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
80.2423 1.2856 0.0172 42.6196 -12.3466 0.1601929 11.169 TRIG_01073893
Foreground time interval of the image:
0.052 0.236 (delta_t = 0.184 [sec])
Background time interval of the image:
-239.312 0.052 (delta_t = 239.364 [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 0.256000
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 0.256000
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 0.256000
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 0.052 sec. to 0.236 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57652 ( -0.261337 0.284584 )
Norm@50keV : 5.07332E-02 ( -0.00895201 0.0087584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.40 using 59 bins.
Reduced chi-squared = 0.708772
# Null hypothesis probability of 9.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.184 sec: 6.47313 ( -1.05376 1.0541 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.75726e-08 ( -1.654e-08 1.66754e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.052 sec. to 0.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14456 ( -1.10238 0.676514 )
Epeak [keV] : 107.595 ( -49.5811 -107.59 )
Norm@50keV : 8.22471E-02 ( -0.0822497 0.194258 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.75 using 59 bins.
Reduced chi-squared = 0.709821
# Null hypothesis probability of 9.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.184 sec: 6.41966 ( -1.06217 1.06068 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.36189e-08 ( -1.95375e-08 1.49612e-08 ) ergs/cm2
Band function
Time interval is from 0.052 sec. to 0.236 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] : 15.0689 (-3.20418 4.05672)
R^2/D10^2 : 0.738701 (-0.408946 0.921893)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.34e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.457e-09 1.910e-09
25- 50 2.576e-08 6.670e-09
50-150 3.989e-08 1.525e-08
15-150 7.212e-08 1.703e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.324 (-102.783 -199.341)
Norm : 26.5605 (-4.28566 4.29978)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.59e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.217e-08 7.098e-09
25- 50 2.341e-08 1.297e-08
50-150 5.134e-08 2.853e-08
15-150 8.692e-08 4.980e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.36297 (-2.27473 5.30849)
R1^2/D10^2 : 39.4464 (-36.7239 160.639)
kT2 [keV] : 21.6068 (-5.88575 14.5461)
R2^2/D10^2 : 0.188118 (-0.161991 0.412998)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.43e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.292e-08 6.944e-09
25- 50 2.032e-08 1.015e-08
50-150 5.507e-08 2.940e-08
15-150 8.831e-08 4.248e-08
Peak spectrum fit
Power-law model
Time interval is from -0.354 sec. to 0.646 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31044 ( -0.421185 0.422539 )
Norm@50keV : 1.23179E-02 ( -0.00283687 0.0028283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.63 using 59 bins.
Reduced chi-squared = 0.870702
# Null hypothesis probability of 7.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.47244 ( -0.34498 0.34645 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21431e-07 ( -3.11638e-08 3.1639e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.354 sec. to 0.646 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.71290 ( -3.06167 1.35011 )
Epeak [keV] : 220.521 ( )
Norm@50keV : 1.83020E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.85 using 59 bins.
Reduced chi-squared = 0.872321
# Null hypothesis probability of 7.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.47622 ( -0.36664 0.3471 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21776e-07 ( -3.42595e-08 2.7727e-08 ) ergs/cm2
Band function
Time interval is from -0.354 sec. to 0.646 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] : 17.2408 (-4.41096 6.74129)
R^2/D10^2 : 0.107848 (-0.072102 0.185318)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.503e-09 3.019e-09
25- 50 2.910e-08 1.498e-08
50-150 6.202e-08 3.461e-08
15-150 9.762e-08 4.106e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-97.1073 -199.363)
Norm : 6.07734 (-1.40468 1.40473)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.06e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.513e-08 9.050e-09
25- 50 2.911e-08 1.711e-08
50-150 6.385e-08 3.793e-08
15-150 1.081e-07 6.330e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.83238 (-1.68821 14.7287)
R1^2/D10^2 : 1596.13 (-1249.79 -1250.7)
kT2 [keV] : 19.2207 (-5.23696 9.62948)
R2^2/D10^2 : 7.18863E-02 (-0.0627791 0.0827428)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.89e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.57652 ( -0.261337 0.284584 )
Norm@50keV : 5.07332E-02 ( -0.00895201 0.0087584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.184 sec: 6.47292 ( -1.05371 1.05405 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.75616e-08 ( -1.65376e-08 1.66876e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14468 ( -1.10238 0.67652 )
Epeak [keV] : 107.610 ( -49.5814 -107.59 )
Norm@50keV : 8.22362E-02 ( -0.0822496 0.194258 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.184 sec: 6.41887 ( -1.06196 1.06046 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.72114e-08 ( -1.70307e-08 1.70134e-08 ) 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) = 2.24e-08
S(50-100 keV) = 3.02e-08
T90 vs. Hardness ratio plot
T90 = 0.163999915122986 sec.
Hardness ratio (energy fluence ratio) = 1.34821
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.20502
Count Ratio (50-100 keV) / (15-25 keV) = 1.11869
Mask shadow pattern
IMX = 8.988959412444540E-01, IMY = 1.967562249808670E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.312000 0.052000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6328 22.0115 0.5 30.9 -42.0 10.4923 21.7 0.2 Crab
40.2931 0.8442 2.9 34.8 52.8 2.4503 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.052000 0.236000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7709 22.0775 8.4 31.0 -42.2 0.0163 1.4 8.5 Crab
348.3355 38.8512 2.1 49.7 148.2 0.1705 5.5 ------ UNKNOWN
80.2424 1.2856 1.0 42.6 -12.3 0.1601 11.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.788600 962.748100
1285.688000 1375.790400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6357 22.0150 0.3 21.0 -169.3 40.0605 33.9 0.1 Crab
43.4723 -8.4313 3.7 37.9 76.3 12.8674 3.2 ------ UNKNOWN
66.3651 -20.3486 2.6 25.5 33.2 5.2119 4.4 ------ UNKNOWN
81.8026 -24.3867 3.5 25.7 -1.5 3.3998 3.3 ------ UNKNOWN
106.5941 -48.0863 3.2 54.4 -19.6 11.9327 3.6 ------ UNKNOWN
105.9571 20.5816 3.0 31.7 -127.5 6.5197 3.8 ------ UNKNOWN
121.1070 7.9544 3.4 41.3 -98.8 16.8106 3.5 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:18:56 EDT 2022