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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
67.3660 28.8776 0.0092 14.0972 -70.6305 0.9028433 20.940 TRIG_00582184
Foreground time interval of the image:
-1.188 10.045 (delta_t = 11.233 [sec])
Background time interval of the image:
-239.656 -1.188 (delta_t = 238.468 [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)
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 -1.188 sec. to 19.228 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35321 ( -0.121854 0.121943 )
Norm@50keV : 4.21747E-03 ( -0.000281327 0.000280541 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.10 using 59 PHA bins.
# Reduced chi-squared = 1.072 for 57 degrees of freedom
# Null hypothesis probability = 3.307946e-01
Photon flux (15-150 keV) in 20.42 sec: 0.508420 ( -0.0343784 0.0344393 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.4052e-07 ( -6.31791e-08 6.36169e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.188 sec. to 19.228 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33979 ( -0.428699 0.123809 )
Epeak [keV] : 9956.07 ( -9999.34 -9999.34 )
Norm@50keV : 4.27646E-03 ( -0.000282087 0.00244047 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.18 using 59 PHA bins.
# Reduced chi-squared = 1.092 for 56 degrees of freedom
# Null hypothesis probability = 2.953976e-01
Photon flux (15-150 keV) in 20.42 sec: 0.508343 ( -0.035373 0.034297 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.39397e-07 ( -6.57218e-08 6.44312e-08 ) ergs/cm2
Band function
Time interval is from -1.188 sec. to 19.228 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.06575 ( 1.10302 1.10302 )
beta : -1.35251 ( -0.121958 0.121894 )
Epeak [keV] : 48.3819 ( -36.4647 -36.4647 )
Norm@50keV : 7.95823E-03 ( -0.00312892 0.603277 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.11 using 59 PHA bins.
# Reduced chi-squared = 1.111 for 55 degrees of freedom
# Null hypothesis probability = 2.659650e-01
Photon flux (15-150 keV) in 20.42 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] : 17.3175 ( )
R^2/D10^2 : 3.54282E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 122.53 using 59 PHA bins.
# Reduced chi-squared = 2.1496 for 57 degrees of freedom
# Null hypothesis probability = 1.077577e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.395e-08 6.034e-09
25- 50 1.974e-07 2.022e-08
50-150 4.250e-07 5.228e-08
15-150 6.663e-07 6.003e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 2.09352 (-0.138916 0.138905)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.16 using 59 PHA bins.
# Reduced chi-squared = 1.231 for 57 degrees of freedom
# Null hypothesis probability = 1.130976e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.064e-07 7.709e-09
25- 50 2.048e-07 1.947e-08
50-150 4.491e-07 1.358e-07
15-150 7.603e-07 1.507e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.62465 (-1.31707 1.53783)
R1^2/D10^2 : 0.598879 (-0.305519 0.757772)
kT2 [keV] : 29.0910 (-4.98205 8.31754)
R2^2/D10^2 : 5.36211E-03 (-0.00296061 0.00478167)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.14 using 59 PHA bins.
# Reduced chi-squared = 1.094 for 55 degrees of freedom
# Null hypothesis probability = 2.949075e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.590e-08 2.516e-08
25- 50 1.896e-07 3.878e-08
50-150 5.573e-07 1.527e-07
15-150 8.428e-07 1.886e-07
Peak spectrum fit
Power-law model
Time interval is from 1.608 sec. to 2.608 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53424 ( -0.241638 0.25083 )
Norm@50keV : 9.12013E-03 ( -0.00136803 0.00134162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.94 using 59 PHA bins.
# Reduced chi-squared = 0.5603 for 57 degrees of freedom
# Null hypothesis probability = 9.970679e-01
Photon flux (15-150 keV) in 1 sec: 1.14936 ( -0.157737 0.157792 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.60554e-08 ( -1.41099e-08 1.43886e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.608 sec. to 2.608 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25361 ( -0.992139 0.515238 )
Epeak [keV] : 131.377 ( -131.364 -131.364 )
Norm@50keV : 1.27222E-02 ( -0.0127228 0.0267481 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.63 using 59 PHA bins.
# Reduced chi-squared = 0.5648 for 56 degrees of freedom
# Null hypothesis probability = 9.964774e-01
Photon flux (15-150 keV) in 1 sec: 1.13702 ( -0.162193 0.16135 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.43513e-08 ( -1.49789e-08 1.52465e-08 ) ergs/cm2
Band function
Time interval is from 1.608 sec. to 2.608 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.20484 ( -0.440078 0.945097 )
beta : -9.37164 ( 9.37166 19.3717 )
Epeak [keV] : 121.864 ( -61.9256 -122.236 )
Norm@50keV : 1.34124E-02 ( -0.00547748 0.0153537 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.64 using 59 PHA bins.
# Reduced chi-squared = 0.5753 for 55 degrees of freedom
# Null hypothesis probability = 9.951881e-01
Photon flux (15-150 keV) in 1 sec: 1.13657 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.40924e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.3493 (-2.68435 3.19697)
R^2/D10^2 : 0.120483 (-0.0573239 0.113091)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.46 using 59 PHA bins.
# Reduced chi-squared = 0.7975 for 57 degrees of freedom
# Null hypothesis probability = 8.644849e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.919e-09 1.566e-09
25- 50 2.402e-08 5.080e-09
50-150 3.890e-08 1.114e-08
15-150 6.883e-08 1.442e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-94.2539 -199.363)
Norm : 4.69036 (-0.640935 0.64111)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.71 using 59 PHA bins.
# Reduced chi-squared = 0.5563 for 57 degrees of freedom
# Null hypothesis probability = 9.973430e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.168e-08 6.520e-09
25- 50 2.247e-08 1.275e-08
50-150 4.927e-08 2.747e-08
15-150 8.342e-08 4.587e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.47649 (-1.56038 2.32182)
R1^2/D10^2 : 6.29315 (-5.11943 44.3181)
kT2 [keV] : 21.2850 (-4.45662 7.22454)
R2^2/D10^2 : 3.40777E-02 (-0.0219813 0.0446874)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 28.82 using 59 PHA bins.
# Reduced chi-squared = 0.5241 for 55 degrees of freedom
# Null hypothesis probability = 9.986180e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.252e-08 6.210e-09
25- 50 1.977e-08 7.662e-09
50-150 5.091e-08 2.664e-08
15-150 8.320e-08 3.794e-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: 1.39229 ( -0.134072 0.134719 )
Norm@50keV : 5.09041E-03 ( -0.000383301 0.00038215 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.56 using 59 PHA bins.
# Reduced chi-squared = 1.027 for 57 degrees of freedom
# Null hypothesis probability = 4.179422e-01
Photon flux (15-150 keV) in 11.23 sec: 0.618841 ( -0.046573 0.0466451 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.53247e-07 ( -4.68639e-08 4.72545e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25786 ( -0.533428 0.255228 )
Epeak [keV] : 285.468 ( -285.461 -285.461 )
Norm@50keV : 5.92790E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.34 using 59 PHA bins.
# Reduced chi-squared = 1.042 for 56 degrees of freedom
# Null hypothesis probability = 3.892575e-01
Photon flux (15-150 keV) in 11.23 sec: 0.614667 ( -0.048947 0.04881 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.47891e-07 ( -5.14514e-08 5.08876e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.20196 ( 1.20196 1.20196 )
beta : -1.39231 ( -0.1347 0.134096 )
Epeak [keV] : 18.9841 ( )
Norm@50keV : 9.72676E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.56 using 59 PHA bins.
# Reduced chi-squared = 1.065 for 55 degrees of freedom
# Null hypothesis probability = 3.461731e-01
Photon flux (15-150 keV) in 11.23 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) = 1.93e-07
S(50-100 keV) = 3.02e-07
T90 vs. Hardness ratio plot
T90 = 17.9879999756813 sec.
Hardness ratio (energy fluence ratio) = 1.56477
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28841
Count Ratio (50-100 keV) / (15-25 keV) = 1.09636
Mask shadow pattern
IMX = 8.328994264363478E-02, IMY = 2.369173205339976E-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:
-239.656000 -1.188000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6358 22.0139 0.2 3.1 57.8 9.9504 47.4 0.2 Crab
96.7573 17.5866 2.7 15.8 84.1 0.9867 4.3 ------ UNKNOWN
35.9365 28.9454 2.0 40.8 -86.1 5.6271 5.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.188000 10.044590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7951 21.9921 4.7 3.2 58.9 0.1004 2.4 9.1 Crab
74.2050 -25.4852 2.3 47.1 171.4 0.4513 4.9 ------ UNKNOWN
67.3660 28.8776 0.5 14.1 -70.6 0.9029 20.9 ------ UNKNOWN
55.7342 18.7838 2.9 23.3 -107.8 0.1989 4.0 ------ UNKNOWN
36.8910 71.8233 2.4 56.3 -31.2 1.1115 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
46.044610 838.865900
840.344000 962.379100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6403 22.0145 0.2 16.2 106.1 39.0140 49.9 0.4 Crab
63.9811 37.9038 3.1 9.5 -21.9 2.5092 3.7 ------ UNKNOWN
61.7705 3.6223 3.4 25.8 -172.3 2.4579 3.4 ------ UNKNOWN
57.3295 18.8256 3.6 13.6 -140.6 2.2928 3.2 ------ UNKNOWN
53.1627 -10.3451 2.8 41.6 -163.9 5.1452 4.1 ------ UNKNOWN
351.0732 74.5252 3.0 58.6 -23.0 21.7799 3.9 ------ UNKNOWN
29.2680 -2.2677 2.7 48.0 -129.1 17.4311 4.3 ------ UNKNOWN
Plot creation:
Sat May 30 14:54:56 EDT 2015