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
29.1063 -27.2979 0.0112 17.6978 -68.5708 0.8305010 17.198 TRIG_01136936
Foreground time interval of the image:
-0.408 9.736 (delta_t = 10.144 [sec])
Background time interval of the image:
-239.744 -0.408 (delta_t = 239.336 [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 -0.408 sec. to 9.736 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41483 ( -0.161927 0.163191 )
Norm@50keV : 5.23574E-03 ( -0.000492738 0.000490232 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.99 using 59 bins.
Reduced chi-squared = 0.806842
# Null hypothesis probability of 8.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.14 sec: 0.639806 ( -0.059267 0.059333 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.11526e-07 ( -5.38191e-08 5.44495e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.408 sec. to 9.736 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27596 ( -0.700034 0.411718 )
Epeak [keV] : 261.800 ( -261.826 -261.826 )
Norm@50keV : 6.15882E-03 ( -0.00212731 0.00751026 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.85 using 59 bins.
Reduced chi-squared = 0.81875
# Null hypothesis probability of 8.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.14 sec: 0.636102 ( -0.061696 0.061419 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.05881e-07 ( -6.02572e-08 5.85987e-08 ) ergs/cm2
Band function
Time interval is from -0.408 sec. to 9.736 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] : 15.4152 (-1.76312 2.04216)
R^2/D10^2 : 6.69483E-02 (-0.0233569 0.0348829)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.45e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.361e-08 5.536e-09
25- 50 1.369e-07 1.810e-08
50-150 2.240e-07 4.299e-08
15-150 3.945e-07 5.303e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-44.5165 -200)
Norm : 2.61390 (-0.240435 0.240435)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.631e-08 7.889e-09
25- 50 1.276e-07 6.326e-08
50-150 2.798e-07 1.356e-07
15-150 4.736e-07 1.955e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.77996 (-3.80157 4.00438)
R1^2/D10^2 : 0.442345 (-0.270617 0.803107)
kT2 [keV] : 29.3756 (-11.0915 -29.8858)
R2^2/D10^2 : 5.71424E-03 (-0.00523184 0.0250021)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.02e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.597e-08 2.416e-08
25- 50 1.285e-07 5.306e-08
50-150 3.168e-07 1.643e-07
15-150 5.013e-07 2.221e-07
Peak spectrum fit
Power-law model
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57113 ( -0.267204 0.279067 )
Norm@50keV : 8.88504E-03 ( -0.00165935 0.00162996 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.29 using 59 bins.
Reduced chi-squared = 1.04018
# Null hypothesis probability of 3.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.13183 ( -0.191349 0.19137 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.34084e-08 ( -1.66232e-08 1.70185e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.240567 ( -2.10062 1.46421 )
Epeak [keV] : 55.0054 ( -11.2457 45.9874 )
Norm@50keV : 8.84589E-02 ( -0.0911009 1.10494 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.50 using 59 bins.
Reduced chi-squared = 0.973214
# Null hypothesis probability of 5.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.07790 ( -0.196336 0.19674 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.2267e-08 ( -1.60471e-08 1.84733e-08 ) ergs/cm2
Band function
Time interval is from 0.516 sec. to 1.516 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] : 13.0223 (-2.05457 2.44098)
R^2/D10^2 : 0.226465 (-0.104368 0.188155)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.145e-09 2.727e-09
25- 50 2.810e-08 6.675e-09
50-150 3.016e-08 1.171e-08
15-150 6.641e-08 1.706e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 161.689 (-82.3926 -159.722)
Norm : 4.72195 (-0.816314 1.02589)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.58e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.204e-08 6.870e-09
25- 50 2.256e-08 1.249e-08
50-150 4.590e-08 2.709e-08
15-150 8.051e-08 4.643e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.32895 (-4.32895 -4.32895)
R1^2/D10^2 : 2.93745 (-2.93747 -2.93747)
kT2 [keV] : 14.4350 (-2.93351 -14.435)
R2^2/D10^2 : 0.144382 (-0.144383 0.201019)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.020e-08 5.540e-09
25- 50 2.601e-08 1.446e-08
50-150 3.385e-08 2.034e-08
15-150 7.006e-08 3.888e-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: 1.41483 ( -0.161927 0.163191 )
Norm@50keV : 5.23574E-03 ( -0.000492738 0.000490232 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.14 sec: 0.639794 ( -0.0592645 0.0593305 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.11464e-07 ( -5.3913e-08 5.44553e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27597 ( -0.700038 0.411711 )
Epeak [keV] : 261.829 ( -261.829 -261.829 )
Norm@50keV : 6.15869E-03 ( -0.00177817 0.00751806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.14 sec: 0.636030 ( -0.06168 0.061398 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.06075e-07 ( -6.02782e-08 5.845e-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) = 1.21e-07
S(50-100 keV) = 1.82e-07
T90 vs. Hardness ratio plot
T90 = 8.9799998998642 sec.
Hardness ratio (energy fluence ratio) = 1.50413
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38341
Count Ratio (50-100 keV) / (15-25 keV) = 1.07811
Mask shadow pattern
IMX = 1.165831900360716E-01, IMY = 2.970397902554033E-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:
-239.744000 -0.408000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
27.2890 14.4976 2.3 32.5 42.2 3.7322 5.0 ------ UNKNOWN
8.0721 -10.2657 2.9 33.6 -16.9 2.3521 3.9 ------ UNKNOWN
44.7948 -35.3862 2.4 21.0 -116.0 3.1649 4.9 ------ UNKNOWN
17.2047 -49.9251 2.4 40.9 -85.5 11.1152 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.408000 9.736000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
29.1063 -27.2979 0.7 17.7 -68.6 0.8305 17.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.156600 407.356600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
15.0798 2.2973 2.6 32.5 42.2 4.6076 4.5 ------ UNKNOWN
22.5288 -25.6764 3.4 6.1 -7.0 2.6266 3.4 ------ UNKNOWN
353.0592 -20.2725 2.7 33.6 -16.9 3.7544 4.3 ------ UNKNOWN
353.5843 -32.4067 2.8 31.1 -39.2 3.8618 4.1 ------ UNKNOWN
10.2274 -65.1226 3.7 39.7 -98.7 9.7876 3.1 ------ UNKNOWN
Plot creation:
Fri Oct 13 23:09:28 EDT 2023