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
326.0534 -34.4140 0.0085 15.6966 -18.1638 2.9078890 22.738 TRIG_01144698
Foreground time interval of the image:
-38.296 11.741 (delta_t = 50.037 [sec])
Background time interval of the image:
-239.360 -38.296 (delta_t = 201.064 [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 -38.296 sec. to 267.908 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67658 ( -0.0884508 0.0894647 )
Norm@50keV : 1.92691E-03 ( -9.82413e-05 9.77392e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.40 using 59 bins.
Reduced chi-squared = 1.00702
# Null hypothesis probability of 4.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 306.2 sec: 0.253868 ( -0.01247 0.012489 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.4744e-06 ( -2.95167e-07 2.97322e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -38.296 sec. to 267.908 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11779 ( -0.406674 0.372257 )
Epeak [keV] : 76.2478 ( -14.5114 54.5881 )
Norm@50keV : 3.72630E-03 ( -0.00129912 0.00224334 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.57 using 59 bins.
Reduced chi-squared = 0.903036
# Null hypothesis probability of 6.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 306.2 sec: 0.245440 ( -0.013582 0.013597 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.20326e-06 ( -3.40693e-07 3.43706e-07 ) ergs/cm2
Band function
Time interval is from -38.296 sec. to 267.908 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] : 13.4694 ( )
R^2/D10^2 : 3.99987E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 120.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.07e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.707e-07 4.379e-08
25- 50 1.683e-06 1.001e-07
50-150 1.970e-06 2.010e-07
15-150 4.124e-06 2.266e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 140.718 (-29.3735 39.0256)
Norm : 1.04855 (-0.0599503 0.0712782)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.288e-07 6.461e-08
25- 50 1.522e-06 1.312e-07
50-150 2.923e-06 8.927e-07
15-150 5.274e-06 1.063e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.54375 (-1.3515 1.69753)
R1^2/D10^2 : 0.553308 (-0.329057 1.17081)
kT2 [keV] : 19.1934 (-2.48153 4.09633)
R2^2/D10^2 : 9.19384E-03 (-0.00502511 0.00693178)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.04e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.151e-07 2.235e-07
25- 50 1.495e-06 2.240e-07
50-150 2.702e-06 4.588e-07
15-150 5.012e-06 7.594e-07
Peak spectrum fit
Power-law model
Time interval is from 0.228 sec. to 1.228 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15841 ( -0.211992 0.209287 )
Norm@50keV : 1.50695E-02 ( -0.00189184 0.00189127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.95 using 59 bins.
Reduced chi-squared = 0.771053
# Null hypothesis probability of 8.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.75920 ( -0.22649 0.22691 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5476e-07 ( -2.13311e-08 2.14619e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.228 sec. to 1.228 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.534878 ( -1.05957 0.740117 )
Epeak [keV] : 131.194 ( -51.502 -131.194 )
Norm@50keV : 2.92007E-02 ( -0.0135784 0.0564217 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.45 using 59 bins.
Reduced chi-squared = 0.758036
# Null hypothesis probability of 9.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.72194 ( -0.23432 0.23305 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50702e-07 ( -2.27138e-08 2.24789e-08 ) ergs/cm2
Band function
Time interval is from 0.228 sec. to 1.228 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] : 19.4989 (-2.90866 3.57113)
R^2/D10^2 : 9.14073E-02 (-0.0386581 0.0639961)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.33e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.766e-09 1.680e-09
25- 50 3.313e-08 6.860e-09
50-150 9.302e-08 2.069e-08
15-150 1.329e-07 2.425e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-35.2263 -200)
Norm : 7.23987 (-0.932426 0.932426)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.69 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 1.802e-08 1.020e-08
25- 50 3.467e-08 1.970e-08
50-150 7.604e-08 4.169e-08
15-150 1.287e-07 7.130e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.0654 (-9.05142 -10.0402)
R1^2/D10^2 : 0.413613 (-0.293968 -0.416798)
kT2 [keV] : 31.8694 (-30.7643 -31.7549)
R2^2/D10^2 : 1.38767E-02 (-0.0133345 0.0957521)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.76e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.224e-08 5.090e-09
25- 50 2.972e-08 8.060e-09
50-150 9.951e-08 2.512e-08
15-150 1.415e-07 3.325e-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: 1.45963 ( -0.109108 0.109923 )
Norm@50keV : 3.83108E-03 ( -0.000243687 0.000242956 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 50.04 sec: 0.473266 ( -0.0298477 0.0298794 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.83127e-06 ( -1.2897e-07 1.29937e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.764330 ( -0.525364 0.468599 )
Epeak [keV] : 89.5597 ( -19.4312 77.8727 )
Norm@50keV : 8.50234E-03 ( -0.00346894 0.00679325 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 50.04 sec: 0.456749 ( -0.031808 0.031754 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.73445e-06 ( -1.44165e-07 1.45241e-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) = 1.47e-06
S(50-100 keV) = 1.84e-06
T90 vs. Hardness ratio plot
T90 = 228.531999945641 sec.
Hardness ratio (energy fluence ratio) = 1.2517
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29502
Count Ratio (50-100 keV) / (15-25 keV) = 0.806423
Mask shadow pattern
IMX = 2.670204085641351E-01, IMY = 8.760484207718193E-02
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:
-239.360000 -38.296000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
306.6117 -1.8629 2.4 52.7 -26.6 7.8640 4.8 ------ UNKNOWN
252.3222 -59.7813 2.4 46.3 -126.3 6.5103 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-38.296000 11.740590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0534 -34.4140 0.5 15.7 -18.2 2.9078 22.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
59.940600 327.940600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.2359 -24.8363 0.0 36.5 -79.9 0.1075 0.1 12.0 HT1900.1-2455
20.3348 -45.8088 2.7 42.2 128.7 8.0505 4.2 ------ UNKNOWN
24.3125 -72.8575 3.8 48.1 166.4 5.3828 3.1 ------ UNKNOWN
325.9948 -34.4317 1.2 0.0 -142.2 4.6936 9.9 ------ UNKNOWN
322.1972 -28.9872 2.4 6.3 -26.0 2.2820 4.9 ------ UNKNOWN
301.7506 -21.8636 2.5 24.7 -59.8 2.7218 4.6 ------ UNKNOWN
282.0081 -63.3444 2.5 39.5 -144.6 3.3616 4.5 ------ UNKNOWN
Plot creation:
Wed Jun 14 13:54:13 EDT 2023