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
27.9298 -3.1936 0.0228 19.2844 18.8145 0.0245257 8.463 TRIG_00567163
Foreground time interval of the image:
-0.004 0.044 (delta_t = 0.048 [sec])
Background time interval of the image:
-185.911 -0.004 (delta_t = 185.907 [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 0.032000
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 0.032000
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 0.032000
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 -0.004 sec. to 0.044 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67252 ( -0.288156 0.301636 )
Norm@50keV : 2.73438E-02 ( -0.00577729 0.00570914 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.58 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 57 degrees of freedom
# Null hypothesis probability = 3.819274e-01
Photon flux (15-150 keV) in 0.048 sec: 3.59740 ( -0.736857 0.73766 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21809e-08 ( -2.6501e-09 2.66797e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.004 sec. to 0.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.455998 ( -2.24264 1.56082 )
Epeak [keV] : 60.3008 ( -10.9144 26.2581 )
Norm@50keV : 0.309363 ( -0.309523 2.56825 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.82 using 59 PHA bins.
# Reduced chi-squared = 0.9611 for 56 degrees of freedom
# Null hypothesis probability = 5.576796e-01
Photon flux (15-150 keV) in 0.048 sec: 3.53490 ( -0.38763 0.75855 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21491e-08 ( -2.52058e-09 2.57486e-09 ) ergs/cm2
Band function
Time interval is from -0.004 sec. to 0.044 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.452381 ( -1.23079 2.69945 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 60.2790 ( -10.8941 26.2661 )
Norm@50keV : 0.308488 ( -0.308488 2.56931 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.82 using 59 PHA bins.
# Reduced chi-squared = 0.9786 for 55 degrees of freedom
# Null hypothesis probability = 5.195995e-01
Photon flux (15-150 keV) in 0.048 sec: 3.54124 ( 3.45876 -0.76983 ) 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] : 15.2118 (-2.29762 2.6224)
R^2/D10^2 : 0.447379 (-0.20739 0.364821)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.25 using 59 PHA bins.
# Reduced chi-squared = 0.9518 for 57 degrees of freedom
# Null hypothesis probability = 5.787635e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.038e-09 3.550e-10
25- 50 4.177e-09 1.169e-09
50-150 6.619e-09 2.019e-09
15-150 1.183e-08 3.118e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 137.294 (-62.253 -134.824)
Norm : 15.4202 (-3.39968 4.27013)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.32 using 59 PHA bins.
# Reduced chi-squared = 1.006 for 57 degrees of freedom
# Null hypothesis probability = 4.630568e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.914e-09 1.104e-09
25- 50 3.501e-09 1.976e-09
50-150 6.653e-09 4.342e-09
15-150 1.207e-08 7.193e-09
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.50506 (-2.48728 4.75533)
R1^2/D10^2 : 269.384 (-265.092 -266.121)
kT2 [keV] : 16.1790 (-2.56003 3.12684)
R2^2/D10^2 : 0.336783 (-0.181042 0.239887)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.78 using 59 PHA bins.
# Reduced chi-squared = 0.9232 for 55 degrees of freedom
# Null hypothesis probability = 6.365912e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.592e-09 7.276e-10
25- 50 3.761e-09 1.613e-09
50-150 6.811e-09 3.017e-09
15-150 1.216e-08 5.073e-09
Peak spectrum fit
Power-law model
Time interval is from -0.478 sec. to 0.522 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86624 ( -0.657105 0.852833 )
Norm@50keV : 2.27462E-03 ( -0.00115102 0.0010457 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.24 using 59 PHA bins.
# Reduced chi-squared = 0.7761 for 57 degrees of freedom
# Null hypothesis probability = 8.914561e-01
Photon flux (15-150 keV) in 1 sec: 0.321852 ( -0.119822 0.119847 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.09063e-08 ( -9.53168e-09 1.03102e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.478 sec. to 0.522 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01093 ( -4.95401 1.18741 )
Epeak [keV] : 53.5205 ( )
Norm@50keV : 6.60850E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.95 using 59 PHA bins.
# Reduced chi-squared = 0.7848 for 56 degrees of freedom
# Null hypothesis probability = 8.786558e-01
Photon flux (15-150 keV) in 1 sec: 0.314494 ( -0.118164 0.120456 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.99267e-08 ( -9.98584e-09 1.07172e-08 ) ergs/cm2
Band function
Time interval is from -0.478 sec. to 0.522 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.15286 ( -1.29936 5.14058 )
beta : -9.37159 ( 9.37165 19.3717 )
Epeak [keV] : 57.1531 ( -56.714 -56.714 )
Norm@50keV : 5.43386E-03 ( -0.0054524 707383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.96 using 59 PHA bins.
# Reduced chi-squared = 0.7993 for 55 degrees of freedom
# Null hypothesis probability = 8.571564e-01
Photon flux (15-150 keV) in 1 sec: 0.316978 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.0048e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.9182 (-4.70123 6.53364)
R^2/D10^2 : 6.20329E-02 (-0.0620304 0.247036)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.00 using 59 PHA bins.
# Reduced chi-squared = 0.7894 for 57 degrees of freedom
# Null hypothesis probability = 8.751146e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.196e-09 1.461e-09
25- 50 7.511e-09 4.592e-09
50-150 7.895e-09 6.120e-09
15-150 1.760e-08 1.157e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 87.6495 (-87.6214 -87.6214)
Norm : 1.48600 (-0.617933 1.16261)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.00 using 59 PHA bins.
# Reduced chi-squared = 0.7719 for 57 degrees of freedom
# Null hypothesis probability = 8.964380e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.874e-09 2.480e-09
25- 50 6.514e-09 4.262e-09
50-150 9.757e-09 8.215e-09
15-150 2.014e-08 1.413e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.66863 (-2.5429 11.0861)
R1^2/D10^2 : 25.3044 (-36.1401 -36.1401)
kT2 [keV] : 15.2824 (-5.548 10.5453)
R2^2/D10^2 : 3.01600E-02 (-0.0308281 0.0771018)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.33 using 59 PHA bins.
# Reduced chi-squared = 0.7697 for 55 degrees of freedom
# Null hypothesis probability = 8.944258e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.671e-09 2.126e-09
25- 50 6.150e-09 3.892e-09
50-150 9.521e-09 6.615e-09
15-150 1.934e-08 1.129e-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: 1.67252 ( -0.288156 0.301636 )
Norm@50keV : 2.73438E-02 ( -0.00577729 0.00570914 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.58 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 57 degrees of freedom
# Null hypothesis probability = 3.819274e-01
Photon flux (15-150 keV) in 0.048 sec: 3.59740 ( -0.736857 0.73766 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21809e-08 ( -2.6501e-09 2.66797e-09 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.455998 ( -2.24264 1.56082 )
Epeak [keV] : 60.3008 ( -10.9144 26.2581 )
Norm@50keV : 0.309363 ( -0.309523 2.56825 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.82 using 59 PHA bins.
# Reduced chi-squared = 0.9611 for 56 degrees of freedom
# Null hypothesis probability = 5.576796e-01
Photon flux (15-150 keV) in 0.048 sec: 3.53490 ( -0.38763 0.75855 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21491e-08 ( -2.52058e-09 2.57486e-09 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.452381 ( -1.23079 2.69945 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 60.2790 ( -10.8941 26.2661 )
Norm@50keV : 0.308488 ( -0.308488 2.56931 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.82 using 59 PHA bins.
# Reduced chi-squared = 0.9786 for 55 degrees of freedom
# Null hypothesis probability = 5.195995e-01
Photon flux (15-150 keV) in 0.048 sec: 3.54124 ( 3.45876 -0.76983 ) 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) = 3.26e-09
S(50-100 keV) = 4.09e-09
T90 vs. Hardness ratio plot
T90 = 0.043999969959259 sec.
Hardness ratio (energy fluence ratio) = 1.2546
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.0653
Count Ratio (50-100 keV) / (15-25 keV) = 1.21735
Mask shadow pattern
IMX = 3.311932371978128E-01, IMY = -1.128406262777303E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
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:
-185.911420 -0.004000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
353.7746 -9.5915 2.7 39.4 82.0 2.7143 4.3 ------ UNKNOWN
356.4952 -12.4155 3.8 39.3 75.9 1.7679 3.1 ------ UNKNOWN
13.5692 -12.9624 2.6 30.6 50.8 0.9600 4.4 ------ UNKNOWN
337.0685 35.1031 2.6 46.3 153.9 1.8815 4.4 ------ UNKNOWN
72.4493 -1.6551 2.6 50.7 -44.3 3.4524 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.004000 0.044000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
27.9298 -3.1936 1.4 19.3 18.8 0.0245 8.5 ------ UNKNOWN
14.9506 57.3254 2.5 42.2 -157.4 0.0211 4.7 ------ UNKNOWN
66.2100 -11.0324 2.1 49.4 -29.7 0.0416 5.6 ------ UNKNOWN
38.3748 61.6090 2.3 47.0 -140.8 0.0328 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
57.088600 962.818600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
352.7849 10.5965 2.5 37.6 124.0 5.2316 4.6 ------ UNKNOWN
3.2628 46.4721 2.8 54.3 171.2 8.3658 4.1 ------ UNKNOWN
28.2558 -25.8586 3.3 22.6 11.2 1.4864 3.5 ------ UNKNOWN
19.1858 20.4165 2.9 25.2 172.4 1.9481 4.0 ------ UNKNOWN
39.8513 -36.6085 3.4 35.1 -4.8 1.9968 3.4 ------ UNKNOWN
Plot creation:
Sat May 30 15:49:32 EDT 2015