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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
120.6614 -26.1489 0.0191 38.7053 154.8100 0.4024027 10.056 TRIG_00311762
Foreground time interval of the image:
0.084 6.056 (delta_t = 5.972 [sec])
Background time interval of the image:
-239.824 -65.655 (delta_t = 174.169 [sec])
-64.824 0.084 (delta_t = 64.908 [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 0.512000
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 0.512000
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 0.512000
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 0.084 sec. to 6.056 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82046 ( -0.254713 0.270577 )
Norm@50keV : 4.86370E-03 ( -0.000818354 0.000794245 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.14 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 57 degrees of freedom
# Null hypothesis probability = 3.973626e-01
Photon flux (15-150 keV) in 5.972 sec: 0.675597 ( -0.0969042 0.0969645 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.6723e-07 ( -4.46637e-08 4.55556e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.084 sec. to 6.056 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55746 ( -1.18775 0.699756 )
Epeak [keV] : 76.5674 ( -76.3547 -76.5674 )
Norm@50keV : 6.77901E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.93 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 56 degrees of freedom
# Null hypothesis probability = 3.687305e-01
Photon flux (15-150 keV) in 5.972 sec: 0.668993 ( -0.100128 0.09957 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.61411e-07 ( -4.97079e-08 4.93843e-08 ) ergs/cm2
Band function
Time interval is from 0.084 sec. to 6.056 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.55425 ( 1.5525 6.49224 )
beta : -2.23331 ( 2.23227 11.5635 )
Epeak [keV] : 76.0685 ( -75.5142 -75.5142 )
Norm@50keV : 6.80614E-03 ( -0.00272649 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.93 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 55 degrees of freedom
# Null hypothesis probability = 3.337813e-01
Photon flux (15-150 keV) in 5.972 sec: 0.669157 ( ) 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] : 11.4484 (-1.89587 2.33192)
R^2/D10^2 : 0.191949 (-0.0955138 0.184264)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.56 using 59 PHA bins.
# Reduced chi-squared = 1.238 for 57 degrees of freedom
# Null hypothesis probability = 1.069621e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.161e-08 9.086e-09
25- 50 9.399e-08 2.138e-08
50-150 7.169e-08 2.485e-08
15-150 1.973e-07 3.983e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.8799 (-38.8812 100.202)
Norm : 2.99760 (-0.553901 0.730851)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.11 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 57 degrees of freedom
# Null hypothesis probability = 3.984233e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.678e-08 9.361e-09
25- 50 8.054e-08 1.436e-08
50-150 1.289e-07 6.866e-08
15-150 2.563e-07 7.349e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.79267 (-3.65569 3.96167)
R1^2/D10^2 : 1.55401 (-1.17629 173.219)
kT2 [keV] : 20.2265 (-8.29179 59.767)
R2^2/D10^2 : 1.75005E-02 (-0.0154666 0.0598417)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.42 using 59 PHA bins.
# Reduced chi-squared = 1.099 for 55 degrees of freedom
# Null hypothesis probability = 2.864404e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.748e-08 2.605e-08
25- 50 7.742e-08 4.049e-08
50-150 1.279e-07 7.358e-08
15-150 2.528e-07 1.325e-07
Peak spectrum fit
Power-law model
Time interval is from 0.052 sec. to 1.052 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45682 ( -0.23077 0.231912 )
Norm@50keV : 1.37446E-02 ( -0.00202049 0.00201417 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.89 using 59 PHA bins.
# Reduced chi-squared = 1.121 for 57 degrees of freedom
# Null hypothesis probability = 2.473386e-01
Photon flux (15-150 keV) in 1 sec: 1.69670 ( -0.251889 0.252493 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.31363e-07 ( -2.07471e-08 2.09467e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.052 sec. to 1.052 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.267762 ( -1.4537 1.06561 )
Epeak [keV] : 71.2597 ( -18.0807 164.644 )
Norm@50keV : 5.63803E-02 ( -0.0563854 0.25818 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.19 using 59 PHA bins.
# Reduced chi-squared = 1.075 for 56 degrees of freedom
# Null hypothesis probability = 3.267838e-01
Photon flux (15-150 keV) in 1 sec: 1.63676 ( -0.25952 0.25931 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21636e-07 ( -2.28763e-08 2.3192e-08 ) ergs/cm2
Band function
Time interval is from 0.052 sec. to 1.052 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.965026 ( -2.14769 -0.994337 )
beta : -1.98150 ( 1.98269 0.504922 )
Epeak [keV] : 48.8723 ( -19.1377 69.7168 )
Norm@50keV : 0.340665 ( -0.395932 105.494 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.88 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 55 degrees of freedom
# Null hypothesis probability = 3.353274e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24385e-07 ( -1.24378e-07 -2.1503e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.6015 (-2.18002 2.67546)
R^2/D10^2 : 0.224764 (-0.101919 0.174776)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.13 using 59 PHA bins.
# Reduced chi-squared = 1.125 for 57 degrees of freedom
# Null hypothesis probability = 2.408135e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.007e-08 2.619e-09
25- 50 3.903e-08 7.565e-09
50-150 5.594e-08 1.661e-08
15-150 1.050e-07 2.160e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.355 (-81.7662 -199.36)
Norm : 7.05625 (-1.01602 1.01746)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.58 using 59 PHA bins.
# Reduced chi-squared = 1.098 for 57 degrees of freedom
# Null hypothesis probability = 2.847216e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.757e-08 9.995e-09
25- 50 3.380e-08 1.894e-08
50-150 7.413e-08 4.152e-08
15-150 1.255e-07 6.910e-08
Double BB
R1^2/D10^2 : 3.50193E-03 ( )
kT2 [keV] : 10.9409 (-5.53816 3.42165)
R2^2/D10^2 : 0.483677 (-0.279449 2.09083)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.81 using 59 PHA bins.
#Fit statistic : Chi-Squared = 58.95 using 59 PHA bins.
#Fit statistic : Chi-Squared = 58.94 using 59 PHA bins.
# Reduced chi-squared = 1.087 for 55 degrees of freedom
# Reduced chi-squared = 1.072 for 55 degrees of freedom
# Reduced chi-squared = 1.072 for 55 degrees of freedom
# Null hypothesis probability = 3.053464e-01
# Null hypothesis probability = 3.332134e-01
# Null hypothesis probability = 3.335996e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.325e-08 8.180e-09
25- 50 3.674e-08 2.070e-08
50-150 6.542e-08 3.899e-08
15-150 1.154e-07 6.150e-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: 1.82046 ( -0.254713 0.270577 )
Norm@50keV : 4.86370E-03 ( -0.000818354 0.000794245 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.14 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 57 degrees of freedom
# Null hypothesis probability = 3.973626e-01
Photon flux (15-150 keV) in 5.972 sec: 0.675597 ( -0.0969042 0.0969645 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.6723e-07 ( -4.46637e-08 4.55556e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55746 ( -1.18775 0.699756 )
Epeak [keV] : 76.5674 ( -76.3547 -76.5674 )
Norm@50keV : 6.77901E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.93 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 56 degrees of freedom
# Null hypothesis probability = 3.687305e-01
Photon flux (15-150 keV) in 5.972 sec: 0.668993 ( -0.100128 0.09957 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.61411e-07 ( -4.97079e-08 4.93843e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.55425 ( 1.5525 6.49222 )
beta : -2.23331 ( 2.23227 11.5635 )
Epeak [keV] : 76.0685 ( -75.5142 -75.5142 )
Norm@50keV : 6.80614E-03 ( -0.00272649 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.93 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 55 degrees of freedom
# Null hypothesis probability = 3.337813e-01
Photon flux (15-150 keV) in 5.972 sec: 0.669157 ( ) 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) = 7.58e-08
S(50-100 keV) = 8.59e-08
T90 vs. Hardness ratio plot
T90 = 5.76400002837181 sec.
Hardness ratio (energy fluence ratio) = 1.13325
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17662
Count Ratio (50-100 keV) / (15-25 keV) = 0.677709
Mask shadow pattern
IMX = -7.251013151863204E-01, IMY = -3.410517312909804E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.824000 -65.654800
-64.824000 0.084000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6305 22.0240 0.5 35.0 -92.2 10.4337 24.3 0.6 Crab
158.9303 18.7139 2.8 38.8 52.8 1.7250 4.2 ------ UNKNOWN
164.9035 57.4247 3.2 56.7 4.7 3.7985 3.6 ------ UNKNOWN
108.9960 -1.6591 2.9 17.3 -167.1 0.6223 3.9 ------ UNKNOWN
148.1573 66.5624 2.6 57.4 -9.6 3.5508 4.3 ------ UNKNOWN
88.1625 -28.2782 2.6 50.6 -167.0 1.8318 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.084000 6.056000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4855 22.0936 5.5 35.2 -92.1 -0.1004 -2.1 9.5 Crab
119.1174 -31.3095 2.2 43.8 157.0 0.2815 5.3 ------ UNKNOWN
120.6613 -26.1489 1.1 38.7 154.8 0.4021 10.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
66.876610 962.274200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5126 -40.5765 1.1 19.0 115.9 5.4663 10.7 1.5 Vela X-1
89.9315 -67.5319 2.3 45.4 168.6 5.3786 5.1 ------ UNKNOWN
70.1656 -69.7376 2.8 52.3 172.4 6.6566 4.1 ------ UNKNOWN
108.4363 -46.0654 2.9 22.2 175.6 1.7083 3.9 ------ UNKNOWN
53.7984 -66.0701 4.4 56.9 179.2 8.3807 2.7 ------ UNKNOWN
87.6726 -41.9093 2.7 31.3 -156.0 2.2792 4.3 ------ UNKNOWN
137.7218 28.9122 2.8 57.5 -9.5 10.5551 4.1 ------ UNKNOWN
105.1478 5.7571 2.2 35.3 -54.7 3.8796 5.3 ------ UNKNOWN
Plot creation:
Sun May 31 07:36:15 EDT 2015