0.0162 35.9590 -38.2473 1.6418399 11.829 TRIG_00663179
Foreground time interval of the image:
-0.064 69.024 (delta_t = 69.088 [sec])
Background time interval of the image:
-239.488 -0.064 (delta_t = 239.424 [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 0.512000
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 0.512000
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 0.512000
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 -0.064 sec. to 69.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88008 ( -0.217691 0.229938 )
Norm@50keV : 1.46218E-03 ( -0.000203439 0.000197332 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.97 using 59 PHA bins.
# Reduced chi-squared = 1.245 for 57 degrees of freedom
# Null hypothesis probability = 1.010607e-01
Photon flux (15-150 keV) in 69.09 sec: 0.208086 ( -0.0240912 0.0241165 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.28687e-07 ( -1.25879e-07 1.28049e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.064 sec. to 69.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87952 ( -0.713716 1.16182 )
Epeak [keV] : 830.730 ( )
Norm@50keV : 1.46174E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.98 using 59 PHA bins.
# Reduced chi-squared = 1.267 for 56 degrees of freedom
# Null hypothesis probability = 8.575130e-02
Photon flux (15-150 keV) in 69.09 sec: 0.208169 ( -0.024274 0.023979 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.27112e-07 ( -1.29606e-07 1.281e-07 ) ergs/cm2
Band function
Time interval is from -0.064 sec. to 69.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.53199 ( 1.53199 1.53199 )
beta : -1.88007 ( 1.88007 0.21769 )
Epeak [keV] : 15.2142 ( -15.188 -15.188 )
Norm@50keV : 3.47366E-03 ( -0.00219061 0.216302 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.97 using 59 PHA bins.
# Reduced chi-squared = 1.290 for 55 degrees of freedom
# Null hypothesis probability = 7.242565e-02
Photon flux (15-150 keV) in 69.09 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] : 11.2131 (-1.7011 2.01303)
R^2/D10^2 : 6.13797E-02 (-0.0280666 0.0522944)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 96.60 using 59 PHA bins.
# Reduced chi-squared = 1.695 for 57 degrees of freedom
# Null hypothesis probability = 8.256062e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.118e-07 2.328e-08
25- 50 3.240e-07 5.413e-08
50-150 2.335e-07 6.636e-08
15-150 6.692e-07 1.110e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 91.6550 (-31.5616 66.6067)
Norm : 0.928583 (-0.149695 0.193179)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.02 using 59 PHA bins.
# Reduced chi-squared = 1.281 for 57 degrees of freedom
# Null hypothesis probability = 7.493247e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.675e-07 2.815e-08
25- 50 2.844e-07 3.848e-08
50-150 4.379e-07 2.016e-07
15-150 8.898e-07 2.145e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.03899 (-1.86215 2.28788)
R1^2/D10^2 : 0.918227 (-0.661673 6.52807)
kT2 [keV] : 20.4594 (-5.74004 14.288)
R2^2/D10^2 : 5.22585E-03 (-0.00435855 0.0117571)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.94 using 59 PHA bins.
# Reduced chi-squared = 1.326 for 55 degrees of freedom
# Null hypothesis probability = 5.308965e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.880e-07 9.507e-08
25- 50 2.519e-07 1.150e-07
50-150 4.587e-07 2.584e-07
15-150 8.986e-07 3.581e-07
Peak spectrum fit
Power-law model
Time interval is from -0.012 sec. to 0.988 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65599 ( -0.201893 0.208766 )
Norm@50keV : 1.43314E-02 ( -0.00182636 0.00180265 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.80 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.456678e-01
Photon flux (15-150 keV) in 1 sec: 1.87499 ( -0.227457 0.227824 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33209e-07 ( -1.78381e-08 1.79943e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.012 sec. to 0.988 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15316 ( -0.998857 0.719826 )
Epeak [keV] : 85.1179 ( -33.5379 -85.1171 )
Norm@50keV : 2.57424E-02 ( -0.0128263 0.0536685 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.77 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 56 degrees of freedom
# Null hypothesis probability = 4.461475e-01
Photon flux (15-150 keV) in 1 sec: 1.84088 ( -0.23628 0.23511 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.29934e-07 ( -1.8749e-08 1.8883e-08 ) ergs/cm2
Band function
Time interval is from -0.012 sec. to 0.988 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.17432 ( -0.492857 0.739616 )
beta : -9.36769 ( 9.37073 19.3707 )
Epeak [keV] : 87.5603 ( -30.1105 -87.4342 )
Norm@50keV : 2.50084E-02 ( -0.0120889 0.00941826 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.77 using 59 PHA bins.
# Reduced chi-squared = 1.032 for 55 degrees of freedom
# Null hypothesis probability = 4.087413e-01
Photon flux (15-150 keV) in 1 sec: 1.84298 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3017e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.5500 (-1.86833 2.15014)
R^2/D10^2 : 0.236459 (-0.0928768 0.15044)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.63 using 59 PHA bins.
# Reduced chi-squared = 1.222 for 57 degrees of freedom
# Null hypothesis probability = 1.216919e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.053e-08 2.458e-09
25- 50 4.065e-08 7.070e-09
50-150 5.776e-08 1.347e-08
15-150 1.089e-07 1.774e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 160.212 (-65.9775 -158.778)
Norm : 7.71462 (-0.986248 1.26512)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.91 using 59 PHA bins.
# Reduced chi-squared = 0.9984 for 57 degrees of freedom
# Null hypothesis probability = 4.784885e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.970e-08 5.971e-09
25- 50 3.685e-08 1.923e-08
50-150 7.469e-08 4.163e-08
15-150 1.312e-07 7.305e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.98989 (-1.10983 1.73271)
R1^2/D10^2 : 74.6294 (-67.4444 1613.98)
kT2 [keV] : 17.1682 (-2.549 3.41702)
R2^2/D10^2 : 0.120040 (-0.0597928 0.0613809)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.00 using 59 PHA bins.
# Reduced chi-squared = 0.9637 for 55 degrees of freedom
# Null hypothesis probability = 5.512657e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.085e-08 8.907e-09
25- 50 3.401e-08 8.775e-09
50-150 6.765e-08 2.056e-08
15-150 1.225e-07 2.471e-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: 1.88008 ( -0.217691 0.229938 )
Norm@50keV : 1.46218E-03 ( -0.000203439 0.000197332 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.97 using 59 PHA bins.
# Reduced chi-squared = 1.245 for 57 degrees of freedom
# Null hypothesis probability = 1.010607e-01
Photon flux (15-150 keV) in 69.09 sec: 0.208086 ( -0.0240912 0.0241165 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.28687e-07 ( -1.25879e-07 1.28049e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87952 ( -0.713716 1.16182 )
Epeak [keV] : 830.730 ( )
Norm@50keV : 1.46174E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.98 using 59 PHA bins.
# Reduced chi-squared = 1.267 for 56 degrees of freedom
# Null hypothesis probability = 8.575130e-02
Photon flux (15-150 keV) in 69.09 sec: 0.208169 ( -0.024274 0.023979 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.27112e-07 ( -1.29606e-07 1.281e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.53199 ( 1.53199 1.53199 )
beta : -1.88007 ( 1.88007 0.21769 )
Epeak [keV] : 15.2142 ( -15.188 -15.188 )
Norm@50keV : 3.47366E-03 ( -0.00219061 3.65737 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.97 using 59 PHA bins.
# Reduced chi-squared = 1.290 for 55 degrees of freedom
# Null hypothesis probability = 7.242565e-02
Photon flux (15-150 keV) in 69.09 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) = 2.69e-07
S(50-100 keV) = 2.92e-07
T90 vs. Hardness ratio plot
T90 = 58.8640000224113 sec.
Hardness ratio (energy fluence ratio) = 1.0855
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.03292
Count Ratio (50-100 keV) / (15-25 keV) = 0.677149
Mask shadow pattern
IMX = 5.697283094631234E-01, IMY = 4.490948199953240E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.488000 -0.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
38.2522 -6.9890 2.1 40.6 71.3 3.8558 5.5 ------ UNKNOWN
73.4591 -7.0346 2.6 39.9 126.7 2.3328 4.4 ------ UNKNOWN
11.3604 -25.2023 2.8 41.3 22.4 1.3281 4.0 ------ UNKNOWN
106.0974 -27.7744 2.7 42.4 -175.3 1.1980 4.3 ------ UNKNOWN
342.6739 -31.0523 3.1 58.2 -3.7 4.3229 3.7 ------ UNKNOWN
14.9085 -53.4893 2.7 28.7 -23.6 0.8289 4.3 ------ UNKNOWN
132.5091 -54.3277 2.7 48.0 -129.1 3.4966 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.064000 69.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
15.4746 -11.1946 2.3 48.4 40.4 1.9938 5.0 ------ UNKNOWN
85.6790 -16.0006 2.5 37.2 150.5 0.7519 4.7 ------ UNKNOWN
2.0541 -61.6687 1.0 36.0 -38.2 1.6416 11.8 ------ UNKNOWN
20.2433 -69.4912 2.1 31.3 -55.9 0.6827 5.4 ------ UNKNOWN
108.5020 -81.1551 2.1 40.8 -90.2 2.0789 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
414.812600 427.412600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
188.2363 46.9224 2.8 33.1 -108.8 0.4412 4.1 ------ UNKNOWN
217.8339 51.7559 2.6 48.0 -129.0 1.2724 4.5 ------ UNKNOWN
Plot creation:
Sun Dec 13 19:50:45 EST 2015