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
352.3016 42.4946 0.0265 33.9638 -30.4332 0.0838499 7.262 TRIG_00525451
Foreground time interval of the image:
-0.032 0.608 (delta_t = 0.640 [sec])
Background time interval of the image:
-239.144 -0.032 (delta_t = 239.112 [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)
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 -0.032 sec. to 0.608 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03003 ( -0.421338 0.394991 )
Norm@50keV : 8.78548E-03 ( -0.00203013 0.0019696 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.56 using 59 PHA bins.
# Reduced chi-squared = 0.7992 for 57 degrees of freedom
# Null hypothesis probability = 8.620880e-01
Photon flux (15-150 keV) in 0.64 sec: 1.01326 ( -0.237513 0.238944 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.01684e-08 ( -1.36124e-08 1.36276e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.032 sec. to 0.608 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02374 ( -0.587791 0.398656 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 8.83555E-03 ( -0.00202587 0.0131939 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.56 using 59 PHA bins.
# Reduced chi-squared = 0.8137 for 56 degrees of freedom
# Null hypothesis probability = 8.391208e-01
Photon flux (15-150 keV) in 0.64 sec: 1.01882 ( -0.243576 0.23298 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.02477e-08 ( -1.36116e-08 1.34918e-08 ) ergs/cm2
Band function
Time interval is from -0.032 sec. to 0.608 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.865581 ( 0.865573 0.865573 )
beta : -1.03005 ( 1.03002 0.421323 )
Epeak [keV] : 44.2698 ( -44.2629 -44.2629 )
Norm@50keV : 1.45152E-02 ( -0.00763565 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.56 using 59 PHA bins.
# Reduced chi-squared = 0.8283 for 55 degrees of freedom
# Null hypothesis probability = 8.141484e-01
Photon flux (15-150 keV) in 0.64 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] : 29.1969 (-7.94603 13.1616)
R^2/D10^2 : 1.50006E-02 (-0.00989917 0.0247466)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.89 using 59 PHA bins.
# Reduced chi-squared = 0.9104 for 57 degrees of freedom
# Null hypothesis probability = 6.665091e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.302e-09 6.037e-10
25- 50 7.939e-09 3.667e-09
50-150 4.829e-08 2.313e-08
15-150 5.753e-08 2.937e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 4.26953 (-0.972087 0.97196)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.38 using 59 PHA bins.
# Reduced chi-squared = 0.9013 for 57 degrees of freedom
# Null hypothesis probability = 6.851317e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.804e-09 4.064e-09
25- 50 1.309e-08 7.763e-09
50-150 2.871e-08 1.700e-08
15-150 4.860e-08 2.836e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.06845 (-2.64799 4.00653)
R1^2/D10^2 : 1.67332 (-1.43911 6.7472)
kT2 [keV] : 40.1797 (-13.2297 43.6442)
R2^2/D10^2 : 5.34221E-03 (-0.00442193 0.0121536)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.05 using 59 PHA bins.
# Reduced chi-squared = 0.7828 for 55 degrees of freedom
# Null hypothesis probability = 8.787708e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.035e-09 3.728e-09
25- 50 1.029e-08 5.770e-09
50-150 4.713e-08 2.741e-08
15-150 6.345e-08 3.270e-08
Peak spectrum fit
Power-law model
Time interval is from -0.212 sec. to 0.788 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.960109 ( -0.54844 0.487181 )
Norm@50keV : 5.31465E-03 ( -0.0015915 0.00152664 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.48 using 59 PHA bins.
# Reduced chi-squared = 0.8330 for 57 degrees of freedom
# Null hypothesis probability = 8.114182e-01
Photon flux (15-150 keV) in 1 sec: 0.610819 ( -0.1797 0.182376 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83053e-08 ( -1.65889e-08 1.67168e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.212 sec. to 0.788 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.75003 ( )
Epeak [keV] : 212.133 ( )
Norm@50keV : 1.79923E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.23 using 59 PHA bins.
# Reduced chi-squared = 0.8434 for 56 degrees of freedom
# Null hypothesis probability = 7.916497e-01
Photon flux (15-150 keV) in 1 sec: 0.607503 ( -0.093821 0.184113 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.81926e-08 ( -8.4784e-09 1.65521e-08 ) ergs/cm2
Band function
Time interval is from -0.212 sec. to 0.788 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.714460 ( -0.718733 1.5472 )
beta : 10.0000 ( -10 -10 )
Epeak [keV] : 324.087 ( -324.087 -324.087 )
Norm@50keV : 1.85856E-21 ( -5.32005e-22 7.95726e-15 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.27 using 59 PHA bins.
# Reduced chi-squared = 0.8595 for 55 degrees of freedom
# Null hypothesis probability = 7.612233e-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] : 28.8165 (-9.45792 17.9165)
R^2/D10^2 : 9.60833E-03 (-0.00960675 0.0228686)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.14 using 59 PHA bins.
# Reduced chi-squared = 0.8797 for 57 degrees of freedom
# Null hypothesis probability = 7.279633e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.279e-09 8.165e-10
25- 50 7.758e-09 4.713e-09
50-150 4.617e-08 2.807e-08
15-150 5.521e-08 3.298e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 2.58221 (-0.750146 0.750046)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.66 using 59 PHA bins.
# Reduced chi-squared = 0.9063 for 57 degrees of freedom
# Null hypothesis probability = 6.750508e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.430e-09 4.014e-09
25- 50 1.237e-08 7.600e-09
50-150 2.713e-08 1.686e-08
15-150 4.593e-08 2.787e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.27206 (-3.11602 5.37387)
R1^2/D10^2 : 0.495787 (-0.442225 2.79124)
kT2 [keV] : 41.2382 (-19.7743 102.581)
R2^2/D10^2 : 3.00678E-03 (-0.00262325 0.00954707)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.29 using 59 PHA bins.
# Reduced chi-squared = 0.8235 for 55 degrees of freedom
# Null hypothesis probability = 8.217300e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.020e-09 3.188e-09
25- 50 1.088e-08 6.255e-09
50-150 4.528e-08 2.625e-08
15-150 6.118e-08 3.167e-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: 1.03003 ( -0.421338 0.394991 )
Norm@50keV : 8.78548E-03 ( -0.00203013 0.0019696 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.56 using 59 PHA bins.
# Reduced chi-squared = 0.7992 for 57 degrees of freedom
# Null hypothesis probability = 8.620880e-01
Photon flux (15-150 keV) in 0.64 sec: 1.01326 ( -0.237513 0.238944 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.01684e-08 ( -1.36124e-08 1.36276e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02374 ( -0.5878 0.398644 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 8.83555E-03 ( -0.00202587 0.0131939 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.56 using 59 PHA bins.
# Reduced chi-squared = 0.8137 for 56 degrees of freedom
# Null hypothesis probability = 8.391208e-01
Photon flux (15-150 keV) in 0.64 sec: 1.01882 ( -0.243576 0.23298 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.02477e-08 ( -1.36116e-08 1.34918e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.865581 ( 0.865573 0.865573 )
beta : -1.03005 ( 1.03002 0.421323 )
Epeak [keV] : 44.2698 ( -44.2629 -44.2629 )
Norm@50keV : 1.45152E-02 ( -0.00763565 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.56 using 59 PHA bins.
# Reduced chi-squared = 0.8283 for 55 degrees of freedom
# Null hypothesis probability = 8.141484e-01
Photon flux (15-150 keV) in 0.64 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) = 1.14e-08
S(50-100 keV) = 2.23e-08
T90 vs. Hardness ratio plot
T90 = 0.595999896526337 sec.
Hardness ratio (energy fluence ratio) = 1.95614
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.18326
Count Ratio (50-100 keV) / (15-25 keV) = 1.40746
Mask shadow pattern
IMX = 5.807817109795863E-01, IMY = 3.411954567137049E-01
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:
-239.144000 -0.032000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4354 35.3268 6.4 39.4 169.5 0.5167 1.8 1.4 Her X-1
288.8342 10.9480 1.6 35.8 102.2 3.2226 7.1 2.1 GRS 1915+105
299.6738 35.2085 2.3 9.6 101.9 0.9232 5.0 4.1 Cyg X-1
308.1110 40.9859 2.0 3.6 35.3 1.0183 5.7 2.0 Cyg X-3
326.1696 38.3214 6.3 16.7 -3.9 0.3349 1.8 0.1 Cyg X-2
351.3533 24.0645 2.6 42.4 -3.6 1.3399 4.4 ------ UNKNOWN
236.0637 72.1149 2.9 42.4 -131.0 1.7112 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.032000 0.608000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6365 35.3774 4.0 39.2 169.4 0.0375 2.9 9.0 Her X-1
288.6826 11.0559 12.5 35.7 102.5 0.0193 0.9 9.5 GRS 1915+105
299.7789 35.2139 4.9 9.5 101.5 -0.0198 -2.3 9.3 Cyg X-1
308.2214 40.7681 5.5 3.8 36.2 0.0170 2.1 12.2 Cyg X-3
326.2918 38.4331 8.5 16.8 -4.4 0.0114 1.4 8.8 Cyg X-2
6.8137 18.3063 2.1 57.2 -10.1 0.2241 5.7 ------ UNKNOWN
352.3048 42.4939 1.6 34.0 -30.4 0.0857 7.4 ------ UNKNOWN
2.1781 53.9664 2.3 37.7 -52.1 0.0784 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
72.556610 962.906500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5903 35.2016 25.1 41.0 127.0 0.7656 0.5 0.0 Cyg X-1
308.0663 40.9291 2.4 32.7 131.6 4.3147 4.9 2.4 Cyg X-3
325.9772 38.3657 4.7 20.4 116.2 1.3435 2.5 9.5 Cyg X-2
314.0453 26.6441 3.4 34.9 104.5 3.9118 3.4 ------ UNKNOWN
217.8670 79.0579 2.9 55.6 -160.4 7.2019 4.0 ------ UNKNOWN
205.5908 76.9222 4.9 58.8 -159.3 11.2292 2.4 ------ UNKNOWN
198.2196 78.6186 4.9 57.9 -156.8 8.8406 2.4 ------ UNKNOWN
119.7717 81.1718 3.2 53.2 -142.2 11.0816 3.6 ------ UNKNOWN
43.9474 22.7757 2.9 46.9 -53.0 11.4080 3.9 ------ UNKNOWN
54.3878 55.0924 3.1 41.3 -100.9 11.9363 3.8 ------ UNKNOWN
Plot creation:
Sat May 30 19:21:27 EDT 2015