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
98.5712 49.8440 0.0163 10.6025 132.3715 1.4034154 11.788 TRIG_01149293
Foreground time interval of the image:
1.144 53.144 (delta_t = 52.000 [sec])
Background time interval of the image:
-239.856 1.144 (delta_t = 241.000 [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 12.160000
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 12.160000
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 12.160000
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 1.144 sec. to 53.144 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38497 ( -0.220555 0.219852 )
Norm@50keV : 1.61197E-03 ( -0.000216061 0.000215091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.89 using 59 bins.
Reduced chi-squared = 0.945439
# Null hypothesis probability of 5.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52 sec: 0.195652 ( -0.025943 0.025971 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.12594e-07 ( -1.20741e-07 1.22496e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.144 sec. to 53.144 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.576979 ( -1.2597 0.508536 )
Epeak [keV] : 82.7418 ( -27.246 -82.7335 )
Norm@50keV : 4.34290E-03 ( -0.00434374 0.0160926 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.85 using 59 bins.
Reduced chi-squared = 0.925893
# Null hypothesis probability of 6.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52 sec: 0.189779 ( -0.027107 0.026983 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.50334e-07 ( -1.42026e-07 1.43698e-07 ) ergs/cm2
Band function
Time interval is from 1.144 sec. to 53.144 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] : 14.1458 (-2.0864 2.60486)
R^2/D10^2 : 2.83254E-02 (-0.0126978 0.0214309)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.30e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.220e-08 1.628e-08
25- 50 2.337e-07 4.391e-08
50-150 3.096e-07 9.006e-08
15-150 6.054e-07 1.098e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-67.9942 -200)
Norm : 0.807429 (-0.105759 0.105759)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.92e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.046e-07 5.897e-08
25- 50 2.011e-07 1.115e-07
50-150 4.411e-07 2.439e-07
15-150 7.468e-07 4.196e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.81685 (-3.34718 3.07792)
R1^2/D10^2 : 7.59338E-02 (-0.0363675 0.107743)
kT2 [keV] : 39.9075 (-36.2833 -57.5723)
R2^2/D10^2 : 5.18935E-04 (-0.000155946 0.00474787)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.01e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.254e-08 4.831e-08
25- 50 2.243e-07 1.257e-07
50-150 4.531e-07 2.582e-07
15-150 7.599e-07 4.046e-07
Peak spectrum fit
Power-law model
Time interval is from 12.144 sec. to 13.144 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45137 ( -0.578574 0.620522 )
Norm@50keV : 4.26174E-03 ( -0.00157623 0.00154214 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.10 using 59 bins.
Reduced chi-squared = 0.896491
# Null hypothesis probability of 6.95e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.525389 ( -0.188124 0.188626 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07774e-08 ( -1.60317e-08 1.64442e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 12.144 sec. to 13.144 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.21474 ( 1.28643 3.49079 )
Epeak [keV] : 63.1553 ( -15.0874 -62.7842 )
Norm@50keV : 7.83051E-02 ( -0.091093 2326.4 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.63 using 59 bins.
Reduced chi-squared = 0.88625
# Null hypothesis probability of 7.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.469914 ( -0.222649 0.21179 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.61352e-08 ( -1.72179e-08 1.79004e-08 ) ergs/cm2
Band function
Time interval is from 12.144 sec. to 13.144 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] : 15.9400 (-4.45667 6.94919)
R^2/D10^2 : 5.39348E-02 (-0.0539348 0.113308)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.48e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.836e-09 1.853e-09
25- 50 1.189e-08 7.295e-09
50-150 2.109e-08 1.500e-08
15-150 3.582e-08 2.285e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-199.363 -199.363)
Norm : 2.18112 (-0.767951 0.768427)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.431e-09 3.572e-09
25- 50 1.045e-08 6.735e-09
50-150 2.291e-08 1.429e-08
15-150 3.879e-08 2.434e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.36718 (-1.75736 16.3935)
R1^2/D10^2 : 8504.58 (-7750.74 -7750.74)
kT2 [keV] : 17.0077 (-4.86055 8.18201)
R2^2/D10^2 : 4.12378E-02 (-0.0307731 0.0508433)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.474e-09 2.158e-09
25- 50 1.053e-08 6.585e-09
50-150 2.247e-08 1.592e-08
15-150 3.748e-08 2.233e-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: 1.38497 ( -0.220555 0.219852 )
Norm@50keV : 1.61197E-03 ( -0.000216061 0.000215091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52 sec: 0.195648 ( -0.0259421 0.0259709 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.1249e-07 ( -1.20697e-07 1.22547e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.576552 ( -1.25956 0.892908 )
Epeak [keV] : 82.7162 ( -27.2611 -82.7309 )
Norm@50keV : 4.34543E-03 ( -0.00434385 0.0160922 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52 sec: 0.189762 ( -0.027101 0.02697 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.50604e-07 ( -1.42334e-07 1.43863e-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) = 1.89e-07
S(50-100 keV) = 2.90e-07
T90 vs. Hardness ratio plot
T90 = 41 sec.
Hardness ratio (energy fluence ratio) = 1.53439
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.98035
Count Ratio (50-100 keV) / (15-25 keV) = 1.29541
Mask shadow pattern
IMX = -1.261539998935572E-01, IMY = -1.382944636345954E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
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:
-239.856000 1.144000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6486 21.9700 2.2 40.8 134.3 8.2212 5.2 2.8 Crab
119.0579 22.0036 3.2 38.0 81.7 5.2599 3.7 ------ UNKNOWN
70.3296 44.4882 1.7 26.7 172.8 3.5412 6.8 ------ UNKNOWN
43.1979 43.1471 2.7 41.5 -163.8 3.1769 4.2 ------ UNKNOWN
206.6215 50.5283 3.3 52.3 -28.3 7.4601 3.5 ------ UNKNOWN
227.2853 86.6905 3.4 32.7 -75.4 2.5607 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
1.144000 53.144000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6844 22.1701 6.0 40.6 134.3 0.6250 1.9 9.8 Crab
141.3476 19.5050 2.6 46.5 52.9 2.3579 4.5 ------ UNKNOWN
98.5712 49.8440 1.0 10.6 132.4 1.4036 11.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
112.044600 962.214600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6297 21.9929 0.6 30.3 154.3 34.4477 18.1 1.3 Crab
128.4274 16.9825 2.1 40.7 79.1 42.7499 5.6 ------ UNKNOWN
70.2868 44.5143 1.6 19.8 -148.8 9.9904 7.3 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:16:36 EDT 2023