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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
87.7797 -24.7912 0.0181 32.2416 -141.7938 1.0141090 10.612 TRIG_00514586
Foreground time interval of the image:
-2.296 50.133 (delta_t = 52.429 [sec])
Background time interval of the image:
-566.567 -546.830 (delta_t = 19.737 [sec])
-239.968 -2.296 (delta_t = 237.672 [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 8.192000
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 8.192000
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 8.192000
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 -2.296 sec. to 71.688 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41329 ( -0.223277 0.224352 )
Norm@50keV : 1.20912E-03 ( -0.000160086 0.000159319 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.93 using 59 PHA bins.
# Reduced chi-squared = 0.8410 for 57 degrees of freedom
# Null hypothesis probability = 7.982454e-01
Photon flux (15-150 keV) in 73.98 sec: 0.147697 ( -0.0194339 0.0194689 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.62022e-07 ( -1.26057e-07 1.27894e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.296 sec. to 71.688 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.574992 ( -1.26275 0.922052 )
Epeak [keV] : 84.8081 ( -23.9315 -84.8067 )
Norm@50keV : 3.19315E-03 ( -0.00319328 0.00988341 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.86 using 59 PHA bins.
# Reduced chi-squared = 0.8188 for 56 degrees of freedom
# Null hypothesis probability = 8.313351e-01
Photon flux (15-150 keV) in 73.98 sec: 0.142116 ( -0.020779 0.020619 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.06656e-07 ( -1.39671e-07 1.43847e-07 ) ergs/cm2
Band function
Time interval is from -2.296 sec. to 71.688 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.507342 ( 0.70563 0.70563 )
beta : -2.22829 ( 2.0173 2.26889 )
Epeak [keV] : 80.7993 ( -80.79 374.349 )
Norm@50keV : 3.47987E-03 ( -0.0034878 74.8197 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.71 using 59 PHA bins.
# Reduced chi-squared = 0.8310 for 55 degrees of freedom
# Null hypothesis probability = 8.097839e-01
Photon flux (15-150 keV) in 73.98 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] : 15.6958 (-2.17 2.62023)
R^2/D10^2 : 1.48337E-02 (-0.00617999 0.0100868)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.67 using 59 PHA bins.
# Reduced chi-squared = 0.9066 for 57 degrees of freedom
# Null hypothesis probability = 6.744581e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.613e-08 1.460e-08
25- 50 2.323e-07 4.276e-08
50-150 3.970e-07 9.518e-08
15-150 6.854e-07 1.237e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 0.609158 (-0.0787425 0.0787387)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.75 using 59 PHA bins.
# Reduced chi-squared = 0.8378 for 57 degrees of freedom
# Null hypothesis probability = 8.035366e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.122e-07 6.329e-08
25- 50 2.159e-07 1.187e-07
50-150 4.735e-07 2.618e-07
15-150 8.016e-07 4.494e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.45200 (-2.77524 6.28868)
R1^2/D10^2 : 0.525303 (-0.492925 177.292)
kT2 [keV] : 18.5786 (-3.50668 15.2791)
R2^2/D10^2 : 7.55465E-03 (-0.0069299 0.00882369)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.43 using 59 PHA bins.
# Reduced chi-squared = 0.8260 for 55 degrees of freedom
# Null hypothesis probability = 8.177303e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.623e-08 4.959e-08
25- 50 2.090e-07 8.867e-08
50-150 4.574e-07 2.037e-07
15-150 7.627e-07 2.917e-07
Peak spectrum fit
Power-law model
Time interval is from 41.012 sec. to 42.012 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44507 ( -0.672446 0.672477 )
Norm@50keV : 3.76973E-03 ( -0.00141928 0.0013806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.42 using 59 PHA bins.
# Reduced chi-squared = 0.9898 for 57 degrees of freedom
# Null hypothesis probability = 4.969213e-01
Photon flux (15-150 keV) in 1 sec: 0.464002 ( -0.168452 0.169318 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.61066e-08 ( -1.44592e-08 1.516e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 41.012 sec. to 42.012 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26388 ( -2.66009 1.12407 )
Epeak [keV] : 198.911 ( -136.164 -136.164 )
Norm@50keV : 4.67121E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.39 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 56 degrees of freedom
# Null hypothesis probability = 4.602449e-01
Photon flux (15-150 keV) in 1 sec: 0.460153 ( -0.173069 0.169911 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.55434e-08 ( -1.54614e-08 1.56128e-08 ) ergs/cm2
Band function
Time interval is from 41.012 sec. to 42.012 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.32840 ( 1.21662 5.66883 )
beta : -1.67208 ( 1.46956 0.688064 )
Epeak [keV] : 26.4695 ( -29.321 160.335 )
Norm@50keV : 97.7396 ( -97.7386 87.646 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.49 using 59 PHA bins.
# Reduced chi-squared = 1.009 for 55 degrees of freedom
# Null hypothesis probability = 4.561178e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.54243e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 18.0414 (-8.84322 12.8456)
R^2/D10^2 : 2.77005E-02 (-0.0276181 0.249541)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.88 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 57 degrees of freedom
# Null hypothesis probability = 4.064154e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.804e-09 1.229e-09
25- 50 8.357e-09 5.390e-09
50-150 1.976e-08 1.336e-08
15-150 2.992e-08 1.894e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 1.90390 (-0.682081 0.682406)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.47 using 59 PHA bins.
# Reduced chi-squared = 0.9906 for 57 degrees of freedom
# Null hypothesis probability = 4.950351e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.741e-09 2.968e-09
25- 50 9.120e-09 5.980e-09
50-150 2.000e-08 1.268e-08
15-150 3.386e-08 2.121e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.62418 (-2.3831 4.95893)
R1^2/D10^2 : 1.22112 (-1.15068 12.1288)
kT2 [keV] : 26.8457 (-11.7156 120.187)
R2^2/D10^2 : 6.13617E-03 (-0.00595684 0.0388317)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.82 using 59 PHA bins.
# Reduced chi-squared = 0.9966 for 55 degrees of freedom
# Null hypothesis probability = 4.816449e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.388e-09 3.168e-09
25- 50 8.354e-09 4.175e-09
50-150 2.316e-08 1.442e-08
15-150 3.690e-08 2.068e-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: 1.44320 ( -0.244122 0.246191 )
Norm@50keV : 1.31077E-03 ( -0.0001944 0.000193122 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.01 using 59 PHA bins.
# Reduced chi-squared = 1.053 for 57 degrees of freedom
# Null hypothesis probability = 3.673237e-01
Photon flux (15-150 keV) in 52.43 sec: 0.161263 ( -0.0235092 0.0235456 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.58468e-07 ( -1.07142e-07 1.08971e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.375962 ( -1.46263 1.11005 )
Epeak [keV] : 74.4578 ( -19.7968 -74.4577 )
Norm@50keV : 4.59495E-03 ( -0.00459496 0.0190406 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.38 using 59 PHA bins.
# Reduced chi-squared = 1.025 for 56 degrees of freedom
# Null hypothesis probability = 4.236541e-01
Photon flux (15-150 keV) in 52.43 sec: 0.153909 ( -0.025037 0.024889 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.04439e-07 ( -1.15143e-07 1.22335e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.376360 ( 0.787077 0.787077 )
beta : -7.73542 ( 4.94587 14.9459 )
Epeak [keV] : 74.4504 ( -74.4528 20.821 )
Norm@50keV : 4.59337E-03 ( -0.00281934 43.9538 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.38 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 55 degrees of freedom
# Null hypothesis probability = 3.868951e-01
Photon flux (15-150 keV) in 52.43 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) = 2.04e-07
S(50-100 keV) = 3.06e-07
T90 vs. Hardness ratio plot
T90 = 64.3199999928474 sec.
Hardness ratio (energy fluence ratio) = 1.5
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31537
Count Ratio (50-100 keV) / (15-25 keV) = 1.27395
Mask shadow pattern
IMX = -4.956360947873087E-01, IMY = 3.901141554868550E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-566.567360 -546.830400
-239.968000 -2.296000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6321 22.0200 0.2 21.5 -19.3 10.4707 53.0 0.3 Crab
109.2785 -41.4897 2.1 48.4 -170.8 2.1773 5.4 ------ UNKNOWN
70.5319 -34.4407 2.9 48.0 -128.7 3.7622 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.296000 50.132600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8325 21.9364 0.0 21.3 -19.1 -0.0855 -1.1 12.0 Crab
131.6890 -28.7638 2.3 47.3 159.1 1.0239 5.2 ------ UNKNOWN
86.5394 45.8503 2.2 41.3 8.0 0.6592 5.3 ------ UNKNOWN
87.7797 -24.7911 1.1 32.2 -141.8 1.0129 10.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
103.332590 962.101300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6322 22.0218 0.5 46.9 23.7 31.1518 22.4 0.4 Crab
135.6637 -40.6668 223.4 42.7 152.9 0.0495 0.1 9.1 Vela X-1
95.4036 23.2670 2.5 48.6 38.3 9.6699 4.5 ------ UNKNOWN
150.9449 -67.0901 4.2 57.0 -175.6 6.3875 2.7 ------ UNKNOWN
78.1952 -49.9974 3.1 26.3 -137.1 1.6918 3.7 ------ UNKNOWN
149.4415 -75.3557 3.1 59.1 -166.1 13.0184 3.8 ------ UNKNOWN
60.1098 -34.6271 3.0 25.9 -90.0 2.0087 3.9 ------ UNKNOWN
Plot creation:
Sat May 30 20:34:10 EDT 2015