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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
76.8105 11.3326 0.0130 6.1507 -63.7919 0.7572659 14.809 TRIG_00669319
Foreground time interval of the image:
-1.312 17.648 (delta_t = 18.960 [sec])
Background time interval of the image:
-441.395 -423.506 (delta_t = 17.889 [sec])
-239.496 -1.312 (delta_t = 238.184 [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 -1.312 sec. to 17.648 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75506 ( -0.186115 0.193375 )
Norm@50keV : 2.31946E-03 ( -0.00029207 0.000286854 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.54 using 59 PHA bins.
# Reduced chi-squared = 1.080 for 57 degrees of freedom
# Null hypothesis probability = 3.167058e-01
Photon flux (15-150 keV) in 18.96 sec: 0.314232 ( -0.033755 0.033761 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.0574e-07 ( -5.22981e-08 5.33398e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.312 sec. to 17.648 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01715 ( -0.896727 0.726132 )
Epeak [keV] : 57.9984 ( -14.705 281.262 )
Norm@50keV : 6.03707E-03 ( -0.00362276 0.0133475 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.50 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 56 degrees of freedom
# Null hypothesis probability = 3.837142e-01
Photon flux (15-150 keV) in 18.96 sec: 0.306195 ( -0.034584 0.034612 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.77171e-07 ( -5.70398e-08 5.95943e-08 ) ergs/cm2
Band function
Time interval is from -1.312 sec. to 17.648 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.01704 ( -0.430987 1.0504 )
beta : -10.0000 ( 10 0 )
Epeak [keV] : 57.9866 ( -14.594 276.491 )
Norm@50keV : 6.03740E-03 ( -0.00362364 0.0133503 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.50 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 55 degrees of freedom
# Null hypothesis probability = 3.481590e-01
Photon flux (15-150 keV) in 18.96 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] : 11.2639 (-1.40806 1.65996)
R^2/D10^2 : 9.70009E-02 (-0.0385926 0.0620238)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.27 using 59 PHA bins.
# Reduced chi-squared = 1.285 for 57 degrees of freedom
# Null hypothesis probability = 7.210352e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.897e-08 9.110e-09
25- 50 1.427e-07 1.992e-08
50-150 1.041e-07 3.016e-08
15-150 2.958e-07 4.076e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.9578 (-30.883 71.6686)
Norm : 1.39959 (-0.197717 0.220725)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.84 using 59 PHA bins.
# Reduced chi-squared = 1.032 for 57 degrees of freedom
# Null hypothesis probability = 4.078649e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.936e-08 1.114e-08
25- 50 1.199e-07 1.579e-08
50-150 1.943e-07 8.586e-08
15-150 3.836e-07 1.004e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.49963 (-2.00726 2.16078)
R1^2/D10^2 : 0.475558 (-0.285173 1.20827)
kT2 [keV] : 21.0629 (-6.01444 13.0401)
R2^2/D10^2 : 6.83780E-03 (-0.00573067 0.0115622)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.46 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 55 degrees of freedom
# Null hypothesis probability = 3.841755e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.713e-08 3.630e-08
25- 50 1.224e-07 6.054e-08
50-150 1.932e-07 1.088e-07
15-150 3.827e-07 1.872e-07
Peak spectrum fit
Power-law model
Time interval is from -0.164 sec. to 0.836 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48142 ( -0.252201 0.25787 )
Norm@50keV : 8.23338E-03 ( -0.00133271 0.0013162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.81 using 59 PHA bins.
# Reduced chi-squared = 0.9616 for 57 degrees of freedom
# Null hypothesis probability = 5.576729e-01
Photon flux (15-150 keV) in 1 sec: 1.02282 ( -0.156266 0.15633 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.83592e-08 ( -1.38889e-08 1.41596e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.164 sec. to 0.836 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.723957 ( -1.36073 0.877379 )
Epeak [keV] : 77.8484 ( -25.7313 -77.8485 )
Norm@50keV : 2.11819E-02 ( -0.0211818 0.0962996 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.27 using 59 PHA bins.
# Reduced chi-squared = 0.9513 for 56 degrees of freedom
# Null hypothesis probability = 5.788264e-01
Photon flux (15-150 keV) in 1 sec: 0.998123 ( -0.160412 0.160177 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.29995e-08 ( -1.56367e-08 1.59739e-08 ) ergs/cm2
Band function
Time interval is from -0.164 sec. to 0.836 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.34025 ( -12.6491 -4.34025 )
beta : -1.76458 ( -0.557725 0.348632 )
Epeak [keV] : 30.4045 ( -12.1157 20.6404 )
Norm@50keV : 102.515 ( -102.511 38.597 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.81 using 59 PHA bins.
# Reduced chi-squared = 0.9420 for 55 degrees of freedom
# Null hypothesis probability = 5.972307e-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] : 13.2563 (-2.29406 2.92945)
R^2/D10^2 : 0.184051 (-0.0930297 0.1758)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.37 using 59 PHA bins.
# Reduced chi-squared = 1.042 for 57 degrees of freedom
# Null hypothesis probability = 3.893823e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.856e-09 2.078e-09
25- 50 2.411e-08 5.910e-09
50-150 2.709e-08 1.008e-08
15-150 5.806e-08 1.460e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.344 (-96.5965 -199.356)
Norm : 4.20343 (-0.637072 0.63746)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.95 using 59 PHA bins.
# Reduced chi-squared = 0.9464 for 57 degrees of freedom
# Null hypothesis probability = 5.903953e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.047e-08 5.950e-09
25- 50 2.014e-08 1.153e-08
50-150 4.416e-08 2.491e-08
15-150 7.476e-08 4.234e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.67864 (-3.29054 3.57961)
R1^2/D10^2 : 0.579429 (-0.365195 1.69313)
kT2 [keV] : 31.1909 (-14.2741 -31.1909)
R2^2/D10^2 : 6.11602E-03 (-0.0057598 0.0564293)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.84 using 59 PHA bins.
# Reduced chi-squared = 0.9425 for 55 degrees of freedom
# Null hypothesis probability = 5.962483e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.237e-09 5.350e-09
25- 50 2.240e-08 1.279e-08
50-150 4.419e-08 2.557e-08
15-150 7.583e-08 3.850e-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: 1.75506 ( -0.186115 0.193375 )
Norm@50keV : 2.31946E-03 ( -0.00029207 0.000286854 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.54 using 59 PHA bins.
# Reduced chi-squared = 1.080 for 57 degrees of freedom
# Null hypothesis probability = 3.167058e-01
Photon flux (15-150 keV) in 18.96 sec: 0.314217 ( -0.0337533 0.0337582 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.0568e-07 ( -5.2274e-08 5.33508e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01715 ( -0.896727 0.726132 )
Epeak [keV] : 57.9984 ( -14.705 281.262 )
Norm@50keV : 6.03707E-03 ( -0.00362276 0.0133475 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.50 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 56 degrees of freedom
# Null hypothesis probability = 3.837142e-01
Photon flux (15-150 keV) in 18.96 sec: 0.306149 ( -0.034575 0.0346 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.77283e-07 ( -5.70563e-08 5.96576e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.01704 ( -0.430987 1.0504 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 57.9866 ( -14.594 276.491 )
Norm@50keV : 6.03740E-03 ( -0.00362364 0.0133503 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.50 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 55 degrees of freedom
# Null hypothesis probability = 3.481590e-01
Photon flux (15-150 keV) in 18.96 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) = 1.12e-07
S(50-100 keV) = 1.33e-07
T90 vs. Hardness ratio plot
T90 = 16.5639999508858 sec.
Hardness ratio (energy fluence ratio) = 1.1875
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.23819
Count Ratio (50-100 keV) / (15-25 keV) = 0.679424
Mask shadow pattern
IMX = 4.759261233783420E-02, IMY = 9.668638485343777E-02
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:
-441.395410 -423.506000
-239.496000 -1.312000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6310 22.0164 0.3 8.5 52.5 10.9065 44.5 0.2 Crab
125.6737 -1.7056 2.4 45.3 152.9 3.4296 4.9 ------ UNKNOWN
24.6960 42.3113 2.7 57.4 -1.5 6.2363 4.4 ------ UNKNOWN
84.6440 -33.5671 3.1 47.1 -135.6 2.8443 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.312000 17.648000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6400 22.0172 605.0 8.5 52.5 0.0010 0.0 0.4 Crab
76.8105 11.3326 0.8 6.2 -63.8 0.7573 14.8 ------ UNKNOWN
108.5411 -38.2945 2.5 57.2 -157.4 1.1765 4.5 ------ UNKNOWN
39.7305 7.5833 2.2 42.6 -46.9 0.5913 5.2 ------ UNKNOWN
45.0414 -1.9440 2.3 40.4 -63.1 0.6504 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
60.804600 840.264000
840.504000 962.598600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6364 22.0159 0.2 12.5 57.7 38.8349 60.3 0.2 Crab
113.2743 13.1835 3.3 35.7 110.2 5.4131 3.5 ------ UNKNOWN
98.5182 -39.2773 2.9 54.5 -173.5 10.3499 3.9 ------ UNKNOWN
29.4864 50.7475 3.9 55.0 -7.5 6.1475 3.0 ------ UNKNOWN
84.7337 -39.2377 3.4 51.1 -160.8 6.3081 3.4 ------ UNKNOWN
65.5559 -40.7484 3.5 53.1 -142.3 15.9527 3.3 ------ UNKNOWN
Plot creation:
Fri Mar 18 11:57:38 EDT 2016