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
192.2769 22.9105 0.0097 42.8204 37.1462 2.8220343 19.678 TRIG_01093742
Foreground time interval of the image:
-3.896 9.544 (delta_t = 13.440 [sec])
Background time interval of the image:
-114.859 -3.896 (delta_t = 110.963 [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
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)
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 -3.896 sec. to 9.544 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66734 ( -0.120095 0.122046 )
Norm@50keV : 1.43326E-02 ( -0.00106796 0.00106136 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.98 using 59 bins.
Reduced chi-squared = 0.771579
# Null hypothesis probability of 8.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.44 sec: 1.88240 ( -0.13619 0.13636 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.78878e-06 ( -1.39902e-07 1.4087e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.896 sec. to 9.544 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10710 ( -0.543304 0.484191 )
Epeak [keV] : 77.6276 ( -18.2321 152.887 )
Norm@50keV : 2.79617E-02 ( -0.012035 0.0247284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.01 using 59 bins.
Reduced chi-squared = 0.714464
# Null hypothesis probability of 9.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.44 sec: 1.84061 ( -0.14103 0.14102 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72211e-06 ( -1.52145e-07 1.52625e-07 ) ergs/cm2
Band function
Time interval is from -3.896 sec. to 9.544 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] : 13.6340 (-1.16532 1.27211)
R^2/D10^2 : 0.292513 (-0.0809424 0.111845)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.30e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.547e-07 1.938e-08
25- 50 5.602e-07 5.174e-08
50-150 6.762e-07 1.078e-07
15-150 1.391e-06 1.217e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 148.086 (-41.3065 -145.452)
Norm : 7.75315 (-0.625555 0.782343)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.679e-07 3.004e-08
25- 50 4.957e-07 6.707e-08
50-150 9.732e-07 3.820e-07
15-150 1.737e-06 4.570e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.50541 (-1.41224 1.69432)
R1^2/D10^2 : 2.57796 (-1.3661 3.60928)
kT2 [keV] : 22.1026 (-3.85634 6.85324)
R2^2/D10^2 : 3.87046E-02 (-0.0251972 0.0450055)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.49e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.638e-07 7.814e-08
25- 50 5.055e-07 1.425e-07
50-150 9.407e-07 3.942e-07
15-150 1.710e-06 4.859e-07
Peak spectrum fit
Power-law model
Time interval is from 0.684 sec. to 1.684 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54691 ( -0.24328 0.254002 )
Norm@50keV : 2.59553E-02 ( -0.0040113 0.00397818 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.14 using 59 bins.
Reduced chi-squared = 0.809474
# Null hypothesis probability of 8.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.28295 ( -0.50522 0.50601 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44489e-07 ( -4.03199e-08 4.0475e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.684 sec. to 1.684 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29927 ( -1.04244 0.488773 )
Epeak [keV] : 154.407 ( -154.406 -154.406 )
Norm@50keV : 3.41761E-02 ( -0.025347 0.0701244 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.91 using 59 bins.
Reduced chi-squared = 0.819821
# Null hypothesis probability of 8.30e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.26276 ( -0.51075 0.51114 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43461e-07 ( -4.11218e-08 4.09e-08 ) ergs/cm2
Band function
Time interval is from 0.684 sec. to 1.684 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] : 16.3506 (-2.97722 3.53848)
R^2/D10^2 : 0.281762 (-0.138941 0.279577)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.550e-08 4.651e-09
25- 50 6.642e-08 1.517e-08
50-150 1.251e-07 3.532e-08
15-150 2.070e-07 4.920e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-88.2628 -199.363)
Norm : 13.4836 (-2.0184 2.01944)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.51e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.358e-08 1.912e-08
25- 50 6.459e-08 3.599e-08
50-150 1.417e-07 7.880e-08
15-150 2.398e-07 1.337e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.32101 (-2.13241 3.53094)
R1^2/D10^2 : 9.14753 (-7.68262 81.516)
kT2 [keV] : 23.3022 (-5.6683 12.1651)
R2^2/D10^2 : 6.91911E-02 (-0.0546679 0.12516)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.12e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.512e-08 1.929e-08
25- 50 5.850e-08 3.018e-08
50-150 1.511e-07 8.646e-08
15-150 2.447e-07 1.185e-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: 1.66734 ( -0.120095 0.122046 )
Norm@50keV : 1.43326E-02 ( -0.00106796 0.00106136 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.44 sec: 1.88232 ( -0.136176 0.136358 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.78853e-06 ( -1.40066e-07 1.40887e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10710 ( -0.543302 0.484192 )
Epeak [keV] : 77.6275 ( -18.232 152.887 )
Norm@50keV : 2.79617E-02 ( -0.012035 0.0247283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.44 sec: 1.84036 ( -0.14098 0.14097 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.7227e-06 ( -1.52436e-07 1.52732e-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) = 4.77e-07
S(50-100 keV) = 6.02e-07
T90 vs. Hardness ratio plot
T90 = 10.6080000400543 sec.
Hardness ratio (energy fluence ratio) = 1.26205
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.5459
Count Ratio (50-100 keV) / (15-25 keV) = 1.10023
Mask shadow pattern
IMX = 7.386484562865351E-01, IMY = -5.595721947618852E-01
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:
-114.859400 -3.896000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4323 35.3556 1.7 27.1 -67.2 1.4848 7.0 1.5 Her X-1
184.2484 27.7601 2.7 42.6 50.0 1.8258 4.3 ------ UNKNOWN
201.2413 26.1630 2.6 36.1 28.2 1.0829 4.5 ------ UNKNOWN
220.9009 12.3564 3.0 44.4 -5.6 1.0329 3.9 ------ UNKNOWN
259.7799 39.3587 2.7 26.3 -80.1 0.8815 4.2 ------ UNKNOWN
298.8954 51.2945 2.5 39.8 -130.4 1.3655 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.896000 9.544000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4107 35.3709 3.4 27.1 -67.2 -0.2199 -3.4 2.9 Her X-1
192.2769 22.9105 0.6 42.8 37.1 2.8223 19.7 ------ UNKNOWN
252.8949 11.5701 2.1 48.4 -49.0 1.2005 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
79.140600 435.540600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
182.9225 -34.5513 3.2 58.1 -3.8 7.6281 3.6 ------ UNKNOWN
186.1193 -33.5740 3.1 56.8 -6.8 5.7703 3.8 ------ UNKNOWN
255.6687 67.9346 2.3 59.0 -169.8 12.7674 5.1 ------ UNKNOWN
255.2395 47.0453 2.1 55.2 -145.2 11.6758 5.4 ------ UNKNOWN
248.1772 37.1645 2.3 49.7 -133.0 8.2131 5.0 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:08:30 EDT 2022