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
110.0502 -2.2073 0.0152 30.1286 83.9451 1.2338653 12.664 TRIG_00998344
Foreground time interval of the image:
-4.016 14.288 (delta_t = 18.304 [sec])
Background time interval of the image:
-129.275 -4.016 (delta_t = 125.259 [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 8.192000
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 8.192000
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 8.192000
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 -4.016 sec. to 14.288 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.940419 ( -0.230551 0.218375 )
Norm@50keV : 4.05613E-03 ( -0.000545238 0.000539011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.67 using 59 bins.
Reduced chi-squared = 0.994211
# Null hypothesis probability of 4.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.3 sec: 0.465879 ( -0.062883 0.063273 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.20373e-07 ( -1.09436e-07 1.09859e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.016 sec. to 14.288 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.143310 ( -1.20284 0.924723 )
Epeak [keV] : 138.338 ( -51.7272 -138.338 )
Norm@50keV : 8.87224E-03 ( -0.00887224 0.018083 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.63 using 59 bins.
Reduced chi-squared = 0.975536
# Null hypothesis probability of 5.27e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.3 sec: 0.450376 ( -0.065646 0.06595 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.93618e-07 ( -1.17969e-07 1.16193e-07 ) ergs/cm2
Band function
Time interval is from -4.016 sec. to 14.288 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] : 22.9932 (-3.50728 4.57531)
R^2/D10^2 : 1.49139E-02 (-0.00647969 0.0104753)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.08e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.615e-08 6.744e-09
25- 50 1.419e-07 3.079e-08
50-150 5.603e-07 1.217e-07
15-150 7.283e-07 1.524e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-26.6935 -200)
Norm : 1.94172 (-0.263097 0.263097)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.92e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.851e-08 4.993e-08
25- 50 1.703e-07 9.534e-08
50-150 3.734e-07 2.076e-07
15-150 6.322e-07 3.556e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.7530 (-1.43974 3.35431)
R1^2/D10^2 : 6.01166E-02 (-1963.91 1.87759e+10)
kT2 [keV] : 36.8315 (-37.2675 -37.2677)
R2^2/D10^2 : 2.66700E-03 (-0.00246766 0.0106399)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.07e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.696e-08 9.608e-09
25- 50 1.361e-07 3.213e-08
50-150 5.688e-07 1.297e-07
15-150 7.418e-07 1.439e-07
Peak spectrum fit
Power-law model
Time interval is from 10.788 sec. to 11.788 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42759 ( -0.431443 0.445177 )
Norm@50keV : 7.75943E-03 ( -0.00225183 0.00224027 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.87 using 59 bins.
Reduced chi-squared = 1.01526
# Null hypothesis probability of 4.43e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.950976 ( -0.27603 0.277144 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.45916e-08 ( -2.30533e-08 2.34951e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 10.788 sec. to 11.788 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.94952 ( 2.98095 3.46898 )
Epeak [keV] : 54.8536 ( -10.9518 32.0207 )
Norm@50keV : 3.20078 ( -3.1648 3041.32 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.26 using 59 bins.
Reduced chi-squared = 0.933214
# Null hypothesis probability of 6.17e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.806341 ( -0.282722 0.313539 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.01381e-08 ( -2.12175e-08 2.63109e-08 ) ergs/cm2
Band function
Time interval is from 10.788 sec. to 11.788 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] : 15.4035 (-3.26352 4.54677)
R^2/D10^2 : 0.114756 (-0.0701818 0.149418)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.37e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.674e-09 3.302e-09
25- 50 2.309e-08 1.159e-08
50-150 3.772e-08 2.008e-08
15-150 6.649e-08 3.289e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-121.322 -199.362)
Norm : 3.99052 (-1.12685 1.12819)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.937e-09 6.185e-09
25- 50 1.911e-08 1.179e-08
50-150 4.192e-08 2.536e-08
15-150 7.097e-08 4.253e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.962908 (-0.962908 1.7196)
R1^2/D10^2 : 9.36331E+05 (-936345 3.3043e+07)
kT2 [keV] : 15.9061 (-3.42607 4.91744)
R2^2/D10^2 : 0.100099 (-0.0629178 0.101204)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.32e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.313e-09 3.235e-09
25- 50 2.195e-08 1.324e-08
50-150 3.873e-08 2.358e-08
15-150 6.700e-08 4.076e-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: 0.940419 ( -0.230551 0.218375 )
Norm@50keV : 4.05613E-03 ( -0.000545238 0.000539011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.3 sec: 0.465874 ( -0.0628731 0.0632946 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.20254e-07 ( -1.09381e-07 1.09917e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.143309 ( -1.20284 0.924725 )
Epeak [keV] : 138.338 ( -51.725 -138.338 )
Norm@50keV : 8.87225E-03 ( -0.00887225 0.018083 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.27e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.3 sec: 0.450371 ( -0.065638 0.065938 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.93999e-07 ( -1.18026e-07 1.16324e-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) = 1.46e-07
S(50-100 keV) = 3.04e-07
T90 vs. Hardness ratio plot
T90 = 15.8880000114441 sec.
Hardness ratio (energy fluence ratio) = 2.08219
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.42876
Count Ratio (50-100 keV) / (15-25 keV) = 2.61694
Mask shadow pattern
IMX = 6.121586613625030E-02, IMY = -5.771094880487742E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-129.275400 -4.016000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6762 -40.6137 15.4 41.5 4.6 0.2230 0.7 7.6 Vela X-1
104.4826 39.3044 2.9 50.4 143.8 4.0328 4.0 ------ UNKNOWN
108.0417 -2.2523 2.4 32.1 84.2 1.6374 4.8 ------ UNKNOWN
112.7443 44.7971 2.9 50.3 154.5 2.8034 4.0 ------ UNKNOWN
118.1844 -49.5848 2.1 53.7 17.0 4.1925 5.4 ------ UNKNOWN
120.1837 -27.8234 2.4 34.3 31.8 1.2701 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.016000 14.288000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6764 -40.5980 5.8 41.5 4.6 0.1954 2.0 7.2 Vela X-1
106.5972 -16.2876 2.5 37.1 60.8 0.6138 4.7 ------ UNKNOWN
110.0502 -2.2073 0.9 30.1 83.9 1.2339 12.7 ------ UNKNOWN
111.7679 15.8592 1.9 31.7 119.5 0.5989 6.0 ------ UNKNOWN
179.7918 40.5230 2.4 53.7 -143.3 1.3908 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
100.324600 962.754000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6370 22.0196 0.5 35.4 131.7 34.5225 21.7 0.4 Crab
135.5472 -40.6761 7.3 44.8 -30.4 2.3242 1.6 7.3 Vela X-1
82.7256 -0.0536 3.3 27.5 91.3 4.3855 3.5 ------ UNKNOWN
112.2224 52.0996 3.0 54.4 178.7 11.6823 3.8 ------ UNKNOWN
127.8768 -56.5862 5.5 56.2 -14.5 6.0759 2.1 ------ UNKNOWN
Plot creation:
Thu Oct 20 00:47:26 EDT 2022