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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
82.9607 -5.3753 0.0097 33.3861 -140.5415 1.8316622 19.960 TRIG_00650977
Foreground time interval of the image:
-30.160 9.717 (delta_t = 39.877 [sec])
Background time interval of the image:
-239.584 -30.160 (delta_t = 209.424 [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 0.256000
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 0.256000
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 0.256000
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 -30.160 sec. to 433.944 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.79645 ( -0.135584 0.138793 )
Norm@50keV : 6.89691E-04 ( -5.53153e-05 5.45356e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.27 using 59 PHA bins.
# Reduced chi-squared = 0.8820 for 57 degrees of freedom
# Null hypothesis probability = 7.235761e-01
Photon flux (15-150 keV) in 464.1 sec: 9.49074E-02 ( -0.00688214 0.00689532 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.94709e-06 ( -2.40491e-07 2.42874e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -30.160 sec. to 433.944 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80099 ( -0.153843 0.135978 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 6.88401E-04 ( -0.000356316 0.000400762 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.28 using 59 PHA bins.
# Reduced chi-squared = 0.8979 for 56 degrees of freedom
# Null hypothesis probability = 6.901256e-01
Photon flux (15-150 keV) in 464.1 sec: 9.49147E-02 ( -0.0069276 0.0068453 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.94404e-06 ( -2.43546e-07 2.41527e-07 ) ergs/cm2
Band function
Time interval is from -30.160 sec. to 433.944 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.44669 ( 1.46242 1.46242 )
beta : -1.79601 ( -0.138935 0.13549 )
Epeak [keV] : 22.4852 ( -19.4256 -19.4256 )
Norm@50keV : 1.51847E-03 ( -0.000687997 0.0996147 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.27 using 59 PHA bins.
# Reduced chi-squared = 0.9141 for 55 degrees of freedom
# Null hypothesis probability = 6.554343e-01
Photon flux (15-150 keV) in 464.1 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] : 12.0809 (-1.16535 1.307)
R^2/D10^2 : 2.12221E-02 (-0.00670301 0.00972755)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 113.87 using 59 PHA bins.
# Reduced chi-squared = 1.9977 for 57 degrees of freedom
# Null hypothesis probability = 1.153706e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.042e-07 3.982e-08
25- 50 9.649e-07 8.307e-08
50-150 8.506e-07 1.390e-07
15-150 2.120e-06 2.072e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 105.870 (-25.6924 52.1897)
Norm : 0.411460 (-0.0424161 0.0439392)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.43 using 59 PHA bins.
# Reduced chi-squared = 0.9550 for 57 degrees of freedom
# Null hypothesis probability = 5.719912e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.990e-07 6.012e-08
25- 50 8.726e-07 7.565e-08
50-150 1.459e-06 4.527e-07
15-150 2.831e-06 5.511e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.62039 (-1.21351 1.40938)
R1^2/D10^2 : 0.264535 (-0.147891 0.448589)
kT2 [keV] : 22.7337 (-4.47869 7.97755)
R2^2/D10^2 : 1.67705E-03 (-0.00110225 0.00218087)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.06 using 59 PHA bins.
# Reduced chi-squared = 0.9830 for 55 degrees of freedom
# Null hypothesis probability = 5.104239e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.396e-07 1.568e-07
25- 50 7.970e-07 1.636e-07
50-150 1.554e-06 4.864e-07
15-150 2.890e-06 7.245e-07
Peak spectrum fit
Power-law model
Time interval is from 9.324 sec. to 10.324 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81896 ( -0.152411 0.157302 )
Norm@50keV : 1.83577E-02 ( -0.00184075 0.00181407 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.32 using 59 PHA bins.
# Reduced chi-squared = 1.111 for 57 degrees of freedom
# Null hypothesis probability = 2.633432e-01
Photon flux (15-150 keV) in 1 sec: 2.54847 ( -0.227816 0.22798 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68902e-07 ( -1.7048e-08 1.72167e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 9.324 sec. to 10.324 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33124 ( -0.72684 0.573818 )
Epeak [keV] : 61.8843 ( -17.2128 -61.8856 )
Norm@50keV : 3.40813E-02 ( -0.0165981 0.0513671 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.49 using 59 PHA bins.
# Reduced chi-squared = 1.098 for 56 degrees of freedom
# Null hypothesis probability = 2.860653e-01
Photon flux (15-150 keV) in 1 sec: 2.50634 ( -0.23493 0.23399 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62332e-07 ( -1.9154e-08 1.9181e-08 ) ergs/cm2
Band function
Time interval is from 9.324 sec. to 10.324 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.04691 ( 1.04324 5.82398 )
beta : -2.19083 ( 2.18796 0.43809 )
Epeak [keV] : 50.7572 ( -50.3275 -50.3275 )
Norm@50keV : 5.12323E-02 ( -0.0523473 1588.94 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.81 using 59 PHA bins.
# Reduced chi-squared = 1.106 for 55 degrees of freedom
# Null hypothesis probability = 2.746048e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62531e-07 ( -1.62524e-07 -1.8385e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.3956 (-1.14767 1.29935)
R^2/D10^2 : 0.745085 (-0.249057 0.366168)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.51 using 59 PHA bins.
# Reduced chi-squared = 1.518 for 57 degrees of freedom
# Null hypothesis probability = 7.066992e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.034e-08 2.955e-09
25- 50 6.015e-08 6.605e-09
50-150 4.530e-08 9.470e-09
15-150 1.258e-07 1.310e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 96.0306 (-25.679 43.8107)
Norm : 11.4132 (-1.38271 1.62776)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.45 using 59 PHA bins.
# Reduced chi-squared = 1.078 for 57 degrees of freedom
# Null hypothesis probability = 3.198728e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.982e-08 4.225e-09
25- 50 5.114e-08 5.005e-09
50-150 8.096e-08 3.161e-08
15-150 1.619e-07 3.285e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.60132 (-2.3021 2.58414)
R1^2/D10^2 : 3.80740 (-2.36549 13.0563)
kT2 [keV] : 21.7637 (-6.90724 26.147)
R2^2/D10^2 : 4.62258E-02 (-0.0409249 0.170391)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.17 using 59 PHA bins.
# Reduced chi-squared = 1.149 for 55 degrees of freedom
# Null hypothesis probability = 2.099985e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.905e-08 9.860e-09
25- 50 5.184e-08 1.962e-08
50-150 7.975e-08 4.304e-08
15-150 1.606e-07 5.777e-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: 1.93122 ( -0.147604 0.15226 )
Norm@50keV : 2.75901E-03 ( -0.000251111 0.00024627 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.52 using 59 PHA bins.
# Reduced chi-squared = 0.9214 for 57 degrees of freedom
# Null hypothesis probability = 6.435753e-01
Photon flux (15-150 keV) in 39.88 sec: 0.401294 ( -0.030993 0.0310664 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01206e-06 ( -8.88411e-08 8.98357e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07417 ( -0.445555 0.0355918 )
Epeak [keV] : 34.1534 ( )
Norm@50keV : 2.31131E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.07 using 59 PHA bins.
# Reduced chi-squared = 0.9298 for 56 degrees of freedom
# Null hypothesis probability = 6.245168e-01
Photon flux (15-150 keV) in 39.88 sec: 0.401141 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0081e-06 ( -4.34413e-08 9.19473e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.45950 ( 1.4594 6.367 )
beta : -1.94260 ( 1.94283 0.157329 )
Epeak [keV] : 26.7851 ( -26.2999 -26.2999 )
Norm@50keV : 6.38574E-03 ( -0.00303949 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.45 using 59 PHA bins.
# Reduced chi-squared = 0.9537 for 55 degrees of freedom
# Null hypothesis probability = 5.724678e-01
Photon flux (15-150 keV) in 39.88 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) = 8.29e-07
S(50-100 keV) = 9.54e-07
T90 vs. Hardness ratio plot
T90 = 408.707999944687 sec.
Hardness ratio (energy fluence ratio) = 1.15078
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.05976
Count Ratio (50-100 keV) / (15-25 keV) = 0.699137
Mask shadow pattern
IMX = -5.088279037210258E-01, IMY = 4.188262261616247E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.584000 -30.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5630 -40.5356 2.0 44.4 -39.1 1.8918 5.6 1.9 Vela X-1
103.7777 -3.5790 2.7 42.4 -109.6 3.2363 4.3 ------ UNKNOWN
104.1965 -3.8650 3.3 42.4 -108.8 2.6177 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-30.160000 9.716590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5185 -40.4758 6.7 44.4 -39.2 -0.2534 -1.7 4.8 Vela X-1
30.2486 -14.1890 2.6 47.8 136.0 1.3534 4.4 ------ UNKNOWN
37.8865 -2.7494 2.6 50.4 153.8 1.3832 4.5 ------ UNKNOWN
38.8438 1.9109 2.9 53.5 158.5 1.6034 4.0 ------ UNKNOWN
59.9911 -7.1825 2.3 34.8 178.0 0.4353 5.0 ------ UNKNOWN
82.9607 -5.3753 0.6 33.4 -140.5 1.8318 20.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
62.716580 962.459200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6294 22.0118 0.2 27.4 -151.4 36.0501 57.1 0.3 Crab
135.5623 -40.5534 5.5 58.6 -17.8 7.2764 2.1 1.5 Vela X-1
62.5719 -48.5928 3.8 46.5 45.7 7.4909 3.0 ------ UNKNOWN
57.6185 -30.7269 3.4 34.7 67.4 4.7678 3.4 ------ UNKNOWN
69.4350 7.9832 3.0 19.0 161.9 2.3438 3.9 ------ UNKNOWN
82.9365 -5.4220 2.0 0.0 65.1 3.4084 5.8 ------ UNKNOWN
Plot creation:
Sun Aug 30 19:03:21 EDT 2015