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
150.2766 -33.7897 0.0120 23.8425 -107.2257 0.5670870 15.940 TRIG_00671447
Foreground time interval of the image:
-2.048 3.000 (delta_t = 5.048 [sec])
Background time interval of the image:
-239.904 -2.048 (delta_t = 237.856 [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 -2.048 sec. to 3.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50898 ( -0.161363 0.162291 )
Norm@50keV : 7.34386E-03 ( -0.00075043 0.000746272 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.72 using 59 PHA bins.
# Reduced chi-squared = 0.8371 for 57 degrees of freedom
# Null hypothesis probability = 8.046777e-01
Photon flux (15-150 keV) in 5.048 sec: 0.919055 ( -0.091252 0.091325 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.5122e-07 ( -3.89868e-08 3.94042e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.048 sec. to 3.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.565751 ( -0.914924 0.731694 )
Epeak [keV] : 69.6151 ( -16.0464 80.8233 )
Norm@50keV : 2.38976E-02 ( -0.0141581 0.0514935 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.64 using 59 PHA bins.
# Reduced chi-squared = 0.7614 for 56 degrees of freedom
# Null hypothesis probability = 9.057651e-01
Photon flux (15-150 keV) in 5.048 sec: 0.890187 ( -0.094382 0.094252 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.21514e-07 ( -4.47499e-08 4.56328e-08 ) ergs/cm2
Band function
Time interval is from -2.048 sec. to 3.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.75884 ( -1.68541 -1.2079 )
beta : -1.96985 ( -0.541547 0.347198 )
Epeak [keV] : 39.7829 ( -10.8507 20.2488 )
Norm@50keV : 0.821888 ( -0.871051 69.2981 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.17 using 59 PHA bins.
# Reduced chi-squared = 0.6940 for 55 degrees of freedom
# Null hypothesis probability = 9.591018e-01
Photon flux (15-150 keV) in 5.048 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] : 13.0739 (-1.40723 1.64741)
R^2/D10^2 : 0.174303 (-0.0609968 0.0890136)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.66 using 59 PHA bins.
# Reduced chi-squared = 0.9415 for 57 degrees of freedom
# Null hypothesis probability = 6.010310e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.189e-08 5.772e-09
25- 50 1.105e-07 1.489e-08
50-150 1.198e-07 2.501e-08
15-150 2.622e-07 3.304e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.130 (-77.2379 -199.154)
Norm : 3.78051 (-0.368202 0.402844)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.92 using 59 PHA bins.
# Reduced chi-squared = 0.7881 for 57 degrees of freedom
# Null hypothesis probability = 8.768063e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.753e-08 1.852e-08
25- 50 9.141e-08 3.390e-08
50-150 2.004e-07 1.083e-07
15-150 3.394e-07 1.717e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.57515 (-2.09466 2.11192)
R1^2/D10^2 : 0.412634 (-0.185722 0.403189)
kT2 [keV] : 38.7296 (-31.4261 -38.9101)
R2^2/D10^2 : 2.43689E-03 (-0.00215266 0.0167677)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.79 using 59 PHA bins.
# Reduced chi-squared = 0.6872 for 55 degrees of freedom
# Null hypothesis probability = 9.629693e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.070e-08 1.342e-08
25- 50 1.058e-07 3.807e-08
50-150 1.922e-07 9.854e-08
15-150 3.387e-07 1.322e-07
Peak spectrum fit
Power-law model
Time interval is from 0.008 sec. to 1.008 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54662 ( -0.25804 0.264181 )
Norm@50keV : 1.03844E-02 ( -0.0017489 0.00172745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.05 using 59 PHA bins.
# Reduced chi-squared = 1.001 for 57 degrees of freedom
# Null hypothesis probability = 4.733039e-01
Photon flux (15-150 keV) in 1 sec: 1.31337 ( -0.20993 0.21009 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.78205e-08 ( -1.76675e-08 1.79639e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.008 sec. to 1.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.530726 ( -1.50206 1.10159 )
Epeak [keV] : 66.8982 ( -19.0731 -66.8981 )
Norm@50keV : 3.67180E-02 ( -0.0367181 0.198496 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.71 using 59 PHA bins.
# Reduced chi-squared = 0.9770 for 56 degrees of freedom
# Null hypothesis probability = 5.236351e-01
Photon flux (15-150 keV) in 1 sec: 1.27434 ( -0.21528 0.21513 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.00596e-08 ( -1.89759e-08 1.99271e-08 ) ergs/cm2
Band function
Time interval is from 0.008 sec. to 1.008 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.402733 ( -1.62399 -1.62399 )
beta : -2.02837 ( 1.93419 0.513297 )
Epeak [keV] : 47.2102 ( -38.5398 65.1886 )
Norm@50keV : 0.150676 ( -0.151755 290.311 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.33 using 59 PHA bins.
# Reduced chi-squared = 0.9878 for 55 degrees of freedom
# Null hypothesis probability = 5.001822e-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] : 13.4002 (-2.27371 2.80603)
R^2/D10^2 : 0.229411 (-0.113848 0.216239)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.28 using 59 PHA bins.
# Reduced chi-squared = 1.040 for 57 degrees of freedom
# Null hypothesis probability = 3.922787e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.729e-09 2.532e-09
25- 50 3.105e-08 7.690e-09
50-150 3.586e-08 1.229e-08
15-150 7.564e-08 1.925e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 188.239 (-97.0755 -185.913)
Norm : 5.40990 (-0.866581 1.05244)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.77 using 59 PHA bins.
# Reduced chi-squared = 0.9784 for 57 degrees of freedom
# Null hypothesis probability = 5.214016e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.357e-08 7.755e-09
25- 50 2.592e-08 1.424e-08
50-150 5.577e-08 3.118e-08
15-150 9.526e-08 5.310e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.22041 (-4.94963 -8.22067)
R1^2/D10^2 : 0.807703 (-0.572549 15.3608)
kT2 [keV] : 24.0391 (-19.3366 -24.0424)
R2^2/D10^2 : 1.84980E-02 (-0.0180806 0.125807)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.38 using 59 PHA bins.
# Reduced chi-squared = 0.9888 for 55 degrees of freedom
# Null hypothesis probability = 4.982164e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.196e-08 6.955e-09
25- 50 2.899e-08 1.576e-08
50-150 5.064e-08 3.043e-08
15-150 9.159e-08 4.636e-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: 1.50898 ( -0.161363 0.162291 )
Norm@50keV : 7.34386E-03 ( -0.00075043 0.000746272 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.72 using 59 PHA bins.
# Reduced chi-squared = 0.8371 for 57 degrees of freedom
# Null hypothesis probability = 8.046777e-01
Photon flux (15-150 keV) in 5.048 sec: 0.919031 ( -0.0912474 0.0913214 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.51174e-07 ( -3.89783e-08 3.94078e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.565869 ( -0.91496 0.731658 )
Epeak [keV] : 69.6196 ( -16.0468 80.8248 )
Norm@50keV : 2.38936E-02 ( -0.0141586 0.0514935 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.64 using 59 PHA bins.
# Reduced chi-squared = 0.7614 for 56 degrees of freedom
# Null hypothesis probability = 9.057651e-01
Photon flux (15-150 keV) in 5.048 sec: 0.890094 ( -0.094358 0.094224 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.2162e-07 ( -4.47864e-08 4.56718e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.75884 ( -1.68541 -1.2079 )
beta : -1.96985 ( -0.541547 0.347198 )
Epeak [keV] : 39.7829 ( -10.8507 20.2488 )
Norm@50keV : 0.821888 ( -0.871051 69.2749 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.17 using 59 PHA bins.
# Reduced chi-squared = 0.6940 for 55 degrees of freedom
# Null hypothesis probability = 9.591018e-01
Photon flux (15-150 keV) in 5.048 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) = 8.73e-08
S(50-100 keV) = 1.23e-07
T90 vs. Hardness ratio plot
T90 = 3.95199990272522 sec.
Hardness ratio (energy fluence ratio) = 1.40893
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.83176
Count Ratio (50-100 keV) / (15-25 keV) = 1.01152
Mask shadow pattern
IMX = -1.308747690339830E-01, IMY = 4.221164039280391E-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:
-239.904000 -2.048000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5351 -40.5329 1.7 24.3 -73.7 1.8387 6.7 1.3 Vela X-1
151.8719 25.1273 3.1 45.7 137.7 3.8587 3.7 ------ UNKNOWN
160.1718 25.3614 2.8 49.8 146.2 4.5450 4.1 ------ UNKNOWN
108.9571 -7.5885 2.5 24.3 40.9 1.1458 4.6 ------ UNKNOWN
155.9693 4.4414 2.8 31.4 163.0 1.2295 4.1 ------ UNKNOWN
114.2628 -53.3720 2.3 39.6 -50.8 2.2450 5.1 ------ UNKNOWN
170.8698 -43.6563 3.2 42.6 -109.5 3.7182 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.048000 3.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6419 -40.6142 47.4 24.4 -73.9 0.0089 0.2 6.3 Vela X-1
143.5082 11.7155 2.3 30.2 134.9 0.2043 4.9 ------ UNKNOWN
171.6769 -15.1069 2.2 38.0 -153.8 0.2042 5.2 ------ UNKNOWN
150.2766 -33.7897 0.7 23.8 -107.2 0.5671 15.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
62.396640 962.194500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5434 -40.5346 0.8 13.5 -6.0 9.8239 14.2 1.4 Vela X-1
170.3475 -60.6191 4.9 29.9 -81.5 -2.4597 -2.4 1.0 Cen X-3
186.7574 -62.7994 14.1 36.9 -88.6 1.7076 0.8 3.3 GX 301-2
169.9998 5.1835 2.3 43.2 147.7 9.7034 5.0 ------ UNKNOWN
196.1837 1.2092 4.8 55.5 178.9 8.2241 2.4 ------ UNKNOWN
69.7233 -67.0119 2.9 55.6 -33.9 17.7810 4.0 ------ UNKNOWN
86.7206 -75.1989 3.8 50.8 -44.5 13.2501 3.1 ------ UNKNOWN
Plot creation:
Fri Mar 18 11:48:07 EDT 2016