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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
98.3949 6.9511 0.0074 20.7333 148.5971 1.3842848 26.006 TRIG_00629578
Foreground time interval of the image:
-0.804 20.061 (delta_t = 20.865 [sec])
Background time interval of the image:
-119.640 -0.804 (delta_t = 118.836 [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 -0.804 sec. to 28.724 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81000 ( -0.109235 0.111008 )
Norm@50keV : 3.44253E-03 ( -0.000225158 0.000223035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.40 using 59 PHA bins.
# Reduced chi-squared = 0.8316 for 57 degrees of freedom
# Null hypothesis probability = 8.137181e-01
Photon flux (15-150 keV) in 29.53 sec: 0.476226 ( -0.0286398 0.0286787 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.35558e-07 ( -6.2093e-08 6.25853e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.804 sec. to 28.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61104 ( -0.445195 0.210637 )
Epeak [keV] : 89.6101 ( -32.267 -89.6107 )
Norm@50keV : 4.40758E-03 ( -0.00115635 0.0031757 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.71 using 59 PHA bins.
# Reduced chi-squared = 0.8341 for 56 degrees of freedom
# Null hypothesis probability = 8.072900e-01
Photon flux (15-150 keV) in 29.53 sec: 0.471254 ( -0.0303 0.030276 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.17654e-07 ( -7.24489e-08 7.22717e-08 ) ergs/cm2
Band function
Time interval is from -0.804 sec. to 28.724 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.520811 ( -0.518959 -0.518959 )
beta : -1.89664 ( -0.17357 0.149434 )
Epeak [keV] : 28.3646 ( -28.3676 112.277 )
Norm@50keV : 0.169782 ( -0.167962 372.367 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.06 using 59 PHA bins.
# Reduced chi-squared = 0.8192 for 55 degrees of freedom
# Null hypothesis probability = 8.282489e-01
Photon flux (15-150 keV) in 29.53 sec: 0.467091 ( 6.53291 -0.467091 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.18548e-07 ( -9.18342e-07 -6.49808e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.5876 ( )
R^2/D10^2 : 0.125755 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 115.66 using 59 PHA bins.
# Reduced chi-squared = 2.0292 for 57 degrees of freedom
# Null hypothesis probability = 7.137378e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.051e-07 1.128e-08
25- 50 3.171e-07 2.244e-08
50-150 2.499e-07 3.674e-08
15-150 6.721e-07 5.005e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8263 (-19.4638 32.9089)
Norm : 2.08732 (-0.185295 0.191935)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.06 using 59 PHA bins.
# Reduced chi-squared = 0.8431 for 57 degrees of freedom
# Null hypothesis probability = 7.945529e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.611e-07 1.686e-08
25- 50 2.785e-07 1.925e-08
50-150 4.508e-07 1.367e-07
15-150 8.904e-07 1.474e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.79100 (-1.20932 1.2549)
R1^2/D10^2 : 0.676836 (-0.293165 0.671265)
kT2 [keV] : 25.6311 (-5.72252 10.4825)
R2^2/D10^2 : 4.88144E-03 (-0.00334652 0.00787161)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.92 using 59 PHA bins.
# Reduced chi-squared = 0.8712 for 55 degrees of freedom
# Null hypothesis probability = 7.397543e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.596e-07 3.135e-08
25- 50 2.782e-07 4.707e-08
50-150 4.799e-07 1.827e-07
15-150 9.177e-07 2.284e-07
Peak spectrum fit
Power-law model
Time interval is from 16.772 sec. to 17.772 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75268 ( -0.26219 0.277169 )
Norm@50keV : 6.79267E-03 ( -0.00123847 0.00120833 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.60 using 59 PHA bins.
# Reduced chi-squared = 0.9930 for 57 degrees of freedom
# Null hypothesis probability = 4.899358e-01
Photon flux (15-150 keV) in 1 sec: 0.919391 ( -0.145291 0.145325 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.26693e-08 ( -1.1592e-08 1.18603e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 16.772 sec. to 17.772 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.885242 ( -1.45855 1.01492 )
Epeak [keV] : 56.7387 ( -17.2221 -56.7388 )
Norm@50keV : 2.07870E-02 ( -0.0207868 0.118489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.74 using 59 PHA bins.
# Reduced chi-squared = 0.9776 for 56 degrees of freedom
# Null hypothesis probability = 5.224987e-01
Photon flux (15-150 keV) in 1 sec: 0.898098 ( -0.147833 0.147792 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83506e-08 ( -1.22831e-08 1.29945e-08 ) ergs/cm2
Band function
Time interval is from 16.772 sec. to 17.772 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.885190 ( -2.68804 1.60891 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 56.7274 ( -17.2153 8412.38 )
Norm@50keV : 2.07875E-02 ( -0.0207875 0.118907 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.74 using 59 PHA bins.
# Reduced chi-squared = 0.9953 for 55 degrees of freedom
# Null hypothesis probability = 4.843709e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.84238e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.5732 (-1.9609 2.42485)
R^2/D10^2 : 0.263505 (-0.13374 0.258697)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.82 using 59 PHA bins.
# Reduced chi-squared = 1.067 for 57 degrees of freedom
# Null hypothesis probability = 3.402467e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.436e-09 2.445e-09
25- 50 2.241e-08 5.315e-09
50-150 1.760e-08 6.626e-09
15-150 4.745e-08 1.149e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8731 (-39.1994 -99.8944)
Norm : 4.12062 (-0.769044 0.967087)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.09 using 59 PHA bins.
# Reduced chi-squared = 0.9664 for 57 degrees of freedom
# Null hypothesis probability = 5.472516e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.077e-08 2.452e-09
25- 50 1.862e-08 4.165e-09
50-150 3.015e-08 1.832e-08
15-150 5.954e-08 2.044e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.88466 (-4.1943 69.3189)
R1^2/D10^2 : 1.10907 (-0.803279 41.649)
kT2 [keV] : 20.6965 (-18.0131 55.8383)
R2^2/D10^2 : 2.07448E-02 (-0.0204034 0.16458)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.72 using 59 PHA bins.
# Reduced chi-squared = 0.9949 for 55 degrees of freedom
# Null hypothesis probability = 4.853874e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.987e-09 5.765e-09
25- 50 1.960e-08 1.032e-08
50-150 2.915e-08 1.732e-08
15-150 5.874e-08 2.941e-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: 1.72105 ( -0.110966 0.112352 )
Norm@50keV : 4.11937E-03 ( -0.000267274 0.000265144 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.12 using 59 PHA bins.
# Reduced chi-squared = 0.6862 for 57 degrees of freedom
# Null hypothesis probability = 9.661605e-01
Photon flux (15-150 keV) in 20.86 sec: 0.551183 ( -0.0339409 0.0340085 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.94368e-07 ( -5.37681e-08 5.4164e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65501 ( -0.426517 0.430418 )
Epeak [keV] : 246.295 ( )
Norm@50keV : 4.46521E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.04 using 59 PHA bins.
# Reduced chi-squared = 0.6971 for 56 degrees of freedom
# Null hypothesis probability = 9.587546e-01
Photon flux (15-150 keV) in 20.86 sec: 0.549238 ( -0.035683 0.035222 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.89745e-07 ( -6.16538e-08 5.81222e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.401100 ( -1.47336 -1.47336 )
beta : -1.78118 ( 1.77408 0.139518 )
Epeak [keV] : 28.5855 ( -25.2918 66.5767 )
Norm@50keV : 0.153650 ( -0.153328 484.832 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.78 using 59 PHA bins.
# Reduced chi-squared = 0.6870 for 55 degrees of freedom
# Null hypothesis probability = 9.630732e-01
Photon flux (15-150 keV) in 20.86 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) = 2.64e-07
S(50-100 keV) = 3.02e-07
T90 vs. Hardness ratio plot
T90 = 24.4359999299049 sec.
Hardness ratio (energy fluence ratio) = 1.14394
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1905
Count Ratio (50-100 keV) / (15-25 keV) = 0.641379
Mask shadow pattern
IMX = -3.230877964462633E-01, IMY = -1.972357388319213E-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:
-119.640000 -0.804000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6613 22.0330 0.3 0.0 87.3 5.0002 43.2 1.9 Crab
110.9537 24.5736 2.7 25.2 93.0 0.7037 4.2 ------ UNKNOWN
84.7452 26.3256 0.9 4.4 27.1 1.5542 12.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.804000 20.060600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5383 21.9260 4.4 0.1 -122.7 0.1216 2.6 7.5 Crab
122.0222 7.9792 2.0 39.5 119.0 0.9148 5.6 ------ UNKNOWN
98.3949 6.9511 0.4 20.7 148.6 1.3842 26.0 ------ UNKNOWN
74.9797 10.0263 2.7 14.6 -129.8 0.2185 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.260580 1190.439600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6342 22.0187 0.2 20.7 -23.6 46.4916 66.9 0.3 Crab
126.9250 -43.6270 3.0 56.8 173.9 16.0683 3.8 ------ UNKNOWN
103.0736 19.9358 2.7 13.7 37.1 2.7952 4.3 ------ UNKNOWN
102.9902 -10.2670 2.8 17.8 -176.6 2.6607 4.1 ------ UNKNOWN
118.1328 -44.0618 3.8 54.1 -179.2 8.0858 3.1 ------ UNKNOWN
84.7342 26.3177 0.5 23.3 -14.1 17.0734 22.1 ------ UNKNOWN
109.6577 -49.5359 3.4 57.4 -170.4 10.7976 3.4 ------ UNKNOWN
Plot creation:
Thu May 28 13:34:38 EDT 2015