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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
92.3878 -13.2851 0.0058 29.4378 9.2610 1.2914191 32.692 TRIG_00566228
Foreground time interval of the image:
-0.332 8.460 (delta_t = 8.792 [sec])
Background time interval of the image:
-114.187 -0.332 (delta_t = 113.855 [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 0.256000
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 0.256000
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 0.256000
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 -0.332 sec. to 8.460 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42828 ( -0.105006 0.108629 )
Norm@50keV : 7.25697E-03 ( -0.000519811 0.000515353 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 93.66 using 59 PHA bins.
# Reduced chi-squared = 1.643 for 57 degrees of freedom
# Null hypothesis probability = 1.589920e-03
Photon flux (15-150 keV) in 8.792 sec: 1.36528 ( -0.0726272 0.0727793 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.26493e-07 ( -3.53919e-08 3.56751e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.332 sec. to 8.460 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09839 ( -0.612177 0.539376 )
Epeak [keV] : 26.5104 ( -9.08041 4.84539 )
Norm@50keV : 4.42033E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.58 using 59 PHA bins.
# Reduced chi-squared = 1.296 for 56 degrees of freedom
# Null hypothesis probability = 6.732149e-02
Photon flux (15-150 keV) in 8.792 sec: 1.27928 ( -0.07844 0.07879 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.61672e-07 ( -3.83929e-08 4.02208e-08 ) ergs/cm2
Band function
Time interval is from -0.332 sec. to 8.460 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.09823 ( -0.377597 0.265571 )
beta : -10.00000 ( 10 3.12157e-06 )
Epeak [keV] : 26.5053 ( -2.69112 4.84433 )
Norm@50keV : 4.42118E-02 ( -0.00225047 0.0582894 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.58 using 59 PHA bins.
# Reduced chi-squared = 1.320 for 55 degrees of freedom
# Null hypothesis probability = 5.623758e-02
Photon flux (15-150 keV) in 8.792 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] : 8.51483 (-0.474913 0.500332)
R^2/D10^2 : 1.10300 (-0.233925 0.299138)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 109.34 using 59 PHA bins.
# Reduced chi-squared = 1.9182 for 57 degrees of freedom
# Null hypothesis probability = 3.769451e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.327e-07 1.064e-08
25- 50 2.580e-07 1.495e-08
50-150 8.283e-08 1.415e-08
15-150 4.735e-07 2.761e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 37.5808 (-4.34193 5.1238)
Norm : 9.03205 (-0.943164 1.07143)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.09 using 59 PHA bins.
# Reduced chi-squared = 1.282 for 57 degrees of freedom
# Null hypothesis probability = 7.413436e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.784e-07 1.270e-08
25- 50 2.283e-07 1.161e-08
50-150 1.647e-07 2.897e-08
15-150 5.713e-07 3.403e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.82329 (-1.08179 1.17886)
R1^2/D10^2 : 6.87867 (-3.6837 12.3601)
kT2 [keV] : 12.4490 (-1.84212 3.06923)
R2^2/D10^2 : 0.161590 (-0.109349 0.20116)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.59 using 59 PHA bins.
# Reduced chi-squared = 1.320 for 55 degrees of freedom
# Null hypothesis probability = 5.613119e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.737e-07 5.837e-08
25- 50 2.291e-07 6.190e-08
50-150 1.488e-07 5.725e-08
15-150 5.517e-07 1.389e-07
Peak spectrum fit
Power-law model
Time interval is from -0.140 sec. to 0.860 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.47838 ( -0.152616 0.160775 )
Norm@50keV : 1.47766E-02 ( -0.0016791 0.00166 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.15 using 59 PHA bins.
# Reduced chi-squared = 0.9675 for 57 degrees of freedom
# Null hypothesis probability = 5.448078e-01
Photon flux (15-150 keV) in 1 sec: 2.86478 ( -0.220827 0.220981 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46917e-07 ( -1.27609e-08 1.29344e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.140 sec. to 0.860 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51215 ( -0.909122 0.491348 )
Epeak [keV] : 18.5152 ( -15.1856 9.17572 )
Norm@50keV : 5.89513E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.32 using 59 PHA bins.
# Reduced chi-squared = 0.8807 for 56 degrees of freedom
# Null hypothesis probability = 7.239045e-01
Photon flux (15-150 keV) in 1 sec: 2.77780 ( -0.22835 0.22865 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.35147e-07 ( -1.4066e-08 1.4904e-08 ) ergs/cm2
Band function
Time interval is from -0.140 sec. to 0.860 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.614955 ( -2.07651 -0.618798 )
beta : -2.92524 ( -0.46386 0.338595 )
Epeak [keV] : 24.5635 ( -4.85053 3.33398 )
Norm@50keV : 2.08126 ( -2.12826 2030.61 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.86 using 59 PHA bins.
# Reduced chi-squared = 0.8338 for 55 degrees of freedom
# Null hypothesis probability = 8.052097e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3489e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.36385 (-0.587319 0.646121)
R^2/D10^2 : 4.32183 (-1.30396 1.85177)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.08 using 59 PHA bins.
# Reduced chi-squared = 1.194 for 57 degrees of freedom
# Null hypothesis probability = 1.495459e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.956e-08 4.640e-09
25- 50 5.966e-08 5.770e-09
50-150 1.183e-08 3.096e-09
15-150 1.111e-07 1.004e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.5781 (-5.55469 7.03939)
Norm : 20.8855 (-3.24532 3.96412)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.35 using 59 PHA bins.
# Reduced chi-squared = 0.8658 for 57 degrees of freedom
# Null hypothesis probability = 7.543348e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.483e-08 4.740e-09
25- 50 5.436e-08 4.720e-09
50-150 3.434e-08 8.250e-09
15-150 1.335e-07 1.280e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.71226 (-0.840321 0.822011)
R1^2/D10^2 : 10.2842 (-4.13231 7.44311)
kT2 [keV] : 18.0061 (-4.75732 8.29498)
R2^2/D10^2 : 5.38600E-02 (-0.0428635 0.161489)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.47 using 59 PHA bins.
# Reduced chi-squared = 0.8086 for 55 degrees of freedom
# Null hypothesis probability = 8.440383e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.490e-08 1.051e-08
25- 50 5.320e-08 1.340e-08
50-150 4.082e-08 2.238e-08
15-150 1.389e-07 4.053e-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: 2.42828 ( -0.105006 0.108629 )
Norm@50keV : 7.25697E-03 ( -0.000519811 0.000515353 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 93.66 using 59 PHA bins.
# Reduced chi-squared = 1.643 for 57 degrees of freedom
# Null hypothesis probability = 1.589920e-03
Photon flux (15-150 keV) in 8.792 sec: 1.36528 ( -0.0726272 0.0727793 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.26493e-07 ( -3.53919e-08 3.56751e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09839 ( -0.612177 0.539376 )
Epeak [keV] : 26.5104 ( -9.08041 4.84539 )
Norm@50keV : 4.42033E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.58 using 59 PHA bins.
# Reduced chi-squared = 1.296 for 56 degrees of freedom
# Null hypothesis probability = 6.732149e-02
Photon flux (15-150 keV) in 8.792 sec: 1.27928 ( -0.07844 0.07879 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.61672e-07 ( -3.83929e-08 4.02208e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.09823 ( -0.377597 0.265571 )
beta : -10.00000 ( 10 3.12157e-06 )
Epeak [keV] : 26.5053 ( -2.69112 4.84433 )
Norm@50keV : 4.42118E-02 ( -0.00225047 0.0582894 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.58 using 59 PHA bins.
# Reduced chi-squared = 1.320 for 55 degrees of freedom
# Null hypothesis probability = 5.623758e-02
Photon flux (15-150 keV) in 8.792 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) = 2.06e-07
S(50-100 keV) = 1.53e-07
T90 vs. Hardness ratio plot
T90 = 7.62799996137619 sec.
Hardness ratio (energy fluence ratio) = 0.742718
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.977984
Count Ratio (50-100 keV) / (15-25 keV) = 0.324435
Mask shadow pattern
IMX = 5.569857683129329E-01, IMY = -9.082077752527755E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-114.187410 -0.332000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6293 22.0123 0.3 7.5 163.7 4.7507 40.6 0.3 Crab
61.6577 -11.6405 2.2 38.0 62.9 1.8010 5.3 ------ UNKNOWN
115.8541 -24.5361 2.1 48.6 -16.6 1.2771 5.5 ------ UNKNOWN
124.2164 -8.4003 2.9 43.2 -40.7 0.9255 4.0 ------ UNKNOWN
130.3582 -23.2152 3.2 56.8 -29.8 2.6717 3.6 ------ UNKNOWN
129.8990 39.5891 2.7 43.4 -113.9 2.1836 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.332000 8.460000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7866 22.0588 37.4 7.4 164.9 0.0093 0.3 8.9 Crab
66.0652 -26.3134 2.4 47.3 45.0 0.7455 4.8 ------ UNKNOWN
92.3878 -13.2851 0.3 29.4 9.3 1.2915 32.7 ------ UNKNOWN
71.9299 68.4560 3.5 53.6 -169.6 0.2998 3.3 ------ UNKNOWN
116.9827 18.9988 2.5 27.7 -83.1 0.2207 4.6 ------ UNKNOWN
128.2305 53.2456 2.5 48.8 -131.5 0.6887 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.212590 962.533900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6309 22.0162 0.2 36.4 -166.1 37.3370 58.7 0.2 Crab
135.5393 -40.5648 3.0 46.4 -18.0 4.1766 3.9 0.8 Vela X-1
54.3191 27.3029 3.2 54.9 165.7 11.5184 3.5 ------ UNKNOWN
75.3511 17.5032 2.9 35.1 178.6 2.5326 4.0 ------ UNKNOWN
107.5464 -31.5097 2.8 22.9 -7.1 2.0144 4.1 ------ UNKNOWN
72.1318 40.9608 3.3 57.4 -170.4 8.9477 3.5 ------ UNKNOWN
145.1528 -22.0702 2.5 50.8 -44.5 14.3165 4.7 ------ UNKNOWN
125.4660 11.6855 4.6 41.2 -98.1 7.7861 2.5 ------ UNKNOWN
Plot creation:
Sat May 30 15:55:02 EDT 2015