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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
99.4212 5.7527 0.0126 17.2182 -141.8376 1.1024749 15.294 TRIG_00680017
Foreground time interval of the image:
-20.884 19.100 (delta_t = 39.984 [sec])
Background time interval of the image:
-239.232 -20.884 (delta_t = 218.348 [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 8.192000
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 8.192000
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 8.192000
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 -20.884 sec. to 19.100 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88831 ( -0.186858 0.196075 )
Norm@50keV : 1.46141E-03 ( -0.000190173 0.000186354 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.84 using 59 PHA bins.
# Reduced chi-squared = 0.9269 for 57 degrees of freedom
# Null hypothesis probability = 6.319662e-01
Photon flux (15-150 keV) in 39.98 sec: 0.208707 ( -0.021286 0.021287 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37207e-07 ( -6.80128e-08 6.97983e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -20.884 sec. to 19.100 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14517 ( -0.982405 0.772679 )
Epeak [keV] : 46.7941 ( -13.5 -46.7941 )
Norm@50keV : 3.99099E-03 ( -0.00255057 0.0113853 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.16 using 59 PHA bins.
# Reduced chi-squared = 0.8957 for 56 degrees of freedom
# Null hypothesis probability = 6.944532e-01
Photon flux (15-150 keV) in 39.98 sec: 0.202712 ( -0.022049 0.022111 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.91886e-07 ( -7.67092e-08 8.27102e-08 ) ergs/cm2
Band function
Time interval is from -20.884 sec. to 19.100 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.136889 ( -3.60857 -0.673426 )
beta : -2.21139 ( 2.21243 0.385622 )
Epeak [keV] : 33.1303 ( -12.6177 43.9873 )
Norm@50keV : 3.28712E-02 ( -0.0323166 104.091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.66 using 59 PHA bins.
# Reduced chi-squared = 0.9029 for 55 degrees of freedom
# Null hypothesis probability = 6.781675e-01
Photon flux (15-150 keV) in 39.98 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] : 9.91351 (-1.14472 1.32893)
R^2/D10^2 : 0.101605 (-0.0385259 0.0603171)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.95 using 59 PHA bins.
# Reduced chi-squared = 1.122 for 57 degrees of freedom
# Null hypothesis probability = 2.456252e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.106e-08 1.543e-08
25- 50 1.991e-07 2.653e-08
50-150 1.013e-07 2.743e-08
15-150 3.814e-07 4.942e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 75.8587 (-22.301 39.2732)
Norm : 1.00044 (-0.147345 0.181996)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.23 using 59 PHA bins.
# Reduced chi-squared = 0.8813 for 57 degrees of freedom
# Null hypothesis probability = 7.249709e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.034e-07 1.443e-08
25- 50 1.680e-07 1.985e-08
50-150 2.286e-07 9.969e-08
15-150 5.000e-07 9.375e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.47926 (-1.98383 1.88122)
R1^2/D10^2 : 0.355543 (-0.197919 0.833685)
kT2 [keV] : 20.6046 (-6.87118 18.2613)
R2^2/D10^2 : 4.15716E-03 (-0.00373707 0.00794911)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.37 using 59 PHA bins.
# Reduced chi-squared = 0.8977 for 55 degrees of freedom
# Null hypothesis probability = 6.886266e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.013e-07 4.945e-08
25- 50 1.713e-07 7.476e-08
50-150 2.284e-07 1.334e-07
15-150 5.010e-07 2.259e-07
Peak spectrum fit
Power-law model
Time interval is from 1.796 sec. to 2.796 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65862 ( -0.592658 0.628491 )
Norm@50keV : 3.25115E-03 ( -0.00121527 0.00112766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.98 using 59 PHA bins.
# Reduced chi-squared = 0.8592 for 57 degrees of freedom
# Null hypothesis probability = 7.663193e-01
Photon flux (15-150 keV) in 1 sec: 0.425751 ( -0.12955 0.129556 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.02155e-08 ( -1.12751e-08 1.20504e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.796 sec. to 2.796 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.47593 ( -0.607131 0.618761 )
Epeak [keV] : 161.504 ( -9999.35 -9999.36 )
Norm@50keV : 1.20977E-03 ( -0.00121349 0.0343154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.79 using 59 PHA bins.
# Reduced chi-squared = 0.8712 for 56 degrees of freedom
# Null hypothesis probability = 7.419215e-01
Photon flux (15-150 keV) in 1 sec: 0.426517 ( -0.130771 0.128842 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.1746e-08 ( -1.33601e-08 7.09432e-09 ) ergs/cm2
Band function
Time interval is from 1.796 sec. to 2.796 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -1.92442 ( -1.52896 0.742839 )
Epeak [keV] : 24.6252 ( -24.6221 9.45045 )
Norm@50keV : 478.362 ( -143.994 3.77228e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.19 using 59 PHA bins.
# Reduced chi-squared = 0.8761 for 55 degrees of freedom
# Null hypothesis probability = 7.305285e-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] : 8.45748 (-2.72171 5.43483)
R^2/D10^2 : 0.364287 (-0.363133 1.25551)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.96 using 59 PHA bins.
# Reduced chi-squared = 0.9292 for 57 degrees of freedom
# Null hypothesis probability = 6.272133e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.895e-09 2.921e-09
25- 50 9.415e-09 6.130e-09
50-150 2.959e-09 2.437e-09
15-150 1.727e-08 1.087e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 149.995 (-117.315 -154.894)
Norm : 1.73267 (-0.553402 1.09292)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.49 using 59 PHA bins.
# Reduced chi-squared = 0.8683 for 57 degrees of freedom
# Null hypothesis probability = 7.496081e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.306e-09 2.722e-09
25- 50 8.230e-09 4.913e-09
50-150 1.772e-08 1.089e-08
15-150 3.025e-08 1.794e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.53503 (-2.19308 2.89075)
R1^2/D10^2 : 0.848464 (-0.66744 2.88147)
kT2 [keV] : 69.8238 (-69.9683 -69.9684)
R2^2/D10^2 : 4.28923E-04 (-0.000394333 0.00533262)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.14 using 59 PHA bins.
# Reduced chi-squared = 0.8389 for 55 degrees of freedom
# Null hypothesis probability = 7.968972e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.563e-09 3.428e-09
25- 50 7.776e-09 4.560e-09
50-150 2.235e-08 1.321e-08
15-150 3.569e-08 1.916e-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: 1.88831 ( -0.186858 0.196075 )
Norm@50keV : 1.46141E-03 ( -0.000190173 0.000186354 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.84 using 59 PHA bins.
# Reduced chi-squared = 0.9269 for 57 degrees of freedom
# Null hypothesis probability = 6.319662e-01
Photon flux (15-150 keV) in 39.98 sec: 0.208695 ( -0.0212848 0.0212849 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37127e-07 ( -6.7978e-08 6.98067e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14519 ( -0.982409 0.772677 )
Epeak [keV] : 46.7943 ( -13.5001 -46.7941 )
Norm@50keV : 3.99088E-03 ( -0.00255055 0.0113853 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.16 using 59 PHA bins.
# Reduced chi-squared = 0.8957 for 56 degrees of freedom
# Null hypothesis probability = 6.944532e-01
Photon flux (15-150 keV) in 39.98 sec: 0.202675 ( -0.022042 0.022103 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.9201e-07 ( -7.67736e-08 8.27466e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.136846 ( -3.61613 -0.673206 )
beta : -2.21138 ( 2.21243 0.385624 )
Epeak [keV] : 33.1304 ( -12.6178 43.9895 )
Norm@50keV : 3.28690E-02 ( -0.0323166 104.156 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.66 using 59 PHA bins.
# Reduced chi-squared = 0.9029 for 55 degrees of freedom
# Null hypothesis probability = 6.781675e-01
Photon flux (15-150 keV) in 39.98 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) = 1.56e-07
S(50-100 keV) = 1.69e-07
T90 vs. Hardness ratio plot
T90 = 33.4759999513626 sec.
Hardness ratio (energy fluence ratio) = 1.08333
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.14812
Count Ratio (50-100 keV) / (15-25 keV) = 0.567047
Mask shadow pattern
IMX = -2.436630703935760E-01, IMY = 1.914851246551121E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.232000 -20.884000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6377 22.0138 0.4 27.8 -87.5 8.9247 30.4 0.3 Crab
124.6432 -33.4501 2.8 51.7 154.8 4.2085 4.2 ------ UNKNOWN
102.9741 -36.2761 3.3 54.1 177.1 2.6883 3.5 ------ UNKNOWN
143.2494 68.9934 3.0 55.4 0.2 3.0874 3.8 ------ UNKNOWN
100.7812 -29.5439 2.4 48.0 -178.5 2.0560 4.9 ------ UNKNOWN
97.8382 22.3378 2.3 15.0 -79.4 0.9872 4.9 ------ UNKNOWN
71.2333 40.2776 2.1 42.7 -60.8 3.7750 5.5 ------ UNKNOWN
70.3234 12.7402 2.2 41.1 -102.6 4.3506 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-20.884000 19.100000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7262 21.8781 6.7 27.7 -87.8 0.1829 1.7 9.7 Crab
150.7317 33.2709 2.2 37.8 44.6 0.7775 5.2 ------ UNKNOWN
99.4212 5.7527 0.8 17.2 -141.8 1.1027 15.3 ------ UNKNOWN
81.4213 65.8749 2.1 53.1 -28.0 1.3701 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
94.468600 962.827700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6350 22.0253 0.2 22.3 -42.8 35.5011 59.0 0.7 Crab
121.5777 -37.2727 3.0 47.7 154.9 7.1830 3.9 ------ UNKNOWN
112.4243 44.1202 3.4 40.0 13.3 3.1407 3.4 ------ UNKNOWN
108.9840 54.4456 2.5 49.3 6.1 5.6196 4.6 ------ UNKNOWN
101.6289 -48.3707 3.8 54.1 177.0 7.1693 3.1 ------ UNKNOWN
101.6124 -41.5692 3.9 47.3 176.6 3.6030 3.0 ------ UNKNOWN
96.7306 40.6732 3.6 35.0 -4.8 2.4914 3.2 ------ UNKNOWN
64.7433 -12.4020 2.8 39.0 -119.1 5.5745 4.1 ------ UNKNOWN
61.6653 44.7315 3.9 51.0 -35.2 5.9417 3.0 ------ UNKNOWN
Plot creation:
Fri Apr 15 11:54:14 EDT 2016