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
18.1355 55.7922 0.0042 12.1656 106.6889 1.7526899 45.819 TRIG_00226382
Foreground time interval of the image:
-3.624 7.000 (delta_t = 10.624 [sec])
Background time interval of the image:
-239.104 -3.624 (delta_t = 235.480 [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 -3.624 sec. to 7.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69065 ( -0.0655201 0.0659846 )
Norm@50keV : 1.03078E-02 ( -0.00038195 0.000380709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.38 using 59 PHA bins.
# Reduced chi-squared = 1.428 for 57 degrees of freedom
# Null hypothesis probability = 1.871530e-02
Photon flux (15-150 keV) in 10.62 sec: 1.36455 ( -0.0499391 0.0500233 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01431e-06 ( -3.9556e-08 3.974e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.624 sec. to 7.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06516 ( -0.301807 0.281002 )
Epeak [keV] : 71.3598 ( -9.7975 20.7626 )
Norm@50keV : 2.16475E-02 ( -0.00602186 0.00917112 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.68 using 59 PHA bins.
# Reduced chi-squared = 1.173 for 56 degrees of freedom
# Null hypothesis probability = 1.764728e-01
Photon flux (15-150 keV) in 10.62 sec: 1.31123 ( -0.05463 0.05472 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.55128e-07 ( -4.68852e-08 4.71294e-08 ) ergs/cm2
Band function
Time interval is from -3.624 sec. to 7.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.06514 ( -0.210462 0.381106 )
beta : -10.0000 ( 10 3.37508e-14 )
Epeak [keV] : 71.3460 ( -8.08637 20.7637 )
Norm@50keV : 2.16463E-02 ( -0.00602421 0.0091708 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.68 using 59 PHA bins.
# Reduced chi-squared = 1.194 for 55 degrees of freedom
# Null hypothesis probability = 1.534921e-01
Photon flux (15-150 keV) in 10.62 sec: 1.31656 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.62983e-07 ( -9.62909e-07 -4.4244e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.9788 ( )
R^2/D10^2 : 0.243453 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 184.41 using 59 PHA bins.
# Reduced chi-squared = 3.2353 for 57 degrees of freedom
# Null hypothesis probability = 2.393955e-15
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.237e-08 6.144e-09
25- 50 3.176e-07 1.333e-08
50-150 3.379e-07 2.602e-08
15-150 7.478e-07 3.308e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 132.297 ( )
Norm : 5.68414 (-0.250429 0.298026)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.03 using 59 PHA bins.
# Reduced chi-squared = 1.176 for 57 degrees of freedom
# Null hypothesis probability = 1.707650e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.556e-07 1.009e-08
25- 50 2.835e-07 1.720e-08
50-150 5.330e-07 1.335e-07
15-150 9.720e-07 1.492e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.88463 (-0.895247 0.897221)
R1^2/D10^2 : 1.01893 (-0.287655 0.467465)
kT2 [keV] : 26.0011 (-3.88952 5.76206)
R2^2/D10^2 : 1.34754E-02 (-0.00699872 0.0119244)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.51 using 59 PHA bins.
# Reduced chi-squared = 1.100 for 55 degrees of freedom
# Null hypothesis probability = 2.837163e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.368e-07 1.561e-08
25- 50 3.005e-07 2.883e-08
50-150 5.254e-07 1.168e-07
15-150 9.627e-07 1.643e-07
Peak spectrum fit
Power-law model
Time interval is from 0.072 sec. to 1.072 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36312 ( -0.095728 0.0963172 )
Norm@50keV : 2.24282E-02 ( -0.00131145 0.00130894 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.24 using 59 PHA bins.
# Reduced chi-squared = 1.215 for 57 degrees of freedom
# Null hypothesis probability = 1.282873e-01
Photon flux (15-150 keV) in 1 sec: 2.70935 ( -0.156725 0.156804 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.18414e-07 ( -1.43467e-08 1.44432e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.072 sec. to 1.072 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.343012 ( -0.480413 0.431187 )
Epeak [keV] : 82.7631 ( -12.4096 24.8183 )
Norm@50keV : 7.16592E-02 ( -0.0272669 0.0503768 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.61 using 59 PHA bins.
# Reduced chi-squared = 0.9037 for 56 degrees of freedom
# Null hypothesis probability = 6.784175e-01
Photon flux (15-150 keV) in 1 sec: 2.59551 ( -0.16358 0.16349 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03534e-07 ( -1.5637e-08 1.5775e-08 ) ergs/cm2
Band function
Time interval is from 0.072 sec. to 1.072 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.342834 ( -0.330209 0.565089 )
beta : -10.0000 ( 10 3.90799e-14 )
Epeak [keV] : 82.7437 ( -12.3967 24.8255 )
Norm@50keV : 7.16771E-02 ( -0.0272528 0.0504379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.61 using 59 PHA bins.
# Reduced chi-squared = 0.9202 for 55 degrees of freedom
# Null hypothesis probability = 6.429586e-01
Photon flux (15-150 keV) in 1 sec: 2.61985 ( 4.38015 -0.19493 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03555e-07 ( -2.03548e-07 -1.5713e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 16.1140 (-1.07931 1.17453)
R^2/D10^2 : 0.253998 (-0.0541479 0.0677801)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.67 using 59 PHA bins.
# Reduced chi-squared = 1.380 for 57 degrees of freedom
# Null hypothesis probability = 3.017578e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.361e-08 1.515e-09
25- 50 5.764e-08 4.155e-09
50-150 1.049e-07 1.142e-08
15-150 1.761e-07 1.340e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 11.1601 (-0.639049 0.639048)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.23 using 59 PHA bins.
# Reduced chi-squared = 1.232 for 57 degrees of freedom
# Null hypothesis probability = 1.120515e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.779e-08 1.710e-09
25- 50 5.345e-08 4.970e-09
50-150 1.172e-07 2.455e-08
15-150 1.985e-07 2.615e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.34701 (-1.96459 2.68056)
R1^2/D10^2 : 2.47029 (-1.58526 5.32643)
kT2 [keV] : 21.0326 (-2.73161 4.76347)
R2^2/D10^2 : 8.75398E-02 (-0.0499376 0.0501778)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.81 using 59 PHA bins.
# Reduced chi-squared = 0.9057 for 55 degrees of freedom
# Null hypothesis probability = 6.725206e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.158e-08 8.724e-09
25- 50 5.366e-08 1.380e-08
50-150 1.259e-07 3.077e-08
15-150 2.011e-07 3.770e-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: 1.69065 ( -0.0655201 0.0659846 )
Norm@50keV : 1.03078E-02 ( -0.00038195 0.000380709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.38 using 59 PHA bins.
# Reduced chi-squared = 1.428 for 57 degrees of freedom
# Null hypothesis probability = 1.871530e-02
Photon flux (15-150 keV) in 10.62 sec: 1.36455 ( -0.0499391 0.0500233 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01431e-06 ( -3.9556e-08 3.974e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06516 ( -0.301807 0.281002 )
Epeak [keV] : 71.3598 ( -9.7975 20.7626 )
Norm@50keV : 2.16475E-02 ( -0.00602186 0.00917112 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.68 using 59 PHA bins.
# Reduced chi-squared = 1.173 for 56 degrees of freedom
# Null hypothesis probability = 1.764728e-01
Photon flux (15-150 keV) in 10.62 sec: 1.31123 ( -0.05463 0.05472 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.55128e-07 ( -4.68852e-08 4.71294e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.06514 ( -0.210462 0.381106 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 71.3460 ( -8.08635 20.7637 )
Norm@50keV : 2.16463E-02 ( -0.00602421 0.0091708 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.68 using 59 PHA bins.
# Reduced chi-squared = 1.194 for 55 degrees of freedom
# Null hypothesis probability = 1.534921e-01
Photon flux (15-150 keV) in 10.62 sec: 1.31656 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.62983e-07 ( -9.62909e-07 -4.4244e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.74e-07
S(50-100 keV) = 3.39e-07
T90 vs. Hardness ratio plot
T90 = 7.97600001096725 sec.
Hardness ratio (energy fluence ratio) = 1.23723
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39596
Count Ratio (50-100 keV) / (15-25 keV) = 0.804453
Mask shadow pattern
IMX = -6.190908599602463E-02, IMY = -2.064984497034719E-01
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:
-239.104000 -3.624000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6150 22.0112 0.6 49.5 -25.7 8.6481 20.4 1.0 Crab
64.6639 6.9789 3.3 57.3 2.3 3.3761 3.5 ------ UNKNOWN
53.4431 47.9566 2.6 15.4 -5.5 0.6616 4.4 ------ UNKNOWN
96.9197 48.9698 2.5 33.9 -63.3 1.2209 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.624000 7.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6598 22.1134 3.2 49.5 -25.8 -0.3301 -3.6 6.1 Crab
18.1355 55.7922 0.3 12.2 106.7 1.7523 45.8 ------ UNKNOWN
72.1308 39.3778 2.5 29.6 -25.4 0.2013 4.7 ------ UNKNOWN
138.1706 73.1337 2.4 35.4 -117.6 0.2933 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
49.796600 480.996660
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1878 41.0674 23.4 46.5 147.4 0.3993 0.5 7.7 Cyg X-3
326.2452 38.4500 7.0 38.2 130.4 0.9238 1.7 8.4 Cyg X-2
12.4766 54.2921 2.6 3.6 112.4 0.9792 4.5 ------ UNKNOWN
319.2760 67.7958 2.8 28.9 -177.0 1.0224 4.1 ------ UNKNOWN
58.0326 11.7669 2.1 53.8 -6.0 3.6433 5.4 ------ UNKNOWN
56.2749 20.3063 2.2 45.4 -9.3 2.0072 5.3 ------ UNKNOWN
242.2373 76.0076 3.7 45.2 -148.7 1.5481 3.2 ------ UNKNOWN
83.1912 31.4839 2.7 50.6 -44.6 5.5626 4.3 ------ UNKNOWN
Plot creation:
Sun May 31 12:15:23 EDT 2015