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
124.1571 57.5832 0.0113 41.8961 -8.3363 1.6635942 16.988 TRIG_01034721
Foreground time interval of the image:
-1.924 16.693 (delta_t = 18.617 [sec])
Background time interval of the image:
-239.808 -1.924 (delta_t = 237.884 [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 -1.924 sec. to 20.952 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44065 ( -0.144909 0.14499 )
Norm@50keV : 5.67314E-03 ( -0.000491298 0.000490672 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.61 using 59 bins.
Reduced chi-squared = 1.25632
# Null hypothesis probability of 9.22e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 22.88 sec: 0.697542 ( -0.062145 0.062281 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24442e-06 ( -1.16322e-07 1.17171e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.924 sec. to 20.952 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.862411 ( -0.63519 0.554909 )
Epeak [keV] : 101.319 ( -29.9122 627.034 )
Norm@50keV : 1.09621E-02 ( -0.00503154 0.0112204 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.41 using 59 bins.
Reduced chi-squared = 1.22161
# Null hypothesis probability of 1.23e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 22.88 sec: 0.681656 ( -0.063931 0.064046 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20115e-06 ( -1.2551e-07 1.25135e-07 ) ergs/cm2
Band function
Time interval is from -1.924 sec. to 20.952 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] : 15.7931 (-1.71401 1.96027)
R^2/D10^2 : 6.76609E-02 (-0.0227857 0.0337692)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 94.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.47e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.006e-08 1.422e-08
25- 50 3.331e-07 4.164e-08
50-150 5.779e-07 9.427e-08
15-150 9.911e-07 1.123e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-42.9549 -200)
Norm : 2.89379 (-0.248202 0.248202)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.649e-07 1.993e-08
25- 50 3.172e-07 6.678e-08
50-150 6.956e-07 2.612e-07
15-150 1.178e-06 3.442e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.20732 (-1.69804 1.95147)
R1^2/D10^2 : 0.421070 (-0.204697 0.461212)
kT2 [keV] : 29.4476 (-6.78883 13.9392)
R2^2/D10^2 : 5.85496E-03 (-0.00419005 0.0093648)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.84e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.379e-07 5.824e-08
25- 50 3.311e-07 1.182e-07
50-150 7.565e-07 3.717e-07
15-150 1.225e-06 4.718e-07
Peak spectrum fit
Power-law model
Time interval is from 0.024 sec. to 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30563 ( -0.202438 0.203283 )
Norm@50keV : 2.37059E-02 ( -0.0027357 0.00272871 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.12 using 59 bins.
Reduced chi-squared = 1.37053
# Null hypothesis probability of 3.31e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.83116 ( -0.33319 0.33388 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.33965e-07 ( -3.00919e-08 3.02941e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.024 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.02836 ( -0.0357975 0.00389424 )
Epeak [keV] : 10.8513 ( )
Norm@50keV : 7.43198E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.12 using 59 bins.
Reduced chi-squared = 1.35929
# Null hypothesis probability of 3.81e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.83208 ( -0.34126 0.3319 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34062e-07 ( -3.13544e-08 3.02397e-08 ) ergs/cm2
Band function
Time interval is from 0.024 sec. to 1.024 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] : 17.2804 (-2.72048 3.44919)
R^2/D10^2 : 0.204320 (-0.0927197 0.160076)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 98.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.18e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.237e-08 2.715e-09
25- 50 5.544e-08 1.068e-08
50-150 1.188e-07 2.721e-08
15-150 1.866e-07 3.290e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-41.537 -200)
Norm : 11.6917 (-1.35688 1.35688)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.41e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.911e-08 1.628e-08
25- 50 5.601e-08 3.059e-08
50-150 1.228e-07 6.780e-08
15-150 2.080e-07 1.148e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.19608 (-3.32138 3.04936)
R1^2/D10^2 : 1.16204 (-0.679598 3.65126)
kT2 [keV] : 40.7453 (-15.2504 90.1695)
R2^2/D10^2 : 9.94898E-03 (-0.00870925 0.0373099)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.84e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.144e-08 1.131e-08
25- 50 5.692e-08 2.805e-08
50-150 1.583e-07 8.321e-08
15-150 2.367e-07 1.152e-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: 1.40960 ( -0.155827 0.155399 )
Norm@50keV : 5.88422E-03 ( -0.000544118 0.000543682 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.62 sec: 0.718164 ( -0.0687386 0.068906 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.05663e-06 ( -1.05665e-07 1.06263e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.859061 ( -0.687381 0.592388 )
Epeak [keV] : 107.298 ( -34.9077 -107.298 )
Norm@50keV : 1.09883E-02 ( -0.0052425 0.0125068 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.62 sec: 0.702619 ( -0.070687 0.070832 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02212e-06 ( -1.14263e-07 1.1372e-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) = 3.00e-07
S(50-100 keV) = 4.39e-07
T90 vs. Hardness ratio plot
T90 = 20.8040000200272 sec.
Hardness ratio (energy fluence ratio) = 1.46333
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.69212
Count Ratio (50-100 keV) / (15-25 keV) = 1.2893
Mask shadow pattern
IMX = 8.876470664433727E-01, IMY = 1.300681625568585E-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:
-239.808000 -1.924000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6448 22.0262 0.5 30.0 -89.8 10.5810 21.2 1.0 Crab
133.3891 -28.8570 2.9 48.6 142.4 5.9263 4.0 ------ UNKNOWN
158.6531 32.0132 3.2 42.6 44.3 2.8716 3.6 ------ UNKNOWN
122.7691 -21.4930 2.9 38.6 152.3 2.2279 4.0 ------ UNKNOWN
157.3589 61.0460 3.5 54.0 8.1 4.1475 3.3 ------ UNKNOWN
118.0108 8.4583 3.6 8.4 142.3 0.9348 3.2 ------ UNKNOWN
91.1689 -13.5527 2.7 37.9 -156.3 1.9590 4.2 ------ UNKNOWN
93.4420 68.6592 3.1 54.1 -25.2 4.4677 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.924000 16.692600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6797 21.8799 4.7 29.9 -90.1 -0.2294 -2.5 8.5 Crab
126.0103 -19.6796 2.2 37.6 146.8 0.5754 5.2 ------ UNKNOWN
131.0507 42.2278 2.9 29.4 9.1 0.2786 4.0 ------ UNKNOWN
124.1572 57.5832 0.7 41.9 -8.3 1.6648 17.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
81.692630 962.282000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6276 21.9998 0.5 46.0 -169.4 33.0587 22.0 0.9 Crab
158.3838 37.9569 3.0 29.7 70.2 5.3876 3.8 ------ UNKNOWN
221.3842 48.5541 4.2 54.0 8.1 9.7055 2.8 ------ UNKNOWN
171.0412 58.9687 3.2 24.2 20.5 3.1511 3.7 ------ UNKNOWN
202.0549 60.3771 3.0 37.9 5.7 4.3563 3.9 ------ UNKNOWN
240.6515 52.3381 5.8 58.5 -6.3 13.7012 2.0 ------ UNKNOWN
241.8116 62.9519 3.7 50.3 -14.6 6.7704 3.1 ------ UNKNOWN
68.2871 19.1633 4.1 55.8 -155.3 9.7763 2.9 ------ UNKNOWN
55.2730 37.2277 2.8 48.3 -129.9 18.4054 4.1 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:13:19 EDT 2022