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
41.1945 -43.4611 0.0218 21.7582 -24.8531 0.1334408 8.815 TRIG_00666378
Foreground time interval of the image:
-0.220 1.316 (delta_t = 1.536 [sec])
Background time interval of the image:
-239.048 -0.220 (delta_t = 238.828 [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 1.408000
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 1.408000
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 1.408000
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 -0.220 sec. to 1.316 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60453 ( -0.307598 0.32219 )
Norm@50keV : 5.58738E-03 ( -0.00109827 0.00106645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.79 using 59 PHA bins.
# Reduced chi-squared = 0.8911 for 57 degrees of freedom
# Null hypothesis probability = 7.057520e-01
Photon flux (15-150 keV) in 1.536 sec: 0.719039 ( -0.124216 0.124243 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.0229e-08 ( -1.67498e-08 1.72636e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.220 sec. to 1.316 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39185 ( -1.2494 0.526329 )
Epeak [keV] : 132.033 ( -131.538 -131.538 )
Norm@50keV : 7.28951E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.67 using 59 PHA bins.
# Reduced chi-squared = 0.9048 for 56 degrees of freedom
# Null hypothesis probability = 6.761575e-01
Photon flux (15-150 keV) in 1.536 sec: 0.713103 ( -0.127478 0.127289 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.85346e-08 ( -1.84199e-08 1.85033e-08 ) ergs/cm2
Band function
Time interval is from -0.220 sec. to 1.316 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97525 ( -4.97525 -4.97525 )
beta : -1.71403 ( -0.421324 0.34825 )
Epeak [keV] : 22.6887 ( -22.6887 6.01589 )
Norm@50keV : 1181.72 ( -202.351 3.88408e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.45 using 59 PHA bins.
# Reduced chi-squared = 0.8990 for 55 degrees of freedom
# Null hypothesis probability = 6.858864e-01
Photon flux (15-150 keV) in 1.536 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] : 13.6559 (-3.18865 3.98339)
R^2/D10^2 : 0.110210 (-0.0645486 0.170329)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.71 using 59 PHA bins.
# Reduced chi-squared = 1.065 for 57 degrees of freedom
# Null hypothesis probability = 3.436943e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.682e-09 2.152e-09
25- 50 2.424e-08 8.587e-09
50-150 2.937e-08 1.226e-08
15-150 6.029e-08 1.617e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.047 (-90.1436 -165.1)
Norm : 2.93010 (-0.529649 0.678124)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.72 using 59 PHA bins.
# Reduced chi-squared = 0.8898 for 57 degrees of freedom
# Null hypothesis probability = 7.082983e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.144e-08 6.361e-09
25- 50 2.153e-08 1.205e-08
50-150 4.446e-08 2.584e-08
15-150 7.743e-08 4.362e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.01450 (-1.62767 3.02959)
R1^2/D10^2 : 2.77752 (-2.15324 12.0842)
kT2 [keV] : 21.8802 (-6.15167 13.4811)
R2^2/D10^2 : 1.75832E-02 (-0.0140278 0.040256)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.68 using 59 PHA bins.
# Reduced chi-squared = 0.8852 for 55 degrees of freedom
# Null hypothesis probability = 7.131446e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.290e-08 7.410e-09
25- 50 1.955e-08 1.025e-08
50-150 4.550e-08 2.721e-08
15-150 7.795e-08 4.065e-08
Peak spectrum fit
Power-law model
Time interval is from 0.112 sec. to 1.112 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81695 ( -0.425919 0.470491 )
Norm@50keV : 5.22253E-03 ( -0.00150886 0.00140391 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.12 using 59 PHA bins.
# Reduced chi-squared = 0.8968 for 57 degrees of freedom
# Null hypothesis probability = 6.943532e-01
Photon flux (15-150 keV) in 1 sec: 0.724476 ( -0.154914 0.154917 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.80607e-08 ( -1.32847e-08 1.40233e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.112 sec. to 1.112 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83285 ( )
Epeak [keV] : 9999.36 ( )
Norm@50keV : 5.18956E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.12 using 59 PHA bins.
# Reduced chi-squared = 0.9129 for 56 degrees of freedom
# Null hypothesis probability = 6.596634e-01
Photon flux (15-150 keV) in 1 sec: 0.551793 ( -0.222474 0.309474 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.24033e-08 ( -1.63298e-08 1.24812e-08 ) ergs/cm2
Band function
Time interval is from 0.112 sec. to 1.112 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98345 ( -4.98345 -4.98345 )
beta : -1.92710 ( -0.661996 0.479531 )
Epeak [keV] : 20.5337 ( -20.5337 64.1848 )
Norm@50keV : 2612.11 ( -555.116 6.83051e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.41 using 59 PHA bins.
# Reduced chi-squared = 0.9166 for 55 degrees of freedom
# Null hypothesis probability = 6.503210e-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] : 8.00442 (-2.6073 6.01888)
R^2/D10^2 : 0.729591 (-0.613553 2.71276)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.50 using 59 PHA bins.
# Reduced chi-squared = 1.096 for 57 degrees of freedom
# Null hypothesis probability = 2.873314e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.457e-09 4.522e-09
25- 50 1.482e-08 7.085e-09
50-150 3.897e-09 2.516e-09
15-150 2.717e-08 1.513e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.7535 (-58.1859 -99.9563)
Norm : 3.17132 (-0.845525 1.38316)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.57 using 59 PHA bins.
# Reduced chi-squared = 0.9223 for 57 degrees of freedom
# Null hypothesis probability = 6.416686e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.289e-09 3.551e-09
25- 50 1.433e-08 6.514e-09
50-150 2.318e-08 1.707e-08
15-150 4.580e-08 2.332e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.94041 (-1.42114 2.0806)
R1^2/D10^2 : 4.18376 (-3.18345 13.1726)
kT2 [keV] : 30.6106 (-13.6103 131.024)
R2^2/D10^2 : 5.36812E-03 (-0.0050207 0.0306771)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.37 using 59 PHA bins.
# Reduced chi-squared = 0.8795 for 55 degrees of freedom
# Null hypothesis probability = 7.240943e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.047e-08 5.910e-09
25- 50 1.098e-08 5.820e-09
50-150 3.197e-08 2.082e-08
15-150 5.342e-08 2.845e-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: 1.60453 ( -0.307598 0.32219 )
Norm@50keV : 5.58738E-03 ( -0.00109827 0.00106645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.79 using 59 PHA bins.
# Reduced chi-squared = 0.8911 for 57 degrees of freedom
# Null hypothesis probability = 7.057520e-01
Photon flux (15-150 keV) in 1.536 sec: 0.719015 ( -0.124211 0.124238 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.02181e-08 ( -1.67402e-08 1.72737e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39048 ( -1.24948 0.526282 )
Epeak [keV] : 131.537 ( -131.533 -131.533 )
Norm@50keV : 7.30179E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.67 using 59 PHA bins.
# Reduced chi-squared = 0.9048 for 56 degrees of freedom
# Null hypothesis probability = 6.761575e-01
Photon flux (15-150 keV) in 1.536 sec: 0.713000 ( -0.127448 0.127242 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.85638e-08 ( -1.83933e-08 1.85196e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97525 ( -4.97525 -4.97525 )
beta : -1.71403 ( -0.421324 0.34825 )
Epeak [keV] : 22.6887 ( -22.6887 6.01589 )
Norm@50keV : 1181.72 ( -202.351 3.88408e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.45 using 59 PHA bins.
# Reduced chi-squared = 0.8990 for 55 degrees of freedom
# Null hypothesis probability = 6.858864e-01
Photon flux (15-150 keV) in 1.536 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) = 2.09e-08
S(50-100 keV) = 2.73e-08
T90 vs. Hardness ratio plot
T90 = 1.43599992990494 sec.
Hardness ratio (energy fluence ratio) = 1.30622
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.905422
Count Ratio (50-100 keV) / (15-25 keV) = 0.926746
Mask shadow pattern
IMX = 3.621614184850643E-01, IMY = 1.677496858247010E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000
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:
-239.048000 -0.220000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6095 -40.6382 3.2 47.5 -169.1 1.6469 3.6 6.2 Vela X-1
68.9732 -2.5480 2.1 39.3 76.5 4.9731 5.5 ------ UNKNOWN
103.6878 -32.2672 3.0 27.7 160.0 1.0199 3.8 ------ UNKNOWN
136.1720 -27.7063 3.2 54.2 176.5 2.9230 3.6 ------ UNKNOWN
2.8813 -28.8823 3.2 55.5 -20.4 2.8722 3.7 ------ UNKNOWN
356.5996 -48.2141 4.8 50.8 -44.7 3.4605 2.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.220000 1.316000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4479 -40.7403 21.6 47.4 -169.0 -0.0167 -0.5 11.7 Vela X-1
105.7352 -23.0831 2.6 34.5 147.6 0.1037 4.4 ------ UNKNOWN
41.1945 -43.4611 1.3 21.8 -24.9 0.1335 8.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
388.252600 963.043200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6277 22.0154 0.2 11.5 53.1 23.9116 51.8 0.3 Crab
102.6101 55.1267 2.7 29.0 173.3 2.2446 4.3 ------ UNKNOWN
96.2805 29.3254 3.1 2.8 -175.7 1.6587 3.7 ------ UNKNOWN
130.4894 66.2763 2.8 45.2 -176.4 3.4546 4.2 ------ UNKNOWN
95.9044 -26.3049 3.1 53.0 -16.3 4.7511 3.7 ------ UNKNOWN
116.9470 20.9473 3.4 20.7 -94.1 1.7670 3.4 ------ UNKNOWN
96.7245 -32.9141 3.0 59.6 -17.0 11.3294 3.9 ------ UNKNOWN
158.5695 44.1392 3.0 53.1 -142.2 12.8093 3.9 ------ UNKNOWN
118.5550 -18.7702 3.5 50.8 -44.5 9.1636 3.3 ------ UNKNOWN
141.8523 22.0630 3.2 42.5 -109.8 8.6472 3.6 ------ UNKNOWN
Plot creation:
Fri Mar 18 13:49:48 EDT 2016