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
67.0815 37.4296 0.0054 44.9420 -147.1295 4.9927045 35.658 TRIG_01036227
Foreground time interval of the image:
-0.040 8.792 (delta_t = 8.832 [sec])
Background time interval of the image:
-239.488 -0.040 (delta_t = 239.448 [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 0.512000
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 0.512000
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 0.512000
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 -0.040 sec. to 8.792 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38757 ( -0.0638512 0.0638111 )
Norm@50keV : 3.94060E-02 ( -0.00146619 0.00146617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.05 using 59 bins.
Reduced chi-squared = 1.19386
# Null hypothesis probability of 1.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 8.832 sec: 4.78563 ( -0.19138 0.19178 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.37201e-06 ( -1.32431e-07 1.32591e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.040 sec. to 8.792 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.844099 ( -0.28573 0.268852 )
Epeak [keV] : 119.833 ( -23.0674 60.4021 )
Norm@50keV : 6.95510E-02 ( -0.016626 0.0233043 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.46 using 59 bins.
Reduced chi-squared = 0.990357
# Null hypothesis probability of 4.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 8.832 sec: 4.65535 ( -0.20046 0.20116 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.29874e-06 ( -1.39165e-07 1.38886e-07 ) ergs/cm2
Band function
Time interval is from -0.040 sec. to 8.792 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] : 18.1520 ( )
R^2/D10^2 : 0.293098 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 168.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.12e-13 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.703e-07 1.250e-08
25- 50 7.926e-07 4.116e-08
50-150 1.900e-06 1.201e-07
15-150 2.863e-06 1.329e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-7.68534 -200)
Norm : 20.1084 (-0.751029 0.751029)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.38e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.424e-07 1.753e-08
25- 50 8.509e-07 3.453e-08
50-150 1.866e-06 7.905e-08
15-150 3.160e-06 1.356e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.06481 (-1.14659 1.33052)
R1^2/D10^2 : 3.78977 (-1.62119 3.30847)
kT2 [keV] : 25.4793 (-2.40015 3.3616)
R2^2/D10^2 : 7.62951E-02 (-0.0287195 0.0350568)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.38e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.462e-07 5.255e-08
25- 50 8.086e-07 8.201e-08
50-150 2.133e-06 2.014e-07
15-150 3.288e-06 2.950e-07
Peak spectrum fit
Power-law model
Time interval is from 2.124 sec. to 3.124 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19472 ( -0.0836204 0.0836211 )
Norm@50keV : 0.115541 ( -0.005965 0.00596428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.55 using 59 bins.
Reduced chi-squared = 1.20263
# Null hypothesis probability of 1.40e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 13.5522 ( -0.7235 0.7242 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17409e-06 ( -6.54514e-08 6.55912e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.124 sec. to 3.124 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.523147 ( -0.388506 0.358351 )
Epeak [keV] : 128.535 ( -27.0608 77.4114 )
Norm@50keV : 0.229619 ( -0.0688193 0.106577 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.68 using 59 bins.
Reduced chi-squared = 1.03
# Null hypothesis probability of 4.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 13.2877 ( -0.7359 0.7371 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16003e-06 ( -6.74833e-08 6.7381e-08 ) ergs/cm2
Band function
Time interval is from 2.124 sec. to 3.124 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] : 20.3658 (-1.22213 1.31198)
R^2/D10^2 : 0.621052 (-0.115367 0.139762)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 104.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.29e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.929e-08 4.815e-09
25- 50 2.485e-07 1.815e-08
50-150 7.658e-07 6.275e-08
15-150 1.064e-06 7.010e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 ( )
Norm : 56.2766 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 115.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.88e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.401e-07 8.250e-09
25- 50 2.696e-07 1.630e-08
50-150 5.912e-07 4.030e-08
15-150 1.001e-06 6.095e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.15472 (-1.52466 2.02668)
R1^2/D10^2 : 13.6299 (-8.39284 27.8503)
kT2 [keV] : 25.5138 (-2.48166 3.5544)
R2^2/D10^2 : 0.263084 (-0.10104 0.117693)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.60e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.005e-07 3.901e-08
25- 50 2.436e-07 4.340e-08
50-150 8.192e-07 9.460e-08
15-150 1.163e-06 1.560e-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: 1.38757 ( -0.0638512 0.0638111 )
Norm@50keV : 3.94060E-02 ( -0.00146619 0.00146617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 8.832 sec: 4.78555 ( -0.191364 0.191757 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.3716e-06 ( -1.32465e-07 1.32616e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.844099 ( -0.28573 0.268852 )
Epeak [keV] : 119.833 ( -23.0674 60.4021 )
Norm@50keV : 6.95510E-02 ( -0.016626 0.0233043 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 8.832 sec: 4.65497 ( -0.20041 0.20109 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.30012e-06 ( -1.39351e-07 1.38945e-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) = 7.87e-07
S(50-100 keV) = 1.20e-06
T90 vs. Hardness ratio plot
T90 = 6.18799984455109 sec.
Hardness ratio (energy fluence ratio) = 1.52478
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.63174
Count Ratio (50-100 keV) / (15-25 keV) = 1.62449
Mask shadow pattern
IMX = -8.381999683979031E-01, IMY = 5.416433501750929E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.488000 -0.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6239 22.0024 0.7 49.9 -175.0 10.7087 16.4 0.9 Crab
192.6539 50.8667 3.0 35.3 20.4 1.6421 3.9 ------ UNKNOWN
93.0293 14.6840 2.7 52.8 170.7 4.1535 4.3 ------ UNKNOWN
155.5468 56.5209 2.5 13.9 38.1 1.2862 4.7 ------ UNKNOWN
186.1576 61.2547 2.7 26.7 6.9 1.4070 4.3 ------ UNKNOWN
67.1384 22.1140 3.8 57.5 -158.5 4.3596 3.1 ------ UNKNOWN
287.2655 68.5162 2.7 50.2 -45.5 5.7632 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.040000 8.792000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7346 22.1361 6.6 49.8 -175.0 -0.2649 -1.8 9.2 Crab
190.1388 33.5312 2.3 46.8 40.6 0.7832 5.1 ------ UNKNOWN
97.4551 10.5058 2.5 55.2 163.9 1.3377 4.6 ------ UNKNOWN
67.0815 37.4296 0.3 44.9 -147.1 4.9929 35.6 ------ UNKNOWN
16.6771 85.9648 2.7 31.6 -63.2 0.4122 4.3 ------ UNKNOWN
54.9549 55.3299 2.6 38.1 -119.0 0.5548 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.612590 710.792000
720.512000 962.529900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6433 22.0146 0.3 21.0 143.8 37.1452 34.1 0.6 Crab
174.9477 85.2399 4.5 54.2 16.8 12.7856 2.6 ------ UNKNOWN
64.1729 76.7099 3.4 39.3 10.1 4.8804 3.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:10:28 EDT 2022