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
40.9059 -65.6611 0.0144 17.2781 135.8566 0.5367789 13.417 TRIG_01150429
Foreground time interval of the image:
-1.248 4.748 (delta_t = 5.996 [sec])
Background time interval of the image:
-239.552 -1.248 (delta_t = 238.304 [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 -1.248 sec. to 4.748 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.06189 ( -0.230193 0.2478 )
Norm@50keV : 4.81542E-03 ( -0.000816691 0.000794275 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 29.70 using 59 bins.
Reduced chi-squared = 0.521053
# Null hypothesis probability of 9.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.996 sec: 0.743712 ( -0.092506 0.092509 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.67413e-07 ( -4.08847e-08 4.20026e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.248 sec. to 4.748 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44643 ( -1.38673 0.680991 )
Epeak [keV] : 35.2389 ( -33.5101 -35.2418 )
Norm@50keV : 1.13365E-02 ( -0.0113507 0.0692555 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 28.77 using 59 bins.
Reduced chi-squared = 0.51375
# Null hypothesis probability of 9.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.996 sec: 0.729451 ( -0.095743 0.095782 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.49461e-07 ( -4.66916e-08 5.18203e-08 ) ergs/cm2
Band function
Time interval is from -1.248 sec. to 4.748 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] : 9.17573 (-1.23657 1.42157)
R^2/D10^2 : 0.485712 (-0.208494 0.367255)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.820e-08 1.030e-08
25- 50 1.056e-07 1.859e-08
50-150 4.272e-08 1.476e-08
15-150 1.965e-07 3.208e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 56.6981 (-17.3977 30.3922)
Norm : 4.01613 (-0.794955 0.991717)
------------------------------------------------------------
#Fit statistic : Chi-Squared 28.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.99e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.993e-08 1.010e-08
25- 50 8.960e-08 1.388e-08
50-150 9.718e-08 3.392e-08
15-150 2.467e-07 4.308e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.81989 (-2.59122 4.31401)
R1^2/D10^2 : 3.51243 (-3.00412 130.534)
kT2 [keV] : 14.1511 (-4.28498 -14.2005)
R2^2/D10^2 : 6.54114E-02 (-0.0642101 0.262819)
------------------------------------------------------------
#Fit statistic : Chi-Squared 29.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.98e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.070e-08 3.277e-08
25- 50 8.859e-08 4.491e-08
50-150 8.349e-08 4.878e-08
15-150 2.328e-07 1.173e-07
Peak spectrum fit
Power-law model
Time interval is from 0.116 sec. to 1.116 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83469 ( -0.344617 0.371189 )
Norm@50keV : 8.14141E-03 ( -0.00197195 0.00189509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.72 using 59 bins.
Reduced chi-squared = 0.837193
# Null hypothesis probability of 8.04e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.13737 ( -0.230153 0.23021 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.48893e-08 ( -1.77349e-08 1.81722e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.116 sec. to 1.116 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60115 ( -1.89319 0.638527 )
Epeak [keV] : 73.1892 ( -73.2079 -73.2373 )
Norm@50keV : 1.11165E-02 ( -0.0111117 0.139285 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.64 using 59 bins.
Reduced chi-squared = 0.850714
# Null hypothesis probability of 7.79e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.13179 ( -0.23291 0.23234 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.32251e-08 ( -2.02405e-08 1.94899e-08 ) ergs/cm2
Band function
Time interval is from 0.116 sec. to 1.116 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] : 10.3689 (-2.20707 2.88327)
R^2/D10^2 : 0.479363 (-0.291547 0.701628)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.21e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.062e-08 4.079e-09
25- 50 2.776e-08 9.735e-09
50-150 1.607e-08 8.595e-09
15-150 5.445e-08 1.996e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.3946 (-43.4617 -89.3952)
Norm : 5.21181 (-1.26706 1.90836)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.360e-08 4.163e-09
25- 50 2.296e-08 7.935e-09
50-150 3.482e-08 2.393e-08
15-150 7.138e-08 3.219e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.16138 (-4.40511 3.54988)
R1^2/D10^2 : 1.51442 (-0.96739 29.6571)
kT2 [keV] : 30.5502 (-31.9433 -35.077)
R2^2/D10^2 : 5.61742E-03 (-0.00355634 0.26558)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.49e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.358e-08 8.050e-09
25- 50 2.331e-08 1.271e-08
50-150 3.627e-08 2.307e-08
15-150 7.316e-08 4.006e-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: 2.06189 ( -0.230193 0.2478 )
Norm@50keV : 4.81542E-03 ( -0.000816691 0.000794275 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 29.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.996 sec: 0.743652 ( -0.0924988 0.0924999 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.6736e-07 ( -4.0856e-08 4.20172e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44671 ( -1.38685 0.680856 )
Epeak [keV] : 35.2379 ( -34.3674 -35.2417 )
Norm@50keV : 1.13320E-02 ( -0.0113503 0.0692564 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 28.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.996 sec: 0.729280 ( -0.095702 0.091755 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4951e-07 ( -4.67148e-08 5.18906e-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) = 8.21e-08
S(50-100 keV) = 7.85e-08
T90 vs. Hardness ratio plot
T90 = 5.36800003051758 sec.
Hardness ratio (energy fluence ratio) = 0.956151
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.05549
Count Ratio (50-100 keV) / (15-25 keV) = 0.421125
Mask shadow pattern
IMX = -2.232059560038941E-01, IMY = -2.166296740017700E-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:
-239.552000 -1.248000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
228.4768 -79.0569 2.4 44.0 -173.2 3.4459 4.8 ------ UNKNOWN
357.7617 2.2809 2.1 58.8 -19.5 10.6714 5.6 191.7 UNKNOWN
354.3318 -1.6489 2.7 55.6 -24.4 7.3345 4.3 354.1 UNKNOWN
335.6887 -19.8616 2.3 44.8 -55.1 6.9167 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.248000 4.748000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
40.9058 -65.6610 0.9 17.3 135.9 0.5368 13.4 ------ UNKNOWN
281.7572 -64.8916 2.3 42.1 -143.2 0.4316 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
71.348600 710.038000
720.448000 782.558200
840.448000 898.763700
900.448000 962.687700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.5426 -60.6619 107.4 48.3 163.0 -0.7948 -0.1 7.1 Cen X-3
186.5091 -62.7488 7.2 49.1 173.3 8.5176 1.6 4.3 GX 301-2
108.4815 -62.4934 2.8 28.2 128.9 7.2817 4.1 ------ UNKNOWN
245.0632 -59.9352 2.5 53.1 -151.8 14.4455 4.6 ------ UNKNOWN
0.6702 -23.2804 2.5 49.5 -37.9 17.7376 4.5 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:15:57 EDT 2023