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
123.9705 30.3389 0.0162 16.3717 29.6809 1.0779759 11.897 TRIG_01102281
Foreground time interval of the image:
-11.940 40.236 (delta_t = 52.176 [sec])
Background time interval of the image:
-239.168 -11.940 (delta_t = 227.228 [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 8.192000
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 8.192000
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 8.192000
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 -11.940 sec. to 40.236 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54743 ( -0.208003 0.212775 )
Norm@50keV : 1.24582E-03 ( -0.000166159 0.000164327 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.25 using 59 bins.
Reduced chi-squared = 1.00439
# Null hypothesis probability of 4.66e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52.18 sec: 0.157601 ( -0.019695 0.019706 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.12285e-07 ( -8.83543e-08 8.99197e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -11.940 sec. to 40.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.465204 ( -1.18658 0.91575 )
Epeak [keV] : 65.5312 ( -14.8832 98.0619 )
Norm@50keV : 4.73945E-03 ( -0.00473945 0.0158465 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.03 using 59 bins.
Reduced chi-squared = 0.946964
# Null hypothesis probability of 5.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52.18 sec: 0.151243 ( -0.020414 0.020419 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.56014e-07 ( -9.59762e-08 1.00727e-07 ) ergs/cm2
Band function
Time interval is from -11.940 sec. to 40.236 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] : 13.2213 (-1.80651 2.17696)
R^2/D10^2 : 2.84795E-02 (-0.0119745 0.0197174)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.48 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 5.507e-08 1.237e-08
25- 50 1.931e-07 3.520e-08
50-150 2.155e-07 6.079e-08
15-150 4.637e-07 7.417e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 181.054 (-79.2502 -177.821)
Norm : 0.647363 (-0.0827429 0.0962344)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.513e-08 4.696e-08
25- 50 1.619e-07 8.698e-08
50-150 3.434e-07 1.917e-07
15-150 5.904e-07 3.180e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.51561 (-3.73688 3.37692)
R1^2/D10^2 : 8.61066E-02 (-0.0521309 0.352102)
kT2 [keV] : 24.4810 (-19.6242 58.7087)
R2^2/D10^2 : 1.99067E-03 (-0.00200466 0.0124733)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.76e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.241e-08 4.214e-08
25- 50 1.809e-07 9.914e-08
50-150 3.118e-07 1.775e-07
15-150 5.652e-07 2.972e-07
Peak spectrum fit
Power-law model
Time interval is from 6.876 sec. to 7.876 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49858 ( -0.494537 0.507033 )
Norm@50keV : 4.26320E-03 ( -0.00122339 0.00118176 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.17 using 59 bins.
Reduced chi-squared = 0.985439
# Null hypothesis probability of 5.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.532023 ( -0.142778 0.142994 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.04585e-08 ( -1.24629e-08 1.28676e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.876 sec. to 7.876 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49028 ( -0.4951 0.689802 )
Epeak [keV] : 9999.26 ( -9999.36 -9999.36 )
Norm@50keV : 4.27874E-03 ( -0.00122949 0.0357934 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.17 using 59 bins.
Reduced chi-squared = 1.00304
# Null hypothesis probability of 4.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.534059 ( -0.149554 0.143795 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.06799e-08 ( -1.36061e-08 9.19132e-09 ) ergs/cm2
Band function
Time interval is from 6.876 sec. to 7.876 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] : 15.4388 (-5.08607 7.57301)
R^2/D10^2 : 5.35371E-02 (-0.0532791 0.161633)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.37e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.658e-09 1.636e-09
25- 50 1.084e-08 6.510e-09
50-150 1.781e-08 1.111e-08
15-150 3.131e-08 1.696e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 2.17014 (-0.577977 0.578183)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.97e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.404e-09 3.272e-09
25- 50 1.039e-08 6.240e-09
50-150 2.280e-08 1.383e-08
15-150 3.860e-08 2.292e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.08881 (-3.06872 7.17806)
R1^2/D10^2 : 1.86221 (-1.72102 205.471)
kT2 [keV] : 23.5900 (-9.28886 -23.5967)
R2^2/D10^2 : 1.06155E-02 (-0.0102879 0.0359813)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.41e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.914e-09 3.525e-09
25- 50 9.130e-09 4.723e-09
50-150 2.430e-08 1.508e-08
15-150 3.934e-08 2.061e-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: 1.54743 ( -0.208003 0.212775 )
Norm@50keV : 1.24582E-03 ( -0.000166159 0.000164327 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.66e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52.18 sec: 0.157596 ( -0.019694 0.0197054 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.12202e-07 ( -8.83079e-08 8.99521e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.465203 ( -1.18658 0.915751 )
Epeak [keV] : 65.5311 ( -14.8832 98.062 )
Norm@50keV : 4.73946E-03 ( -0.00473946 0.0158465 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52.18 sec: 0.151227 ( -0.020409 0.020415 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.56207e-07 ( -9.60931e-08 1.00827e-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) = 1.55e-07
S(50-100 keV) = 2.12e-07
T90 vs. Hardness ratio plot
T90 = 44.2599999904633 sec.
Hardness ratio (energy fluence ratio) = 1.36774
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.89723
Count Ratio (50-100 keV) / (15-25 keV) = 1.04291
Mask shadow pattern
IMX = 2.552340665624958E-01, IMY = -1.454701450132551E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.168000 -11.940000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6424 22.0241 0.6 29.9 -73.6 9.1538 20.5 0.8 Crab
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-11.940000 40.236000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4549 22.1105 0.0 30.1 -73.4 0.4176 2.8 11.5 Crab
123.9704 30.3389 1.0 16.4 29.7 1.0780 11.9 ------ UNKNOWN
96.0116 31.3919 2.3 22.8 -44.7 0.4782 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
105.332600 653.893200
654.832000 659.167400
660.832000 838.671800
840.832000 963.017500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6367 22.0053 1.1 36.9 -107.3 27.0476 10.9 0.6 Crab
196.4775 68.2167 7.3 55.6 11.3 5.2505 1.6 ------ UNKNOWN
117.7374 49.5448 2.8 19.8 -26.1 3.8940 4.1 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:02:25 EDT 2022