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
201.7989 37.5988 0.0224 17.4829 139.1656 0.0696343 8.613 TRIG_00600951
Foreground time interval of the image:
-0.040 0.352 (delta_t = 0.392 [sec])
Background time interval of the image:
-87.899 -0.040 (delta_t = 87.859 [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 0.128000
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 0.128000
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 0.128000
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 -0.040 sec. to 0.352 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.525033 ( -0.375533 0.337895 )
Norm@50keV : 9.85348E-03 ( -0.00230442 0.00221817 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.37 using 59 PHA bins.
# Reduced chi-squared = 1.147 for 57 degrees of freedom
# Null hypothesis probability = 2.089210e-01
Photon flux (15-150 keV) in 0.392 sec: 1.16240 ( -0.238018 0.239896 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12434e-08 ( -1.03547e-08 1.03891e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.040 sec. to 0.352 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.04460 ( -2.98163 1.69169 )
Epeak [keV] : 134.488 ( -43.6445 -134.261 )
Norm@50keV : 3.45684E-02 ( -0.035096 0.227518 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.13 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 56 degrees of freedom
# Null hypothesis probability = 2.390300e-01
Photon flux (15-150 keV) in 0.392 sec: 1.10566 ( -0.24261 0.24836 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.04872e-08 ( -1.09341e-08 1.07808e-08 ) ergs/cm2
Band function
Time interval is from -0.040 sec. to 0.352 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.06431 ( -0.581677 3.81088 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 134.219 ( -32.7608 145.262 )
Norm@50keV : 3.51053E-02 ( -0.0351051 0.227998 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.12 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 55 degrees of freedom
# Null hypothesis probability = 2.111647e-01
Photon flux (15-150 keV) in 0.392 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] : 31.6983 (-7.05968 11.5324)
R^2/D10^2 : 1.65684E-02 (-0.00939053 0.0174338)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.07 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 57 degrees of freedom
# Null hypothesis probability = 2.704120e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.863e-10 4.431e-10
25- 50 6.219e-09 2.634e-09
50-150 4.311e-08 1.757e-08
15-150 5.032e-08 1.941e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 4.22524 (-0.997233 0.99722)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 88.09 using 59 PHA bins.
# Reduced chi-squared = 1.545 for 57 degrees of freedom
# Null hypothesis probability = 5.154307e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.125e-09 2.489e-09
25- 50 7.936e-09 4.655e-09
50-150 1.740e-08 1.025e-08
15-150 2.947e-08 1.770e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.59974 (-2.33287 2.66438)
R1^2/D10^2 : 1023.52 (-63.7625 -63.7625)
kT2 [keV] : 32.2738 (-7.4439 157.644)
R2^2/D10^2 : 1.56651E-02 (-0.00901348 0.0155977)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.44 using 59 PHA bins.
# Reduced chi-squared = 1.135 for 55 degrees of freedom
# Null hypothesis probability = 2.288105e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.379e-09 4.731e-10
25- 50 6.071e-09 2.835e-09
50-150 4.323e-08 2.090e-08
15-150 5.068e-08 2.250e-08
Peak spectrum fit
Power-law model
Time interval is from -0.342 sec. to 0.658 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.126273 ( -0.624273 0.492691 )
Norm@50keV : 3.59574E-03 ( -0.00142443 0.00135952 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.79 using 59 PHA bins.
# Reduced chi-squared = 0.9436 for 57 degrees of freedom
# Null hypothesis probability = 5.964388e-01
Photon flux (15-150 keV) in 1 sec: 0.465460 ( -0.128898 0.132815 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.94057e-08 ( -1.48475e-08 1.48526e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.342 sec. to 0.658 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.29953 ( -4.45385 1.69965 )
Epeak [keV] : 175.197 ( -175.197 -175.197 )
Norm@50keV : 9.77689E-03 ( -0.00977691 0.130891 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.94 using 59 PHA bins.
# Reduced chi-squared = 0.9453 for 56 degrees of freedom
# Null hypothesis probability = 5.915686e-01
Photon flux (15-150 keV) in 1 sec: 0.451105 ( -0.123371 0.132907 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.93948e-08 ( -1.55891e-08 1.5202e-08 ) ergs/cm2
Band function
Time interval is from -0.342 sec. to 0.658 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.966701 ( 0.966701 0.966701 )
beta : -0.126277 ( -0.493179 0.623642 )
Epeak [keV] : 15.6806 ( -15.6806 -15.6806 )
Norm@50keV : 4.97008E-03 ( -0.00265772 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.79 using 59 PHA bins.
# Reduced chi-squared = 0.9779 for 55 degrees of freedom
# Null hypothesis probability = 5.211082e-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] : 43.7861 (-14.7822 48.3631)
R^2/D10^2 : 3.12207E-03 (-0.00312207 0.00604846)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.97 using 59 PHA bins.
# Reduced chi-squared = 0.9294 for 57 degrees of freedom
# Null hypothesis probability = 6.268076e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.229e-10 4.420e-10
25- 50 5.057e-09 2.950e-09
50-150 5.377e-08 3.093e-08
15-150 5.955e-08 3.464e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.62486 (-0.57939 0.579365)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.10 using 59 PHA bins.
# Reduced chi-squared = 1.335 for 57 degrees of freedom
# Null hypothesis probability = 4.633581e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.044e-09 2.589e-09
25- 50 7.780e-09 5.015e-09
50-150 1.706e-08 1.101e-08
15-150 2.889e-08 1.925e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 27.2514 ( )
R1^2/D10^2 : 3.12853E-03 (-0.00309837 -0.00309837)
kT2 [keV] : 56.7834 (-59.17 -59.17)
R2^2/D10^2 : 1.26604E-03 (-0.00104098 -0.00104098)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.97 using 59 PHA bins.
#Fit statistic : Chi-Squared = 52.95 using 59 PHA bins.
# Reduced chi-squared = 0.9632 for 55 degrees of freedom
# Reduced chi-squared = 0.9628 for 55 degrees of freedom
# Null hypothesis probability = 5.523987e-01
# Null hypothesis probability = 5.532881e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 0.525033 ( -0.375533 0.337895 )
Norm@50keV : 9.85348E-03 ( -0.00230442 0.00221817 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.37 using 59 PHA bins.
# Reduced chi-squared = 1.147 for 57 degrees of freedom
# Null hypothesis probability = 2.089210e-01
Photon flux (15-150 keV) in 0.392 sec: 1.16240 ( -0.238018 0.239896 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12434e-08 ( -1.03547e-08 1.03891e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.04460 ( -2.98163 1.69169 )
Epeak [keV] : 134.488 ( -43.6445 -134.261 )
Norm@50keV : 3.45684E-02 ( -0.035096 0.227518 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.13 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 56 degrees of freedom
# Null hypothesis probability = 2.390300e-01
Photon flux (15-150 keV) in 0.392 sec: 1.10566 ( -0.24261 0.24836 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.04872e-08 ( -1.09341e-08 1.07808e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.06431 ( -0.581677 3.81088 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 134.219 ( -32.7608 145.262 )
Norm@50keV : 3.51053E-02 ( -0.0351051 0.227998 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.12 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 55 degrees of freedom
# Null hypothesis probability = 2.111647e-01
Photon flux (15-150 keV) in 0.392 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) = 6.71e-09
S(50-100 keV) = 1.87e-08
T90 vs. Hardness ratio plot
T90 = 0.339999973773956 sec.
Hardness ratio (energy fluence ratio) = 2.78689
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.15683
Count Ratio (50-100 keV) / (15-25 keV) = 3.99817
Mask shadow pattern
IMX = -2.383069636509457E-01, IMY = -2.059508394812140E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
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:
-87.899390 -0.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6195 35.3750 4.3 39.3 50.8 0.7178 2.7 8.2 Her X-1
172.2052 14.7761 2.6 47.3 176.7 1.0760 4.4 ------ UNKNOWN
147.7925 16.5925 3.3 57.6 -156.3 2.3723 3.5 ------ UNKNOWN
140.2915 28.8165 3.0 52.1 -140.5 2.0541 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.040000 0.352000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6122 35.2948 23.8 39.4 50.9 0.0098 0.5 8.1 Her X-1
201.7989 37.5988 1.3 17.5 139.2 0.0696 8.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
48.500590 962.466100
1325.400000 1465.093700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5725 35.4153 8.2 41.9 35.1 1.6664 1.4 7.1 Her X-1
246.8055 67.5193 2.7 38.9 -15.7 3.1465 4.3 ------ UNKNOWN
184.5726 40.3347 3.1 13.6 -114.3 2.2567 3.7 ------ UNKNOWN
164.2212 36.1712 3.0 29.9 -122.3 2.9754 3.8 ------ UNKNOWN
152.7545 -0.0592 5.3 58.8 -159.2 12.6602 2.2 ------ UNKNOWN
155.1087 17.1648 3.1 45.6 -144.7 5.8526 3.7 ------ UNKNOWN
310.2279 76.7469 3.6 57.6 -26.3 12.6000 3.3 ------ UNKNOWN
314.3524 75.9210 3.3 58.8 -26.0 16.3225 3.5 ------ UNKNOWN
Plot creation:
Sat May 30 13:26:16 EDT 2015