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
286.617 68.778 0.000 32.336 -6.729 0.026 8.686 TRIG_00310785
Image time interval: 0.000 to 0.064 [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 0.064000
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 0.064000
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 0.064000
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 -2.192 sec. to 221.808 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87271 ( -0.118815 0.12159 )
Norm@50keV : 9.88582E-04 ( -7.23395e-05 7.14028e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.34 using 59 PHA bins.
# Reduced chi-squared = 0.7077 for 57 degrees of freedom
# Null hypothesis probability = 9.536366e-01
Photon flux (15-150 keV) in 224 sec: 0.140257 ( -0.00876362 0.00877098 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03573e-06 ( -1.4748e-07 1.49243e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.192 sec. to 221.808 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67943 ( -0.488465 0.417134 )
Epeak [keV] : 73.2223 ( -56.876 -73.2228 )
Norm@50keV : 1.26439E-03 ( -0.000413436 0.00106474 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.80 using 59 PHA bins.
# Reduced chi-squared = 0.7106 for 56 degrees of freedom
# Null hypothesis probability = 9.500640e-01
Photon flux (15-150 keV) in 224 sec: 0.138771 ( -0.009378 0.009344 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.99252e-06 ( -1.77076e-07 1.76615e-07 ) ergs/cm2
Band function
Time interval is from -2.192 sec. to 221.808 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.62289 ( -2.62289 -2.62289 )
beta : -1.92725 ( -0.166027 0.139718 )
Epeak [keV] : 22.2927 ( -22.2927 96.1778 )
Norm@50keV : 3.97412 ( -3.97407 145.916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.09 using 59 PHA bins.
# Reduced chi-squared = 0.7107 for 55 degrees of freedom
# Null hypothesis probability = 9.483364e-01
Photon flux (15-150 keV) in 224 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.99881e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.0289 (-0.886228 0.970673)
R^2/D10^2 : 4.37427E-02 (-0.0119014 0.0163148)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 103.30 using 59 PHA bins.
# Reduced chi-squared = 1.8123 for 57 degrees of freedom
# Null hypothesis probability = 1.707338e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.492e-07 2.929e-08
25- 50 7.069e-07 5.107e-08
50-150 4.867e-07 7.750e-08
15-150 1.443e-06 1.159e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 87.1501 (-18.0961 26.7703)
Norm : 0.634588 (-0.0589723 0.0687498)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.46 using 59 PHA bins.
# Reduced chi-squared = 0.7273 for 57 degrees of freedom
# Null hypothesis probability = 9.394484e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.705e-07 3.640e-08
25- 50 6.222e-07 3.830e-08
50-150 9.286e-07 3.152e-07
15-150 1.921e-06 3.054e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.54978 (-0.995376 1.15806)
R1^2/D10^2 : 0.407684 (-0.201734 0.477398)
kT2 [keV] : 20.1276 (-3.48287 5.64375)
R2^2/D10^2 : 3.55631E-03 (-0.00215907 0.00396612)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.41 using 59 PHA bins.
# Reduced chi-squared = 0.7347 for 55 degrees of freedom
# Null hypothesis probability = 9.296069e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.932e-07 8.333e-08
25- 50 5.878e-07 1.100e-07
50-150 9.513e-07 3.064e-07
15-150 1.932e-06 4.627e-07
Peak spectrum fit
Power-law model
Time interval is from 37.308 sec. to 38.308 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40498 ( -0.327633 0.332562 )
Norm@50keV : 5.50960E-03 ( -0.00104355 0.00103161 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.57 using 59 PHA bins.
# Reduced chi-squared = 1.028 for 57 degrees of freedom
# Null hypothesis probability = 4.175866e-01
Photon flux (15-150 keV) in 1 sec: 0.671729 ( -0.124242 0.124449 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.31833e-08 ( -1.12164e-08 1.1442e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 37.308 sec. to 38.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20242 ( -1.30545 1.59997 )
Epeak [keV] : 203.809 ( -224.027 -224.027 )
Norm@50keV : 6.89533E-03 ( -0.00676418 0.0194401 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.49 using 59 PHA bins.
# Reduced chi-squared = 1.044 for 56 degrees of freedom
# Null hypothesis probability = 3.840467e-01
Photon flux (15-150 keV) in 1 sec: 0.666408 ( -0.125142 0.127395 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.26274e-08 ( -1.17191e-08 1.18408e-08 ) ergs/cm2
Band function
Time interval is from 37.308 sec. to 38.308 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.25678 ( -0.426149 0.883341 )
beta : -9.37166 ( 9.37167 19.3717 )
Epeak [keV] : 288.785 ( -221.564 -287.151 )
Norm@50keV : 6.46071E-03 ( -0.00193172 0.0168889 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.50 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 55 degrees of freedom
# Null hypothesis probability = 3.482427e-01
Photon flux (15-150 keV) in 1 sec: 0.665808 ( ) 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] : 18.7175 (-4.20904 5.30288)
R^2/D10^2 : 3.65626E-02 (-0.020482 0.0487279)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.33 using 59 PHA bins.
# Reduced chi-squared = 1.164 for 57 degrees of freedom
# Null hypothesis probability = 1.863091e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.531e-09 1.039e-09
25- 50 1.205e-08 4.704e-09
50-150 3.092e-08 1.211e-08
15-150 4.550e-08 1.537e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-89.4828 -199.363)
Norm : 2.75542 (-0.505246 0.505246)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.20 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 57 degrees of freedom
# Null hypothesis probability = 3.953673e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.861e-09 4.006e-09
25- 50 1.320e-08 7.605e-09
50-150 2.895e-08 1.648e-08
15-150 4.901e-08 2.817e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.89165 (-2.00069 2.64241)
R1^2/D10^2 : 2.52308 (-2.07169 25.2681)
kT2 [keV] : 24.6654 (-6.16843 11.2541)
R2^2/D10^2 : 1.29694E-02 (-0.00905698 0.0226488)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.45 using 59 PHA bins.
# Reduced chi-squared = 1.008 for 55 degrees of freedom
# Null hypothesis probability = 4.576547e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.997e-09 4.104e-09
25- 50 1.125e-08 5.956e-09
50-150 3.528e-08 2.087e-08
15-150 5.353e-08 2.852e-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: 1.91933 ( -0.474427 0.540937 )
Norm@50keV : 9.47516E-04 ( -0.000334956 0.000319268 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.91 using 59 PHA bins.
# Reduced chi-squared = 0.9984 for 57 degrees of freedom
# Null hypothesis probability = 4.785894e-01
Photon flux (15-150 keV) in 14.1 sec: 0.137108 ( -0.0370707 0.0370711 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22858e-07 ( -4.01939e-08 4.27392e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.918742 ( -4.11211 1.22895 )
Epeak [keV] : 41.7723 ( )
Norm@50keV : 3.85222E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.38 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 56 degrees of freedom
# Null hypothesis probability = 4.606644e-01
Photon flux (15-150 keV) in 14.1 sec: 0.132932 ( -0.0376987 0.038266 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08969e-07 ( -4.20865e-08 5.2204e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.78591 ( -4.78591 -4.78591 )
beta : -2.36466 ( -1.36358 0.715963 )
Epeak [keV] : 26.9651 ( -26.9651 8.11879 )
Norm@50keV : 68.6017 ( -18.2401 1.46536e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.65 using 59 PHA bins.
# Reduced chi-squared = 1.012 for 55 degrees of freedom
# Null hypothesis probability = 4.502166e-01
Photon flux (15-150 keV) in 14.1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.1437e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.88e-07
S(50-100 keV) = 6.43e-07
T90 vs. Hardness ratio plot
T90 = 176 sec.
Hardness ratio (energy fluence ratio) = 1.09354
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.05448
Count Ratio (50-100 keV) / (15-25 keV) = 0.633453
Mask shadow pattern
IMX = 0.628686079164, IMY = 0.0741715436521
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-751.791400 -634.155000
-239.192000 -2.192000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
136.8662 19.4539 4.9 56.9 179.2 3.2774 2.4 ------ UNKNOWN
107.1371 56.0783 2.6 31.7 -128.5 1.1799 4.4 ------ UNKNOWN
332.2716 50.8877 4.8 56.3 -28.3 2.8038 2.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.192000 11.908590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
255.9805 65.7414 2.5 27.4 15.6 0.1868 4.6 ------ UNKNOWN
286.6595 68.7730 2.1 32.3 -6.7 0.2189 5.4 ------ UNKNOWN
4.9828 71.6963 2.2 36.5 -50.8 0.2830 5.2 ------ UNKNOWN
72.1440 59.0365 2.2 39.1 -98.4 0.5789 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.108580 962.902000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4698 35.2915 3.1 37.9 73.3 5.2145 3.7 3.1 Her X-1
299.5883 35.1989 0.2 34.3 9.4 31.2079 49.0 0.2 Cyg X-1
308.0662 40.9672 2.1 30.0 -5.1 3.1084 5.5 2.2 Cyg X-3
326.1119 38.3791 3.5 37.1 -27.4 2.2533 3.3 4.4 Cyg X-2
279.7490 58.4702 3.2 10.7 48.0 1.5419 3.6 ------ UNKNOWN
146.7658 50.7235 5.2 56.9 179.2 7.5359 2.2 ------ UNKNOWN
302.1740 61.9005 3.0 9.4 -22.3 1.7427 3.8 ------ UNKNOWN
314.5537 13.7849 2.4 57.8 -4.2 13.0364 4.8 ------ UNKNOWN
137.4894 51.8710 3.4 57.2 -173.8 9.9532 3.4 ------ UNKNOWN
319.0851 15.0524 3.0 57.5 -9.6 9.8358 3.8 ------ UNKNOWN
7.4905 50.1753 3.4 41.2 -77.8 8.5033 3.4 ------ UNKNOWN
Plot creation:
Thu Oct 8 20:31:30 EDT 2015