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
147.4259 70.5081 0.0030 1.5516 118.8398 4.7144720 63.309 TRIG_00657750
Foreground time interval of the image:
-4.832 13.381 (delta_t = 18.213 [sec])
Background time interval of the image:
-239.120 -4.832 (delta_t = 234.288 [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 -4.832 sec. to 311.296 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50078 ( -0.0596992 0.0598692 )
Norm@50keV : 2.40760E-03 ( -7.33652e-05 7.33105e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.96 using 59 PHA bins.
# Reduced chi-squared = 0.7712 for 57 degrees of freedom
# Null hypothesis probability = 8.971696e-01
Photon flux (15-150 keV) in 316.1 sec: 0.300626 ( -0.00982275 0.00986294 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.21868e-06 ( -2.38214e-07 2.3928e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.832 sec. to 311.296 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49873 ( -0.0604159 0.0597608 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.41441E-03 ( -7.3536e-05 0.000642606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.96 using 59 PHA bins.
# Reduced chi-squared = 0.7850 for 56 degrees of freedom
# Null hypothesis probability = 8.783696e-01
Photon flux (15-150 keV) in 316.1 sec: 0.300551 ( -0.009488 0.009765 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.21865e-06 ( -2.5563e-07 2.36601e-07 ) ergs/cm2
Band function
Time interval is from -4.832 sec. to 311.296 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97837 ( -4.97837 -4.97837 )
beta : -1.51093 ( -0.0633348 0.0610984 )
Epeak [keV] : 20.3222 ( -20.3222 3.78067 )
Norm@50keV : 876.438 ( -26.5046 830649 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.31 using 59 PHA bins.
# Reduced chi-squared = 0.7874 for 55 degrees of freedom
# Null hypothesis probability = 8.729855e-01
Photon flux (15-150 keV) in 316.1 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] : 16.1313 ( )
R^2/D10^2 : 2.50888E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 291.23 using 59 PHA bins.
# Reduced chi-squared = 5.1094 for 57 degrees of freedom
# Null hypothesis probability = 3.794475e-33
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.259e-07 2.813e-08
25- 50 1.805e-06 8.171e-08
50-150 3.293e-06 1.906e-07
15-150 5.523e-06 2.055e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-12.4566 -200)
Norm : 1.22537 (-0.0371181 0.0371181)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.08 using 59 PHA bins.
# Reduced chi-squared = 0.9312 for 57 degrees of freedom
# Null hypothesis probability = 6.229261e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.647e-07 3.240e-08
25- 50 1.856e-06 6.559e-08
50-150 4.070e-06 1.249e-07
15-150 6.890e-06 2.260e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.84432 (-0.77421 0.878376)
R1^2/D10^2 : 0.333549 (-0.112766 0.184793)
kT2 [keV] : 27.3548 (-2.86951 3.99518)
R2^2/D10^2 : 3.36936E-03 (-0.00125443 0.0016183)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.27 using 59 PHA bins.
# Reduced chi-squared = 0.9685 for 55 degrees of freedom
# Null hypothesis probability = 5.410146e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.064e-07 1.045e-07
25- 50 1.796e-06 1.285e-07
50-150 4.408e-06 3.762e-07
15-150 7.110e-06 4.536e-07
Peak spectrum fit
Power-law model
Time interval is from 1.700 sec. to 2.700 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38422 ( -0.115197 0.115982 )
Norm@50keV : 2.20194E-02 ( -0.00155886 0.00155261 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.66 using 59 PHA bins.
# Reduced chi-squared = 1.257 for 57 degrees of freedom
# Null hypothesis probability = 9.153157e-02
Photon flux (15-150 keV) in 1 sec: 2.67210 ( -0.183249 0.183287 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.13464e-07 ( -1.70901e-08 1.7242e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.700 sec. to 2.700 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.827543 ( -0.527116 0.46892 )
Epeak [keV] : 101.766 ( -28.9012 241.646 )
Norm@50keV : 4.30221E-02 ( -0.0182081 0.0371095 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.47 using 59 PHA bins.
# Reduced chi-squared = 1.205 for 56 degrees of freedom
# Null hypothesis probability = 1.400961e-01
Photon flux (15-150 keV) in 1 sec: 2.61617 ( -0.18977 0.18934 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03087e-07 ( -1.9394e-08 1.9432e-08 ) ergs/cm2
Band function
Time interval is from 1.700 sec. to 2.700 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.72574 ( -2.60126 -1.73165 )
beta : -1.57306 ( -1.7386 0.184325 )
Epeak [keV] : 35.5601 ( -8.2612 96.1956 )
Norm@50keV : 2.86902 ( -2.98565 367.166 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.12 using 59 PHA bins.
# Reduced chi-squared = 1.184 for 55 degrees of freedom
# Null hypothesis probability = 1.649504e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07066e-07 ( -2.07059e-07 -1.8413e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.8499 (-1.26353 1.40913)
R^2/D10^2 : 0.323876 (-0.0867697 0.116011)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 102.43 using 59 PHA bins.
# Reduced chi-squared = 1.7971 for 57 degrees of freedom
# Null hypothesis probability = 2.105450e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.498e-08 2.025e-09
25- 50 5.896e-08 5.365e-09
50-150 8.808e-08 1.248e-08
15-150 1.620e-07 1.420e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-28.1555 -200)
Norm : 10.9465 (-0.748116 0.748116)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.30 using 59 PHA bins.
# Reduced chi-squared = 1.286 for 57 degrees of freedom
# Null hypothesis probability = 7.175082e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.727e-08 2.170e-09
25- 50 5.246e-08 5.990e-09
50-150 1.151e-07 3.143e-08
15-150 1.948e-07 3.585e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.85818 (-1.76025 2.12758)
R1^2/D10^2 : 1.73196 (-0.835818 1.98028)
kT2 [keV] : 27.0587 (-6.04001 15.5256)
R2^2/D10^2 : 3.10443E-02 (-0.0241865 0.0485889)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.71 using 59 PHA bins.
# Reduced chi-squared = 1.195 for 55 degrees of freedom
# Null hypothesis probability = 1.528542e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.286e-08 6.760e-09
25- 50 5.465e-08 1.579e-08
50-150 1.272e-07 5.910e-08
15-150 2.047e-07 7.241e-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: 1.30966 ( -0.0450069 0.0449334 )
Norm@50keV : 1.71089E-02 ( -0.000402365 0.000402323 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.93 using 59 PHA bins.
# Reduced chi-squared = 0.7006 for 57 degrees of freedom
# Null hypothesis probability = 9.581227e-01
Photon flux (15-150 keV) in 18.21 sec: 2.04481 ( -0.0520856 0.0522009 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.07152e-06 ( -7.74599e-08 7.75839e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13546 ( -0.183122 0.089974 )
Epeak [keV] : 279.925 ( -113.991 9521.61 )
Norm@50keV : 2.04604E-02 ( -0.00286855 0.00410329 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.08 using 59 PHA bins.
# Reduced chi-squared = 0.6622 for 56 degrees of freedom
# Null hypothesis probability = 9.759143e-01
Photon flux (15-150 keV) in 18.21 sec: 2.01932 ( -0.05753 0.05768 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.03776e-06 ( -8.56416e-08 8.52956e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.392779 ( -1.60951 -0.322698 )
beta : -1.35183 ( 1.34571 0.0582672 )
Epeak [keV] : 57.8492 ( -28.5298 224.305 )
Norm@50keV : 6.46168E-02 ( -0.0391904 596.203 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.32 using 59 PHA bins.
# Reduced chi-squared = 0.6604 for 55 degrees of freedom
# Null hypothesis probability = 9.755562e-01
Photon flux (15-150 keV) in 18.21 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) = 1.79e-06
S(50-100 keV) = 2.52e-06
T90 vs. Hardness ratio plot
T90 = 211.056000053883 sec.
Hardness ratio (energy fluence ratio) = 1.40782
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.2441
Count Ratio (50-100 keV) / (15-25 keV) = 0.982424
Mask shadow pattern
IMX = -1.306597232928468E-02, IMY = -2.372788338045695E-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:
-239.120000 -4.832000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
65.3966 71.4309 3.0 26.1 94.0 1.2108 3.9 ------ UNKNOWN
264.0344 79.6434 2.6 26.9 161.1 1.0088 4.4 ------ UNKNOWN
260.1167 42.4677 2.7 57.6 -165.4 4.1960 4.2 ------ UNKNOWN
207.4730 38.0683 3.0 43.7 -116.2 3.1771 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.832000 13.380610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
147.4259 70.5081 0.2 1.6 118.8 4.7143 63.3 ------ UNKNOWN
239.2723 73.5369 2.1 26.4 179.5 0.4706 5.6 ------ UNKNOWN
181.4065 32.3858 2.3 41.0 -83.6 1.4586 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
34.580600 962.982600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
21.1631 64.3488 3.5 40.2 102.2 7.0374 3.3 ------ UNKNOWN
96.5075 47.6733 3.0 33.0 28.7 3.0482 3.9 ------ UNKNOWN
100.9872 43.9685 2.6 34.9 20.7 3.5081 4.5 ------ UNKNOWN
181.6500 87.7619 3.6 17.7 139.2 1.7587 3.2 ------ UNKNOWN
268.5713 65.1275 3.0 38.5 170.3 3.1434 3.8 ------ UNKNOWN
105.4162 24.9154 3.1 51.5 5.8 5.3676 3.8 ------ UNKNOWN
263.9458 67.4099 2.8 35.6 171.2 2.9484 4.1 ------ UNKNOWN
147.4318 70.4813 0.9 0.0 -43.1 5.8168 13.0 ------ UNKNOWN
241.2119 35.2163 2.0 58.3 -151.6 16.9782 5.9 ------ UNKNOWN
215.5475 37.3260 3.7 47.9 -129.0 6.9672 3.1 ------ UNKNOWN
207.7194 37.3185 3.5 45.3 -121.2 7.0318 3.3 ------ UNKNOWN
Plot creation:
Sun Nov 1 14:28:47 EST 2015