Special notes of this burst
Image
Pre-slew 25.0-100.0 keV image (Event data)
#RAcent DECcent POSerr Theta Phi Peak_Cts SNR Name
27.245 22.744 0.000 41.044 165.735 0.318 8.898 TRIG_00433065
Image time interval: 0.000 to 8.192 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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)
The mask-weighted light curves based on cleaned DPHs
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 -2.420 sec. to 458.424 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40216 ( -0.204463 0.204133 )
Norm@50keV : 4.39118E-04 ( -5.17692e-05 5.14189e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.26 using 59 PHA bins.
# Reduced chi-squared = 0.8817 for 57 degrees of freedom
# Null hypothesis probability = 7.240799e-01
Photon flux (15-150 keV) in 460.8 sec: 5.35026E-02 ( -0.00617913 0.00618523 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95433e-06 ( -2.58668e-07 2.62377e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.420 sec. to 458.424 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40416 ( -0.20923 0.201834 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 4.39711E-04 ( -0.000118358 0.000482153 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.27 using 59 PHA bins.
# Reduced chi-squared = 0.8976 for 56 degrees of freedom
# Null hypothesis probability = 6.907239e-01
Photon flux (15-150 keV) in 460.8 sec: 5.34820E-02 ( -0.0061504 0.0061439 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95241e-06 ( -2.69057e-07 2.60997e-07 ) ergs/cm2
Band function
Time interval is from -2.420 sec. to 458.424 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.94336 ( -4.94336 -4.94336 )
beta : -1.53369 ( -0.290698 0.241661 )
Epeak [keV] : 25.5976 ( -25.5976 5.12721 )
Norm@50keV : 35.0189 ( -3.96989 149727 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.68 using 59 PHA bins.
# Reduced chi-squared = 0.8669 for 55 degrees of freedom
# Null hypothesis probability = 7.476965e-01
Photon flux (15-150 keV) in 460.8 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] : 14.8132 (-2.40473 3.01949)
R^2/D10^2 : 6.24169E-03 (-0.00290506 0.00530361)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.01 using 59 PHA bins.
# Reduced chi-squared = 1.316 for 57 degrees of freedom
# Null hypothesis probability = 5.510061e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.324e-07 3.117e-08
25- 50 5.200e-07 9.237e-08
50-150 7.721e-07 1.928e-07
15-150 1.424e-06 2.170e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-58.334 -200)
Norm : 0.219186 (-0.0251228 0.0251228)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.21 using 59 PHA bins.
# Reduced chi-squared = 0.9159 for 57 degrees of freedom
# Null hypothesis probability = 6.551739e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.515e-07 1.409e-07
25- 50 4.838e-07 2.684e-07
50-150 1.061e-06 5.834e-07
15-150 1.796e-06 9.707e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.16690 (-1.80475 2.64066)
R1^2/D10^2 : 5.71474E-02 (-0.0362617 0.0990197)
kT2 [keV] : 35.4824 (-12.4997 108.817)
R2^2/D10^2 : 2.84334E-04 (-0.000269228 0.000861971)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.22 using 59 PHA bins.
# Reduced chi-squared = 0.8767 for 55 degrees of freedom
# Null hypothesis probability = 7.294091e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.457e-07 1.013e-07
25- 50 4.708e-07 1.901e-07
50-150 1.300e-06 6.916e-07
15-150 2.016e-06 9.076e-07
Peak spectrum fit
Power-law model
Time interval is from -1.808 sec. to -0.808 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84020 ( -0.576779 0.650236 )
Norm@50keV : 5.64543E-03 ( -0.00204903 0.00182125 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.44 using 59 PHA bins.
# Reduced chi-squared = 0.9901 for 57 degrees of freedom
# Null hypothesis probability = 4.961470e-01
Photon flux (15-150 keV) in 1 sec: 0.790399 ( -0.221193 0.220953 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.19153e-08 ( -1.74014e-08 1.79455e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.808 sec. to -0.808 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.74680 ( )
Epeak [keV] : 242.616 ( )
Norm@50keV : 1.99431E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.07 using 59 PHA bins.
# Reduced chi-squared = 0.9834 for 56 degrees of freedom
# Null hypothesis probability = 5.100380e-01
Photon flux (15-150 keV) in 1 sec: 0.791755 ( -0.2194 0.219595 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.10953e-08 ( -1.66334e-08 1.78139e-08 ) ergs/cm2
Band function
Time interval is from -1.808 sec. to -0.808 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.45399 ( 1.45427 1.45427 )
beta : -1.84026 ( 1.84042 0.576802 )
Epeak [keV] : 17.1316 ( -17.033 -17.033 )
Norm@50keV : 1.43610E-02 ( -0.0143742 11322.1 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.44 using 59 PHA bins.
# Reduced chi-squared = 1.026 for 55 degrees of freedom
# Null hypothesis probability = 4.209986e-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] : 7.90489 (-2.64473 4.87194)
R^2/D10^2 : 0.848338 (-0.84462 3.60438)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.63 using 59 PHA bins.
# Reduced chi-squared = 1.116 for 57 degrees of freedom
# Null hypothesis probability = 2.546276e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.500e-09 5.835e-09
25- 50 1.628e-08 9.975e-09
50-150 4.110e-09 3.187e-09
15-150 2.989e-08 1.842e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8454 (-99.9046 -99.9046)
Norm : 3.41445 (-1.21298 2.41504)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.06 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.361470e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.924e-09 5.370e-09
25- 50 1.543e-08 9.260e-09
50-150 2.498e-08 1.889e-08
15-150 4.933e-08 3.464e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.12207 (-2.20326 3.07964)
R1^2/D10^2 : 2.14981 (-1.69396 13.2371)
kT2 [keV] : 98.7805 (-74.4033 -99.6656)
R2^2/D10^2 : 3.63102E-04 (-0.00029381 0.00941611)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.36 using 59 PHA bins.
#Fit statistic : Chi-Squared = 53.29 using 59 PHA bins.
# Reduced chi-squared = 0.9702 for 55 degrees of freedom
# Reduced chi-squared = 0.9688 for 55 degrees of freedom
# Null hypothesis probability = 5.375531e-01
# Null hypothesis probability = 5.404070e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.131e-08 6.760e-09
25- 50 1.305e-08 7.230e-09
50-150 3.584e-08 2.067e-08
15-150 6.020e-08 3.077e-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: 1.80851 ( -0.481713 0.542595 )
Norm@50keV : 8.12106E-04 ( -0.000263364 0.000247606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.71 using 59 PHA bins.
# Reduced chi-squared = 0.8545 for 57 degrees of freedom
# Null hypothesis probability = 7.748103e-01
Photon flux (15-150 keV) in 53.81 sec: 0.112278 ( -0.0301829 0.0302167 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02187e-07 ( -1.25798e-07 1.30648e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66404 ( -2.33358 0.7174 )
Epeak [keV] : 106.168 ( )
Norm@50keV : 9.73477E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.69 using 59 PHA bins.
# Reduced chi-squared = 0.8694 for 56 degrees of freedom
# Null hypothesis probability = 7.453408e-01
Photon flux (15-150 keV) in 53.81 sec: 0.111691 ( -0.0310988 0.030648 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.9763e-07 ( -1.35942e-07 1.33935e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.69402 ( 6.69402 6.69402 )
beta : -1.80851 ( -0.542595 0.481524 )
Epeak [keV] : 79.0008 ( -79.0008 -79.0008 )
Norm@50keV : 0.110377 ( -0.0357949 0.0336551 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.71 using 59 PHA bins.
# Reduced chi-squared = 0.8856 for 55 degrees of freedom
# Null hypothesis probability = 7.124094e-01
Photon flux (15-150 keV) in 53.81 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) = 4.60e-07
S(50-100 keV) = 6.96e-07
T90 vs. Hardness ratio plot
T90 = 436.655999958515 sec.
Hardness ratio (energy fluence ratio) = 1.51304
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.42719
Count Ratio (50-100 keV) / (15-25 keV) = 1.09776
Mask shadow pattern
IMX = -0.843794285758, IMY = -0.214535657933
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-239.512000 -2.420000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
39.8396 33.6801 3.1 54.3 176.9 2.3632 3.7 ------ UNKNOWN
54.4826 32.0424 3.2 58.7 -169.2 3.5980 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.420000 51.388600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
27.2549 22.7543 2.2 41.1 165.7 0.6884 5.2 ------ UNKNOWN
27.2924 11.3554 2.1 29.8 168.5 0.4801 5.4 ------ UNKNOWN
24.5745 -3.7907 2.4 14.4 167.2 0.3600 4.9 ------ UNKNOWN
63.0742 -55.6500 2.5 48.4 -50.1 1.5872 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
127.588610 625.388600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
27.2676 22.7560 1.3 0.1 -167.3 2.6975 9.2 ------ UNKNOWN
Plot creation:
Thu Oct 8 20:27:26 EDT 2015