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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
97.8780 24.3487 0.0123 49.3476 -170.8726 4.4950832 15.593 TRIG_00451343
Foreground time interval of the image:
-38.000 67.325 (delta_t = 105.325 [sec])
Background time interval of the image:
-239.376 -38.000 (delta_t = 201.376 [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 16.384000
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 16.384000
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 16.384000
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 -38.000 sec. to 133.296 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67222 ( -0.142771 0.145105 )
Norm@50keV : 2.18976E-03 ( -0.000179086 0.000177611 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.09 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 57 degrees of freedom
# Null hypothesis probability = 2.699496e-01
Photon flux (15-150 keV) in 171.3 sec: 0.288059 ( -0.0231321 0.023204 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.48123e-06 ( -2.99828e-07 3.01908e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -38.000 sec. to 133.296 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67600 ( -0.147181 0.142694 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 2.18710E-03 ( -0.00219201 0.00152576 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.10 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 56 degrees of freedom
# Null hypothesis probability = 2.399251e-01
Photon flux (15-150 keV) in 171.3 sec: 0.287911 ( -0.023086 0.023455 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.48061e-06 ( -2.98422e-07 3.00323e-07 ) ergs/cm2
Band function
Time interval is from -38.000 sec. to 133.296 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.961378 ( 1.21732 1.21732 )
beta : -1.69441 ( 1.68878 0.156751 )
Epeak [keV] : 38.5334 ( -38.5028 -38.5028 )
Norm@50keV : 7.15334E-03 ( -0.0071564 359881 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.98 using 59 PHA bins.
# Reduced chi-squared = 1.145 for 55 degrees of freedom
# Null hypothesis probability = 2.148908e-01
Photon flux (15-150 keV) in 171.3 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] : 13.5792 ( )
R^2/D10^2 : 4.33522E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 115.92 using 59 PHA bins.
# Reduced chi-squared = 2.0337 for 57 degrees of freedom
# Null hypothesis probability = 6.657327e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.900e-07 4.651e-08
25- 50 1.046e-06 1.084e-07
50-150 1.249e-06 2.197e-07
15-150 2.585e-06 2.501e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 162.403 (-55.0367 -161.404)
Norm : 1.16612 (-0.0996662 0.132478)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.21 using 59 PHA bins.
# Reduced chi-squared = 1.144 for 57 degrees of freedom
# Null hypothesis probability = 2.127690e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.093e-07 6.552e-08
25- 50 9.547e-07 2.043e-07
50-150 1.945e-06 9.196e-07
15-150 3.409e-06 1.075e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.72446 (-1.40235 1.58091)
R1^2/D10^2 : 0.406238 (-0.211821 0.563554)
kT2 [keV] : 28.2226 (-6.54944 13.4287)
R2^2/D10^2 : 2.51560E-03 (-0.00179618 0.00403668)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.02 using 59 PHA bins.
# Reduced chi-squared = 1.164 for 55 degrees of freedom
# Null hypothesis probability = 1.894130e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.397e-07 1.415e-07
25- 50 9.472e-07 2.201e-07
50-150 2.012e-06 9.365e-07
15-150 3.499e-06 1.101e-06
Peak spectrum fit
Power-law model
Time interval is from 8.704 sec. to 9.704 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61587 ( -0.417824 0.432474 )
Norm@50keV : 1.03006E-02 ( -0.00263978 0.00260633 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.58 using 59 PHA bins.
# Reduced chi-squared = 1.010 for 57 degrees of freedom
# Null hypothesis probability = 4.536137e-01
Photon flux (15-150 keV) in 1 sec: 1.33027 ( -0.341342 0.343336 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.61519e-08 ( -2.56462e-08 2.59923e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.704 sec. to 9.704 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.997673 ( -2.2229 1.28462 )
Epeak [keV] : 82.7792 ( -72.656 -82.7792 )
Norm@50keV : 2.10044E-02 ( -0.01312 0.218166 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.17 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 56 degrees of freedom
# Null hypothesis probability = 4.315087e-01
Photon flux (15-150 keV) in 1 sec: 1.30014 ( -0.352408 0.35242 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.33308e-08 ( -2.67301e-08 2.71142e-08 ) ergs/cm2
Band function
Time interval is from 8.704 sec. to 9.704 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97015 ( -4.97015 -4.97015 )
beta : -1.70065 ( -0.678295 0.456638 )
Epeak [keV] : 23.8606 ( -23.8606 25.5223 )
Norm@50keV : 1545.49 ( -380.233 9.89595e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.12 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 55 degrees of freedom
# Null hypothesis probability = 3.962284e-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] : 15.3268 (-4.06984 5.3193)
R^2/D10^2 : 0.139888 (-0.0924714 0.279273)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.36 using 59 PHA bins.
# Reduced chi-squared = 1.059 for 57 degrees of freedom
# Null hypothesis probability = 3.555186e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.854e-09 4.030e-09
25- 50 2.777e-08 1.365e-08
50-150 4.482e-08 2.433e-08
15-150 7.945e-08 3.447e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 166.786 (-101.192 -166.751)
Norm : 5.49263 (-1.41711 2.00101)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.24 using 59 PHA bins.
# Reduced chi-squared = 1.004 for 57 degrees of freedom
# Null hypothesis probability = 4.662177e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.397e-08 8.050e-09
25- 50 2.627e-08 1.499e-08
50-150 5.409e-08 3.253e-08
15-150 9.433e-08 5.655e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.49644 (-3.47385 8.62283)
R1^2/D10^2 : 3.13624 (-2.97609 10.0085)
kT2 [keV] : 20.7543 (-6.97876 -20.7596)
R2^2/D10^2 : 3.91691E-02 (-0.0387326 0.152022)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.76 using 59 PHA bins.
# Reduced chi-squared = 1.032 for 55 degrees of freedom
# Null hypothesis probability = 4.093668e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.418e-08 7.950e-09
25- 50 2.534e-08 1.319e-08
50-150 5.299e-08 3.452e-08
15-150 9.250e-08 4.734e-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: 1.65679 ( -0.145531 0.147798 )
Norm@50keV : 3.16390E-03 ( -0.000260653 0.000258806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.29 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 57 degrees of freedom
# Null hypothesis probability = 4.276472e-01
Photon flux (15-150 keV) in 105.3 sec: 0.414058 ( -0.0341159 0.0342417 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.09642e-06 ( -2.69155e-07 2.70799e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65942 ( -0.200874 0.145708 )
Epeak [keV] : 9999.36 ( -9999.99 -10000 )
Norm@50keV : 3.16411E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.30 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 56 degrees of freedom
# Null hypothesis probability = 3.909077e-01
Photon flux (15-150 keV) in 105.3 sec: 0.414137 ( -0.035831 0.033954 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.09329e-06 ( -2.68599e-07 2.7119e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.26935 ( 1.28753 6.26833 )
beta : -1.66822 ( 1.66706 0.155749 )
Epeak [keV] : 49.9041 ( -50.8843 -50.8843 )
Norm@50keV : 6.01407E-03 ( -0.00295912 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.29 using 59 PHA bins.
# Reduced chi-squared = 1.060 for 55 degrees of freedom
# Null hypothesis probability = 3.553378e-01
Photon flux (15-150 keV) in 105.3 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) = 9.31e-07
S(50-100 keV) = 1.17e-06
T90 vs. Hardness ratio plot
T90 = 153.115999937057 sec.
Hardness ratio (energy fluence ratio) = 1.25671
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.40788
Count Ratio (50-100 keV) / (15-25 keV) = 1.00512
Mask shadow pattern
IMX = -1.149816202800094E+00, IMY = 1.847357461875183E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
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:
-239.376000 -38.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6197 22.0097 0.9 54.8 -155.5 7.8492 12.6 0.8 Crab
217.1377 53.4216 3.3 40.7 39.3 1.4157 3.5 ------ UNKNOWN
173.2606 63.4178 2.6 18.9 62.9 0.8923 4.5 ------ UNKNOWN
117.3881 28.3447 2.7 42.8 165.9 1.5597 4.3 ------ UNKNOWN
68.3340 30.6103 3.7 51.1 -135.8 2.8131 3.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-38.000000 67.324600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5362 21.9693 21.7 54.9 -155.4 -0.2802 -0.5 6.0 Crab
165.3894 39.4300 2.1 36.9 100.4 2.2079 5.4 ------ UNKNOWN
97.8780 24.3487 0.7 49.3 -170.9 4.4937 15.6 ------ UNKNOWN
314.3012 78.5219 2.4 30.7 -29.5 0.7154 4.7 ------ UNKNOWN
80.2211 54.2288 2.3 26.1 -131.2 0.7748 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
131.324590 962.727800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6284 22.0244 0.2 13.3 -99.9 34.5353 62.6 0.7 Crab
139.2826 53.6837 2.6 42.5 32.8 5.3154 4.5 ------ UNKNOWN
111.8183 21.7282 2.8 13.1 96.3 2.2491 4.2 ------ UNKNOWN
105.5595 -13.7429 2.7 38.8 165.5 3.5839 4.3 ------ UNKNOWN
100.4772 -21.1956 2.5 45.6 174.0 5.1608 4.7 ------ UNKNOWN
105.3518 46.0454 2.2 22.5 11.0 2.7179 5.2 ------ UNKNOWN
65.4605 -20.9065 4.7 55.2 -145.0 8.3668 2.5 ------ UNKNOWN
Plot creation:
Sat May 30 22:29:40 EDT 2015