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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
127.0016 46.2340 0.0037 36.5222 142.3095 10.1894655 51.851 TRIG_00596426
Foreground time interval of the image:
-8.688 17.725 (delta_t = 26.413 [sec])
Background time interval of the image:
-239.976 -8.688 (delta_t = 231.288 [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 -8.688 sec. to 125.348 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15453 ( -0.0340804 0.0339422 )
Norm@50keV : 1.14163E-02 ( -0.000210092 0.00020952 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.33 using 59 PHA bins.
# Reduced chi-squared = 0.7952 for 57 degrees of freedom
# Null hypothesis probability = 8.674891e-01
Photon flux (15-150 keV) in 134 sec: 1.33210 ( -0.026639 0.0267472 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57269e-05 ( -2.83473e-07 2.83573e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.688 sec. to 125.348 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14925 ( -0.107471 0.0678821 )
Epeak [keV] : 9997.16 ( )
Norm@50keV : 1.14732E-02 ( -0.000200533 0.00175636 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.29 using 59 PHA bins.
# Reduced chi-squared = 0.8088 for 56 degrees of freedom
# Null hypothesis probability = 8.462556e-01
Photon flux (15-150 keV) in 134 sec: 1.33091 ( -0.0261 0.02716 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56915e-05 ( -2.81132e-07 3.3299e-07 ) ergs/cm2
Band function
Time interval is from -8.688 sec. to 125.348 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.757762 ( 0.703091 0.703091 )
beta : -1.16270 ( 1.17069 0.0438509 )
Epeak [keV] : 34.7943 ( -55.8452 171.276 )
Norm@50keV : 0.314206 ( -0.31421 404.312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.15 using 59 PHA bins.
# Reduced chi-squared = 0.8027 for 55 degrees of freedom
# Null hypothesis probability = 8.524474e-01
Photon flux (15-150 keV) in 134 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] : 22.2831 ( )
R^2/D10^2 : 4.26813E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 614.48 using 59 PHA bins.
# Reduced chi-squared = 10.780 for 57 degrees of freedom
# Null hypothesis probability = 1.795592e-94
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.225e-07 2.077e-08
25- 50 2.784e-06 7.705e-08
50-150 1.033e-05 2.499e-07
15-150 1.363e-05 2.687e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 5.82688 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 512.48 using 59 PHA bins.
# Reduced chi-squared = 8.9909 for 57 degrees of freedom
# Null hypothesis probability = 1.755426e-74
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.944e-06 4.020e-08
25- 50 3.740e-06 7.169e-08
50-150 8.203e-06 1.655e-07
15-150 1.389e-05 2.613e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.28246 (-0.73575 0.779893)
R1^2/D10^2 : 0.438544 (-0.0950762 0.130149)
kT2 [keV] : 38.7434 (-3.21847 4.22143)
R2^2/D10^2 : 6.22930E-03 (-0.00169091 0.00198056)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.96 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 55 degrees of freedom
# Null hypothesis probability = 4.021203e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.166e-06 7.611e-08
25- 50 3.349e-06 1.226e-07
50-150 1.120e-05 4.924e-07
15-150 1.571e-05 5.762e-07
Peak spectrum fit
Power-law model
Time interval is from 51.424 sec. to 52.424 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03015 ( -0.0796724 0.079213 )
Norm@50keV : 3.90456E-02 ( -0.00174721 0.00174637 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.22 using 59 PHA bins.
# Reduced chi-squared = 0.9162 for 57 degrees of freedom
# Null hypothesis probability = 6.545507e-01
Photon flux (15-150 keV) in 1 sec: 4.50337 ( -0.204569 0.204631 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17803e-07 ( -2.10877e-08 2.11588e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 51.424 sec. to 52.424 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.754132 ( -0.328113 0.295517 )
Epeak [keV] : 255.401 ( -108.387 -255.401 )
Norm@50keV : 5.20718E-02 ( -0.0105558 0.0204951 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.85 using 59 PHA bins.
# Reduced chi-squared = 0.8902 for 56 degrees of freedom
# Null hypothesis probability = 7.054621e-01
Photon flux (15-150 keV) in 1 sec: 4.45146 ( -0.21225 0.21218 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.11854e-07 ( -2.252e-08 2.2385e-08 ) ergs/cm2
Band function
Time interval is from 51.424 sec. to 52.424 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.902982 ( 0.902982 0.902982 )
beta : -1.03016 ( -0.0792039 0.079703 )
Epeak [keV] : 30.6028 ( )
Norm@50keV : 6.20774E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.22 using 59 PHA bins.
# Reduced chi-squared = 0.9495 for 55 degrees of freedom
# Null hypothesis probability = 5.814083e-01
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] : 21.0715 ( )
R^2/D10^2 : 0.183413 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 126.07 using 59 PHA bins.
# Reduced chi-squared = 2.2118 for 57 degrees of freedom
# Null hypothesis probability = 3.928666e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.536e-08 1.430e-09
25- 50 7.914e-08 5.115e-09
50-150 2.620e-07 2.170e-08
15-150 3.565e-07 2.115e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 18.0622 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 162.94 using 59 PHA bins.
# Reduced chi-squared = 2.8585 for 57 degrees of freedom
# Null hypothesis probability = 3.867158e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.498e-08 2.240e-09
25- 50 8.652e-08 4.900e-09
50-150 1.897e-07 9.650e-09
15-150 3.212e-07 1.855e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.99264 (-1.78544 2.02077)
R1^2/D10^2 : 1.44722 (-0.609164 1.3317)
kT2 [keV] : 35.6171 (-6.00384 11.1743)
R2^2/D10^2 : 2.97711E-02 (-0.0167784 0.0247563)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.11 using 59 PHA bins.
# Reduced chi-squared = 0.9111 for 55 degrees of freedom
# Null hypothesis probability = 6.615989e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.806e-08 6.505e-09
25- 50 8.311e-08 1.361e-08
50-150 3.040e-07 7.785e-08
15-150 4.151e-07 8.495e-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: 0.953871 ( -0.0441001 0.0437723 )
Norm@50keV : 2.58157E-02 ( -0.000635729 0.000632676 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.10 using 59 PHA bins.
# Reduced chi-squared = 0.6334 for 57 degrees of freedom
# Null hypothesis probability = 9.861369e-01
Photon flux (15-150 keV) in 26.41 sec: 2.96634 ( -0.074353 0.0745343 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.49677e-06 ( -1.80627e-07 1.80858e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.947257 ( -0.0350842 0.0562281 )
Epeak [keV] : 9999.98 ( )
Norm@50keV : 2.59754E-02 ( -0.00063619 0.000595318 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.08 using 59 PHA bins.
# Reduced chi-squared = 0.6443 for 56 degrees of freedom
# Null hypothesis probability = 9.822302e-01
Photon flux (15-150 keV) in 26.41 sec: 2.96385 ( -0.07271 0.0755 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.48628e-06 ( -1.81331e-07 1.98682e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -4.99995 -4.99995 )
beta : -0.963868 ( -0.04515 0.045195 )
Epeak [keV] : 24.4848 ( -24.4848 3.93845 )
Norm@50keV : 1853.42 ( -42.4742 3.44318e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.24 using 59 PHA bins.
# Reduced chi-squared = 0.6407 for 55 degrees of freedom
# Null hypothesis probability = 9.824713e-01
Photon flux (15-150 keV) in 26.41 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) = 3.21e-06
S(50-100 keV) = 5.77e-06
T90 vs. Hardness ratio plot
T90 = 80.0759999155998 sec.
Hardness ratio (energy fluence ratio) = 1.79751
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.64325
Count Ratio (50-100 keV) / (15-25 keV) = 1.65177
Mask shadow pattern
IMX = -5.860254435949162E-01, IMY = -4.527762847548107E-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:
-239.976000 -8.688000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6345 22.0140 0.5 44.1 -150.4 9.6959 24.7 0.1 Crab
105.6044 59.8504 2.4 18.0 139.5 0.9080 4.7 ------ UNKNOWN
107.0313 25.1793 2.5 47.0 179.3 1.7226 4.6 ------ UNKNOWN
325.1336 45.7394 3.0 54.3 -6.0 2.3436 3.8 ------ UNKNOWN
357.4361 39.5795 2.3 46.6 -36.2 2.3009 5.0 ------ UNKNOWN
60.1914 20.7233 2.4 44.4 -118.9 4.3452 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.688000 17.724610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4246 22.0275 5.4 44.1 -150.2 0.3562 2.1 11.6 Crab
168.2072 63.2786 3.0 39.3 95.3 1.6937 3.8 ------ UNKNOWN
167.0277 69.4303 2.6 34.6 88.7 1.0660 4.4 ------ UNKNOWN
127.0016 46.2340 0.2 36.5 142.3 10.1892 51.8 ------ UNKNOWN
302.1078 63.2345 3.9 45.8 20.3 0.5910 3.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
75.524600 962.164700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6294 22.0114 0.4 42.5 -124.3 40.0589 28.0 0.3 Crab
120.0616 -9.3329 3.0 55.9 173.6 10.7198 3.9 ------ UNKNOWN
180.0497 75.3703 2.8 36.5 5.2 2.4446 4.1 ------ UNKNOWN
129.5903 39.3641 2.9 7.1 148.9 1.8408 3.9 ------ UNKNOWN
126.9697 46.2348 1.9 0.0 -107.0 3.0350 6.0 ------ UNKNOWN
102.5680 -8.6167 3.6 59.0 -166.2 11.4319 3.2 ------ UNKNOWN
Plot creation:
Sat May 30 13:51:45 EDT 2015