Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
76.9329 -32.8412 0.0268 43.6700 -174.1642 1.7990393 7.180 TRIG_00982201
Foreground time interval of the image:
18.448 65.980 (delta_t = 47.532 [sec])
Background time interval of the image:
-11.699 18.448 (delta_t = 30.147 [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 64.000000
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 64.000000
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 64.000000
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 18.448 sec. to 65.980 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.47473 ( -0.298945 0.340055 )
Norm@50keV : 1.71061E-03 ( -0.00041329 0.000407989 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.81 using 59 bins.
Reduced chi-squared = 0.751053
# Null hypothesis probability of 9.19e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 47.53 sec: 0.330961 ( -0.047237 0.047228 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.07806e-07 ( -1.4324e-07 1.49913e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 18.448 sec. to 65.980 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25114 ( -2.25513 0.745727 )
Epeak [keV] : 21.5296 ( -18.9323 11.3201 )
Norm@50keV : 1.02970E-02 ( -0.0103021 0.315025 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.95 using 59 bins.
Reduced chi-squared = 0.73125
# Null hypothesis probability of 9.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 47.53 sec: 0.319775 ( -0.048422 0.048897 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24647e-07 ( -1.41635e-07 1.74453e-07 ) ergs/cm2
Band function
Time interval is from 18.448 sec. to 65.980 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 7.38368 (-1.09907 1.26491)
R^2/D10^2 : 0.501080 (-0.239806 0.476558)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.75e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.197e-07 5.754e-08
25- 50 3.330e-07 8.458e-08
50-150 6.668e-08 3.234e-08
15-150 6.194e-07 1.389e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 32.5055 (-9.59498 15.154)
Norm : 2.48828 (-0.658081 0.983748)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.502e-07 4.561e-08
25- 50 2.984e-07 6.825e-08
50-150 1.811e-07 8.867e-08
15-150 7.298e-07 1.630e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.269373 (-0.268427 3.178)
R1^2/D10^2 : 2.83693E+19 (-1.08143e+19 -2.79098e+19)
kT2 [keV] : 7.69706 (-1.14677 1.33412)
R2^2/D10^2 : 0.412718 (-0.199487 0.393168)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.16e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.475e-07 1.324e-07
25- 50 3.038e-07 1.612e-07
50-150 1.419e-07 8.871e-08
15-150 6.932e-07 3.465e-07
Peak spectrum fit
Power-law model
Time interval is from 49.936 sec. to 50.936 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62775 ( -0.813346 0.938474 )
Norm@50keV : 5.97708E-03 ( -0.00276015 0.00244191 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.71 using 59 bins.
Reduced chi-squared = 0.784386
# Null hypothesis probability of 8.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.774879 ( -0.311265 0.312291 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57237e-08 ( -2.48989e-08 2.5492e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 49.936 sec. to 50.936 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.18010 ( -4.29731 0.610028 )
Epeak [keV] : 498.736 ( )
Norm@50keV : 3.97153E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.14 using 59 bins.
Reduced chi-squared = 0.788214
# Null hypothesis probability of 8.74e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.582443 ( -0.582443 0.482077 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.30491e-08 ( -3.25261e-08 2.18637e-07 ) ergs/cm2
Band function
Time interval is from 49.936 sec. to 50.936 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 18.7992 (-12.5674 21.1728)
R^2/D10^2 : 3.72089E-02 (-0.0365365 1.87364)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.82e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.595e-09 1.776e-09
25- 50 1.239e-08 8.285e-09
50-150 3.210e-08 2.339e-08
15-150 4.708e-08 3.125e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.359 (-199.362 -199.362)
Norm : 3.09422 (-1.21686 2.19067)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.705e-09 4.948e-09
25- 50 1.482e-08 9.695e-09
50-150 3.251e-08 2.147e-08
15-150 5.503e-08 3.450e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.46090 (-3.9522 5.60342)
R1^2/D10^2 : 6.64877 (-6.43772 -6.6445)
kT2 [keV] : 29.6299 (-14.9724 -29.6339)
R2^2/D10^2 : 7.18636E-03 (-0.00713116 0.0681143)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.67e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.101e-08 6.215e-09
25- 50 1.099e-08 5.585e-09
50-150 3.814e-08 2.530e-08
15-150 6.014e-08 3.266e-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: 2.47473 ( -0.298945 0.340055 )
Norm@50keV : 1.71061E-03 ( -0.00041329 0.000407989 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.19e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 47.53 sec: 0.330908 ( -0.0472278 0.0472293 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.0762e-07 ( -1.43035e-07 1.49967e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25091 ( -2.255 1.08136 )
Epeak [keV] : 21.5320 ( -19.1674 11.3103 )
Norm@50keV : 1.03005E-02 ( -0.0103026 0.315023 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 47.53 sec: 0.319683 ( -0.048395 0.048859 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24733e-07 ( -1.41725e-07 1.7589e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 2.67e-07
S(50-100 keV) = 1.92e-07
T90 vs. Hardness ratio plot
T90 = 41.972000002861 sec.
Hardness ratio (energy fluence ratio) = 0.719101
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.06737
Count Ratio (50-100 keV) / (15-25 keV) = 0.342093
Mask shadow pattern
IMX = -9.496713393525639E-01, IMY = 9.706305275166674E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-11.699400 18.448000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4196 -40.7497 0.0 6.8 73.3 -0.0744 -1.0 12.7 Vela X-1
170.0314 -60.5670 1572.0 35.8 76.1 0.0012 0.0 9.0 Cen X-3
83.4410 -64.4687 2.8 40.3 137.6 0.7672 4.1 ------ UNKNOWN
188.0014 -13.9100 2.6 55.9 11.5 2.1154 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
18.448000 65.980000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6110 -40.3677 5.2 6.6 70.3 -0.3160 -2.2 11.8 Vela X-1
170.5543 -60.7146 5.6 36.1 76.1 0.7400 2.1 8.9 Cen X-3
116.2347 -55.2351 2.1 22.2 130.0 0.8942 5.4 ------ UNKNOWN
77.8598 -45.6201 2.2 40.4 167.3 1.2084 5.2 ------ UNKNOWN
76.9329 -32.8412 1.6 43.7 -174.2 1.7992 7.2 ------ UNKNOWN
87.2181 -5.1812 2.2 49.7 -134.3 3.7215 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
138.900600 496.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6075 -40.5298 8.1 46.8 -10.3 1.0544 1.4 3.9 Vela X-1
38.0071 8.6343 2.6 55.6 -176.2 7.2447 4.4 ------ UNKNOWN
79.5099 12.8391 2.4 45.8 -123.9 7.5571 4.7 ------ UNKNOWN
Plot creation:
Mon Nov 16 14:56:15 EST 2020