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
230.3409 68.3430 0.0087 43.9202 -149.4753 3.9481260 22.248 TRIG_00652603
Foreground time interval of the image:
-25.256 13.365 (delta_t = 38.621 [sec])
Background time interval of the image:
-65.635 -25.256 (delta_t = 40.379 [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 -25.256 sec. to 176.020 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87493 ( -0.090832 0.092134 )
Norm@50keV : 2.30203E-03 ( -0.000116681 0.000115771 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.52 using 59 PHA bins.
# Reduced chi-squared = 0.9741 for 57 degrees of freedom
# Null hypothesis probability = 5.306093e-01
Photon flux (15-150 keV) in 201.3 sec: 0.326905 ( -0.0159337 0.0160008 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.26001e-06 ( -2.14868e-07 2.15969e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -25.256 sec. to 176.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87355 ( -0.0910775 0.402178 )
Epeak [keV] : 9999.23 ( -9999.34 -9999.35 )
Norm@50keV : 2.30496E-03 ( -0.000117192 0.000801217 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.53 using 59 PHA bins.
# Reduced chi-squared = 0.9916 for 56 degrees of freedom
# Null hypothesis probability = 4.926999e-01
Photon flux (15-150 keV) in 201.3 sec: 0.326750 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.25866e-06 ( -2.22296e-07 2.13922e-07 ) ergs/cm2
Band function
Time interval is from -25.256 sec. to 176.020 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.94920 ( -4.9492 -4.9492 )
beta : -1.89945 ( -0.106919 0.095567 )
Epeak [keV] : 20.0147 ( -20.0147 3.47238 )
Norm@50keV : 1269.61 ( -58.1639 2.38528e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.68 using 59 PHA bins.
# Reduced chi-squared = 0.9941 for 55 degrees of freedom
# Null hypothesis probability = 4.869755e-01
Photon flux (15-150 keV) in 201.3 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] : 12.0254 ( )
R^2/D10^2 : 7.16393E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 204.13 using 59 PHA bins.
# Reduced chi-squared = 3.5813 for 57 degrees of freedom
# Null hypothesis probability = 1.962897e-18
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.411e-07 3.905e-08
25- 50 1.392e-06 8.314e-08
50-150 1.212e-06 1.369e-07
15-150 3.045e-06 1.671e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.4304 (-16.347 22.1698)
Norm : 1.41456 (-0.102027 0.11411)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.41 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 57 degrees of freedom
# Null hypothesis probability = 2.078288e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.441e-07 6.693e-08
25- 50 1.280e-06 7.408e-08
50-150 2.044e-06 5.495e-07
15-150 4.068e-06 5.797e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.93506 (-0.705126 0.774542)
R1^2/D10^2 : 0.793101 (-0.300266 0.531993)
kT2 [keV] : 24.1545 (-3.23564 4.4519)
R2^2/D10^2 : 4.26949E-03 (-0.00194712 0.00304886)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.83 using 59 PHA bins.
# Reduced chi-squared = 0.9970 for 55 degrees of freedom
# Null hypothesis probability = 4.809777e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.242e-07 1.197e-07
25- 50 1.210e-06 1.210e-07
50-150 2.210e-06 3.740e-07
15-150 4.244e-06 5.737e-07
Peak spectrum fit
Power-law model
Time interval is from 1.568 sec. to 2.568 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97822 ( -0.263029 0.282286 )
Norm@50keV : 1.58532E-02 ( -0.00276815 0.00266936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.20 using 59 PHA bins.
# Reduced chi-squared = 1.056 for 57 degrees of freedom
# Null hypothesis probability = 3.608438e-01
Photon flux (15-150 keV) in 1 sec: 2.35447 ( -0.334413 0.334937 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46043e-07 ( -2.37899e-08 2.42679e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.568 sec. to 2.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.92188 ( -1.04558 0.298119 )
Epeak [keV] : 62.3145 ( )
Norm@50keV : 1.70320E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.19 using 59 PHA bins.
# Reduced chi-squared = 1.075 for 56 degrees of freedom
# Null hypothesis probability = 3.268249e-01
Photon flux (15-150 keV) in 1 sec: 2.35294 ( -0.34824 0.3332 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45407e-07 ( -2.6256e-08 2.4661e-08 ) ergs/cm2
Band function
Time interval is from 1.568 sec. to 2.568 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.91571 ( -1.10169 0.985647 )
beta : -9.35079 ( 9.37142 19.3714 )
Epeak [keV] : 71.9801 ( -71.0863 -71.0863 )
Norm@50keV : 1.70029E-02 ( -0.00238406 5.22986e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.19 using 59 PHA bins.
# Reduced chi-squared = 1.094 for 55 degrees of freedom
# Null hypothesis probability = 2.935206e-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] : 10.4919 (-1.77952 2.22239)
R^2/D10^2 : 0.883823 (-0.460227 0.928673)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.13 using 59 PHA bins.
# Reduced chi-squared = 1.336 for 57 degrees of freedom
# Null hypothesis probability = 4.610086e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.011e-08 5.235e-09
25- 50 5.342e-08 1.174e-08
50-150 3.198e-08 1.146e-08
15-150 1.055e-07 2.088e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 75.6452 (-27.9974 60.4163)
Norm : 11.1295 (-2.25907 3.05223)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.25 using 59 PHA bins.
# Reduced chi-squared = 1.075 for 57 degrees of freedom
# Null hypothesis probability = 3.260882e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.876e-08 5.810e-09
25- 50 4.670e-08 7.920e-09
50-150 6.343e-08 3.362e-08
15-150 1.389e-07 3.335e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.69459 (-1.75117 2.75624)
R1^2/D10^2 : 14.6946 (-11.977 117.564)
kT2 [keV] : 19.1274 (-6.02151 14.0362)
R2^2/D10^2 : 7.23045E-02 (-0.0625017 0.198068)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.80 using 59 PHA bins.
# Reduced chi-squared = 1.105 for 55 degrees of freedom
# Null hypothesis probability = 2.749841e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.277e-08 1.809e-08
25- 50 4.043e-08 1.765e-08
50-150 6.794e-08 3.916e-08
15-150 1.411e-07 6.579e-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: 1.81323 ( -0.101383 0.103118 )
Norm@50keV : 6.75039E-03 ( -0.000392885 0.000390253 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.91 using 59 PHA bins.
# Reduced chi-squared = 0.7880 for 57 degrees of freedom
# Null hypothesis probability = 8.769509e-01
Photon flux (15-150 keV) in 38.62 sec: 0.935002 ( -0.0535199 0.0536774 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.39899e-06 ( -1.41556e-07 1.42224e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54506 ( -0.411349 0.317885 )
Epeak [keV] : 84.4096 ( -28.6177 -84.4096 )
Norm@50keV : 9.21160E-03 ( -0.00272337 0.00544867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.47 using 59 PHA bins.
# Reduced chi-squared = 0.7763 for 56 degrees of freedom
# Null hypothesis probability = 8.890758e-01
Photon flux (15-150 keV) in 38.62 sec: 0.919265 ( -0.057562 0.057791 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35309e-06 ( -1.56701e-07 1.56538e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.54525 ( -0.331849 0.378133 )
beta : -10.00000 ( 10 20 )
Epeak [keV] : 84.4289 ( -24.7166 -84.4289 )
Norm@50keV : 9.20758E-03 ( -0.000497334 0.00545154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.47 using 59 PHA bins.
# Reduced chi-squared = 0.7904 for 55 degrees of freedom
# Null hypothesis probability = 8.691425e-01
Photon flux (15-150 keV) in 38.62 sec: 0.924133 ( ) 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) = 1.23e-06
S(50-100 keV) = 1.34e-06
T90 vs. Hardness ratio plot
T90 = 143.055999934673 sec.
Hardness ratio (energy fluence ratio) = 1.08943
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.09854
Count Ratio (50-100 keV) / (15-25 keV) = 0.678464
Mask shadow pattern
IMX = -8.295371942011757E-01, IMY = 4.891173970783941E-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:
-65.635410 -25.256000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6464 35.1880 4.1 48.7 139.2 1.0206 2.8 2.9 Cyg X-1
308.1259 41.0065 11.4 40.2 135.9 0.1841 1.0 3.3 Cyg X-3
326.3317 38.1535 0.0 35.0 113.9 0.0909 0.6 12.6 Cyg X-2
18.2349 14.8234 2.5 50.0 37.1 1.5215 4.6 ------ UNKNOWN
25.0579 40.8967 2.3 25.6 18.1 0.3499 5.1 ------ UNKNOWN
53.7720 53.1684 0.8 26.2 -35.8 1.1574 15.3 ------ UNKNOWN
185.6082 83.7154 2.8 32.2 -127.6 0.3891 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-25.256000 13.364600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6950 35.3150 11.7 48.6 139.3 0.4879 1.0 8.5 Cyg X-1
308.2968 40.9532 6.6 40.2 135.7 0.4259 1.7 8.5 Cyg X-3
326.1754 38.3176 23.2 35.0 114.2 -0.1051 -0.5 0.3 Cyg X-2
25.9093 14.3877 2.7 51.5 27.7 1.8573 4.3 ------ UNKNOWN
263.8408 75.0804 3.1 32.3 -155.8 0.4280 3.7 ------ UNKNOWN
230.3409 68.3430 0.5 43.9 -149.5 3.9475 22.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.764600 122.564600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3739 35.4386 3.9 35.5 147.2 0.3548 2.9 7.1 Her X-1
230.3302 68.3036 1.4 0.1 -124.2 0.5959 8.2 ------ UNKNOWN
221.5359 18.0965 2.4 50.6 -167.2 0.8546 4.8 ------ UNKNOWN
86.2547 49.7908 2.9 58.9 -24.4 1.8798 4.0 ------ UNKNOWN
Plot creation:
Wed Sep 30 11:11:22 EDT 2015