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
129.9636 60.2031 0.0033 31.5573 -124.3267 9.6656736 57.055 TRIG_01035994
Foreground time interval of the image:
-0.176 9.241 (delta_t = 9.417 [sec])
Background time interval of the image:
-239.860 -0.176 (delta_t = 239.684 [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 0.064000
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 0.064000
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 0.064000
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 -0.176 sec. to 734.988 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73758 ( -0.112066 0.114076 )
Norm@50keV : 8.02962E-04 ( -5.74465e-05 5.70016e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.89 using 59 bins.
Reduced chi-squared = 0.962982
# Null hypothesis probability of 5.55e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 735.2 sec: 0.108086 ( -0.007088 0.007093 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.45212e-06 ( -4.03698e-07 4.07853e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.176 sec. to 734.988 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.599724 ( -0.646098 0.557756 )
Epeak [keV] : 54.7878 ( -7.02534 13.3586 )
Norm@50keV : 3.37101E-03 ( -0.00168533 0.00422465 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.02 using 59 bins.
Reduced chi-squared = 0.7325
# Null hypothesis probability of 9.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 735.2 sec: 0.102885 ( -0.0074727 0.007486 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.90677e-06 ( -4.51791e-07 4.68814e-07 ) ergs/cm2
Band function
Time interval is from -0.176 sec. to 734.988 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] : 11.9882 (-0.832503 0.90359)
R^2/D10^2 : 2.67867E-02 (-0.00636467 0.00823688)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.986e-07 6.620e-08
25- 50 1.882e-06 1.540e-07
50-150 1.625e-06 2.400e-07
15-150 4.105e-06 3.353e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 105.222 (-22.0883 37.2258)
Norm : 0.477352 (-0.0418812 0.0441328)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.171e-07 9.594e-08
25- 50 1.602e-06 1.268e-07
50-150 2.670e-06 8.359e-07
15-150 5.189e-06 9.664e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.10549 (-2.48835 2.04181)
R1^2/D10^2 : 7.56849E-02 (-0.0340926 0.128013)
kT2 [keV] : 22.6548 (-7.06521 24.8272)
R2^2/D10^2 : 1.50564E-03 (-0.00138622 0.00647472)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.24e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.712e-07 1.892e-07
25- 50 1.753e-06 4.900e-07
50-150 2.467e-06 1.132e-06
15-150 4.991e-06 1.595e-06
Peak spectrum fit
Power-law model
Time interval is from 7.504 sec. to 8.504 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74586 ( -0.0540926 0.05449 )
Norm@50keV : 0.153877 ( -0.00519827 0.00519157 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 103.99 using 59 bins.
Reduced chi-squared = 1.82439
# Null hypothesis probability of 1.44e-04 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 20.7762 ( -0.731 0.7321 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.42043e-06 ( -4.91062e-08 4.91729e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.504 sec. to 8.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.618669 ( -0.278142 0.262511 )
Epeak [keV] : 62.8104 ( -4.11045 5.33028 )
Norm@50keV : 0.552749 ( -0.139608 0.200295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.13 using 59 bins.
Reduced chi-squared = 0.716607
# Null hypothesis probability of 9.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 19.6990 ( -0.7592 0.7616 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3489e-06 ( -5.19895e-08 5.20415e-08 ) ergs/cm2
Band function
Time interval is from 7.504 sec. to 8.504 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] : 14.0524 ( )
R^2/D10^2 : 2.92165 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 150.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.55e-10 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.218e-07 7.850e-09
25- 50 4.548e-07 1.790e-08
50-150 5.925e-07 3.680e-08
15-150 1.169e-06 4.050e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 116.430 (-12.128 19.0505)
Norm : 90.4568 (-4.34581 3.85295)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.85e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.270e-07 1.525e-08
25- 50 4.089e-07 2.075e-08
50-150 7.437e-07 1.710e-07
15-150 1.380e-06 1.855e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.10964 (-1.06663 1.16791)
R1^2/D10^2 : 18.0023 (-6.57259 12.6395)
kT2 [keV] : 20.1341 (-1.86022 2.59846)
R2^2/D10^2 : 0.575328 (-0.244712 0.315583)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.30e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.934e-07 2.830e-08
25- 50 4.339e-07 3.825e-08
50-150 7.115e-07 6.570e-08
15-150 1.339e-06 1.375e-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: 1.90490 ( -0.0390888 0.0392223 )
Norm@50keV : 6.51320E-02 ( -0.00141121 0.00141064 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 107.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.51e-05 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.417 sec: 9.36662 ( -0.23724 0.238215 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.63919e-06 ( -1.21832e-07 1.21851e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14589 ( -0.190712 0.18313 )
Epeak [keV] : 59.1421 ( -3.45177 4.26488 )
Norm@50keV : 0.149116 ( -0.0264993 0.0337982 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.417 sec: 8.79879 ( -0.26289 0.26484 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37606e-06 ( -1.36518e-07 1.36283e-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) = 1.50e-06
S(50-100 keV) = 1.80e-06
T90 vs. Hardness ratio plot
T90 = 637.31199991703 sec.
Hardness ratio (energy fluence ratio) = 1.2
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.46135
Count Ratio (50-100 keV) / (15-25 keV) = 0.757806
Mask shadow pattern
IMX = -3.463410182310839E-01, IMY = 5.072082088400764E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-239.860000 -0.176000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
177.6967 -0.0155 2.6 39.7 71.4 4.2635 4.4 ------ UNKNOWN
208.9944 22.4756 3.1 39.8 10.4 1.6659 3.7 ------ UNKNOWN
228.9031 33.1161 3.0 50.3 -14.8 2.6967 3.9 ------ UNKNOWN
92.7945 38.4551 3.2 55.8 -155.3 4.8507 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.176000 9.240590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
156.8273 20.3095 2.5 19.6 116.5 0.4663 4.5 ------ UNKNOWN
232.9648 22.2109 2.8 58.7 -5.1 2.3476 4.2 ------ UNKNOWN
129.9636 60.2031 0.2 31.6 -124.3 9.6655 57.1 ------ UNKNOWN
100.8076 48.0610 3.0 47.2 -146.1 0.9594 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.040610 902.210000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6099 21.9841 4.2 50.0 -165.6 22.6805 2.7 2.2 Crab
191.3472 34.5439 3.8 46.5 48.0 39.2271 3.1 ------ UNKNOWN
79.7732 15.3055 2.8 57.6 -165.4 55.4716 4.2 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:12:15 EDT 2022