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
279.4751 -11.6816 0.0127 55.8867 -8.8617 9.9180040 15.153 TRIG_00550457
Foreground time interval of the image:
-11.299 154.176 (delta_t = 165.475 [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
Time interval is from -159.472 sec. to 154.176 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74896 ( -0.0489459 0.0491411 )
Norm@50keV : 1.02716E-02 ( -0.000253383 0.000253176 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.03 using 59 PHA bins.
# Reduced chi-squared = 0.7548 for 57 degrees of freedom
# Null hypothesis probability = 9.147120e-01
Photon flux (15-150 keV) in 313.6 sec: 1.38837 ( -0.0393699 0.0395721 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.97249e-05 ( -7.48933e-07 7.49692e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -159.472 sec. to 154.176 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55839 ( -0.202415 0.192361 )
Epeak [keV] : 124.380 ( -37.9665 3992.3 )
Norm@50keV : 1.25852E-02 ( -0.00212822 0.0029483 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.22 using 59 PHA bins.
# Reduced chi-squared = 0.7182 for 56 degrees of freedom
# Null hypothesis probability = 9.447139e-01
Photon flux (15-150 keV) in 313.6 sec: 1.36365 ( -0.04588 0.04621 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.92959e-05 ( -8.73062e-07 8.69299e-07 ) ergs/cm2
Band function
Time interval is from -159.472 sec. to 154.176 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.55044 ( -0.0927396 0.185398 )
beta : -9.14499 ( 9.36706 19.3659 )
Epeak [keV] : 123.365 ( -28.249 4075.03 )
Norm@50keV : 1.26593E-02 ( -0.000308598 0.00123414 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.23 using 59 PHA bins.
# Reduced chi-squared = 0.7314 for 55 degrees of freedom
# Null hypothesis probability = 9.323669e-01
Photon flux (15-150 keV) in 313.6 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.96169e-05 ( -2.96147e-05 -2.96169e-05 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.8001 ( )
R^2/D10^2 : 0.145762 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 383.47 using 59 PHA bins.
# Reduced chi-squared = 6.7276 for 57 degrees of freedom
# Null hypothesis probability = 6.489229e-50
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.101e-06 1.018e-07
25- 50 8.244e-06 2.728e-07
50-150 1.221e-05 5.911e-07
15-150 2.256e-05 5.958e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 135.433 (-14.9247 17.5042)
Norm : 5.63603 (-0.196386 0.215268)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.21 using 59 PHA bins.
# Reduced chi-squared = 0.7931 for 57 degrees of freedom
# Null hypothesis probability = 8.702576e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.574e-06 2.681e-07
25- 50 8.349e-06 3.920e-07
50-150 1.577e-05 3.359e-06
15-150 2.869e-05 3.613e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.68500 (-0.655909 0.699045)
R1^2/D10^2 : 1.79318 (-0.546146 0.87499)
kT2 [keV] : 24.0870 (-1.96588 2.48162)
R2^2/D10^2 : 1.96097E-02 (-0.00617234 0.0077902)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.36 using 59 PHA bins.
# Reduced chi-squared = 0.9702 for 55 degrees of freedom
# Null hypothesis probability = 5.375432e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.471e-06 4.281e-07
25- 50 8.317e-06 4.171e-07
50-150 1.587e-05 9.847e-07
15-150 2.865e-05 1.380e-06
Peak spectrum fit
Power-law model
Time interval is from -138.276 sec. to -137.276 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57337 ( -0.107283 0.107971 )
Norm@50keV : 5.22230E-02 ( -0.0031216 0.00311284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.99 using 59 PHA bins.
# Reduced chi-squared = 0.9472 for 57 degrees of freedom
# Null hypothesis probability = 5.887150e-01
Photon flux (15-150 keV) in 1 sec: 6.65671 ( -0.409469 0.410806 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.90053e-07 ( -3.13903e-08 3.15729e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -138.276 sec. to -137.276 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57630 ( -0.193599 0.105353 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.22213E-02 ( -0.0111899 0.0224848 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.01 using 59 PHA bins.
# Reduced chi-squared = 0.9644 for 56 degrees of freedom
# Null hypothesis probability = 5.506835e-01
Photon flux (15-150 keV) in 1 sec: 6.65443 ( -0.40983 0.40978 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.90003e-07 ( -3.0787e-08 3.1276e-08 ) ergs/cm2
Band function
Time interval is from -138.276 sec. to -137.276 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.63894 ( -4.63894 -4.63894 )
beta : -1.58439 ( -0.112497 0.10951 )
Epeak [keV] : 19.3274 ( -19.3274 5.48889 )
Norm@50keV : 1.46208E+04 ( -853.249 2.83028e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.74 using 59 PHA bins.
# Reduced chi-squared = 0.9771 for 55 degrees of freedom
# Null hypothesis probability = 5.228848e-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] : 14.9265 ( )
R^2/D10^2 : 0.734523 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 141.09 using 59 PHA bins.
# Reduced chi-squared = 2.4753 for 57 degrees of freedom
# Null hypothesis probability = 4.416623e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.429e-08 3.760e-09
25- 50 1.356e-07 1.035e-08
50-150 2.052e-07 2.215e-08
15-150 3.751e-07 2.760e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 26.8896 (-1.57615 1.5737)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.59 using 59 PHA bins.
# Reduced chi-squared = 0.9928 for 57 degrees of freedom
# Null hypothesis probability = 4.903382e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.697e-08 4.825e-09
25- 50 1.288e-07 9.000e-09
50-150 2.825e-07 6.090e-08
15-150 4.783e-07 7.420e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.09967 (-1.29369 1.47866)
R1^2/D10^2 : 7.23651 (-3.38559 7.72829)
kT2 [keV] : 29.9337 (-5.91072 10.9383)
R2^2/D10^2 : 5.14705E-02 (-0.0322856 0.0601369)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.61 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 55 degrees of freedom
# Null hypothesis probability = 3.788493e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.668e-08 1.480e-08
25- 50 1.282e-07 2.261e-08
50-150 2.967e-07 8.535e-08
15-150 4.915e-07 1.174e-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: 1.89411 ( -0.154958 0.159871 )
Norm@50keV : 4.32829E-03 ( -0.000398137 0.000392788 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.78 using 59 PHA bins.
# Reduced chi-squared = 0.7505 for 57 degrees of freedom
# Null hypothesis probability = 9.189711e-01
Photon flux (15-150 keV) in 165.5 sec: 0.619607 ( -0.0543166 0.0546196 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.58544e-06 ( -5.96573e-07 6.0053e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69713 ( -0.66628 0.56994 )
Epeak [keV] : 75.0739 ( )
Norm@50keV : 5.46471E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.47 using 59 PHA bins.
# Reduced chi-squared = 0.7584 for 56 degrees of freedom
# Null hypothesis probability = 9.090246e-01
Photon flux (15-150 keV) in 165.5 sec: 0.612583 ( -0.05816 0.057985 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.49746e-06 ( -6.60345e-07 6.54933e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.64261 ( 1.60006 1.60006 )
beta : -2.12720 ( 2.11473 0.366191 )
Epeak [keV] : 67.1201 ( -65.9763 -65.9763 )
Norm@50keV : 5.86223E-03 ( -0.00172591 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.43 using 59 PHA bins.
# Reduced chi-squared = 0.7715 for 55 degrees of freedom
# Null hypothesis probability = 8.923137e-01
Photon flux (15-150 keV) in 165.5 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.4803e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 8.21e-06
S(50-100 keV) = 9.77e-06
T90 vs. Hardness ratio plot
T90 = 272.379999935627 sec.
Hardness ratio (energy fluence ratio) = 1.19001
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.2219
Count Ratio (50-100 keV) / (15-25 keV) = 0.879547
Mask shadow pattern
IMX = 1.458634699968526E+00, IMY = 2.274181447674928E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-11.299400 154.176000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6371 35.2990 34.0 33.5 63.2 -0.1249 -0.3 9.2 Her X-1
268.4636 -1.4705 8.4 50.4 8.6 -0.6543 -1.4 5.8 SW J1753.5-0127
288.7944 10.9534 0.7 31.7 -14.2 3.3183 16.7 0.5 GRS 1915+105
299.5637 35.2188 1.9 6.9 -46.9 0.9722 6.0 1.7 Cyg X-1
308.1115 40.9375 2.3 8.3 -117.6 0.7883 5.0 0.9 Cyg X-3
326.2472 38.3457 6.4 22.5 -120.8 0.3516 1.8 3.8 Cyg X-2
257.4515 1.7242 2.8 53.6 22.6 4.1932 4.2 ------ UNKNOWN
279.4752 -11.6816 0.8 55.9 -8.9 9.9167 15.2 ------ UNKNOWN
4.3087 52.5882 2.8 45.2 -157.7 1.3664 4.2 ------ UNKNOWN
337.3603 18.6945 6.1 41.2 -98.2 1.6634 1.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
546.400600 963.041900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6081 35.4232 10.0 34.1 69.2 0.7558 1.2 8.8 Her X-1
268.2804 -1.3197 7.7 50.9 15.2 1.7894 1.5 9.6 SW J1753.5-0127
288.7895 10.9529 0.7 32.0 -7.3 6.3593 16.7 0.7 GRS 1915+105
299.5565 35.2688 1.6 6.7 -35.6 2.1875 7.2 4.4 Cyg X-1
308.1564 40.9611 1.3 7.7 -110.9 2.5354 8.6 2.2 Cyg X-3
326.1621 38.1725 6.7 21.8 -114.1 0.6356 1.7 9.0 Cyg X-2
283.7127 22.4600 3.5 22.8 11.5 0.9893 3.3 ------ UNKNOWN
Plot creation:
Sat May 30 17:17:31 EDT 2015