Special notes of this burst
Image
Pre-slew 25.0-100.0 keV image (Event data)
#RAcent DECcent POSerr Theta Phi Peak_Cts SNR Name
108.278 -25.100 0.000 23.376 -39.373 0.160 8.547 TRIG_00361489
Image time interval: 0.000 to 5.504 [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 5.504000
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 5.504000
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 5.504000
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 0.408 sec. to 81.176 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31130 ( -0.518873 0.495123 )
Norm@50keV : 4.77831E-04 ( -0.00012434 0.00012331 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.36 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 57 degrees of freedom
# Null hypothesis probability = 3.895380e-01
Photon flux (15-150 keV) in 80.77 sec: 5.71261E-02 ( -0.0150066 0.0150376 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.80343e-07 ( -1.11247e-07 1.14132e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.408 sec. to 81.176 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32983 ( -0.650855 0.481424 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 4.75610E-04 ( -0.000123567 0.00116803 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.38 using 59 PHA bins.
# Reduced chi-squared = 1.060 for 56 degrees of freedom
# Null hypothesis probability = 3.536285e-01
Photon flux (15-150 keV) in 80.77 sec: 5.73496E-02 ( -0.0152209 0.014841 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.79517e-07 ( -1.10426e-07 1.11173e-07 ) ergs/cm2
Band function
Time interval is from 0.408 sec. to 81.176 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.13093 ( 0.930744 0.930744 )
beta : -1.36154 ( 1.32351 0.528707 )
Epeak [keV] : 23.5914 ( -66.7726 -66.7726 )
Norm@50keV : 13.2753 ( -13.2765 42303.9 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.26 using 59 PHA bins.
# Reduced chi-squared = 1.077 for 55 degrees of freedom
# Null hypothesis probability = 3.229110e-01
Photon flux (15-150 keV) in 80.77 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] : 16.2401 (-6.85144 16.3592)
R^2/D10^2 : 4.74837E-03 (-0.00455433 0.0263615)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.98 using 59 PHA bins.
# Reduced chi-squared = 1.175 for 57 degrees of freedom
# Null hypothesis probability = 1.718554e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.084e-08 1.370e-08
25- 50 8.882e-08 5.258e-08
50-150 1.647e-07 1.083e-07
15-150 2.743e-07 1.762e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-111.497 -199.363)
Norm : 0.234415 (-0.0609904 0.0609895)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.53 using 59 PHA bins.
# Reduced chi-squared = 1.062 for 57 degrees of freedom
# Null hypothesis probability = 3.496929e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.715e-08 2.869e-08
25- 50 9.070e-08 5.468e-08
50-150 1.989e-07 1.201e-07
15-150 3.367e-07 1.998e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.45955 (-3.08425 2.96607)
R1^2/D10^2 : 5.73119E-02 (-0.0470825 0.366917)
kT2 [keV] : 62.4505 (-58.0747 -62.4505)
R2^2/D10^2 : 8.44743E-05 (-7.25731e-05 0.000855189)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.62 using 59 PHA bins.
# Reduced chi-squared = 1.048 for 55 degrees of freedom
# Null hypothesis probability = 3.784142e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.643e-08 2.805e-08
25- 50 8.632e-08 5.266e-08
50-150 2.864e-07 1.575e-07
15-150 4.191e-07 2.140e-07
Peak spectrum fit
Power-law model
Time interval is from 1.924 sec. to 2.924 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18024 ( -0.496432 0.459058 )
Norm@50keV : 4.65709E-03 ( -0.00115817 0.00115718 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.53 using 59 PHA bins.
# Reduced chi-squared = 0.6935 for 57 degrees of freedom
# Null hypothesis probability = 9.622621e-01
Photon flux (15-150 keV) in 1 sec: 0.545170 ( -0.140492 0.140971 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.75161e-08 ( -1.30501e-08 1.32773e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.924 sec. to 2.924 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.77687 ( )
Epeak [keV] : 229.822 ( )
Norm@50keV : 5.46734E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.36 using 59 PHA bins.
# Reduced chi-squared = 0.7029 for 56 degrees of freedom
# Null hypothesis probability = 9.551550e-01
Photon flux (15-150 keV) in 1 sec: 0.547391 ( -0.142488 0.138808 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.74882e-08 ( -7.0063e-09 1.30033e-08 ) ergs/cm2
Band function
Time interval is from 1.924 sec. to 2.924 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.94403 ( -4.94403 -4.94403 )
beta : -1.24545 ( -0.548722 0.52624 )
Epeak [keV] : 23.9946 ( -23.9946 63.1594 )
Norm@50keV : 442.403 ( -109.468 2.11801e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.18 using 59 PHA bins.
# Reduced chi-squared = 0.7123 for 55 degrees of freedom
# Null hypothesis probability = 9.472263e-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] : 16.4647 (-6.08004 15.7375)
R^2/D10^2 : 4.51001E-02 (-0.0385353 0.171057)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.60 using 59 PHA bins.
# Reduced chi-squared = 0.8176 for 57 degrees of freedom
# Null hypothesis probability = 8.357011e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.511e-09 1.547e-09
25- 50 1.082e-08 5.886e-09
50-150 2.073e-08 1.338e-08
15-150 3.406e-08 2.046e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-95.8168 -199.363)
Norm : 2.25460 (-0.574453 0.574475)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.69 using 59 PHA bins.
# Reduced chi-squared = 0.7314 for 57 degrees of freedom
# Null hypothesis probability = 9.361043e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.614e-09 3.380e-09
25- 50 1.080e-08 6.525e-09
50-150 2.368e-08 1.430e-08
15-150 4.010e-08 2.384e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.38167 (-2.95671 4.38581)
R1^2/D10^2 : 0.253283 (-0.211624 0.850823)
kT2 [keV] : 200.000 (-166.56 -200)
R2^2/D10^2 : 1.11952E-04 (-4.86313e-05 0.000568247)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.76 using 59 PHA bins.
#Fit statistic : Chi-Squared = 36.62 using 59 PHA bins.
# Reduced chi-squared = 0.6683 for 55 degrees of freedom
# Reduced chi-squared = 0.6658 for 55 degrees of freedom
# Null hypothesis probability = 9.722602e-01
# Null hypothesis probability = 9.733350e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.649e-09 2.855e-09
25- 50 1.108e-08 6.855e-09
50-150 3.479e-08 2.210e-08
15-150 5.052e-08 2.678e-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: 1.28424 ( -0.540401 0.520203 )
Norm@50keV : 5.78047E-04 ( -0.000154564 0.000153968 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.62 using 59 PHA bins.
# Reduced chi-squared = 0.8706 for 57 degrees of freedom
# Null hypothesis probability = 7.454133e-01
Photon flux (15-150 keV) in 54.12 sec: 6.87666E-02 ( -0.0188063 0.0188577 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.1035e-07 ( -9.3363e-08 9.54579e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29591 ( -0.55879 0.509539 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.76860E-04 ( -0.000155167 0.00161678 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.63 using 59 PHA bins.
# Reduced chi-squared = 0.8863 for 56 degrees of freedom
# Null hypothesis probability = 7.131526e-01
Photon flux (15-150 keV) in 54.12 sec: 6.90512E-02 ( -0.0190577 0.0185875 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10261e-07 ( -9.3239e-08 9.33841e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.995886 ( 0.996839 0.996839 )
beta : -1.28453 ( 1.28424 0.540286 )
Epeak [keV] : 56.5733 ( -56.1208 -56.1208 )
Norm@50keV : 1.06695E-03 ( -0.000642803 0.0984223 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.62 using 59 PHA bins.
# Reduced chi-squared = 0.9022 for 55 degrees of freedom
# Null hypothesis probability = 6.795356e-01
Photon flux (15-150 keV) in 54.12 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) = 8.52e-08
S(50-100 keV) = 1.37e-07
T90 vs. Hardness ratio plot
T90 = 77.9520000219345 sec.
Hardness ratio (energy fluence ratio) = 1.60798
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.04994
Count Ratio (50-100 keV) / (15-25 keV) = 0.847935
Mask shadow pattern
IMX = 0.334132621021, IMY = 0.274198475222
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 5.504000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 5.504000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 5.504000
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:
-239.976000 0.408000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6448 22.0147 0.3 32.8 179.4 9.7479 39.6 0.6 Crab
135.5127 -40.5983 2.2 50.8 -36.2 4.1535 5.3 2.7 Vela X-1
96.2037 1.5188 3.1 13.8 -140.2 0.6907 3.8 ------ UNKNOWN
135.9203 -27.3662 3.2 47.1 -53.1 3.4014 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.408000 54.524600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5060 21.9544 8.2 32.8 179.2 0.1361 1.4 7.9 Crab
135.6260 -40.3996 6.3 50.8 -36.5 0.5570 1.8 10.3 Vela X-1
50.7460 14.5348 2.6 45.5 131.4 1.5700 4.4 ------ UNKNOWN
52.0311 -47.2824 2.1 48.4 42.1 1.9772 5.5 ------ UNKNOWN
70.0226 31.2833 2.6 45.5 165.8 0.8001 4.5 ------ UNKNOWN
108.3298 -25.1560 1.9 23.4 -39.3 0.5489 6.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
101.524580 962.066100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6390 22.0182 0.6 52.8 177.8 32.6171 19.0 0.4 Crab
135.5204 -40.5576 0.3 27.4 -22.2 16.6772 34.4 0.4 Vela X-1
170.3666 -60.6540 12.6 54.7 -5.2 -1.2820 -0.9 2.4 Cen X-3
62.8100 -28.1591 3.7 40.5 102.1 6.0871 3.2 ------ UNKNOWN
72.4185 -41.0040 2.5 33.7 79.7 4.3278 4.6 ------ UNKNOWN
78.7116 22.8248 2.8 55.9 173.5 11.4031 4.2 ------ UNKNOWN
173.6351 -63.7362 2.9 56.8 -1.9 9.9465 4.0 ------ UNKNOWN
139.0214 -53.2853 2.7 36.4 -4.2 3.2061 4.3 ------ UNKNOWN
176.6833 -57.4672 2.7 57.5 -9.5 9.2828 4.3 ------ UNKNOWN
100.8424 26.8958 3.6 52.5 -161.6 4.8308 3.2 ------ UNKNOWN
161.0139 -42.5269 3.5 46.3 -27.4 2.9311 3.3 ------ UNKNOWN
165.7237 -40.8739 2.2 49.7 -29.8 6.1525 5.2 ------ UNKNOWN
160.3025 -23.9089 3.2 47.0 -53.1 9.1808 3.7 ------ UNKNOWN
Plot creation:
Thu Oct 8 20:29:23 EDT 2015