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
131.609 -60.174 0.000 19.729 -33.287 0.090 7.744 TRIG_00580267
Image time interval: 0.000 to 2.048 [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 2.048000
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 2.048000
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 2.048000
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)
The mask-weighted light curves based on cleaned DPHs
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 -0.252 sec. to 20.508 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52162 ( -0.434804 0.457954 )
Norm@50keV : 9.62577E-04 ( -0.000248419 0.000238747 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.09 using 59 PHA bins.
# Reduced chi-squared = 0.9314 for 57 degrees of freedom
# Null hypothesis probability = 6.225723e-01
Photon flux (15-150 keV) in 20.76 sec: 0.120879 ( -0.0284262 0.0284707 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8892e-07 ( -5.24082e-08 5.40213e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.252 sec. to 20.508 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50972 ( -1.47152 3.1125 )
Epeak [keV] : 9988.13 ( -9999.3 -9999.3 )
Norm@50keV : 9.75101E-04 ( -0.000249684 0.00393607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.09 using 59 PHA bins.
# Reduced chi-squared = 0.9481 for 56 degrees of freedom
# Null hypothesis probability = 5.855774e-01
Photon flux (15-150 keV) in 20.76 sec: 0.120896 ( -0.0286954 0.028389 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.88818e-07 ( -5.3642e-08 5.38251e-08 ) ergs/cm2
Band function
Time interval is from -0.252 sec. to 20.508 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51065 ( -2.03567 1.47097 )
beta : -9.37096 ( 5.95674 9.37096 )
Epeak [keV] : 9974.59 ( -9949.64 -9999.36 )
Norm@50keV : 9.73738E-04 ( -0.000250273 0.00394292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.09 using 59 PHA bins.
# Reduced chi-squared = 0.9653 for 55 degrees of freedom
# Null hypothesis probability = 5.478298e-01
Photon flux (15-150 keV) in 20.76 sec: 0.120863 ( 6.87914 -0.0284609 ) 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] : 17.0237 (-5.48955 7.44981)
R^2/D10^2 : 8.65607E-03 (-0.0060054 0.0237213)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.13 using 59 PHA bins.
# Reduced chi-squared = 1.055 for 57 degrees of freedom
# Null hypothesis probability = 3.629953e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.060e-08 5.893e-09
25- 50 4.696e-08 2.307e-08
50-150 9.722e-08 5.785e-08
15-150 1.548e-07 8.322e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-124.029 -199.363)
Norm : 0.491767 (-0.115244 0.115338)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.39 using 59 PHA bins.
# Reduced chi-squared = 0.9366 for 57 degrees of freedom
# Null hypothesis probability = 6.114251e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.542e-08 1.507e-08
25- 50 4.890e-08 2.922e-08
50-150 1.073e-07 6.382e-08
15-150 1.816e-07 1.074e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.54303 (-2.03985 4.26107)
R1^2/D10^2 : 0.727545 (-0.646059 3.77422)
kT2 [keV] : 24.7494 (-8.08905 19.4485)
R2^2/D10^2 : 2.16484E-03 (-0.00180251 0.00335056)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.25 using 59 PHA bins.
# Reduced chi-squared = 0.9318 for 55 degrees of freedom
# Null hypothesis probability = 6.188215e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.944e-08 1.741e-08
25- 50 3.974e-08 2.081e-08
50-150 1.237e-07 7.680e-08
15-150 1.929e-07 1.069e-07
Peak spectrum fit
Power-law model
Time interval is from 19.312 sec. to 20.312 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20217 ( -0.399472 0.388453 )
Norm@50keV : 5.67929E-03 ( -0.00116424 0.0011638 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.68 using 59 PHA bins.
# Reduced chi-squared = 0.6259 for 57 degrees of freedom
# Null hypothesis probability = 9.879541e-01
Photon flux (15-150 keV) in 1 sec: 0.666835 ( -0.139495 0.140117 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.75834e-08 ( -1.34364e-08 1.36669e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 19.312 sec. to 20.312 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20439 ( -0.408599 0.384647 )
Epeak [keV] : 9999.32 ( -9999.36 -9999.36 )
Norm@50keV : 5.70440E-03 ( -0.00116884 0.010803 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.69 using 59 PHA bins.
# Reduced chi-squared = 0.6373 for 56 degrees of freedom
# Null hypothesis probability = 9.843297e-01
Photon flux (15-150 keV) in 1 sec: 0.668355 ( -0.141248 0.138458 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.77297e-08 ( -1.3563e-08 1.3258e-08 ) ergs/cm2
Band function
Time interval is from 19.312 sec. to 20.312 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.977334 ( 0.977332 0.977332 )
beta : -1.20215 ( 1.20216 0.399446 )
Epeak [keV] : 46.6511 ( -46.6533 -46.6533 )
Norm@50keV : 1.01534E-02 ( -0.00562907 0.920013 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.68 using 59 PHA bins.
# Reduced chi-squared = 0.6487 for 55 degrees of freedom
# Null hypothesis probability = 9.798898e-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] : 19.0429 (-5.4045 8.73494)
R^2/D10^2 : 3.47494E-02 (-0.0240168 0.0694206)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.98 using 59 PHA bins.
# Reduced chi-squared = 0.7715 for 57 degrees of freedom
# Null hypothesis probability = 8.968368e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.475e-09 1.095e-09
25- 50 1.192e-08 4.929e-09
50-150 3.179e-08 1.420e-08
15-150 4.619e-08 1.725e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-80.3865 -200)
Norm : 2.72862 (-0.571518 0.571518)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.48 using 59 PHA bins.
# Reduced chi-squared = 0.6752 for 57 degrees of freedom
# Null hypothesis probability = 9.715313e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.795e-09 4.050e-09
25- 50 1.307e-08 7.590e-09
50-150 2.866e-08 1.683e-08
15-150 4.853e-08 2.805e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.58472 (-5.36872 6.92942)
R1^2/D10^2 : 0.501776 (-0.353562 0.917489)
kT2 [keV] : 42.4525 (-28.8711 -49.4883)
R2^2/D10^2 : 2.48879E-03 (-0.00159801 0.0230549)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.07 using 59 PHA bins.
# Reduced chi-squared = 0.6558 for 55 degrees of freedom
# Null hypothesis probability = 9.773389e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.557e-09 3.463e-09
25- 50 1.181e-08 6.525e-09
50-150 4.121e-08 2.363e-08
15-150 5.858e-08 3.148e-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: 1.52162 ( -0.434804 0.457954 )
Norm@50keV : 9.62577E-04 ( -0.000248419 0.000238747 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.09 using 59 PHA bins.
# Reduced chi-squared = 0.9314 for 57 degrees of freedom
# Null hypothesis probability = 6.225723e-01
Photon flux (15-150 keV) in 20.76 sec: 0.120879 ( -0.0284262 0.0284707 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8892e-07 ( -5.24082e-08 5.40213e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50972 ( -1.47152 3.1125 )
Epeak [keV] : 9988.13 ( -9999.3 -9999.3 )
Norm@50keV : 9.75101E-04 ( -0.000249684 0.00393607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.09 using 59 PHA bins.
# Reduced chi-squared = 0.9481 for 56 degrees of freedom
# Null hypothesis probability = 5.855774e-01
Photon flux (15-150 keV) in 20.76 sec: 0.120896 ( -0.0286954 0.028389 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.88818e-07 ( -5.3642e-08 5.38251e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51065 ( -1.16665 1.47449 )
beta : -9.37096 ( 5.95674 9.37096 )
Epeak [keV] : 9974.59 ( -9949.66 -9999.36 )
Norm@50keV : 9.73738E-04 ( -0.000250273 0.00394292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.09 using 59 PHA bins.
# Reduced chi-squared = 0.9653 for 55 degrees of freedom
# Null hypothesis probability = 5.478298e-01
Photon flux (15-150 keV) in 20.76 sec: 0.120863 ( 6.87914 -0.0284609 ) 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) = 4.72e-08
S(50-100 keV) = 6.58e-08
T90 vs. Hardness ratio plot
T90 = 20.3439999222755 sec.
Hardness ratio (energy fluence ratio) = 1.39407
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.825079
Count Ratio (50-100 keV) / (15-25 keV) = 1.06461
Mask shadow pattern
IMX = 0.29977964718, IMY = 0.196822643445
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-50.803400 -0.252000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.8060 -40.5317 0.0 0.3 -140.3 0.0404 0.5 12.7 Vela X-1
170.6514 -60.5704 5.9 29.4 -74.2 0.1949 1.9 10.4 Cen X-3
186.5431 -62.7842 90.1 37.2 -75.0 0.0245 0.1 3.2 GX 301-2
34.8572 -69.7261 2.6 55.8 -14.6 1.2206 4.5 ------ UNKNOWN
195.4022 -59.3864 2.3 41.1 -81.0 1.5789 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.252000 20.508000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.8060 -40.5317 0.0 0.3 -140.1 -0.0436 -0.8 12.7 Vela X-1
170.3339 -60.7537 99.3 29.3 -73.7 0.0090 0.1 7.9 Cen X-3
186.3323 -62.8355 5.7 37.1 -74.9 -0.2586 -2.0 9.7 GX 301-2
134.7376 -65.4172 2.2 24.8 -38.2 0.3055 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
72.796610 962.766000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3735 -40.6557 8.9 19.7 152.0 -0.6336 -1.3 9.3 Vela X-1
170.3037 -60.6188 1.5 18.8 -108.3 3.7531 7.5 0.4 Cen X-3
186.5582 -62.7654 2.0 25.6 -96.8 3.4142 5.8 2.7 GX 301-2
65.4237 -57.3683 2.4 33.0 28.5 3.1446 4.8 ------ UNKNOWN
18.4995 -53.7396 2.9 54.3 5.5 7.1692 3.9 ------ UNKNOWN
13.1610 -52.9065 3.1 56.7 2.8 10.2066 3.7 ------ UNKNOWN
39.0202 -72.4252 4.9 34.9 -4.7 1.4545 2.4 ------ UNKNOWN
125.0178 -69.2295 2.8 9.5 -22.2 1.9739 4.2 ------ UNKNOWN
154.0099 -70.8020 3.4 14.0 -67.9 1.6558 3.4 ------ UNKNOWN
173.7894 -10.0407 2.6 59.1 -166.1 15.4386 4.4 ------ UNKNOWN
196.3998 -73.6931 4.4 26.9 -70.8 1.6199 2.7 ------ UNKNOWN
340.6599 -65.3166 3.0 52.6 -21.8 4.8825 3.8 ------ UNKNOWN
Plot creation:
Thu Oct 8 20:12:31 EDT 2015