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
135.0244 -47.5563 0.0128 42.5817 1.7264 1.2461214 14.978 TRIG_00572308
Foreground time interval of the image:
-1.928 12.408 (delta_t = 14.336 [sec])
Background time interval of the image:
-119.224 -1.928 (delta_t = 117.296 [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)
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 -1.928 sec. to 12.408 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96460 ( -0.179694 0.190435 )
Norm@50keV : 5.35846E-03 ( -0.000675567 0.000661932 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.64 using 59 PHA bins.
# Reduced chi-squared = 0.9059 for 57 degrees of freedom
# Null hypothesis probability = 6.758036e-01
Photon flux (15-150 keV) in 14.34 sec: 0.790965 ( -0.0778136 0.0778268 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.0748e-07 ( -8.43284e-08 8.62627e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.928 sec. to 12.408 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.968183 ( -0.950276 0.778723 )
Epeak [keV] : 43.8469 ( -11.3306 17.9375 )
Norm@50keV : 1.97702E-02 ( -0.0124905 0.0494406 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8327 for 56 degrees of freedom
# Null hypothesis probability = 8.095638e-01
Photon flux (15-150 keV) in 14.34 sec: 0.761072 ( -0.080558 0.080768 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.47095e-07 ( -8.93296e-08 9.54442e-08 ) ergs/cm2
Band function
Time interval is from -1.928 sec. to 12.408 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.968281 ( -0.612253 1.18172 )
beta : -10.0000 ( 10 1.06581e-14 )
Epeak [keV] : 43.8391 ( -11.2948 17.9423 )
Norm@50keV : 1.97666E-02 ( -0.012489 0.0495964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8478 for 55 degrees of freedom
# Null hypothesis probability = 7.817513e-01
Photon flux (15-150 keV) in 14.34 sec: 0.769020 ( 6.23098 -0.090132 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.48015e-07 ( -6.47914e-07 -9.08539e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.4138 (-1.16935 1.31107)
R^2/D10^2 : 0.319034 (-0.114767 0.18078)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.47 using 59 PHA bins.
# Reduced chi-squared = 1.061 for 57 degrees of freedom
# Null hypothesis probability = 3.518191e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.023e-07 1.738e-08
25- 50 2.691e-07 3.542e-08
50-150 1.578e-07 4.202e-08
15-150 5.292e-07 7.005e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.2967 (-18.3907 29.2831)
Norm : 3.91821 (-0.570547 0.660149)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.13 using 59 PHA bins.
# Reduced chi-squared = 0.8268 for 57 degrees of freedom
# Null hypothesis probability = 8.214564e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.440e-07 2.032e-08
25- 50 2.285e-07 2.495e-08
50-150 2.913e-07 7.973e-08
15-150 6.637e-07 9.221e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.24258 (-2.21553 2.43674)
R1^2/D10^2 : 2.42210 (-1.71781 22.5501)
kT2 [keV] : 15.5836 (-3.63895 7.68716)
R2^2/D10^2 : 5.21924E-02 (-0.0435683 0.116273)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.59 using 59 PHA bins.
# Reduced chi-squared = 0.8470 for 55 degrees of freedom
# Null hypothesis probability = 7.831339e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.395e-07 6.922e-08
25- 50 2.300e-07 1.079e-07
50-150 2.649e-07 1.546e-07
15-150 6.343e-07 2.872e-07
Peak spectrum fit
Power-law model
Time interval is from 1.324 sec. to 2.324 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05878 ( -0.347403 0.392056 )
Norm@50keV : 1.09533E-02 ( -0.00284461 0.00270444 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.40 using 59 PHA bins.
# Reduced chi-squared = 1.340 for 57 degrees of freedom
# Null hypothesis probability = 4.413103e-02
Photon flux (15-150 keV) in 1 sec: 1.68901 ( -0.297663 0.297689 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01401e-07 ( -2.30335e-08 2.41823e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.324 sec. to 2.324 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.11204 ( )
Epeak [keV] : 62.5299 ( )
Norm@50keV : 9.98731E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.29 using 59 PHA bins.
# Reduced chi-squared = 1.362 for 56 degrees of freedom
# Null hypothesis probability = 3.704195e-02
Photon flux (15-150 keV) in 1 sec: 1.68728 ( -0.29704 0.29754 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01436e-07 ( -1.29819e-08 2.376e-08 ) ergs/cm2
Band function
Time interval is from 1.324 sec. to 2.324 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.75828 ( -4.75828 -4.75828 )
beta : -2.21259 ( -0.577592 0.425158 )
Epeak [keV] : 21.1318 ( -21.1318 5.80571 )
Norm@50keV : 3727.45 ( -653.267 2.01158e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.59 using 59 PHA bins.
# Reduced chi-squared = 1.374 for 55 degrees of freedom
# Null hypothesis probability = 3.416285e-02
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] : 7.33083 (-1.54636 2.25262)
R^2/D10^2 : 2.52580 (-1.6221 4.06061)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.67 using 59 PHA bins.
# Reduced chi-squared = 1.503 for 57 degrees of freedom
# Null hypothesis probability = 8.333690e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.282e-08 8.470e-09
25- 50 3.412e-08 1.221e-08
50-150 6.663e-09 3.929e-09
15-150 6.361e-08 2.108e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 57.0574 (-25.9417 68.4432)
Norm : 8.98987 (-2.52367 4.06044)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.06 using 59 PHA bins.
# Reduced chi-squared = 1.369 for 57 degrees of freedom
# Null hypothesis probability = 3.347319e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.240e-08 5.175e-09
25- 50 3.356e-08 8.840e-09
50-150 3.659e-08 1.939e-08
15-150 9.255e-08 3.077e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.82540 (-1.59638 2.02771)
R1^2/D10^2 : 5.66200 (-3.77358 14.2836)
kT2 [keV] : 37.7399 (-22.3209 -38.0422)
R2^2/D10^2 : 4.78962E-03 (-0.00447793 0.0526856)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.15 using 59 PHA bins.
# Reduced chi-squared = 1.348 for 55 degrees of freedom
# Null hypothesis probability = 4.354096e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.536e-08 1.307e-08
25- 50 2.899e-08 1.355e-08
50-150 5.643e-08 3.580e-08
15-150 1.108e-07 5.612e-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: 1.96460 ( -0.179694 0.190435 )
Norm@50keV : 5.35846E-03 ( -0.000675567 0.000661932 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.64 using 59 PHA bins.
# Reduced chi-squared = 0.9059 for 57 degrees of freedom
# Null hypothesis probability = 6.758036e-01
Photon flux (15-150 keV) in 14.34 sec: 0.790965 ( -0.0778136 0.0778268 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.0748e-07 ( -8.43284e-08 8.62627e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.968183 ( -0.950276 0.778723 )
Epeak [keV] : 43.8469 ( -11.3306 17.9375 )
Norm@50keV : 1.97702E-02 ( -0.0124905 0.0494406 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8327 for 56 degrees of freedom
# Null hypothesis probability = 8.095638e-01
Photon flux (15-150 keV) in 14.34 sec: 0.761072 ( -0.080558 0.080768 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.47095e-07 ( -8.93296e-08 9.54442e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.968281 ( -0.612253 1.18172 )
beta : -10.0000 ( 10 1.77636e-14 )
Epeak [keV] : 43.8391 ( -11.2948 17.9423 )
Norm@50keV : 1.97666E-02 ( -0.012489 0.0495964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8478 for 55 degrees of freedom
# Null hypothesis probability = 7.817513e-01
Photon flux (15-150 keV) in 14.34 sec: 0.769020 ( 6.23098 -0.090132 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.48015e-07 ( -6.47914e-07 -9.08539e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.11e-07
S(50-100 keV) = 2.16e-07
T90 vs. Hardness ratio plot
T90 = 12.2400000095367 sec.
Hardness ratio (energy fluence ratio) = 1.0237
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36044
Count Ratio (50-100 keV) / (15-25 keV) = 0.666504
Mask shadow pattern
IMX = 9.185392598813594E-01, IMY = -2.768482040946642E-02
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:
-119.224000 -1.928000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4880 -40.5509 1.9 35.6 1.3 1.2795 6.1 1.9 Vela X-1
108.4441 -25.5352 3.3 33.1 50.0 0.9178 3.5 ------ UNKNOWN
139.4625 51.8505 2.7 56.9 -175.8 3.6857 4.2 ------ UNKNOWN
167.7385 -51.3737 2.4 53.6 -23.2 2.2314 4.9 ------ UNKNOWN
176.0594 -23.8025 2.6 43.4 -58.9 2.2979 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.928000 12.408000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6875 -40.5099 5.2 35.5 1.0 0.1502 2.2 7.7 Vela X-1
98.1733 -31.0731 2.1 43.6 50.0 1.1027 5.5 ------ UNKNOWN
135.0243 -47.5563 0.8 42.6 1.7 1.2462 15.0 ------ UNKNOWN
159.5894 45.0508 2.3 54.5 -157.9 0.8349 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
85.076600 962.851800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5137 -40.5664 0.7 7.0 -147.9 9.2105 17.3 1.0 Vela X-1
170.3609 -60.6703 3.2 24.0 -14.4 2.1024 3.5 3.1 Cen X-3
186.6389 -62.7529 0.8 32.0 -13.0 9.8017 15.2 1.2 GX 301-2
88.5375 -63.4385 3.1 29.8 70.4 3.8067 3.8 ------ UNKNOWN
183.8679 -73.8103 2.1 33.6 7.3 3.4426 5.5 ------ UNKNOWN
205.1560 -37.5882 3.4 50.7 -44.5 11.0295 4.0 ------ UNKNOWN
204.8634 -37.4823 5.3 50.6 -44.8 8.4985 3.0 ------ UNKNOWN
Plot creation:
Sat May 30 15:30:03 EDT 2015