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
120.0290 -9.0766 0.0020 5.1274 -12.4952 10.9258662 96.999 TRIG_00512035
Foreground time interval of the image:
-13.016 12.085 (delta_t = 25.101 [sec])
Background time interval of the image:
-239.016 -13.016 (delta_t = 226.000 [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 1.024000
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 1.024000
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 1.024000
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 -13.016 sec. to 213.984 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37738 ( -0.031307 0.0312367 )
Norm@50keV : 7.73524E-03 ( -0.000125383 0.000125236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.02 using 59 PHA bins.
# Reduced chi-squared = 0.7548 for 57 degrees of freedom
# Null hypothesis probability = 9.147804e-01
Photon flux (15-150 keV) in 227 sec: 0.937285 ( -0.0176333 0.0176966 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.7047e-05 ( -2.75335e-07 2.75419e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -13.016 sec. to 213.984 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28105 ( -0.128933 0.0735754 )
Epeak [keV] : 443.256 ( -217.826 -443.4 )
Norm@50keV : 8.49240E-03 ( -0.000574781 0.00110032 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.33 using 59 PHA bins.
# Reduced chi-squared = 0.7381 for 56 degrees of freedom
# Null hypothesis probability = 9.285692e-01
Photon flux (15-150 keV) in 227 sec: 0.929219 ( -0.02022 0.010206 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69604e-05 ( -3.02478e-07 2.98959e-07 ) ergs/cm2
Band function
Time interval is from -13.016 sec. to 213.984 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.688316 ( -0.473972 5.06323 )
beta : -1.41440 ( -0.0830607 0.0447135 )
Epeak [keV] : 69.6817 ( -37.392 162.453 )
Norm@50keV : 1.95988E-02 ( -0.00994898 0.912242 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.06 using 59 PHA bins.
# Reduced chi-squared = 0.6919 for 55 degrees of freedom
# Null hypothesis probability = 9.602968e-01
Photon flux (15-150 keV) in 227 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] : 19.3892 ( )
R^2/D10^2 : 4.34931E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 761.51 using 59 PHA bins.
# Reduced chi-squared = 13.360 for 57 degrees of freedom
# Null hypothesis probability = 7.629867e-124
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.241e-07 2.622e-08
25- 50 3.532e-06 9.534e-08
50-150 9.796e-06 2.463e-07
15-150 1.405e-05 2.508e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 3.98841 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 189.66 using 59 PHA bins.
# Reduced chi-squared = 3.3274 for 57 degrees of freedom
# Null hypothesis probability = 3.710581e-16
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.254e-06 4.143e-08
25- 50 4.337e-06 8.399e-08
50-150 9.511e-06 1.748e-07
15-150 1.610e-05 2.792e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.56977 (-0.586505 0.622381)
R1^2/D10^2 : 0.441081 (-0.0882542 0.116687)
kT2 [keV] : 33.0827 (-2.35142 2.96065)
R2^2/D10^2 : 5.87987E-03 (-0.00146447 0.00170117)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.25 using 59 PHA bins.
# Reduced chi-squared = 1.059 for 55 degrees of freedom
# Null hypothesis probability = 3.566426e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.608e-06 1.068e-07
25- 50 4.114e-06 1.407e-07
50-150 1.107e-05 3.814e-07
15-150 1.679e-05 5.266e-07
Peak spectrum fit
Power-law model
Time interval is from 8.984 sec. to 9.984 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12581 ( -0.0530679 0.052945 )
Norm@50keV : 8.47845E-02 ( -0.00249356 0.00249327 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.81 using 59 PHA bins.
# Reduced chi-squared = 1.137 for 57 degrees of freedom
# Null hypothesis probability = 2.229693e-01
Photon flux (15-150 keV) in 1 sec: 9.86046 ( -0.298556 0.298812 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.79278e-07 ( -2.88203e-08 2.88874e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.984 sec. to 9.984 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.779959 ( -0.231005 0.219525 )
Epeak [keV] : 197.559 ( -57.0361 229.022 )
Norm@50keV : 0.121741 ( -0.0244362 0.0323311 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.42 using 59 PHA bins.
# Reduced chi-squared = 1.025 for 56 degrees of freedom
# Null hypothesis probability = 4.224750e-01
Photon flux (15-150 keV) in 1 sec: 9.69040 ( -0.31586 0.3161 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.61678e-07 ( -3.1489e-08 3.1321e-08 ) ergs/cm2
Band function
Time interval is from 8.984 sec. to 9.984 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.307641 ( -0.513964 0.855958 )
beta : -1.29424 ( -0.203022 0.111066 )
Epeak [keV] : 92.0748 ( -32.3866 103.028 )
Norm@50keV : 0.228349 ( -0.124385 0.583799 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.55 using 59 PHA bins.
# Reduced chi-squared = 0.9736 for 55 degrees of freedom
# Null hypothesis probability = 5.303119e-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] : 19.6506 ( )
R^2/D10^2 : 0.489304 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 217.46 using 59 PHA bins.
# Reduced chi-squared = 3.8150 for 57 degrees of freedom
# Null hypothesis probability = 1.398596e-20
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.668e-08 2.140e-09
25- 50 1.805e-07 7.800e-09
50-150 5.155e-07 2.550e-08
15-150 7.327e-07 2.855e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 40.6136 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 234.85 using 59 PHA bins.
# Reduced chi-squared = 4.1202 for 57 degrees of freedom
# Null hypothesis probability = 1.891280e-23
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.011e-07 3.105e-09
25- 50 1.945e-07 6.150e-09
50-150 4.267e-07 1.265e-08
15-150 7.223e-07 2.150e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.2841 (-1.43225 1.5059)
R1^2/D10^2 : 2.37719 (-0.683697 1.1468)
kT2 [keV] : 39.1330 (-6.93328 13.4934)
R2^2/D10^2 : 4.24783E-02 (-0.0244445 0.0379672)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.18 using 59 PHA bins.
# Reduced chi-squared = 1.076 for 55 degrees of freedom
# Null hypothesis probability = 3.256997e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.019e-08 6.900e-09
25- 50 1.914e-07 1.615e-08
50-150 6.130e-07 1.169e-07
15-150 8.645e-07 1.359e-07
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: 1.23458 ( -0.0304935 0.0304025 )
Norm@50keV : 2.83532E-02 ( -0.000465589 0.000465042 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.65 using 59 PHA bins.
# Reduced chi-squared = 0.6080 for 57 degrees of freedom
# Null hypothesis probability = 9.915464e-01
Photon flux (15-150 keV) in 25.1 sec: 3.34519 ( -0.0610337 0.061194 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.15159e-06 ( -1.16167e-07 1.16205e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09887 ( -0.125784 0.109774 )
Epeak [keV] : 404.652 ( -163.844 2423.86 )
Norm@50keV : 3.22525E-02 ( -0.00346853 0.00397975 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.11 using 59 PHA bins.
# Reduced chi-squared = 0.5555 for 56 degrees of freedom
# Null hypothesis probability = 9.971798e-01
Photon flux (15-150 keV) in 25.1 sec: 3.31043 ( -0.06773 0.06804 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.11136e-06 ( -1.23266e-07 1.22739e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.284663 ( -0.519311 4.4193 )
beta : -1.27456 ( -0.0661862 0.049321 )
Epeak [keV] : 63.6387 ( -33.2088 149.944 )
Norm@50keV : 0.105392 ( -0.0639169 24.6028 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 27.48 using 59 PHA bins.
# Reduced chi-squared = 0.4997 for 55 degrees of freedom
# Null hypothesis probability = 9.993010e-01
Photon flux (15-150 keV) in 25.1 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) = 3.96e-06
S(50-100 keV) = 6.10e-06
T90 vs. Hardness ratio plot
T90 = 68 sec.
Hardness ratio (energy fluence ratio) = 1.5404
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.47171
Count Ratio (50-100 keV) / (15-25 keV) = 1.20466
Mask shadow pattern
IMX = 8.760464921093211E-02, IMY = 1.941371800310528E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.016000 -13.016000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5713 -40.5358 2.4 34.7 -95.1 2.2472 4.9 2.3 Vela X-1
150.8658 13.5764 2.5 33.1 150.6 1.4891 4.6 ------ UNKNOWN
142.0945 -0.5167 2.4 18.4 168.8 0.9095 4.8 ------ UNKNOWN
154.7583 -24.2952 3.0 33.3 -136.5 1.0200 3.9 ------ UNKNOWN
102.9514 -47.9569 3.0 44.8 -59.9 3.4904 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.016000 12.084600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4883 -40.7177 7.4 34.8 -94.9 0.3832 1.6 9.9 Vela X-1
123.3378 18.8244 2.5 26.1 96.1 0.8097 4.7 ------ UNKNOWN
72.5431 -1.0451 2.6 52.5 13.5 2.0252 4.4 ------ UNKNOWN
120.0290 -9.0766 0.1 5.1 -12.5 10.9261 97.0 ------ UNKNOWN
175.3043 -26.1393 2.5 51.5 -142.8 2.1579 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
41.084600 423.034000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6251 21.9966 1.1 47.3 40.7 8.7419 10.8 1.2 Crab
135.4273 -40.5445 4.1 34.3 -111.8 1.1031 2.8 4.7 Vela X-1
173.6423 -1.3558 2.0 53.9 174.2 5.0393 5.8 ------ UNKNOWN
113.3042 -2.3032 2.8 9.5 44.1 0.8491 4.1 ------ UNKNOWN
120.0344 -9.0928 0.8 0.0 -124.5 2.8476 13.7 ------ UNKNOWN
74.7068 -14.8407 2.5 44.6 -12.8 1.5636 4.6 ------ UNKNOWN
66.5239 -17.7709 3.5 52.6 -16.3 1.6905 3.3 ------ UNKNOWN
Plot creation:
Sat May 30 20:37:27 EDT 2015