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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
212.9847 16.9870 0.0145 9.0532 150.5733 0.0999093 13.256 TRIG_00222154
Foreground time interval of the image:
0.040 0.588 (delta_t = 0.548 [sec])
Background time interval of the image:
-239.512 0.040 (delta_t = 239.552 [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 0.040 sec. to 0.588 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.483733 ( -0.241854 0.223854 )
Norm@50keV : 1.08415E-02 ( -0.0015633 0.00152089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.43 using 59 PHA bins.
# Reduced chi-squared = 1.288 for 57 degrees of freedom
# Null hypothesis probability = 7.042899e-02
Photon flux (15-150 keV) in 0.548 sec: 1.28748 ( -0.162011 0.162626 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.04837e-08 ( -1.03694e-08 1.04179e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.040 sec. to 0.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.282647 ( -1.28846 0.851148 )
Epeak [keV] : 190.293 ( )
Norm@50keV : 2.16012E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.74 using 59 PHA bins.
# Reduced chi-squared = 1.281 for 56 degrees of freedom
# Null hypothesis probability = 7.656385e-02
Photon flux (15-150 keV) in 0.548 sec: 1.25491 ( -0.16793 0.16813 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.84358e-08 ( -1.13036e-08 1.1029e-08 ) ergs/cm2
Band function
Time interval is from 0.040 sec. to 0.588 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.732912 ( 0.732986 0.732986 )
beta : -0.483733 ( -0.223854 0.241851 )
Epeak [keV] : 23.3170 ( -23.3297 -23.3297 )
Norm@50keV : 1.41585E-02 ( -0.00542825 133695 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.43 using 59 PHA bins.
# Reduced chi-squared = 1.335 for 55 degrees of freedom
# Null hypothesis probability = 4.906833e-02
Photon flux (15-150 keV) in 0.548 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] : 30.8704 (-5.23506 7.50076)
R^2/D10^2 : 1.92305E-02 (-0.00847923 0.0132063)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.65 using 59 PHA bins.
# Reduced chi-squared = 1.292 for 57 degrees of freedom
# Null hypothesis probability = 6.810223e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.543e-09 4.006e-10
25- 50 9.632e-09 2.261e-09
50-150 6.408e-08 1.428e-08
15-150 7.526e-08 1.591e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 4.56183 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 131.63 using 59 PHA bins.
# Reduced chi-squared = 2.3093 for 57 degrees of freedom
# Null hypothesis probability = 7.761147e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.225e-09 3.551e-09
25- 50 1.197e-08 6.732e-09
50-150 2.626e-08 1.494e-08
15-150 4.446e-08 2.516e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.924344 (-0.917224 1.91321)
R1^2/D10^2 : 5.29194E+05 (-658689 3.1936e+10)
kT2 [keV] : 31.2358 (-5.36678 7.7482)
R2^2/D10^2 : 1.85613E-02 (-0.00825552 0.00972449)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.87 using 59 PHA bins.
# Reduced chi-squared = 1.325 for 55 degrees of freedom
# Null hypothesis probability = 5.373536e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.679e-09 3.965e-10
25- 50 9.492e-09 2.310e-09
50-150 6.432e-08 1.574e-08
15-150 7.550e-08 1.643e-08
Peak spectrum fit
Power-law model
Time interval is from -0.184 sec. to 0.816 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.530925 ( -0.289923 0.265293 )
Norm@50keV : 6.48981E-03 ( -0.00108351 0.00104654 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.32 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 57 degrees of freedom
# Null hypothesis probability = 4.264378e-01
Photon flux (15-150 keV) in 1 sec: 0.764884 ( -0.111776 0.112354 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.58449e-08 ( -1.27909e-08 1.28641e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.184 sec. to 0.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 8.04163E-02 ( -1.50658 0.566851 )
Epeak [keV] : 272.740 ( -272.761 -272.761 )
Norm@50keV : 9.72970E-03 ( -0.00413153 0.0246225 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.90 using 59 PHA bins.
# Reduced chi-squared = 1.034 for 56 degrees of freedom
# Null hypothesis probability = 4.049557e-01
Photon flux (15-150 keV) in 1 sec: 0.751863 ( -0.117264 0.117166 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.45474e-08 ( -1.38764e-08 1.34362e-08 ) ergs/cm2
Band function
Time interval is from -0.184 sec. to 0.816 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.848036 ( 0.848036 0.848036 )
beta : -0.530927 ( -0.265305 0.290183 )
Epeak [keV] : 17.9664 ( -17.9663 -17.9663 )
Norm@50keV : 8.89227E-03 ( -0.0033999 90854.3 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.32 using 59 PHA bins.
# Reduced chi-squared = 1.060 for 55 degrees of freedom
# Null hypothesis probability = 3.541684e-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] : 30.4633 (-5.98748 9.22629)
R^2/D10^2 : 1.16277E-02 (-0.00588514 0.0100435)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.34 using 59 PHA bins.
# Reduced chi-squared = 1.059 for 57 degrees of freedom
# Null hypothesis probability = 3.561123e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.672e-09 5.308e-10
25- 50 1.038e-08 2.863e-09
50-150 6.763e-08 1.901e-08
15-150 7.968e-08 2.329e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 2.82880 (-0.466886 0.466881)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 96.96 using 59 PHA bins.
# Reduced chi-squared = 1.701 for 57 degrees of freedom
# Null hypothesis probability = 7.611902e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.041e-09 4.032e-09
25- 50 1.354e-08 7.685e-09
50-150 2.970e-08 1.684e-08
15-150 5.029e-08 2.854e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.27107 (-1.27709 1.21183)
R1^2/D10^2 : 9028.62 (-8647.54 3.98707e+08)
kT2 [keV] : 31.2358 (-6.27576 9.89675)
R2^2/D10^2 : 1.07858E-02 (-0.0055905 0.00860589)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.71 using 59 PHA bins.
# Reduced chi-squared = 1.067 for 55 degrees of freedom
# Null hypothesis probability = 3.411309e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.235e-09 5.982e-10
25- 50 1.007e-08 3.038e-09
50-150 6.821e-08 1.875e-08
15-150 8.051e-08 2.216e-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: 0.483733 ( -0.241854 0.223854 )
Norm@50keV : 1.08415E-02 ( -0.0015633 0.00152089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.43 using 59 PHA bins.
# Reduced chi-squared = 1.288 for 57 degrees of freedom
# Null hypothesis probability = 7.042899e-02
Photon flux (15-150 keV) in 0.548 sec: 1.28748 ( -0.162011 0.162626 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.04837e-08 ( -1.03694e-08 1.04179e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.282647 ( -1.28846 0.851148 )
Epeak [keV] : 190.293 ( )
Norm@50keV : 2.16012E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.74 using 59 PHA bins.
# Reduced chi-squared = 1.281 for 56 degrees of freedom
# Null hypothesis probability = 7.656385e-02
Photon flux (15-150 keV) in 0.548 sec: 1.25491 ( -0.16793 0.16813 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.84358e-08 ( -1.13036e-08 1.1029e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.732912 ( 0.732986 0.732986 )
beta : -0.483733 ( -0.223854 0.241851 )
Epeak [keV] : 23.3170 ( -23.3297 -23.3297 )
Norm@50keV : 1.41585E-02 ( -0.00542825 133691 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.43 using 59 PHA bins.
# Reduced chi-squared = 1.335 for 55 degrees of freedom
# Null hypothesis probability = 4.906833e-02
Photon flux (15-150 keV) in 0.548 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) = 1.02e-08
S(50-100 keV) = 2.92e-08
T90 vs. Hardness ratio plot
T90 = 0.504000008106232 sec.
Hardness ratio (energy fluence ratio) = 2.86275
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 3.57886
Count Ratio (50-100 keV) / (15-25 keV) = 5.37942
Mask shadow pattern
IMX = -1.387802605343761E-01, IMY = -7.828382608907439E-02
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:
-239.512000 0.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4061 35.4220 5.1 37.9 45.4 0.7933 2.3 5.4 Her X-1
229.8277 -15.6757 2.6 45.3 135.1 2.7189 4.4 ------ UNKNOWN
235.9618 37.5980 2.6 23.9 35.2 0.7209 4.5 ------ UNKNOWN
224.4958 33.1106 2.5 13.5 35.2 0.6702 4.6 ------ UNKNOWN
168.8896 40.3250 2.6 37.9 -76.3 1.9991 4.5 ------ UNKNOWN
165.8988 16.7730 3.5 43.1 -112.3 2.4872 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.040000 0.588000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4936 35.2232 15.6 38.0 45.7 -0.0127 -0.7 7.4 Her X-1
260.5717 28.5425 2.3 43.5 55.5 0.1765 5.1 ------ UNKNOWN
212.9847 16.9870 0.9 9.1 150.6 0.0999 13.3 ------ UNKNOWN
193.8789 5.9810 2.0 26.0 -156.5 0.0465 5.6 ------ UNKNOWN
170.5111 3.7675 2.3 45.0 -132.0 0.1066 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
46.988600 962.568000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4582 35.3455 5.0 41.1 40.2 2.1646 2.3 0.2 Her X-1
225.2253 25.4128 3.4 14.1 36.4 1.2574 3.4 ------ UNKNOWN
227.0607 40.1086 2.9 26.1 9.9 1.5971 3.9 ------ UNKNOWN
227.7178 44.7917 2.4 30.4 5.8 2.1852 4.9 ------ UNKNOWN
178.6260 -19.0276 3.0 49.4 -150.4 4.2166 3.9 ------ UNKNOWN
Plot creation:
Sun May 31 12:28:12 EDT 2015