Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
78.1685 -7.0385 0.0071 23.7670 -92.9450 1.9697471 27.059 TRIG_00672236
Foreground time interval of the image:
-1.492 13.557 (delta_t = 15.049 [sec])
Background time interval of the image:
-239.744 -1.492 (delta_t = 238.252 [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 -1.492 sec. to 773.032 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21193 ( -0.0455391 0.0453108 )
Norm@50keV : 2.56990E-03 ( -6.08443e-05 6.07313e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.43 using 59 PHA bins.
# Reduced chi-squared = 0.9549 for 57 degrees of freedom
# Null hypothesis probability = 5.721771e-01
Photon flux (15-150 keV) in 774.5 sec: 0.302172 ( -0.007807 0.00784 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.0128e-05 ( -4.89376e-07 4.90216e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.492 sec. to 773.032 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20944 ( -0.0478891 0.0437552 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.58082E-03 ( -6.05887e-05 0.000235772 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.54 using 59 PHA bins.
# Reduced chi-squared = 0.9739 for 56 degrees of freedom
# Null hypothesis probability = 5.302476e-01
Photon flux (15-150 keV) in 774.5 sec: 0.304470 ( -0.010203 0.005433 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02279e-05 ( -5.95164e-07 3.8366e-07 ) ergs/cm2
Band function
Time interval is from -1.492 sec. to 773.032 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.830461 ( 0.828501 0.828501 )
beta : -1.22099 ( -0.0608081 0.0523666 )
Epeak [keV] : 91.9356 ( -93.8195 477.325 )
Norm@50keV : 4.61092E-03 ( -0.00205535 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.18 using 59 PHA bins.
# Reduced chi-squared = 0.9850 for 55 degrees of freedom
# Null hypothesis probability = 5.061111e-01
Photon flux (15-150 keV) in 774.5 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] : 20.8103 ( )
R^2/D10^2 : 1.17055E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 450.55 using 59 PHA bins.
# Reduced chi-squared = 7.9044 for 57 degrees of freedom
# Null hypothesis probability = 1.450392e-62
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.446e-07 3.671e-08
25- 50 3.806e-06 1.375e-07
50-150 1.227e-05 4.453e-07
15-150 1.682e-05 4.724e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 1.29809 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 250.77 using 59 PHA bins.
# Reduced chi-squared = 4.3996 for 57 degrees of freedom
# Null hypothesis probability = 3.932136e-26
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.503e-06 6.428e-08
25- 50 4.816e-06 1.301e-07
50-150 1.056e-05 2.749e-07
15-150 1.788e-05 4.492e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.73220 (-0.761006 0.818203)
R1^2/D10^2 : 0.132098 (-0.0324009 0.0457515)
kT2 [keV] : 38.8012 (-4.10307 5.69717)
R2^2/D10^2 : 1.36929E-03 (-0.000452879 0.000565701)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 55 degrees of freedom
# Null hypothesis probability = 3.905106e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.705e-06 1.382e-07
25- 50 4.450e-06 2.064e-07
50-150 1.415e-05 1.084e-06
15-150 2.030e-05 1.204e-06
Peak spectrum fit
Power-law model
Time interval is from 15.972 sec. to 16.972 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06950 ( -0.0977638 0.0972536 )
Norm@50keV : 5.48944E-02 ( -0.00297656 0.00297655 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7477 for 57 degrees of freedom
# Null hypothesis probability = 9.217109e-01
Photon flux (15-150 keV) in 1 sec: 0.299354 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.79709e-07 ( -3.63211e-08 3.6517e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 15.972 sec. to 16.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06432 ( -0.328591 0.235603 )
Epeak [keV] : 9998.11 ( -9998.02 -9998.02 )
Norm@50keV : 5.52024E-02 ( -0.00299326 0.0274489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.61 using 59 PHA bins.
# Reduced chi-squared = 0.7609 for 56 degrees of freedom
# Null hypothesis probability = 9.063104e-01
Photon flux (15-150 keV) in 1 sec: 6.34267 ( -0.35024 0.36289 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.78709e-07 ( -3.99928e-08 3.84968e-08 ) ergs/cm2
Band function
Time interval is from 15.972 sec. to 16.972 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.691968 ( 0.693804 5.33143 )
beta : -1.11924 ( 1.11771 0.135895 )
Epeak [keV] : 132.357 ( -128.492 471.72 )
Norm@50keV : 9.13013E-02 ( -0.042418 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.11 using 59 PHA bins.
# Reduced chi-squared = 0.7657 for 55 degrees of freedom
# Null hypothesis probability = 8.989704e-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] : 20.0184 ( )
R^2/D10^2 : 0.296412 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 117.15 using 59 PHA bins.
# Reduced chi-squared = 2.0552 for 57 degrees of freedom
# Null hypothesis probability = 4.781402e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.289e-08 2.475e-09
25- 50 1.141e-07 9.100e-09
50-150 3.390e-07 3.550e-08
15-150 4.760e-07 3.505e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-8.26833 -200)
Norm : 25.3525 (-1.42475 1.42475)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 106.17 using 59 PHA bins.
# Reduced chi-squared = 1.8626 for 57 degrees of freedom
# Null hypothesis probability = 8.421574e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.313e-08 3.935e-09
25- 50 1.214e-07 7.900e-09
50-150 2.663e-07 6.260e-08
15-150 4.509e-07 7.000e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.09235 (-1.609 1.78926)
R1^2/D10^2 : 2.28302 (-0.913416 1.80804)
kT2 [keV] : 41.4070 (-8.85042 18.8183)
R2^2/D10^2 : 2.66154E-02 (-0.0167622 0.0284419)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.06 using 59 PHA bins.
# Reduced chi-squared = 0.7465 for 55 degrees of freedom
# Null hypothesis probability = 9.187331e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.268e-08 9.055e-09
25- 50 1.193e-07 2.071e-08
50-150 4.257e-07 1.615e-07
15-150 5.878e-07 1.717e-07
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: 1.12595 ( -0.111187 0.109662 )
Norm@50keV : 8.36598E-03 ( -0.000494432 0.000493458 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.99 using 59 PHA bins.
# Reduced chi-squared = 1.158 for 57 degrees of freedom
# Null hypothesis probability = 1.941390e-01
Photon flux (15-150 keV) in 15.05 sec: 0.972983 ( -0.0598504 0.0600906 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30571e-06 ( -8.39188e-08 8.42096e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12618 ( -0.116748 0.105847 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 8.41183E-03 ( -0.000492448 0.00203531 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.04 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 56 degrees of freedom
# Null hypothesis probability = 1.686656e-01
Photon flux (15-150 keV) in 15.05 sec: 0.972884 ( -0.05948 0.059736 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30241e-06 ( -8.04663e-08 8.89229e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.909217 ( 0.909217 0.909217 )
beta : -1.12596 ( 1.12596 0.111198 )
Epeak [keV] : 50.5940 ( -50.594 -50.594 )
Norm@50keV : 1.47110E-02 ( -0.00675498 361048 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.99 using 59 PHA bins.
# Reduced chi-squared = 1.200 for 55 degrees of freedom
# Null hypothesis probability = 1.474399e-01
Photon flux (15-150 keV) in 15.05 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) = 4.26e-06
S(50-100 keV) = 7.35e-06
T90 vs. Hardness ratio plot
T90 = 327.751999974251 sec.
Hardness ratio (energy fluence ratio) = 1.72535
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.54677
Count Ratio (50-100 keV) / (15-25 keV) = 1.38191
Mask shadow pattern
IMX = -2.262474928634723E-02, IMY = 4.397838829652273E-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:
-239.744000 -1.492000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6333 22.0204 0.3 21.5 -10.0 10.2836 40.6 0.4 Crab
137.7041 -12.9898 2.9 43.5 145.4 2.8604 4.0 ------ UNKNOWN
119.3974 -12.5314 3.2 28.0 160.7 1.0571 3.6 ------ UNKNOWN
66.8802 -6.3287 2.4 33.5 -81.2 2.1750 4.8 ------ UNKNOWN
54.3359 5.2262 3.1 43.6 -59.0 4.0934 3.7 ------ UNKNOWN
46.2003 17.8106 3.7 52.1 -42.4 4.4166 3.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.492000 13.556590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4390 22.0740 6.8 21.6 -10.3 -0.0953 -1.7 11.4 Crab
134.7125 20.4425 2.8 38.3 93.6 0.8650 4.0 ------ UNKNOWN
120.6399 25.5193 1.9 29.1 74.6 0.5340 6.1 ------ UNKNOWN
112.3852 5.2936 2.1 14.1 121.0 0.3093 5.5 ------ UNKNOWN
62.4669 40.0264 2.1 46.9 -8.2 0.5231 5.4 ------ UNKNOWN
59.5657 29.1803 2.8 43.3 -23.1 0.3628 4.1 ------ UNKNOWN
78.1686 -7.0385 0.4 23.8 -92.9 1.9695 27.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
58.956600 596.256590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6467 22.0133 0.4 29.5 35.5 21.7736 31.7 0.8 Crab
117.5304 -21.1441 2.0 40.5 139.7 8.0959 5.7 ------ UNKNOWN
115.6033 -53.2756 3.3 55.3 179.0 10.1326 3.4 ------ UNKNOWN
78.1886 -7.0450 0.6 0.0 -65.9 10.1667 19.1 ------ UNKNOWN
29.7844 13.0531 3.7 52.1 -42.2 11.5276 3.1 ------ UNKNOWN
Plot creation:
Fri Mar 18 11:44:21 EDT 2016