Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
135.6447 -40.4686 0.0158 6.2 -177.0 2.8973 12.2 TRIG_00725983
------------------------------------------
Foreground time interval of the image:
0.000 344.000 (delta_t = 344.000 [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
Time interval is from 0.000 sec. to 344.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.51516 ( -0.244519 0.269422 )
Norm@50keV : 3.15181E-04 ( -6.45879e-05 6.51388e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.89 using 59 PHA bins.
# Reduced chi-squared = 0.9630 for 57 degrees of freedom
# Null hypothesis probability = 5.546127e-01
Photon flux (15-150 keV) in 344 sec: 6.24951E-02 ( -0.0073494 0.00735395 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08865e-06 ( -1.63311e-07 1.71335e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 344.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.362755 ( -2.04957 1.55569 )
Epeak [keV] : 23.9570 ( )
Norm@50keV : 9.04387E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.84 using 59 PHA bins.
# Reduced chi-squared = 0.8722 for 56 degrees of freedom
# Null hypothesis probability = 7.400518e-01
Photon flux (15-150 keV) in 344 sec: 6.00274E-02 ( -0.0071931 0.0072651 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.15855e-07 ( -1.36702e-07 1.67858e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 344.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.241544 ( -1.02347 0.57339 )
beta : -3.81177 ( 4.09078 1.46658 )
Epeak [keV] : 23.8301 ( -10.2216 4.98919 )
Norm@50keV : 1.12673E-02 ( -0.0122448 71.558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.68 using 59 PHA bins.
# Reduced chi-squared = 0.8851 for 55 degrees of freedom
# Null hypothesis probability = 7.132486e-01
Photon flux (15-150 keV) in 344 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.64229e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 6.80398 (-0.783389 0.873613)
R^2/D10^2 : 0.136381 (-0.0542043 0.0920651)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.64 using 59 PHA bins.
# Reduced chi-squared = 0.9060 for 57 degrees of freedom
# Null hypothesis probability = 6.756759e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.385e-07 6.675e-08
25- 50 4.384e-07 8.509e-08
50-150 6.548e-08 2.871e-08
15-150 8.424e-07 1.428e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 28.3595 (-6.64918 9.51176)
Norm : 0.532079 (-0.120153 0.164049)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.81 using 59 PHA bins.
# Reduced chi-squared = 0.8738 for 57 degrees of freedom
# Null hypothesis probability = 7.392669e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.615e-07 5.308e-08
25- 50 4.002e-07 6.811e-08
50-150 2.033e-07 9.131e-08
15-150 9.650e-07 1.655e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.81248 (-4.81156 -4.81248)
R1^2/D10^2 : 0.353622 (-0.314678 -0.353622)
kT2 [keV] : 10.1327 (-9.92483 -10.1327)
R2^2/D10^2 : 1.44706E-02 (-0.0144313 0.124242)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.65 using 59 PHA bins.
# Reduced chi-squared = 0.8846 for 55 degrees of freedom
# Null hypothesis probability = 7.143092e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.578e-07 2.030e-07
25- 50 4.151e-07 2.190e-07
50-150 1.486e-07 8.777e-08
15-150 9.215e-07 4.715e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 344.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.51516 ( -0.244519 0.269422 )
Norm@50keV : 3.15181E-04 ( -6.45879e-05 6.51388e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.89 using 59 PHA bins.
# Reduced chi-squared = 0.9630 for 57 degrees of freedom
# Null hypothesis probability = 5.546127e-01
Photon flux (15-150 keV) in 344 sec: 6.24951E-02 ( -0.0073494 0.00735395 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08865e-06 ( -1.63311e-07 1.71335e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 344.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.362755 ( -2.04957 1.55569 )
Epeak [keV] : 23.9570 ( )
Norm@50keV : 9.04387E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.84 using 59 PHA bins.
# Reduced chi-squared = 0.8722 for 56 degrees of freedom
# Null hypothesis probability = 7.400518e-01
Photon flux (15-150 keV) in 344 sec: 6.00274E-02 ( -0.0071931 0.0072651 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.15855e-07 ( -1.36702e-07 1.67858e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 344.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.241544 ( -1.02347 0.57339 )
beta : -3.81177 ( 4.09078 1.46658 )
Epeak [keV] : 23.8301 ( -10.2216 4.98919 )
Norm@50keV : 1.12673E-02 ( -0.0122448 71.5614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.68 using 59 PHA bins.
# Reduced chi-squared = 0.8851 for 55 degrees of freedom
# Null hypothesis probability = 7.132486e-01
Photon flux (15-150 keV) in 344 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.64229e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 6.80398 (-0.783389 0.873613)
R^2/D10^2 : 0.136381 (-0.0542043 0.0920651)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.64 using 59 PHA bins.
# Reduced chi-squared = 0.9060 for 57 degrees of freedom
# Null hypothesis probability = 6.756759e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.385e-07 6.156e-08
25- 50 4.384e-07 8.495e-08
50-150 6.548e-08 2.844e-08
15-150 8.424e-07 1.422e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 28.3595 (-6.64918 9.51176)
Norm : 0.532079 (-0.120153 0.164049)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.81 using 59 PHA bins.
# Reduced chi-squared = 0.8738 for 57 degrees of freedom
# Null hypothesis probability = 7.392669e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.615e-07 5.550e-08
25- 50 4.002e-07 6.792e-08
50-150 2.033e-07 8.937e-08
15-150 9.650e-07 1.705e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.81248 (-4.81171 -4.81248)
R1^2/D10^2 : 0.353622 (-0.314678 -0.353622)
kT2 [keV] : 10.1327 (-9.85757 -10.1327)
R2^2/D10^2 : 1.44706E-02 (-0.0144313 0.124242)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.65 using 59 PHA bins.
# Reduced chi-squared = 0.8846 for 55 degrees of freedom
# Null hypothesis probability = 7.143092e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.578e-07 2.083e-07
25- 50 4.151e-07 2.188e-07
50-150 1.486e-07 8.421e-08
15-150 9.215e-07 4.790e-07
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: 2.51516 ( -0.244519 0.269422 )
Norm@50keV : 3.15181E-04 ( -6.45879e-05 6.51388e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.89 using 59 PHA bins.
# Reduced chi-squared = 0.9630 for 57 degrees of freedom
# Null hypothesis probability = 5.546127e-01
Photon flux (15-150 keV) in 344 sec: 6.24951E-02 ( -0.0073494 0.00735395 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08865e-06 ( -1.63311e-07 1.71335e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.362755 ( -2.04957 1.55569 )
Epeak [keV] : 23.9570 ( )
Norm@50keV : 9.04387E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.84 using 59 PHA bins.
# Reduced chi-squared = 0.8722 for 56 degrees of freedom
# Null hypothesis probability = 7.400518e-01
Photon flux (15-150 keV) in 344 sec: 6.00274E-02 ( -0.0071931 0.0072651 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.15855e-07 ( -1.36702e-07 1.67858e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.241544 ( -1.02347 0.57339 )
beta : -3.81177 ( 4.09078 1.46658 )
Epeak [keV] : 23.8301 ( -10.2216 4.98919 )
Norm@50keV : 1.12673E-02 ( -0.0122448 71.5729 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.68 using 59 PHA bins.
# Reduced chi-squared = 0.8851 for 55 degrees of freedom
# Null hypothesis probability = 7.132486e-01
Photon flux (15-150 keV) in 344 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.64229e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.62e-07
S(50-100 keV) = 2.53e-07
T90 vs. Hardness ratio plot
T90 = 344 sec.
Hardness ratio (energy fluence ratio) = 0.698895
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.762427
Count Ratio (50-100 keV) / (15-25 keV) = 0.132386
Mask shadow pattern
IMX = -1.081805683408513E-01, IMY = 5.638747778110085E-03
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 344.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6301 -40.4763 1.0 6.2 -177.0 2.8763 12.1 6.6 Vela X-1
170.3958 -60.5259 2.1 28.8 -88.6 2.3459 5.5 6.3 Cen X-3
186.8418 -62.6467 5.2 36.8 -86.9 1.8356 2.2 9.0 GX 301-2
67.9946 -30.4018 3.4 49.5 38.0 5.2538 3.4 ------ UNKNOWN
137.6577 5.0481 3.0 50.2 144.0 5.2169 3.9 ------ UNKNOWN
76.0990 -61.5865 3.3 34.9 -4.8 1.1513 3.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
386.400610 643.720000
645.000000 963.049900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5064 -40.5894 0.9 0.1 11.4 4.3540 12.6 2.3 Vela X-1
170.2838 -60.5648 1.5 29.2 -72.0 4.4044 7.8 3.6 Cen X-3
186.7325 -62.7088 3.3 37.2 -73.1 3.5751 3.4 4.2 GX 301-2
77.2774 -44.1934 2.8 42.4 27.9 2.8582 4.1 ------ UNKNOWN
141.5173 -58.8475 2.7 18.7 -46.5 1.8296 4.2 ------ UNKNOWN
188.3680 -49.0404 3.3 37.6 -95.8 4.0881 3.5 ------ UNKNOWN
233.8450 -84.0116 2.8 50.6 -44.7 8.6867 4.2 ------ UNKNOWN
Plot creation:
Sat Dec 10 01:38:04 EST 2016