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
14.3499 -46.7991 0.0022 0.0366 -106.8900 57.8054139 86.977 TRIG_00509337
Foreground time interval of the image:
-16.299 164.560 (delta_t = 180.859 [sec])
166.000 914.212 (delta_t = 748.212 [sec])
Background time interval of the image:
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 64.000000
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 64.000000
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 64.000000
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
Multiple GTIs in the spectrum
tstart tstop
-66.952000 164.560000
166.000000 914.212000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48925 ( -0.029508 0.0294588 )
Norm@50keV : 3.91935E-03 ( -5.92695e-05 5.91967e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.41 using 59 PHA bins.
# Reduced chi-squared = 0.6387 for 57 degrees of freedom
# Null hypothesis probability = 9.847144e-01
Photon flux (15-150 keV) in 979.7 sec: 0.487888 ( -0.00900603 0.00904641 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.6491e-05 ( -5.39986e-07 5.40067e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-66.952000 164.560000
166.000000 914.212000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48780 ( )
Epeak [keV] : 9720.16 ( -9646.41 -9646.41 )
Norm@50keV : 3.93203E-03 ( -5.98322e-05 0.00065929 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.36 using 59 PHA bins.
# Reduced chi-squared = 0.6493 for 56 degrees of freedom
# Null hypothesis probability = 9.806091e-01
Photon flux (15-150 keV) in 979.7 sec: 0.484700 ( -0.009765 0.011484 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.63791e-05 ( -5.63425e-07 6.36903e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-66.952000 164.560000
166.000000 914.212000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.45042 ( 1.11455 5.94631 )
beta : -1.53905 ( 1.59954 0.137876 )
Epeak [keV] : 855.055 ( -863.918 -863.918 )
Norm@50keV : 4.06610E-03 ( -6.03856e-05 0.000228922 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.06 using 59 PHA bins.
# Reduced chi-squared = 0.6557 for 55 degrees of freedom
# Null hypothesis probability = 9.773661e-01
Photon flux (15-150 keV) in 979.7 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] : 18.9910 ( )
R^2/D10^2 : 2.30909E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 943.90 using 59 PHA bins.
# Reduced chi-squared = 16.560 for 57 degrees of freedom
# Null hypothesis probability = 6.843204e-161
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.604e-06 5.192e-08
25- 50 7.712e-06 1.793e-07
50-150 2.044e-05 4.507e-07
15-150 2.976e-05 5.143e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 2.02430 (-0.0298736 0.0298742)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 102.55 using 59 PHA bins.
# Reduced chi-squared = 1.7991 for 57 degrees of freedom
# Null hypothesis probability = 2.048368e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.940e-06 9.356e-08
25- 50 9.503e-06 1.705e-07
50-150 2.084e-05 3.527e-07
15-150 3.528e-05 6.221e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.68779 (-0.492792 0.521975)
R1^2/D10^2 : 0.345523 (-0.0716344 0.0952025)
kT2 [keV] : 29.7429 (-1.5877 1.88171)
R2^2/D10^2 : 4.06472E-03 (-0.00079706 0.000893325)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.73 using 59 PHA bins.
# Reduced chi-squared = 1.231 for 55 degrees of freedom
# Null hypothesis probability = 1.163409e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.061e-06 2.371e-07
25- 50 9.126e-06 2.479e-07
50-150 2.267e-05 6.417e-07
15-150 3.585e-05 8.964e-07
Peak spectrum fit
Power-law model
Time interval is from -64.384 sec. to -63.384 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67788 ( -0.594956 0.638697 )
Norm@50keV : 8.18168E-03 ( -0.00297239 0.0028546 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.58 using 59 PHA bins.
# Reduced chi-squared = 1.308 for 57 degrees of freedom
# Null hypothesis probability = 5.901308e-02
Photon flux (15-150 keV) in 1 sec: 1.07835 ( -0.371952 0.374742 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.58931e-08 ( -2.77618e-08 2.84288e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -64.384 sec. to -63.384 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65759 ( -3.75932 0.935636 )
Epeak [keV] : 814.644 ( )
Norm@50keV : 8.38679E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.58 using 59 PHA bins.
# Reduced chi-squared = 1.332 for 56 degrees of freedom
# Null hypothesis probability = 4.913258e-02
Photon flux (15-150 keV) in 1 sec: 1.07826 ( -0.375659 0.372 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.55397e-08 ( -4.45477e-08 2.87013e-08 ) ergs/cm2
Band function
Time interval is from -64.384 sec. to -63.384 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95003 ( -4.95003 -4.95003 )
beta : -2.03382 ( -2.20114 0.81367 )
Epeak [keV] : 30.8726 ( -30.8726 55.7524 )
Norm@50keV : 263.753 ( -87.3087 1.11098e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.02 using 59 PHA bins.
# Reduced chi-squared = 1.346 for 55 degrees of freedom
# Null hypothesis probability = 4.450198e-02
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] : 10.4495 (-3.49155 8.62948)
R^2/D10^2 : 0.429613 (-0.426938 1.6008)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.14 using 59 PHA bins.
# Reduced chi-squared = 1.353 for 57 degrees of freedom
# Null hypothesis probability = 3.905761e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.683e-09 6.035e-09
25- 50 2.559e-08 1.588e-08
50-150 1.515e-08 1.112e-08
15-150 5.042e-08 3.275e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 136.521 ( )
Norm : 4.52823 (-1.63942 2.86443)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.68 using 59 PHA bins.
# Reduced chi-squared = 1.310 for 57 degrees of freedom
# Null hypothesis probability = 5.807016e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.101e-08 6.780e-09
25- 50 2.083e-08 1.252e-08
50-150 4.358e-08 2.754e-08
15-150 7.542e-08 4.504e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.84028 (-3.33105 5.00179)
R1^2/D10^2 : 1.05128 (-0.664271 2.10334)
kT2 [keV] : 43.1662 (-28.8713 -43.5794)
R2^2/D10^2 : 2.27147E-03 (-0.00220121 0.0852505)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.30 using 59 PHA bins.
# Reduced chi-squared = 1.333 for 55 degrees of freedom
# Null hypothesis probability = 5.008550e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.202e-08 7.420e-09
25- 50 2.304e-08 1.358e-08
50-150 4.244e-08 2.597e-08
15-150 7.751e-08 4.026e-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: 1.49585 ( -0.0296012 0.0295545 )
Norm@50keV : 3.89799E-03 ( -5.90774e-05 5.90092e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.55 using 59 PHA bins.
# Reduced chi-squared = 0.6412 for 57 degrees of freedom
# Null hypothesis probability = 9.839909e-01
Photon flux (15-150 keV) in 929.1 sec: 0.486081 ( -0.00899577 0.00903561 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.43799e-05 ( -5.10913e-07 5.10989e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43193 ( -0.125035 0.0737666 )
Epeak [keV] : 513.350 ( -321.871 -549.842 )
Norm@50keV : 4.14210E-03 ( -0.000293424 0.000494677 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.91 using 59 PHA bins.
# Reduced chi-squared = 0.6413 for 56 degrees of freedom
# Null hypothesis probability = 9.831629e-01
Photon flux (15-150 keV) in 929.1 sec: 0.482915 ( -0.010647 0.010655 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.42699e-05 ( -5.648e-07 5.0924e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.43430 ( 1.10157 5.99891 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 552.675 ( -177.816 -552.746 )
Norm@50keV : 4.13262E-03 ( -0.00022499 0.000496974 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.77 using 59 PHA bins.
# Reduced chi-squared = 0.6504 for 55 degrees of freedom
# Null hypothesis probability = 9.792906e-01
Photon flux (15-150 keV) in 929.1 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) = 8.98e-06
S(50-100 keV) = 1.28e-05
T90 vs. Hardness ratio plot
T90 = 810.96799993515 sec.
Hardness ratio (energy fluence ratio) = 1.42539
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.26603
Count Ratio (50-100 keV) / (15-25 keV) = 0.999958
Mask shadow pattern
IMX = -1.855401688589516E-04, IMY = 6.110664473265062E-04
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-16.299410 164.560000
166.000000 914.212000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
59.1157 -41.4584 2.4 32.1 133.3 5.3548 4.8 ------ UNKNOWN
114.4612 -56.7569 2.5 57.1 176.2 19.4703 4.6 ------ UNKNOWN
115.3314 -59.5268 2.9 55.8 179.2 14.3795 3.9 ------ UNKNOWN
55.8419 -63.9388 2.3 28.4 178.4 3.7535 5.0 ------ UNKNOWN
14.3499 -46.7991 0.1 0.0 -106.9 57.8057 87.0 ------ UNKNOWN
125.2951 -65.1611 2.8 56.0 -172.0 11.0640 4.1 ------ UNKNOWN
329.6172 -3.0686 2.7 58.4 -19.5 16.1338 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-239.000000 164.560000
166.000000 963.057900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
59.1179 -41.4696 2.4 32.1 133.3 6.2729 4.9 ------ UNKNOWN
349.0415 3.8965 3.6 55.4 4.9 11.8919 3.2 ------ UNKNOWN
115.3235 -59.5208 3.0 55.8 179.2 16.6512 3.9 ------ UNKNOWN
55.8509 -63.9284 2.3 28.4 178.4 4.5011 5.1 ------ UNKNOWN
14.3506 -46.8004 0.2 0.0 -108.8 59.6262 75.8 ------ UNKNOWN
125.3151 -65.1603 2.9 56.1 -172.0 12.5274 4.0 ------ UNKNOWN
329.6091 -3.0697 2.5 58.4 -19.5 19.9374 4.6 ------ UNKNOWN
324.3848 -56.5684 3.5 31.7 -90.4 4.6904 3.3 ------ UNKNOWN
Plot creation:
Sat May 30 20:57:25 EDT 2015