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
70.0935 22.5246 0.0122 35.1938 -22.0675 5.8717864 15.710 TRIG_00357072
Foreground time interval of the image:
-112.896 159.752 (delta_t = 272.648 [sec])
Background time interval of the image:
-567.179 -534.007 (delta_t = 33.172 [sec])
-239.080 -112.896 (delta_t = 126.184 [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 4.096000
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 4.096000
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 4.096000
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 -112.896 sec. to 159.752 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36395 ( -0.112236 0.111897 )
Norm@50keV : 1.46132E-03 ( -8.96317e-05 8.95111e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.76 using 59 PHA bins.
# Reduced chi-squared = 1.013 for 57 degrees of freedom
# Null hypothesis probability = 4.469763e-01
Photon flux (15-150 keV) in 272.6 sec: 0.176561 ( -0.0111618 0.0111891 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87866e-06 ( -2.644e-07 2.65945e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -112.896 sec. to 159.752 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28315 ( -0.420825 0.138367 )
Epeak [keV] : 438.421 ( -465.132 -465.132 )
Norm@50keV : 1.59783E-03 ( -0.000217475 0.000902157 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.67 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.133674e-01
Photon flux (15-150 keV) in 272.6 sec: 0.175771 ( -0.011742 0.005887 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.85721e-06 ( -2.88329e-07 2.81378e-07 ) ergs/cm2
Band function
Time interval is from -112.896 sec. to 159.752 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95092 ( -4.95092 -4.95092 )
beta : -1.40768 ( -0.123351 0.121027 )
Epeak [keV] : 23.3363 ( -23.3363 3.84613 )
Norm@50keV : 190.957 ( -11.6179 572725 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.84 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 55 degrees of freedom
# Null hypothesis probability = 4.429389e-01
Photon flux (15-150 keV) in 272.6 sec: 0.175502 ( ) 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] : 17.4849 ( )
R^2/D10^2 : 1.18424E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 123.81 using 59 PHA bins.
# Reduced chi-squared = 2.1720 for 57 degrees of freedom
# Null hypothesis probability = 7.503634e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.994e-07 2.475e-08
25- 50 9.020e-07 8.164e-08
50-150 1.986e-06 2.230e-07
15-150 3.087e-06 2.385e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 0.730381 (-0.0447801 0.0447753)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.69 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 57 degrees of freedom
# Null hypothesis probability = 1.781842e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.959e-07 3.448e-08
25- 50 9.539e-07 7.319e-08
50-150 2.092e-06 4.693e-07
15-150 3.542e-06 5.778e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.44700 (-1.20098 1.44706)
R1^2/D10^2 : 0.228862 (-0.116231 0.267131)
kT2 [keV] : 27.9598 (-4.26778 6.64229)
R2^2/D10^2 : 2.10909E-03 (-0.00106382 0.00161963)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.07 using 59 PHA bins.
# Reduced chi-squared = 1.001 for 55 degrees of freedom
# Null hypothesis probability = 4.718286e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.527e-07 1.186e-07
25- 50 8.796e-07 1.492e-07
50-150 2.537e-06 5.765e-07
15-150 3.869e-06 7.616e-07
Peak spectrum fit
Power-law model
Time interval is from -6.096 sec. to -5.096 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37027 ( -0.353699 0.352536 )
Norm@50keV : 7.03806E-03 ( -0.0015292 0.0015211 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.26 using 59 PHA bins.
# Reduced chi-squared = 1.162 for 57 degrees of freedom
# Null hypothesis probability = 1.878863e-01
Photon flux (15-150 keV) in 1 sec: 0.851501 ( -0.183891 0.184398 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.84311e-08 ( -1.62604e-08 1.66844e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.096 sec. to -5.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.124060 ( -2.03342 1.3759 )
Epeak [keV] : 73.1249 ( -21.2141 -73.1251 )
Norm@50keV : 3.07606E-02 ( -0.0307602 0.281968 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.08 using 59 PHA bins.
# Reduced chi-squared = 1.144 for 56 degrees of freedom
# Null hypothesis probability = 2.142656e-01
Photon flux (15-150 keV) in 1 sec: 0.810403 ( -0.18871 0.190197 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.17677e-08 ( -1.69364e-08 1.836e-08 ) ergs/cm2
Band function
Time interval is from -6.096 sec. to -5.096 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95098 ( -13.6794 -4.95098 )
beta : -1.66317 ( -0.702241 0.458249 )
Epeak [keV] : 30.2963 ( -9.69481 10.3756 )
Norm@50keV : 214.118 ( -44.505 2447.62 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.14 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 55 degrees of freedom
# Null hypothesis probability = 2.108370e-01
Photon flux (15-150 keV) in 1 sec: 0.843608 ( 6.15639 -0.18737 ) 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] : 15.6130 (-3.55214 4.69997)
R^2/D10^2 : 8.88205E-02 (-0.0530556 0.12811)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.94 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 57 degrees of freedom
# Null hypothesis probability = 1.952558e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.500e-09 2.045e-09
25- 50 1.854e-08 8.119e-09
50-150 3.128e-08 1.447e-08
15-150 5.432e-08 2.186e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-101.983 -199.363)
Norm : 3.52720 (-0.750392 0.750406)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.97 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 57 degrees of freedom
# Null hypothesis probability = 1.946010e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.783e-09 5.260e-09
25- 50 1.690e-08 9.990e-09
50-150 3.706e-08 2.170e-08
15-150 6.273e-08 3.645e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21485 (-7.20317 -7.20317)
R1^2/D10^2 : 0.586320 (-0.589671 -0.589671)
kT2 [keV] : 21.6180 (-21.5925 -21.5925)
R2^2/D10^2 : 2.29716E-02 (-0.0230816 0.0936362)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.47 using 59 PHA bins.
# Reduced chi-squared = 1.154 for 55 degrees of freedom
# Null hypothesis probability = 2.026915e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.057e-09 4.467e-09
25- 50 1.781e-08 9.880e-09
50-150 3.792e-08 2.234e-08
15-150 6.279e-08 3.184e-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: 1.36395 ( -0.112236 0.111897 )
Norm@50keV : 1.46132E-03 ( -8.96317e-05 8.95111e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.76 using 59 PHA bins.
# Reduced chi-squared = 1.013 for 57 degrees of freedom
# Null hypothesis probability = 4.469763e-01
Photon flux (15-150 keV) in 272.6 sec: 0.176561 ( -0.0111618 0.0111891 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87866e-06 ( -2.644e-07 2.65945e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28315 ( -0.420825 0.138367 )
Epeak [keV] : 438.421 ( -465.132 -465.132 )
Norm@50keV : 1.59783E-03 ( -0.000217475 0.000902157 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.67 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.133674e-01
Photon flux (15-150 keV) in 272.6 sec: 0.175771 ( -0.011742 0.005887 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.85721e-06 ( -2.88329e-07 2.81378e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95092 ( -4.95092 -4.95092 )
beta : -1.40768 ( -0.123351 0.121027 )
Epeak [keV] : 23.3363 ( -23.3363 3.84613 )
Norm@50keV : 190.957 ( -11.6179 572725 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.84 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 55 degrees of freedom
# Null hypothesis probability = 4.429389e-01
Photon flux (15-150 keV) in 272.6 sec: 0.175502 ( ) 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) = 8.94e-07
S(50-100 keV) = 1.39e-06
T90 vs. Hardness ratio plot
T90 = 202.899999976158 sec.
Hardness ratio (energy fluence ratio) = 1.55481
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31974
Count Ratio (50-100 keV) / (15-25 keV) = 1.22031
Mask shadow pattern
IMX = 6.535952434727554E-01, IMY = 2.649658515032313E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-567.179400 -534.007000
-239.080000 -112.896000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6398 22.0185 0.5 38.1 -42.6 6.5175 24.4 0.4 Crab
47.0779 16.2959 2.7 43.2 11.7 1.1242 4.2 ------ UNKNOWN
151.0239 56.2087 2.6 44.0 -140.2 1.4681 4.5 ------ UNKNOWN
83.4488 5.5931 2.5 54.0 -36.7 3.6626 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-112.896000 159.752000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7784 22.0950 5.3 38.0 -42.8 -1.0009 -2.2 9.4 Crab
35.3829 36.8471 2.5 28.2 42.4 1.7955 4.6 ------ UNKNOWN
70.0935 22.5246 0.7 35.2 -22.1 5.8720 15.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
401.320630 840.230000
840.920000 962.930000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
204.4197 16.3666 3.0 39.9 104.0 5.2927 3.8 ------ UNKNOWN
202.3402 27.5570 2.8 32.1 89.9 2.7890 4.0 ------ UNKNOWN
170.4905 -8.5774 2.9 46.3 166.3 3.2588 4.0 ------ UNKNOWN
170.6734 72.4558 3.4 35.0 -4.9 1.3307 3.4 ------ UNKNOWN
164.4187 58.7021 2.8 21.2 -9.5 1.2895 4.2 ------ UNKNOWN
154.3779 -10.4042 2.7 49.2 -172.4 3.0908 4.3 ------ UNKNOWN
152.1693 87.4022 3.4 49.9 -8.2 2.2827 3.4 ------ UNKNOWN
143.5780 -15.4195 3.0 57.0 -161.5 6.2399 3.8 ------ UNKNOWN
100.9812 72.2983 2.1 46.9 -29.5 3.7649 5.6 ------ UNKNOWN
129.7740 1.9756 2.9 48.6 -135.7 5.4427 4.0 ------ UNKNOWN
Plot creation:
Sun May 31 03:33:40 EDT 2015