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
56.8516 -44.1537 0.0063 27.5265 170.2953 1.6082352 30.455 TRIG_00663074
Foreground time interval of the image:
-5.616 13.285 (delta_t = 18.901 [sec])
Background time interval of the image:
-239.816 -5.616 (delta_t = 234.200 [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 -5.616 sec. to 91.348 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74263 ( )
Norm@50keV : 2.06080E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 116.50 using 59 PHA bins.
# Reduced chi-squared = 2.0439 for 57 degrees of freedom
# Null hypothesis probability = 5.695364e-06
Photon flux (15-150 keV) in 96.96 sec: 0.277902 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84458e-06 ( 0 0 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.616 sec. to 91.348 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.783934 ( -0.474009 0.424193 )
Epeak [keV] : 57.6338 ( -6.9031 12.582 )
Norm@50keV : 6.78563E-03 ( -0.00274906 0.00540997 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 99.67 using 59 PHA bins.
# Reduced chi-squared = 1.780 for 56 degrees of freedom
# Null hypothesis probability = 2.974129e-04
Photon flux (15-150 keV) in 96.96 sec: 0.265975 ( -0.015412 0.015426 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69322e-06 ( -1.20929e-07 1.23052e-07 ) ergs/cm2
Band function
Time interval is from -5.616 sec. to 91.348 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.186022 ( -0.700855 0.129709 )
beta : -2.27674 ( -0.427547 0.382438 )
Epeak [keV] : 47.0051 ( -17.9541 10.2063 )
Norm@50keV : 1.61904E-02 ( -0.0112785 40.9347 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 95.76 using 59 PHA bins.
# Reduced chi-squared = 1.741 for 55 degrees of freedom
# Null hypothesis probability = 5.499303e-04
Photon flux (15-150 keV) in 96.96 sec: 0.265112 ( 6.73489 -0.015295 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72118e-06 ( -1.7205e-06 -1.15101e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.1120 ( )
R^2/D10^2 : 6.56497E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 143.42 using 59 PHA bins.
# Reduced chi-squared = 2.5162 for 57 degrees of freedom
# Null hypothesis probability = 2.140066e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.977e-07 1.794e-08
25- 50 6.288e-07 4.034e-08
50-150 5.581e-07 7.073e-08
15-150 1.385e-06 8.290e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 111.545 (-21.1294 26.4943)
Norm : 1.19930 (-0.0805786 0.0966723)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 103.43 using 59 PHA bins.
# Reduced chi-squared = 1.8145 for 57 degrees of freedom
# Null hypothesis probability = 1.654742e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.036e-07 2.700e-08
25- 50 5.361e-07 3.243e-08
50-150 9.219e-07 2.683e-07
15-150 1.762e-06 2.938e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.26818 (-1.40369 1.2885)
R1^2/D10^2 : 0.192063 (-0.0660475 0.133741)
kT2 [keV] : 25.8252 (-6.41804 13.5538)
R2^2/D10^2 : 2.40836E-03 (-0.00186486 0.0054596)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 95.84 using 59 PHA bins.
# Reduced chi-squared = 1.742 for 55 degrees of freedom
# Null hypothesis probability = 5.398224e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.622e-07 4.669e-08
25- 50 5.897e-07 8.891e-08
50-150 8.817e-07 3.715e-07
15-150 1.734e-06 4.384e-07
Peak spectrum fit
Power-law model
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09331 ( -0.225996 0.217771 )
Norm@50keV : 8.68010E-03 ( -0.00122353 0.00122105 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.62 using 59 PHA bins.
# Reduced chi-squared = 1.239 for 57 degrees of freedom
# Null hypothesis probability = 1.060677e-01
Photon flux (15-150 keV) in 1 sec: 1.00619 ( -0.145582 0.146106 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.09464e-08 ( -1.34909e-08 1.3587e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.719717 ( -1.78105 1.24454 )
Epeak [keV] : 78.2887 ( -17.062 59.5492 )
Norm@50keV : 6.50874E-02 ( -0.0650858 0.385923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.62 using 59 PHA bins.
# Reduced chi-squared = 1.136 for 56 degrees of freedom
# Null hypothesis probability = 2.259466e-01
Photon flux (15-150 keV) in 1 sec: 0.950258 ( -0.15192 0.151912 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.12235e-08 ( -1.54472e-08 1.56524e-08 ) ergs/cm2
Band function
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -4.53486 -5 )
beta : -1.72922 ( -0.695532 0.396406 )
Epeak [keV] : 44.7985 ( -7.89843 7.76701 )
Norm@50keV : 25.7469 ( -3.46227 52.0493 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.79 using 59 PHA bins.
# Reduced chi-squared = 1.087 for 55 degrees of freedom
# Null hypothesis probability = 3.060019e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.52115e-08 ( -8.52045e-08 -1.4028e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 18.1001 (-2.52801 3.18708)
R^2/D10^2 : 6.99109E-02 (-0.0295853 0.046457)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.58 using 59 PHA bins.
# Reduced chi-squared = 1.133 for 57 degrees of freedom
# Null hypothesis probability = 2.288120e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.578e-09 1.333e-09
25- 50 2.126e-08 4.940e-09
50-150 5.062e-08 1.213e-08
15-150 7.646e-08 1.435e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-36.4248 -200)
Norm : 4.18570 (-0.604848 0.604848)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.92 using 59 PHA bins.
# Reduced chi-squared = 1.402 for 57 degrees of freedom
# Null hypothesis probability = 2.425918e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.042e-08 5.930e-09
25- 50 2.004e-08 1.126e-08
50-150 4.396e-08 2.466e-08
15-150 7.442e-08 4.179e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 14.9049 (-4.0722 3.91433)
R1^2/D10^2 : 0.114245 (-0.108364 0.112557)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 9.76662E-05 (-7.64984e-05 0.00107373)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.58 using 59 PHA bins.
#Fit statistic : Chi-Squared = 60.41 using 59 PHA bins.
# Reduced chi-squared = 1.101 for 55 degrees of freedom
# Reduced chi-squared = 1.098 for 55 degrees of freedom
# Null hypothesis probability = 2.815241e-01
# Null hypothesis probability = 2.868836e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.502e-09 2.996e-09
25- 50 2.206e-08 1.117e-08
50-150 5.818e-08 2.983e-08
15-150 8.575e-08 4.786e-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: 1.31229 ( -0.0824815 0.0819869 )
Norm@50keV : 5.62043E-03 ( -0.000285147 0.000285129 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 103.69 using 59 PHA bins.
# Reduced chi-squared = 1.8192 for 57 degrees of freedom
# Null hypothesis probability = 1.551382e-04
Photon flux (15-150 keV) in 18.9 sec: 0.672073 ( -0.0352936 0.0353377 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04661e-06 ( -5.75101e-08 5.76673e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.199222 ( -0.441107 0.398971 )
Epeak [keV] : 82.8003 ( -10.759 19.1161 )
Norm@50keV : 1.99568E-02 ( -0.00714572 0.012613 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.11 using 59 PHA bins.
# Reduced chi-squared = 1.377 for 56 degrees of freedom
# Null hypothesis probability = 3.220831e-02
Photon flux (15-150 keV) in 18.9 sec: 0.645590 ( -0.036496 0.036519 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.74255e-07 ( -6.35021e-08 6.36798e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.967955 ( -0.868232 -0.979334 )
beta : -1.82497 ( -0.289206 0.250537 )
Epeak [keV] : 54.8376 ( -13.8809 14.5237 )
Norm@50keV : 0.102314 ( -0.108656 26.7354 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.58 using 59 PHA bins.
# Reduced chi-squared = 1.265 for 55 degrees of freedom
# Null hypothesis probability = 8.914070e-02
Photon flux (15-150 keV) in 18.9 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.91751e-07 ( -9.91619e-07 -6.0979e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.08e-07
S(50-100 keV) = 6.07e-07
T90 vs. Hardness ratio plot
T90 = 76.0439999103546 sec.
Hardness ratio (energy fluence ratio) = 1.19488
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.401
Count Ratio (50-100 keV) / (15-25 keV) = 0.7779
Mask shadow pattern
IMX = -5.136973580862169E-01, IMY = -8.785136123531888E-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:
-239.816000 -5.616000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
30.7592 -31.6759 2.9 17.6 109.8 0.7322 4.0 ------ UNKNOWN
106.3034 -85.5078 2.8 44.0 -116.6 3.0941 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.616000 13.284600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
56.8517 -44.1537 0.4 27.5 170.3 1.6084 30.5 ------ UNKNOWN
91.9862 -37.1389 2.6 54.3 178.9 0.7881 4.5 ------ UNKNOWN
5.4470 -70.1548 2.5 24.8 -100.4 0.2618 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.684600 962.214000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
92.1933 -6.1458 2.3 49.0 151.4 10.1927 5.0 ------ UNKNOWN
353.6210 -22.2527 3.2 55.7 13.0 10.1550 3.6 ------ UNKNOWN
102.3802 -37.6938 2.5 34.6 -163.0 2.4961 4.7 ------ UNKNOWN
11.0013 -64.8241 3.7 32.5 -43.7 1.9277 3.2 ------ UNKNOWN
99.7979 -59.5076 2.6 29.9 -122.2 3.1420 4.5 ------ UNKNOWN
128.5358 -27.2997 5.4 58.7 -159.2 9.7624 2.1 ------ UNKNOWN
131.9043 -53.4216 2.5 48.0 -129.2 11.0298 4.7 ------ UNKNOWN
Plot creation:
Sun Dec 13 19:52:35 EST 2015