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
111.3496 -37.7910 0.0107 43.7989 -28.5522 1.5736167 17.848 TRIG_00646603
Foreground time interval of the image:
-6.576 16.205 (delta_t = 22.781 [sec])
Background time interval of the image:
-239.296 -6.576 (delta_t = 232.720 [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 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 -6.576 sec. to 115.152 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03226 ( -0.175927 0.184774 )
Norm@50keV : 1.21989E-03 ( -0.000139226 0.000135509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.60 using 59 PHA bins.
# Reduced chi-squared = 0.9580 for 57 degrees of freedom
# Null hypothesis probability = 5.654623e-01
Photon flux (15-150 keV) in 121.7 sec: 0.185751 ( -0.0166771 0.0167045 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.37172e-06 ( -1.436e-07 1.45724e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.576 sec. to 115.152 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12302 ( )
Epeak [keV] : 63.2280 ( )
Norm@50keV : 1.08466E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.37 using 59 PHA bins.
# Reduced chi-squared = 0.9710 for 56 degrees of freedom
# Null hypothesis probability = 5.365984e-01
Photon flux (15-150 keV) in 121.7 sec: 0.185907 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36656e-06 ( -1.40393e-07 1.48097e-07 ) ergs/cm2
Band function
Time interval is from -6.576 sec. to 115.152 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.61818 ( 1.61818 1.61818 )
beta : -2.03225 ( -0.185738 0.175742 )
Epeak [keV] : 10.2719 ( -10.2719 -10.2719 )
Norm@50keV : 3.43690E-03 ( -0.0034369 938.371 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.60 using 59 PHA bins.
# Reduced chi-squared = 0.9928 for 55 degrees of freedom
# Null hypothesis probability = 4.896712e-01
Photon flux (15-150 keV) in 121.7 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] : 9.62447 (-1.30843 1.56548)
R^2/D10^2 : 9.37529E-02 (-0.0408224 0.071924)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 103.22 using 59 PHA bins.
# Reduced chi-squared = 1.8109 for 57 degrees of freedom
# Null hypothesis probability = 1.739101e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.122e-07 3.371e-08
25- 50 4.993e-07 6.237e-08
50-150 2.330e-07 5.945e-08
15-150 9.445e-07 1.165e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.8220 (-18.3992 29.3285)
Norm : 0.896375 (-0.131522 0.155305)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.96 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 57 degrees of freedom
# Null hypothesis probability = 3.688725e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.798e-07 3.371e-08
25- 50 4.449e-07 4.107e-08
50-150 5.703e-07 1.223e-07
15-150 1.295e-06 1.504e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.16273 (-0.928574 1.04388)
R1^2/D10^2 : 0.861488 (-0.453667 1.17012)
kT2 [keV] : 21.8608 (-4.52128 7.38233)
R2^2/D10^2 : 3.23138E-03 (-0.0020915 0.0045702)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.61 using 59 PHA bins.
# Reduced chi-squared = 0.9566 for 55 degrees of freedom
# Null hypothesis probability = 5.664441e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.242e-07 1.155e-07
25- 50 3.881e-07 1.112e-07
50-150 6.657e-07 3.122e-07
15-150 1.378e-06 4.553e-07
Peak spectrum fit
Power-law model
Time interval is from 0.356 sec. to 1.356 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74394 ( -0.252464 0.263818 )
Norm@50keV : 1.25033E-02 ( -0.00213072 0.0020985 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.17 using 59 PHA bins.
# Reduced chi-squared = 1.213 for 57 degrees of freedom
# Null hypothesis probability = 1.294714e-01
Photon flux (15-150 keV) in 1 sec: 1.68689 ( -0.271638 0.272166 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.15415e-07 ( -2.00513e-08 2.02803e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.356 sec. to 1.356 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.452264 ( -1.68157 1.20725 )
Epeak [keV] : 56.3378 ( -12.9597 107.048 )
Norm@50keV : 6.07955E-02 ( -0.0607961 0.427611 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.82 using 59 PHA bins.
# Reduced chi-squared = 1.175 for 56 degrees of freedom
# Null hypothesis probability = 1.734328e-01
Photon flux (15-150 keV) in 1 sec: 1.62562 ( -0.27887 0.27904 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07426e-07 ( -2.10535e-08 2.1729e-08 ) ergs/cm2
Band function
Time interval is from 0.356 sec. to 1.356 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.391095 ( -2.7181 -0.423343 )
beta : -2.37054 ( 2.37569 0.617176 )
Epeak [keV] : 45.5403 ( -14.5054 60.1577 )
Norm@50keV : 0.209503 ( -0.24457 101.69 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.39 using 59 PHA bins.
# Reduced chi-squared = 1.189 for 55 degrees of freedom
# Null hypothesis probability = 1.594081e-01
Photon flux (15-150 keV) in 1 sec: 1.61400 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09375e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.5316 (-1.94339 2.36418)
R^2/D10^2 : 0.370871 (-0.17755 0.320547)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.51 using 59 PHA bins.
# Reduced chi-squared = 1.220 for 57 degrees of freedom
# Null hypothesis probability = 1.235874e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.235e-08 3.385e-09
25- 50 4.085e-08 9.220e-09
50-150 3.966e-08 1.351e-08
15-150 9.286e-08 2.257e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 111.030 (-44.2947 -110.921)
Norm : 7.41276 (-1.29263 1.78184)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.01 using 59 PHA bins.
# Reduced chi-squared = 1.176 for 57 degrees of freedom
# Null hypothesis probability = 1.711336e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.936e-08 4.250e-09
25- 50 3.415e-08 7.895e-09
50-150 5.858e-08 3.435e-08
15-150 1.121e-07 4.542e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.86587 ( )
R1^2/D10^2 : 0.904468 (-0.562503 -0.894783)
kT2 [keV] : 23.7803 (-24.0763 -24.7375)
R2^2/D10^2 : 1.86365E-02 (-0.0153868 0.34479)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.83 using 59 PHA bins.
#Fit statistic : Chi-Squared = 65.48 using 59 PHA bins.
# Reduced chi-squared = 1.215 for 55 degrees of freedom
# Reduced chi-squared = 1.191 for 55 degrees of freedom
# Null hypothesis probability = 1.316882e-01
# Null hypothesis probability = 1.574272e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.563e-08 5.277e-09
25- 50 3.773e-08 1.325e-08
50-150 4.392e-08 1.668e-08
15-150 9.728e-08 2.333e-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: 2.02999 ( -0.149927 0.156213 )
Norm@50keV : 4.59190E-03 ( -0.000450279 0.000441996 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.60 using 59 PHA bins.
# Reduced chi-squared = 0.7124 for 57 degrees of freedom
# Null hypothesis probability = 9.504963e-01
Photon flux (15-150 keV) in 22.78 sec: 0.698459 ( -0.0574448 0.0575186 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.66359e-07 ( -8.82784e-08 8.91621e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71350 ( -0.65966 0.423072 )
Epeak [keV] : 40.1565 ( -32.8084 -40.1565 )
Norm@50keV : 6.87696E-03 ( -0.00351599 0.00895995 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.75 using 59 PHA bins.
# Reduced chi-squared = 0.7098 for 56 degrees of freedom
# Null hypothesis probability = 9.506626e-01
Photon flux (15-150 keV) in 22.78 sec: 0.688786 ( -0.060072 0.060006 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.41304e-07 ( -9.95782e-08 1.00136e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.43616 ( 1.43444 1.43444 )
beta : -2.21648 ( 2.21448 0.301048 )
Epeak [keV] : 35.8596 ( -35.6267 28.5237 )
Norm@50keV : 1.04625E-02 ( -0.006356 939.419 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.52 using 59 PHA bins.
# Reduced chi-squared = 0.7185 for 55 degrees of freedom
# Null hypothesis probability = 9.426687e-01
Photon flux (15-150 keV) in 22.78 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.44288e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.17e-07
S(50-100 keV) = 4.08e-07
T90 vs. Hardness ratio plot
T90 = 97.2640000581741 sec.
Hardness ratio (energy fluence ratio) = 0.978417
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.980515
Count Ratio (50-100 keV) / (15-25 keV) = 0.66851
Mask shadow pattern
IMX = 8.423049718904094E-01, IMY = 4.583284421965760E-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:
-239.296000 -6.576000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6020 -40.6231 31.9 55.7 -9.1 0.2254 0.4 5.3 Vela X-1
259.3158 -85.6548 3.0 40.1 60.4 2.2714 3.9 ------ UNKNOWN
148.1251 -67.7949 3.3 44.2 24.7 1.2538 3.5 ------ UNKNOWN
124.8088 -51.8821 3.4 42.8 -3.8 0.9851 3.4 ------ UNKNOWN
19.0002 -15.0668 3.1 45.9 -167.5 1.2683 3.8 ------ UNKNOWN
14.6072 -2.8481 2.6 58.8 -166.0 5.2494 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.576000 16.204600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5681 -40.6096 6.2 55.7 -9.1 0.3071 1.9 3.8 Vela X-1
111.3496 -37.7910 0.6 43.8 -28.6 1.5739 17.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.004590 962.784000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5275 -40.5500 0.7 18.9 33.5 7.7707 15.8 0.3 Vela X-1
143.4726 -20.6725 2.6 32.6 -5.1 2.6881 4.4 ------ UNKNOWN
87.9874 -16.0686 3.2 29.9 -122.4 2.5842 3.7 ------ UNKNOWN
53.0791 -17.7811 2.5 54.3 -157.9 8.7151 4.6 ------ UNKNOWN
65.9822 -14.7118 3.6 46.2 -145.2 3.7976 3.2 ------ UNKNOWN
78.9722 -3.4172 3.0 45.3 -121.3 9.5498 3.9 ------ UNKNOWN
Plot creation:
Sat Jul 11 00:45:55 EDT 2015