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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
256.0576 -42.5459 0.1325 4.6 141.9 0.2051 1.4 TRIG_00557910
------------------------------------------
Foreground time interval of the image:
0.000 49.271 (delta_t = 49.271 [sec])
60.000 122.000 (delta_t = 62.000 [sec])
361.000 423.080 (delta_t = 62.080 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 49.270500
60.000000 122.000000
361.000000 423.080000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.74129 ( -2.73831 -2.73831 )
Norm@50keV : 3.43884E-05 ( -3.44066e-05 6.49496e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8029 for 57 degrees of freedom
# Null hypothesis probability = 8.569526e-01
Photon flux (15-150 keV) in 173.4 sec: 7.88460E-03 ( -0.0078846 0.00826508 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.43963e-08 ( -6.43963e-08 9.41911e-08 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 49.270500
60.000000 122.000000
361.000000 423.080000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.51372 ( )
Epeak [keV] : 24.7446 ( )
Norm@50keV : 1.25386 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.94 using 59 PHA bins.
# Reduced chi-squared = 0.7847 for 56 degrees of freedom
# Null hypothesis probability = 8.788010e-01
Photon flux (15-150 keV) in 173.4 sec: 9.80346E-03 ( -0.00695797 0.00699484 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.67708e-08 ( -4.74795e-08 4.8359e-08 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 49.270500
60.000000 122.000000
361.000000 423.080000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.44894 ( 9.44894 9.44894 )
beta : -2.73825 ( 2.73907 2.73907 )
Epeak [keV] : 45.4799 ( -45.4799 -45.4799 )
Norm@50keV : 4.68044E-03 ( -0.0046782 0.0088324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8321 for 55 degrees of freedom
# Null hypothesis probability = 8.079630e-01
Photon flux (15-150 keV) in 173.4 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] : 5.95950 (-2.9444 7.09268)
R^2/D10^2 : 3.78025E-02 (-0.0388008 0.748151)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.35 using 59 PHA bins.
# Reduced chi-squared = 0.7781 for 57 degrees of freedom
# Null hypothesis probability = 8.891816e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.063e-08 2.087e-08
25- 50 3.010e-08 2.480e-08
50-150 2.681e-09 3.005e-09
15-150 6.341e-08 5.358e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 20.3976 (-21.3564 -21.3564)
Norm : 0.101803 (-0.101492 1.91229)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.21 using 59 PHA bins.
# Reduced chi-squared = 0.7932 for 57 degrees of freedom
# Null hypothesis probability = 8.701902e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.783e-08 2.181e-08
25- 50 2.474e-08 2.366e-08
50-150 7.659e-09 1.171e-08
15-150 6.024e-08 5.152e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.83911 (-5.92063 -5.92063)
R1^2/D10^2 : 3.42128E-02 (-0.0338502 -0.0338502)
kT2 [keV] : 6.04508 (-5.82397 -5.82397)
R2^2/D10^2 : 6.20513E-03 (-0.00581317 -0.00581317)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.35 using 59 PHA bins.
# Reduced chi-squared = 0.8064 for 55 degrees of freedom
# Null hypothesis probability = 8.472733e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.110e-08 1.011e-01
25- 50 2.961e-08 8.835e-01
50-150 2.490e-09 2.080e+01
15-150 6.320e-08 2.033e+01
Peak spectrum fit
Power-law model
Time interval is from 361.000 sec. to 423.080 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.74129 ( -2.73831 -2.73831 )
Norm@50keV : 3.43884E-05 ( -3.44066e-05 6.49496e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8029 for 57 degrees of freedom
# Null hypothesis probability = 8.569526e-01
Photon flux (15-150 keV) in 173.4 sec: 7.88460E-03 ( -0.0078846 0.00826508 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.43963e-08 ( -6.43963e-08 9.41911e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 361.000 sec. to 423.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.51372 ( )
Epeak [keV] : 24.7446 ( )
Norm@50keV : 1.25386 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.94 using 59 PHA bins.
# Reduced chi-squared = 0.7847 for 56 degrees of freedom
# Null hypothesis probability = 8.788010e-01
Photon flux (15-150 keV) in 173.4 sec: 9.80346E-03 ( -0.00695797 0.00699484 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.67708e-08 ( -4.74795e-08 4.8359e-08 ) ergs/cm2
Band function
Time interval is from 361.000 sec. to 423.080 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.44894 ( 9.44894 9.44894 )
beta : -2.73825 ( 2.73907 2.73907 )
Epeak [keV] : 45.4799 ( -45.4799 -45.4799 )
Norm@50keV : 4.68044E-03 ( -0.0046782 0.0088324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8321 for 55 degrees of freedom
# Null hypothesis probability = 8.079630e-01
Photon flux (15-150 keV) in 173.4 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] : 5.95950 (-2.9444 7.09268)
R^2/D10^2 : 3.78025E-02 (-0.0388008 0.748151)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.35 using 59 PHA bins.
# Reduced chi-squared = 0.7781 for 57 degrees of freedom
# Null hypothesis probability = 8.891816e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.063e-08 2.433e-08
25- 50 3.010e-08 2.266e-08
50-150 2.681e-09 3.059e-09
15-150 6.341e-08 4.615e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 20.3976 (-21.3564 -21.3564)
Norm : 0.101803 (-0.101492 1.91229)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.21 using 59 PHA bins.
# Reduced chi-squared = 0.7932 for 57 degrees of freedom
# Null hypothesis probability = 8.701902e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.783e-08 2.099e-08
25- 50 2.474e-08 1.983e-08
50-150 7.659e-09 1.053e-08
15-150 6.024e-08 5.214e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.83911 (-5.92063 -5.92063)
R1^2/D10^2 : 3.42128E-02 (-0.0338502 -0.0338502)
kT2 [keV] : 6.04508 (-5.82397 -5.82397)
R2^2/D10^2 : 6.20513E-03 (-0.00581317 -0.00581317)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.35 using 59 PHA bins.
# Reduced chi-squared = 0.8064 for 55 degrees of freedom
# Null hypothesis probability = 8.472733e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.110e-08 9.303e-02
25- 50 2.961e-08 8.602e-01
50-150 2.490e-09 2.148e+01
15-150 6.320e-08 2.276e+01
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: 2.74129 ( -2.73831 -2.73831 )
Norm@50keV : 3.43884E-05 ( -3.44066e-05 6.49496e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8029 for 57 degrees of freedom
# Null hypothesis probability = 8.569526e-01
Photon flux (15-150 keV) in 173.4 sec: 7.88460E-03 ( -0.0078846 0.00826508 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.43963e-08 ( -6.43963e-08 9.41911e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.51372 ( )
Epeak [keV] : 24.7446 ( )
Norm@50keV : 1.25386 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.94 using 59 PHA bins.
# Reduced chi-squared = 0.7847 for 56 degrees of freedom
# Null hypothesis probability = 8.788010e-01
Photon flux (15-150 keV) in 173.4 sec: 9.80346E-03 ( -0.00695797 0.00699484 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.67708e-08 ( -4.74795e-08 4.8359e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.44894 ( 9.44894 9.44894 )
beta : -2.73825 ( 2.73907 2.73907 )
Epeak [keV] : 45.4799 ( -45.4799 -45.4799 )
Norm@50keV : 4.68044E-03 ( -0.0046782 0.0088324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8321 for 55 degrees of freedom
# Null hypothesis probability = 8.079630e-01
Photon flux (15-150 keV) in 173.4 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) = 2.16434e-08
S(50-100 keV) = 1.29688e-08
T90 vs. Hardness ratio plot
T90 = 648 sec.
Hardness ratio (energy fluence ratio) = 0.599203
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.429171
Count Ratio (50-100 keV) / (15-25 keV) = 0.0592586
Mask shadow pattern
IMX = -6.290867618276523E-02, IMY = -4.929311036698768E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 49.270500
60.000000 122.000000
361.000000 423.080000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4165 -60.5997 30.7 47.4 -46.6 0.2083 0.4 3.3 Cen X-3
186.6744 -62.7285 4.3 39.4 -47.0 0.6471 2.7 2.6 GX 301-2
244.9922 -15.6140 0.9 30.5 80.2 3.3166 12.6 1.7 Sco X-1
256.0183 -37.9390 5.6 8.4 118.4 0.2673 2.1 5.9 4U 1700-377
256.6256 -36.4606 6.2 10.0 117.6 0.2443 1.9 9.5 GX 349+2
263.1697 -24.7547 8.8 22.9 120.8 0.2363 1.3 8.8 GX 1+4
264.9058 -44.2745 0.0 9.7 179.2 0.1895 1.4 12.6 4U 1735-44
270.3215 -24.9420 3.6 25.7 135.2 0.5375 3.2 8.5 GX 5-1
270.2443 -25.7607 10.6 25.0 136.0 0.1870 1.1 3.3 GRS 1758-258
273.8742 -14.0222 4.3 36.9 130.6 0.8801 2.7 7.7 GX 17+2
276.0156 -30.4078 9.3 24.5 152.5 0.1959 1.2 5.3 H1820-303
284.8183 -24.8495 85.8 33.9 156.0 0.0284 0.1 12.6 HT1900.1-2455
263.1140 -33.7650 3.5 14.9 133.7 0.4928 3.3 7.5 GX 354-0
290.0780 -8.1928 2.0 50.1 146.2 4.1265 5.8 ------ UNKNOWN
203.0838 -43.5200 2.5 33.9 -11.9 0.7580 4.6 ------ UNKNOWN
329.4936 -34.0000 3.4 58.8 -159.3 3.2812 3.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
802.900600 934.547600
936.000000 963.018400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3409 -60.6305 11.1 47.8 0.5 -1.8504 -1.0 0.9 Cen X-3
186.6950 -62.8273 7.5 43.5 10.0 2.6838 1.5 3.6 GX 301-2
264.6390 -44.5937 5.9 37.6 83.7 -7.2809 -2.0 9.7 4U 1735-44
249.5687 -47.1524 3.6 40.5 67.2 11.8716 3.2 ------ UNKNOWN
263.6055 -58.6575 2.6 26.2 67.6 6.3779 4.5 ------ UNKNOWN
278.2582 -73.4976 2.5 13.7 37.4 4.9091 4.6 ------ UNKNOWN
153.3788 -52.5582 2.6 57.2 -9.6 19.1790 4.5 ------ UNKNOWN
55.0218 -68.6726 2.9 29.8 -65.0 5.4578 4.0 ------ UNKNOWN
125.7714 -52.7033 3.3 56.8 -29.5 21.0052 3.6 ------ UNKNOWN
Plot creation:
Sun Jul 7 23:44:47 EDT 2013