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
108.9233 49.6597 0.0183 30.6897 -13.9694 1.5200058 10.484 TRIG_00506074
Foreground time interval of the image:
-47.832 -14.249 (delta_t = 33.583 [sec])
-13.000 60.180 (delta_t = 73.180 [sec])
Background time interval of the image:
-205.699 -47.832 (delta_t = 157.867 [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 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)
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
Multiple GTIs in the spectrum
tstart tstop
-47.832000 -14.248800
-13.000000 60.180000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64852 ( -0.206892 0.210702 )
Norm@50keV : 9.03853E-04 ( -0.000117039 0.000115271 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.57 using 59 PHA bins.
# Reduced chi-squared = 1.080 for 57 degrees of freedom
# Null hypothesis probability = 3.157672e-01
Photon flux (15-150 keV) in 106.8 sec: 0.117963 ( -0.014024 0.0140332 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.97922e-07 ( -1.22838e-07 1.24912e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-47.832000 -14.248800
-13.000000 60.180000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52085 ( -0.878705 0.332284 )
Epeak [keV] : 165.155 ( -168.255 -168.255 )
Norm@50keV : 1.06672E-03 ( -0.000273539 0.0022669 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.49 using 59 PHA bins.
# Reduced chi-squared = 1.098 for 56 degrees of freedom
# Null hypothesis probability = 2.858995e-01
Photon flux (15-150 keV) in 106.8 sec: 0.117413 ( -0.014376 0.014339 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.85387e-07 ( -1.47646e-07 1.35336e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-47.832000 -14.248800
-13.000000 60.180000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99426 ( -5.82199 -4.99426 )
beta : -1.86625 ( -0.389342 0.267287 )
Epeak [keV] : 25.8259 ( -6.29884 4.98421 )
Norm@50keV : 93.4032 ( -10.8632 452.36 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.84 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 55 degrees of freedom
# Null hypothesis probability = 4.062571e-01
Photon flux (15-150 keV) in 106.8 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] : 10.8035 (-1.51084 1.90093)
R^2/D10^2 : 4.19643E-02 (-0.0189543 0.0317809)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.71 using 59 PHA bins.
# Reduced chi-squared = 1.363 for 57 degrees of freedom
# Null hypothesis probability = 3.548524e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.089e-07 2.477e-08
25- 50 3.008e-07 5.057e-08
50-150 1.955e-07 6.050e-08
15-150 6.052e-07 9.697e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 146.931 (-62.9285 -145.612)
Norm : 0.488609 (-0.0640034 0.0863181)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.66 using 59 PHA bins.
# Reduced chi-squared = 1.082 for 57 degrees of freedom
# Null hypothesis probability = 3.131842e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.343e-07 4.690e-08
25- 50 2.481e-07 1.226e-07
50-150 4.855e-07 2.861e-07
15-150 8.679e-07 4.564e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.95936 (-1.41524 1.56354)
R1^2/D10^2 : 0.108845 (-0.0520376 0.107933)
kT2 [keV] : 48.9997 (-21.6982 -48.7069)
R2^2/D10^2 : 1.88176E-04 (-0.000181847 0.000539481)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.92 using 59 PHA bins.
# Reduced chi-squared = 0.9803 for 55 degrees of freedom
# Null hypothesis probability = 5.160330e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.380e-07 4.911e-08
25- 50 2.686e-07 8.667e-08
50-150 5.205e-07 2.692e-07
15-150 9.272e-07 3.720e-07
Peak spectrum fit
Power-law model
Time interval is from 49.536 sec. to 50.536 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10165 ( -1.13578 0.870091 )
Norm@50keV : 3.27518E-03 ( -0.00143824 0.00115349 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.11 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.343542e-01
Photon flux (15-150 keV) in 1 sec: 0.379756 ( -0.379756 0.144152 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.42514e-08 ( -1.37301e-08 1.37391e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 49.536 sec. to 50.536 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11015 ( -1.22092 0.811538 )
Epeak [keV] : 1.00000E+04 ( )
Norm@50keV : 3.29223E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.12 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 56 degrees of freedom
# Null hypothesis probability = 3.970534e-01
Photon flux (15-150 keV) in 1 sec: 0.383801 ( -0.07042 0.140292 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.31055e-08 ( -1.27687e-08 1.50353e-08 ) ergs/cm2
Band function
Time interval is from 49.536 sec. to 50.536 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.955300 ( 0.954456 0.954456 )
beta : -1.10311 ( 1.09904 1.13686 )
Epeak [keV] : 31.7518 ( -30.896 -30.896 )
Norm@50keV : 5.42261E-03 ( -0.00326105 0.596562 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.11 using 59 PHA bins.
# Reduced chi-squared = 1.056 for 55 degrees of freedom
# Null hypothesis probability = 3.616460e-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] : 56.4160 (-40.8068 -57.2595)
R^2/D10^2 : 9.90390E-04 (-0.000943521 0.027909)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.60 using 59 PHA bins.
# Reduced chi-squared = 1.098 for 57 degrees of freedom
# Null hypothesis probability = 2.843741e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.127e-10 2.034e-10
25- 50 2.319e-09 1.426e-09
50-150 3.166e-08 1.854e-08
15-150 3.429e-08 1.967e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-199.363 -199.363)
Norm : 1.57729 (-0.571065 0.57105)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.79 using 59 PHA bins.
# Reduced chi-squared = 1.049 for 57 degrees of freedom
# Null hypothesis probability = 3.747357e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.928e-09 2.523e-09
25- 50 7.555e-09 4.933e-09
50-150 1.657e-08 1.021e-08
15-150 2.805e-08 1.761e-08
Double BB
R1^2/D10^2 : 1.15380 ( )
kT2 [keV] : 200.000 ( )
R2^2/D10^2 : 1.09181E-04 (-4.67979e-05 0.000420651)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.26 using 59 PHA bins.
#Fit statistic : Chi-Squared = 54.11 using 59 PHA bins.
#Fit statistic : Chi-Squared = 54.02 using 59 PHA bins.
# Reduced chi-squared = 0.9866 for 55 degrees of freedom
# Reduced chi-squared = 0.9838 for 55 degrees of freedom
# Reduced chi-squared = 0.9822 for 55 degrees of freedom
# Null hypothesis probability = 5.027914e-01
# Null hypothesis probability = 5.086124e-01
# Null hypothesis probability = 5.119878e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.862e-09 3.204e-09
25- 50 5.029e-09 2.838e-09
50-150 2.995e-08 2.655e-08
15-150 3.984e-08 2.861e-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: 1.64852 ( -0.206892 0.210702 )
Norm@50keV : 9.03853E-04 ( -0.000117039 0.000115271 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.57 using 59 PHA bins.
# Reduced chi-squared = 1.080 for 57 degrees of freedom
# Null hypothesis probability = 3.157672e-01
Photon flux (15-150 keV) in 106.8 sec: 0.117963 ( -0.014024 0.0140332 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.97922e-07 ( -1.22838e-07 1.24912e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52085 ( -0.878705 0.332284 )
Epeak [keV] : 165.155 ( -168.255 -168.255 )
Norm@50keV : 1.06672E-03 ( -0.000273539 0.0022669 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.49 using 59 PHA bins.
# Reduced chi-squared = 1.098 for 56 degrees of freedom
# Null hypothesis probability = 2.858995e-01
Photon flux (15-150 keV) in 106.8 sec: 0.117413 ( -0.014376 0.014339 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.85387e-07 ( -1.47646e-07 1.35336e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99426 ( -14.9553 -4.99426 )
beta : -1.86625 ( -0.389342 0.267287 )
Epeak [keV] : 25.8259 ( -6.29884 4.98421 )
Norm@50keV : 93.4032 ( -10.8632 452.36 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.84 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 55 degrees of freedom
# Null hypothesis probability = 4.062571e-01
Photon flux (15-150 keV) in 106.8 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) = 2.38e-07
S(50-100 keV) = 3.03e-07
T90 vs. Hardness ratio plot
T90 = 83.0279999375343 sec.
Hardness ratio (energy fluence ratio) = 1.27311
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28909
Count Ratio (50-100 keV) / (15-25 keV) = 0.738368
Mask shadow pattern
IMX = 5.759592231643343E-01, IMY = 1.432760321747943E-01
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:
-205.699410 -47.832000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6292 22.0030 1.7 51.3 29.2 5.1426 6.9 0.7 Crab
308.0124 40.9824 325.4 58.0 -178.6 -0.0358 -0.0 4.8 Cyg X-3
326.3786 38.3944 3.8 55.3 164.5 -2.4865 -3.1 10.7 Cyg X-2
294.0733 43.4496 3.0 59.0 -166.2 3.7593 3.9 ------ UNKNOWN
140.8815 35.0265 3.3 53.9 -36.8 2.6783 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-47.832000 -14.248800
-13.000000 60.180000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8265 22.0091 7.6 51.3 28.9 -1.0525 -1.5 10.8 Crab
308.2383 40.9926 3.5 57.9 -178.8 -2.5686 -3.3 6.3 Cyg X-3
326.2287 38.3080 6.5 55.4 164.6 1.3567 1.8 2.8 Cyg X-2
108.9237 49.6602 1.1 30.7 -14.0 1.5437 10.6 ------ UNKNOWN
278.5813 57.1374 2.9 48.6 -149.8 1.2287 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
126.300590 963.085500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6339 22.0123 0.3 34.1 44.0 32.6478 34.6 0.1 Crab
38.7552 83.3155 3.8 38.5 168.8 2.4695 3.0 ------ UNKNOWN
252.5502 68.1748 3.2 59.1 -166.1 16.3021 3.6 ------ UNKNOWN
121.5539 -7.0415 3.8 57.8 -15.9 7.8226 3.0 ------ UNKNOWN
158.5962 55.9342 3.2 30.0 -122.4 2.3579 3.6 ------ UNKNOWN
Plot creation:
Sat May 30 21:18:20 EDT 2015