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
34.3208 1.9621 0.0193 24.0888 112.4001 3.5461153 9.983 TRIG_00762535
Foreground time interval of the image:
-11.899 336.701 (delta_t = 348.600 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -74.360 sec. to 464.232 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67345 ( -0.167627 0.172309 )
Norm@50keV : 5.73229E-04 ( -5.81432e-05 5.72335e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.20 using 59 PHA bins.
# Reduced chi-squared = 0.9509 for 57 degrees of freedom
# Null hypothesis probability = 5.806704e-01
Photon flux (15-150 keV) in 538.6 sec: 7.54419E-02 ( -0.0068863 0.0068932 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.86534e-06 ( -3.06777e-07 3.11945e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -74.360 sec. to 464.232 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49455 ( -0.719334 0.34264 )
Epeak [keV] : 132.203 ( -107.404 -132.402 )
Norm@50keV : 7.13889E-04 ( -0.000306589 0.000985055 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.98 using 59 PHA bins.
# Reduced chi-squared = 0.9640 for 56 degrees of freedom
# Null hypothesis probability = 5.516383e-01
Photon flux (15-150 keV) in 538.6 sec: 7.47746E-02 ( -0.0073027 0.0072512 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.81499e-06 ( -3.55037e-07 3.47846e-07 ) ergs/cm2
Band function
Time interval is from -74.360 sec. to 464.232 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] : 12.7106 (-1.4604 1.67975)
R^2/D10^2 : 1.46572E-02 (-0.00528677 0.0081549)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.49 using 59 PHA bins.
# Reduced chi-squared = 1.447 for 57 degrees of freedom
# Null hypothesis probability = 1.526917e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.705e-07 4.643e-08
25- 50 9.090e-07 1.142e-07
50-150 9.161e-07 1.917e-07
15-150 2.096e-06 2.542e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 144.069 (-51.0994 -142.981)
Norm : 0.311100 (-0.031871 0.040511)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.29 using 59 PHA bins.
# Reduced chi-squared = 0.9525 for 57 degrees of freedom
# Null hypothesis probability = 5.772377e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.318e-07 6.113e-08
25- 50 7.956e-07 1.363e-07
50-150 1.544e-06 7.881e-07
15-150 2.771e-06 9.428e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.02569 (-1.98616 2.27047)
R1^2/D10^2 : 0.139698 (-0.0907635 0.52482)
kT2 [keV] : 22.0972 (-5.40317 12.7327)
R2^2/D10^2 : 1.57836E-03 (-0.00126927 0.00312654)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.67 using 59 PHA bins.
# Reduced chi-squared = 1.012 for 55 degrees of freedom
# Null hypothesis probability = 4.495762e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.419e-07 2.083e-07
25- 50 7.741e-07 2.852e-07
50-150 1.517e-06 8.228e-07
15-150 2.733e-06 1.220e-06
Peak spectrum fit
Power-law model
Time interval is from 0.220 sec. to 1.220 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96655 ( -1.46268 1.46531 )
Norm@50keV : 2.28019E-03 ( -0.00227899 0.00151047 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.77 using 59 PHA bins.
# Reduced chi-squared = 0.9785 for 57 degrees of freedom
# Null hypothesis probability = 5.211329e-01
Photon flux (15-150 keV) in 1 sec: 0.336889 ( -0.167646 0.167631 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.09889e-08 ( -1.28744e-08 1.53825e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.220 sec. to 1.220 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.95594 ( )
Epeak [keV] : 9999.36 ( )
Norm@50keV : 2.29139E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.78 using 59 PHA bins.
# Reduced chi-squared = 0.9960 for 56 degrees of freedom
# Null hypothesis probability = 4.833302e-01
Photon flux (15-150 keV) in 1 sec: 0.250353 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69348e-08 ( -1.68792e-08 1.48478e-08 ) ergs/cm2
Band function
Time interval is from 0.220 sec. to 1.220 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] : 7.22894 (-2.6124 4.06953)
R^2/D10^2 : 0.578242 (-0.578729 2.92696)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.52 using 59 PHA bins.
# Reduced chi-squared = 0.9741 for 57 degrees of freedom
# Null hypothesis probability = 5.306627e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.013e-09 3.253e-09
25- 50 7.302e-09 5.260e-09
50-150 1.357e-09 1.220e-09
15-150 1.367e-08 9.700e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 38.3967 (-38.4425 -38.4425)
Norm : 2.16944 (-2.1672 4.36691)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.30 using 59 PHA bins.
# Reduced chi-squared = 0.9876 for 57 degrees of freedom
# Null hypothesis probability = 5.014634e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.911e-09 3.203e-09
25- 50 6.346e-09 4.336e-09
50-150 4.692e-09 4.547e-09
15-150 1.595e-08 1.175e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 200.000 (-200 -200)
R1^2/D10^2 : 8.14351E-05 (-5.56082e-05 5.46794e-05)
kT2 [keV] : 6.32038 (-2.39534 3.34405)
R2^2/D10^2 : 0.889609 (-0.756156 5.57541)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.52 using 59 PHA bins.
#Fit statistic : Chi-Squared = 49.75 using 59 PHA bins.
# Reduced chi-squared = 1.010 for 55 degrees of freedom
# Reduced chi-squared = 0.9046 for 55 degrees of freedom
# Null hypothesis probability = 4.549107e-01
# Null hypothesis probability = 6.747520e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.013e-09 2.928e-01
25- 50 7.302e-09 2.699e+00
50-150 1.357e-09 6.065e+01
15-150 1.367e-08 6.955e+01
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: 1.70218 ( -0.197964 0.205422 )
Norm@50keV : 6.24663E-04 ( -7.78085e-05 7.63359e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.60 using 59 PHA bins.
# Reduced chi-squared = 0.9579 for 57 degrees of freedom
# Null hypothesis probability = 5.655944e-01
Photon flux (15-150 keV) in 348.6 sec: 8.30254E-02 ( -0.00910845 0.00911317 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01585e-06 ( -2.61851e-07 2.66872e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26684 ( -0.970525 0.605324 )
Epeak [keV] : 77.0118 ( -56.0416 -77.0118 )
Norm@50keV : 1.07496E-03 ( -0.000343986 0.00250327 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.79 using 59 PHA bins.
# Reduced chi-squared = 0.9605 for 56 degrees of freedom
# Null hypothesis probability = 5.591152e-01
Photon flux (15-150 keV) in 348.6 sec: 8.13810E-02 ( -0.0096378 0.0096003 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.93164e-06 ( -3.01595e-07 3.08257e-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) = 7.65e-07
S(50-100 keV) = 9.64e-07
T90 vs. Hardness ratio plot
T90 = 459.216000020504 sec.
Hardness ratio (energy fluence ratio) = 1.26013
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.27093
Count Ratio (50-100 keV) / (15-25 keV) = 0.78147
Mask shadow pattern
IMX = -1.703726376191623E-01, IMY = -4.133521449098388E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-11.899400 336.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6275 22.0153 0.4 33.1 -115.8 14.2201 26.0 0.3 Crab
22.6830 1.6110 3.5 35.7 110.3 2.2994 3.3 ------ UNKNOWN
34.3208 1.9621 1.2 24.1 112.4 3.5460 10.0 ------ UNKNOWN
28.5291 51.0376 2.8 56.9 175.7 7.8687 4.1 ------ UNKNOWN
63.4137 -22.9184 2.2 23.4 5.8 1.4616 5.3 ------ UNKNOWN
32.2354 52.5679 2.7 56.9 179.0 8.4796 4.3 ------ UNKNOWN
86.8140 -53.2844 3.3 58.3 -2.0 6.3450 3.5 ------ UNKNOWN
97.9820 -45.7051 2.3 57.5 -14.3 7.2418 5.0 ------ UNKNOWN
89.7906 38.3120 2.6 48.0 -129.0 6.8270 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
382.100590 963.120400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
358.6768 0.8028 3.2 35.7 110.4 3.4049 3.6 92.9 UNKNOWN
355.3696 23.0613 2.2 43.3 144.2 5.1609 5.1 ------ UNKNOWN
34.3029 1.9818 1.2 0.0 116.1 3.4265 9.3 ------ UNKNOWN
70.9902 2.7012 3.7 36.6 -70.1 2.9467 3.1 ------ UNKNOWN
Plot creation:
Wed Aug 2 18:48:06 EDT 2017