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
301.6059 57.5638 0.0216 22.3794 -24.9060 1.4323674 8.930 TRIG_00711914
Foreground time interval of the image:
-15.099 73.301 (delta_t = 88.400 [sec])
Background time interval of the image:
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 64.000000
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 64.000000
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 64.000000
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 -33.112 sec. to 211.088 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43457 ( -0.108447 0.108985 )
Norm@50keV : 1.55989E-03 ( -9.3659e-05 9.33196e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.82 using 59 PHA bins.
# Reduced chi-squared = 0.6459 for 57 degrees of freedom
# Null hypothesis probability = 9.825965e-01
Photon flux (15-150 keV) in 244.2 sec: 0.191513 ( -0.011302 0.011314 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.65616e-06 ( -2.47643e-07 2.50229e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -33.112 sec. to 211.088 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17698 ( -0.456159 0.309532 )
Epeak [keV] : 158.823 ( -72.0188 -158.823 )
Norm@50keV : 2.10233E-03 ( -0.000609899 0.00141775 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.71 using 59 PHA bins.
# Reduced chi-squared = 0.6377 for 56 degrees of freedom
# Null hypothesis probability = 9.841947e-01
Photon flux (15-150 keV) in 244.2 sec: 0.188580 ( -0.012259 0.012221 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.56324e-06 ( -2.89494e-07 2.89726e-07 ) ergs/cm2
Band function
Time interval is from -33.112 sec. to 211.088 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 15.2088 (-1.15683 1.27608)
R^2/D10^2 : 2.04012E-02 (-0.00495224 0.00644293)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 91.02 using 59 PHA bins.
# Reduced chi-squared = 1.597 for 57 degrees of freedom
# Null hypothesis probability = 2.809585e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.407e-07 2.977e-08
25- 50 9.685e-07 7.277e-08
50-150 1.534e-06 1.875e-07
15-150 2.743e-06 2.027e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-27.91 -200)
Norm : 0.782996 (-0.0454631 0.0454631)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.87 using 59 PHA bins.
# Reduced chi-squared = 0.6819 for 57 degrees of freedom
# Null hypothesis probability = 9.683606e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.762e-07 3.468e-08
25- 50 9.160e-07 7.497e-08
50-150 2.009e-06 4.165e-07
15-150 3.401e-06 4.737e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.01373 (-1.84285 1.9765)
R1^2/D10^2 : 0.175933 (-0.0933317 0.330114)
kT2 [keV] : 25.7174 (-5.10188 9.85733)
R2^2/D10^2 : 2.72883E-03 (-0.00183836 0.00347271)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.98 using 59 PHA bins.
# Reduced chi-squared = 0.7088 for 55 degrees of freedom
# Null hypothesis probability = 9.496925e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.156e-07 1.059e-07
25- 50 9.016e-07 1.808e-07
50-150 2.196e-06 7.558e-07
15-150 3.514e-06 8.433e-07
Peak spectrum fit
Power-law model
Time interval is from 148.564 sec. to 149.564 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26758 ( -0.204819 0.203968 )
Norm@50keV : 1.35623E-02 ( -0.00156648 0.00155734 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.26 using 59 PHA bins.
# Reduced chi-squared = 0.9344 for 57 degrees of freedom
# Null hypothesis probability = 6.160660e-01
Photon flux (15-150 keV) in 1 sec: 1.60876 ( -0.18182 0.1819 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.35126e-07 ( -1.82084e-08 1.84842e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 148.564 sec. to 149.564 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26195 ( -0.355701 0.207032 )
Epeak [keV] : 9999.32 ( -9999.36 -9999.36 )
Norm@50keV : 1.36241E-02 ( -0.013623 0.00825932 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.28 using 59 PHA bins.
# Reduced chi-squared = 0.9514 for 56 degrees of freedom
# Null hypothesis probability = 5.784344e-01
Photon flux (15-150 keV) in 1 sec: 1.61747 ( -0.25174 0.23395 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.49593e-08 ( 0 0 ) ergs/cm2
Band function
Time interval is from 148.564 sec. to 149.564 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 15.8509 (-2.76868 3.6834)
R^2/D10^2 : 0.151156 (-0.0741223 0.136284)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 83.09 using 59 PHA bins.
# Reduced chi-squared = 1.458 for 57 degrees of freedom
# Null hypothesis probability = 1.365270e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.869e-09 1.991e-09
25- 50 3.285e-08 6.250e-09
50-150 5.747e-08 1.343e-08
15-150 9.819e-08 1.691e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-41.7941 -200)
Norm : 6.46608 (-0.742324 0.742324)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.33 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 57 degrees of freedom
# Null hypothesis probability = 3.907142e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.618e-08 9.130e-09
25- 50 3.113e-08 1.721e-08
50-150 6.828e-08 3.784e-08
15-150 1.156e-07 6.360e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.83308 (-1.86541 2.22879)
R1^2/D10^2 : 1.22689 (-0.690578 1.8495)
kT2 [keV] : 49.9141 (-20.1322 -49.9188)
R2^2/D10^2 : 3.92791E-03 (-0.00363157 0.0124302)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.95 using 59 PHA bins.
# Reduced chi-squared = 0.9083 for 55 degrees of freedom
# Null hypothesis probability = 6.673293e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.447e-08 4.482e-09
25- 50 3.032e-08 1.119e-08
50-150 9.982e-08 5.369e-08
15-150 1.446e-07 6.392e-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: 1.71694 ( -0.275367 0.292279 )
Norm@50keV : 9.30551E-04 ( -0.000170037 0.000164581 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.03 using 59 PHA bins.
# Reduced chi-squared = 0.6848 for 57 degrees of freedom
# Null hypothesis probability = 9.669039e-01
Photon flux (15-150 keV) in 88.4 sec: 0.124328 ( -0.0185902 0.0185902 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.6067e-07 ( -1.42506e-07 1.4788e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36076 ( -1.33063 0.928023 )
Epeak [keV] : 78.6647 ( -70.3917 -78.6667 )
Norm@50keV : 1.47345E-03 ( -0.0014734 0.00670916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.71 using 59 PHA bins.
# Reduced chi-squared = 0.6912 for 56 degrees of freedom
# Null hypothesis probability = 9.621379e-01
Photon flux (15-150 keV) in 88.4 sec: 0.122397 ( -0.019425 0.0193 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.30141e-07 ( -1.62432e-07 1.69206e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 8.74e-07
S(50-100 keV) = 1.29e-06
T90 vs. Hardness ratio plot
T90 = 207.307999968529 sec.
Hardness ratio (energy fluence ratio) = 1.47597
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38106
Count Ratio (50-100 keV) / (15-25 keV) = 1.12059
Mask shadow pattern
IMX = 3.734577096126134E-01, IMY = 1.734012259417237E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.099400 73.300590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3165 35.4220 26.2 36.6 -104.0 0.1576 0.4 8.4 Her X-1
268.3344 -1.3854 4.6 46.8 -162.5 -0.8111 -2.5 4.5 SW J1753.5-0127
273.9985 -14.1943 23.4 55.0 -177.1 -0.3734 -0.5 9.5 GX 17+2
288.6537 10.8431 4.9 26.3 176.9 0.4009 2.4 10.5 GRS 1915+105
299.6219 35.2040 0.6 0.1 81.4 2.9464 20.4 1.6 Cyg X-1
308.0537 41.1599 0.0 8.9 18.0 -0.0800 -0.5 12.7 Cyg X-3
326.1717 38.3224 15.1 21.5 46.0 -0.1291 -0.8 0.0 Cyg X-2
349.4214 29.1824 2.9 42.2 55.9 2.2970 4.0 ------ UNKNOWN
331.6195 64.4827 2.8 35.0 -4.3 0.7713 4.2 ------ UNKNOWN
301.6058 57.5638 1.3 22.4 -24.9 1.4319 8.9 ------ UNKNOWN
249.1229 41.8426 2.9 39.4 -92.5 2.3144 4.0 ------ UNKNOWN
249.4127 32.3497 2.5 41.3 -106.9 2.7992 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
117.900600 337.511500
361.000200 365.720000
421.000000 430.094900
482.000000 482.318100
541.000000 547.816500
601.000000 617.898700
776.000000 778.846500
780.000000 903.088400
920.000000 959.079600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4901 35.3194 21.0 38.2 -142.1 -0.2501 -0.6 2.1 Her X-1
288.7467 10.8958 6.0 47.7 159.9 1.6248 1.9 4.3 GRS 1915+105
299.6146 35.2089 0.4 22.4 146.9 7.5943 26.6 1.3 Cyg X-1
308.3908 40.9608 0.0 17.2 125.0 -0.5698 -1.9 12.7 Cyg X-3
326.3085 38.3907 16.8 25.1 91.9 0.2761 0.7 7.7 Cyg X-2
318.3591 35.1321 2.8 25.1 108.8 1.4252 4.1 ------ UNKNOWN
37.4954 52.3703 2.9 50.6 14.5 3.0252 4.1 ------ UNKNOWN
12.6179 63.3848 3.4 33.7 12.6 1.1204 3.3 ------ UNKNOWN
301.5488 57.5503 0.6 0.0 34.2 4.5918 18.0 ------ UNKNOWN
275.0715 56.1138 2.1 14.5 -121.6 1.4588 5.6 ------ UNKNOWN
100.1020 63.8875 4.3 57.5 -26.2 4.7473 2.9 ------ UNKNOWN
100.2897 63.7649 4.1 57.6 -26.3 5.6368 3.5 ------ UNKNOWN
Plot creation:
Thu Oct 6 15:52:25 EDT 2016