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
149.5699 69.7035 0.0065 30.0697 -55.3614 1.8762476 29.803 TRIG_01062150
Foreground time interval of the image:
-0.320 5.012 (delta_t = 5.332 [sec])
Background time interval of the image:
-239.672 -0.320 (delta_t = 239.352 [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 1.024000
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 1.024000
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 1.024000
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 -0.672 sec. to 213.328 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14339 ( -0.266776 0.257627 )
Norm@50keV : 7.20959E-04 ( -0.000105768 0.000105613 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.78 using 59 bins.
Reduced chi-squared = 0.961053
# Null hypothesis probability of 5.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 214 sec: 8.40135E-02 ( -0.0126873 0.0127289 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.59164e-06 ( -2.56567e-07 2.59353e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.672 sec. to 213.328 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.916919 ( -1.1522 0.675519 )
Epeak [keV] : 256.377 ( -256.422 -256.422 )
Norm@50keV : 9.24682E-04 ( -0.000300438 0.0022396 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.62 using 59 bins.
Reduced chi-squared = 0.975357
# Null hypothesis probability of 5.27e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 214 sec: 8.31845E-02 ( -0.0131919 0.0131744 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56615e-06 ( -2.85579e-07 2.7642e-07 ) ergs/cm2
Band function
Time interval is from -0.672 sec. to 213.328 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] : 18.6398 (-3.57566 4.90822)
R^2/D10^2 : 4.85624E-03 (-0.00257671 0.0050176)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.64e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.145e-08 2.326e-08
25- 50 3.390e-07 9.080e-08
50-150 8.622e-07 2.419e-07
15-150 1.273e-06 2.949e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-46.802 -200)
Norm : 0.347310 (-0.0521727 0.0521727)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.27e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.851e-07 1.058e-07
25- 50 3.560e-07 2.022e-07
50-150 7.808e-07 4.435e-07
15-150 1.322e-06 7.485e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.3084 (-3.61165 4.37239)
R1^2/D10^2 : 2.36228E-02 (-0.0152535 0.0584341)
kT2 [keV] : 49.6665 (-24.4999 -49.6665)
R2^2/D10^2 : 1.87427E-04 (-0.000173013 0.00156134)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.47e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.213e-07 7.109e-08
25- 50 3.649e-07 2.019e-07
50-150 1.114e-06 5.778e-07
15-150 1.601e-06 8.116e-07
Peak spectrum fit
Power-law model
Time interval is from 0.172 sec. to 1.172 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18690 ( -0.105448 0.104895 )
Norm@50keV : 5.47189E-02 ( -0.00340792 0.00340767 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.85 using 59 bins.
Reduced chi-squared = 0.874561
# Null hypothesis probability of 7.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.41132 ( -0.40715 0.40738 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57276e-07 ( -3.88103e-08 3.90037e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.172 sec. to 1.172 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.980577 ( -0.423067 0.258607 )
Epeak [keV] : 265.944 ( -265.947 -265.947 )
Norm@50keV : 6.88070E-02 ( -0.0166571 0.0397329 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.05 using 59 bins.
Reduced chi-squared = 0.875893
# Null hypothesis probability of 7.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.37299 ( -0.41373 0.41365 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.51341e-07 ( -4.10005e-08 4.07112e-08 ) ergs/cm2
Band function
Time interval is from 0.172 sec. to 1.172 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] : 20.2348 (-1.56333 1.74359)
R^2/D10^2 : 0.319064 (-0.074474 0.0945152)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.51e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.507e-08 3.035e-09
25- 50 1.258e-07 1.065e-08
50-150 3.825e-07 3.835e-08
15-150 5.334e-07 4.165e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-8.58085 -200)
Norm : 27.3800 (-1.70038 1.70038)
------------------------------------------------------------
#Fit statistic : Chi-Squared 107.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.71e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.815e-08 4.625e-09
25- 50 1.311e-07 1.165e-08
50-150 2.875e-07 5.985e-08
15-150 4.868e-07 9.875e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.1145 (-2.29166 2.65868)
R1^2/D10^2 : 1.69133 (-0.744454 1.67292)
kT2 [keV] : 38.2260 (-9.20864 27.6388)
R2^2/D10^2 : 3.32865E-02 (-0.0260106 0.0503943)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.90e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.185e-08 1.188e-08
25- 50 1.330e-07 3.337e-08
50-150 4.419e-07 1.898e-07
15-150 6.167e-07 2.092e-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: 1.35666 ( -0.086884 0.0869181 )
Norm@50keV : 2.43146E-02 ( -0.00120827 0.00120762 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.78e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.332 sec: 2.93324 ( -0.149725 0.149911 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26433e-06 ( -6.95245e-08 6.98055e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.996272 ( -0.375971 0.344879 )
Epeak [keV] : 146.651 ( -49.7247 2997.8 )
Norm@50keV : 3.63216E-02 ( -0.0113044 0.0183025 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.332 sec: 2.88375 ( -0.15701 0.15686 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23499e-06 ( -7.63063e-08 7.58477e-08 ) 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) = 3.23e-07
S(50-100 keV) = 5.84e-07
T90 vs. Hardness ratio plot
T90 = 3.85999989509583 sec.
Hardness ratio (energy fluence ratio) = 1.80805
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50516
Count Ratio (50-100 keV) / (15-25 keV) = 1.30293
Mask shadow pattern
IMX = 3.290872601135894E-01, IMY = 4.763524701263181E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.672000 -0.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3938 35.2481 6.7 33.0 104.8 0.9524 1.7 6.5 Her X-1
234.0288 17.1920 2.4 43.0 143.7 3.8232 4.8 ------ UNKNOWN
260.0532 57.7529 3.1 21.3 60.0 1.1564 3.7 ------ UNKNOWN
180.9736 37.9453 2.8 32.0 -128.6 1.8709 4.2 ------ UNKNOWN
120.3958 63.9429 2.8 42.7 -54.8 3.4854 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.320000 5.012000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4901 35.1565 0.0 33.1 104.8 -0.1536 -2.1 11.3 Her X-1
239.7581 16.9013 2.8 44.6 136.1 0.6270 4.1 ------ UNKNOWN
268.2280 51.0813 2.3 28.6 68.8 0.3295 5.1 ------ UNKNOWN
277.1849 65.0666 2.4 27.0 37.1 0.2639 4.8 ------ UNKNOWN
149.5699 69.7035 0.4 30.1 -55.4 1.8761 29.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
70.228600 204.628600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
198.7013 70.2246 2.7 16.4 131.4 0.8026 4.3 ------ UNKNOWN
55.7722 38.8943 2.8 55.2 -4.9 2.2284 4.1 ------ UNKNOWN
75.0777 29.1164 3.2 57.5 -27.2 4.5070 3.7 ------ UNKNOWN
82.2382 30.3009 2.4 53.9 -33.5 4.9106 4.8 ------ UNKNOWN
Plot creation:
Thu Nov 10 21:17:55 EST 2022