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
7.3580 9.2245 0.0064 28.0316 132.9764 6.2914612 29.875 TRIG_00756284
Foreground time interval of the image:
-122.995 13.805 (delta_t = 136.800 [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 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 -207.896 sec. to 144.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62528 ( -0.0721692 0.072468 )
Norm@50keV : 2.32298E-03 ( -8.958e-05 8.93247e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.22 using 59 PHA bins.
# Reduced chi-squared = 0.7408 for 57 degrees of freedom
# Null hypothesis probability = 9.280700e-01
Photon flux (15-150 keV) in 352 sec: 0.300910 ( -0.012181 0.01223 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.62576e-06 ( -3.11465e-07 3.12448e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -207.896 sec. to 144.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62335 ( -0.243878 0.111382 )
Epeak [keV] : 9996.03 ( -9995.7 -9995.7 )
Norm@50keV : 2.32821E-03 ( -8.9223e-05 0.000848082 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.22 using 59 PHA bins.
# Reduced chi-squared = 0.7540 for 56 degrees of freedom
# Null hypothesis probability = 9.134945e-01
Photon flux (15-150 keV) in 352 sec: 0.300692 ( -0.013345 0.012407 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.6189e-06 ( -3.55119e-07 3.18581e-07 ) ergs/cm2
Band function
Time interval is from -207.896 sec. to 144.104 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] : 14.4877 ( )
R^2/D10^2 : 3.57598E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 224.50 using 59 PHA bins.
# Reduced chi-squared = 3.9386 for 57 degrees of freedom
# Null hypothesis probability = 9.822845e-22
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.559e-07 4.365e-08
25- 50 2.138e-06 1.056e-07
50-150 3.006e-06 2.306e-07
15-150 5.700e-06 2.429e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 179.451 (-34.7772 -179.004)
Norm : 1.21014 (-0.0520357 0.0574796)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.37 using 59 PHA bins.
# Reduced chi-squared = 0.8136 for 57 degrees of freedom
# Null hypothesis probability = 8.416296e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.075e-06 6.600e-08
25- 50 2.041e-06 2.072e-07
50-150 4.317e-06 1.281e-06
15-150 7.432e-06 1.452e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.31013 (-0.847887 0.899953)
R1^2/D10^2 : 0.297594 (-0.0971898 0.162458)
kT2 [keV] : 29.3227 (-4.16412 6.19915)
R2^2/D10^2 : 2.32851E-03 (-0.00110105 0.00169078)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.32 using 59 PHA bins.
# Reduced chi-squared = 0.8239 for 55 degrees of freedom
# Null hypothesis probability = 8.210034e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.050e-06 1.183e-07
25- 50 2.079e-06 1.734e-07
50-150 4.455e-06 7.836e-07
15-150 7.584e-06 8.096e-07
Peak spectrum fit
Power-law model
Time interval is from 7.604 sec. to 8.604 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66607 ( -0.163981 0.167266 )
Norm@50keV : 2.06408E-02 ( -0.00210146 0.00207279 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.95 using 59 PHA bins.
# Reduced chi-squared = 1.017 for 57 degrees of freedom
# Null hypothesis probability = 4.399693e-01
Photon flux (15-150 keV) in 1 sec: 2.70974 ( -0.25239 0.25253 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.91695e-07 ( -2.06186e-08 2.08691e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.604 sec. to 8.604 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58305 ( -0.627121 0.717751 )
Epeak [keV] : 220.114 ( )
Norm@50keV : 2.28991E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.89 using 59 PHA bins.
# Reduced chi-squared = 1.034 for 56 degrees of freedom
# Null hypothesis probability = 4.053505e-01
Photon flux (15-150 keV) in 1 sec: 2.70123 ( -0.25364 0.25808 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90187e-07 ( -2.31049e-08 2.20201e-08 ) ergs/cm2
Band function
Time interval is from 7.604 sec. to 8.604 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] : 11.9112 (-1.48229 1.78556)
R^2/D10^2 : 0.668293 (-0.266583 0.421582)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 93.68 using 59 PHA bins.
# Reduced chi-squared = 1.644 for 57 degrees of freedom
# Null hypothesis probability = 1.582049e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.004e-08 3.445e-09
25- 50 6.252e-08 7.715e-09
50-150 5.307e-08 1.159e-08
15-150 1.356e-07 1.505e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 148.970 (-54.113 -147.594)
Norm : 11.1444 (-1.14883 1.4665)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.58 using 59 PHA bins.
# Reduced chi-squared = 1.028 for 57 degrees of freedom
# Null hypothesis probability = 4.170765e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.864e-08 5.515e-09
25- 50 5.303e-08 1.581e-08
50-150 1.044e-07 5.448e-08
15-150 1.861e-07 7.243e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.95577 (-1.28661 1.40901)
R1^2/D10^2 : 3.55794 (-1.69016 3.83085)
kT2 [keV] : 30.1867 (-7.96036 16.7878)
R2^2/D10^2 : 1.86783E-02 (-0.0137519 0.0354152)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.06 using 59 PHA bins.
# Reduced chi-squared = 0.9828 for 55 degrees of freedom
# Null hypothesis probability = 5.107034e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.013e-08 9.945e-09
25- 50 5.357e-08 1.602e-08
50-150 1.114e-07 5.735e-08
15-150 1.950e-07 7.053e-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: 1.46504 ( -0.0881133 0.0881966 )
Norm@50keV : 3.07804E-03 ( -0.000148099 0.000147811 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.29 using 59 PHA bins.
# Reduced chi-squared = 0.7419 for 57 degrees of freedom
# Null hypothesis probability = 9.270420e-01
Photon flux (15-150 keV) in 136.8 sec: 0.380761 ( -0.0189562 0.0190087 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.01845e-06 ( -2.11485e-07 2.12404e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38174 ( -0.335087 0.162168 )
Epeak [keV] : 384.874 ( -384.874 -384.874 )
Norm@50keV : 3.38020E-03 ( -0.00043435 0.00149246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.09 using 59 PHA bins.
# Reduced chi-squared = 0.7516 for 56 degrees of freedom
# Null hypothesis probability = 9.158703e-01
Photon flux (15-150 keV) in 136.8 sec: 0.378884 ( -0.020142 0.020068 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.99429e-06 ( -2.2992e-07 2.29619e-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) = 2.00e-06
S(50-100 keV) = 2.59e-06
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 1.295
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29068
Count Ratio (50-100 keV) / (15-25 keV) = 0.919339
Mask shadow pattern
IMX = -3.629465970071011E-01, IMY = -3.895343691985889E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-122.995400 13.804600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
357.3081 15.8868 1.8 39.6 137.9 2.3065 6.3 ------ UNKNOWN
357.4795 25.7640 2.4 43.9 151.3 1.9051 4.8 ------ UNKNOWN
7.3580 9.2245 0.4 28.0 133.0 6.2906 29.9 ------ UNKNOWN
13.4773 25.3928 2.3 32.7 166.2 1.1081 5.0 ------ UNKNOWN
2.0004 49.8441 1.9 57.4 177.7 6.0188 6.0 ------ UNKNOWN
63.4691 -51.7358 3.5 56.8 -0.2 2.6704 3.3 ------ UNKNOWN
69.5285 -23.8268 2.6 41.7 -32.3 1.2838 4.4 ------ UNKNOWN
73.3284 4.4960 3.5 40.0 -76.6 2.2105 3.3 ------ UNKNOWN
77.1245 -3.6513 3.4 43.5 -64.2 2.5482 3.4 ------ UNKNOWN
61.9377 39.6879 3.0 48.1 -129.2 3.4264 3.9 ------ UNKNOWN
62.7977 37.9781 2.8 47.2 -127.0 3.6046 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
62.404590 836.886000
900.104000 962.157600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2369 38.2280 7.0 46.9 156.1 2.6455 1.7 6.4 Cyg X-2
13.5503 -13.5443 3.3 23.6 6.0 1.7877 3.5 ------ UNKNOWN
29.5390 -40.4280 2.5 53.7 0.3 6.9802 4.6 ------ UNKNOWN
15.4297 -2.3488 2.7 14.1 -14.0 2.0825 4.2 ------ UNKNOWN
40.8430 48.1001 3.0 48.0 -129.1 10.9304 3.8 ------ UNKNOWN
46.9500 26.2135 4.9 41.1 -98.4 6.5090 2.4 ------ UNKNOWN
52.4685 -4.2975 3.4 46.9 -54.0 9.6062 3.4 ------ UNKNOWN
Plot creation:
Thu Jun 22 11:31:05 EDT 2017