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
76.9550 -59.8161 0.0208 14.1149 -73.5724 0.6628752 9.296 TRIG_01142997
Foreground time interval of the image:
1.064 21.096 (delta_t = 20.032 [sec])
Background time interval of the image:
-239.896 1.064 (delta_t = 240.960 [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 4.096000
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 4.096000
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 4.096000
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 1.064 sec. to 21.096 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52876 ( -0.259621 0.266231 )
Norm@50keV : 2.18810E-03 ( -0.000359829 0.000354413 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.19 using 59 bins.
Reduced chi-squared = 0.792807
# Null hypothesis probability of 8.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 20.03 sec: 0.275335 ( -0.042158 0.042179 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.13944e-07 ( -7.38718e-08 7.55203e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.064 sec. to 21.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.842201 ( -1.3414 0.870285 )
Epeak [keV] : 77.7986 ( -28.2658 -77.7986 )
Norm@50keV : 5.14139E-03 ( -0.00321049 0.0224365 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.92 using 59 bins.
Reduced chi-squared = 0.784286
# Null hypothesis probability of 8.79e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 20.03 sec: 0.268317 ( -0.043549 0.043495 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87268e-07 ( -8.26742e-08 8.52311e-08 ) ergs/cm2
Band function
Time interval is from 1.064 sec. to 21.096 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] : 13.0335 (-2.30259 2.97521)
R^2/D10^2 : 5.16002E-02 (-0.0267117 0.0516283)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.13e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.724e-08 1.183e-08
25- 50 1.286e-07 3.033e-08
50-150 1.383e-07 5.095e-08
15-150 3.042e-07 7.326e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 196.446 (-103.273 -195.933)
Norm : 1.12845 (-0.172286 0.19949)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.90e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.639e-08 3.195e-08
25- 50 1.083e-07 5.965e-08
50-150 2.363e-07 1.299e-07
15-150 4.010e-07 2.240e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.21480 (-3.36165 3.45239)
R1^2/D10^2 : 0.182241 (-0.117986 0.706096)
kT2 [keV] : 28.3985 (-23.5473 -28.3926)
R2^2/D10^2 : 2.24701E-03 (-0.00221641 0.0175036)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.80e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.127e-08 2.848e-08
25- 50 1.185e-07 6.541e-08
50-150 2.293e-07 1.324e-07
15-150 3.991e-07 2.067e-07
Peak spectrum fit
Power-law model
Time interval is from 3.348 sec. to 4.348 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47294 ( -0.475009 0.485475 )
Norm@50keV : 5.60322E-03 ( -0.00161278 0.00157627 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.93 using 59 bins.
Reduced chi-squared = 0.94614
# Null hypothesis probability of 5.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.694553 ( -0.18927 0.189495 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.34048e-08 ( -1.658e-08 1.71668e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.348 sec. to 4.348 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16234 ( -3.21707 1.29805 )
Epeak [keV] : 124.353 ( -124.708 -124.708 )
Norm@50keV : 8.27841E-03 ( -0.00471339 0.575383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.86 using 59 bins.
Reduced chi-squared = 0.961786
# Null hypothesis probability of 5.56e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.687093 ( -0.197114 0.194343 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.16904e-08 ( -2.01367e-08 1.8544e-08 ) ergs/cm2
Band function
Time interval is from 3.348 sec. to 4.348 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] : 12.6668 (-3.66253 6.07085)
R^2/D10^2 : 0.143871 (-0.107702 0.341276)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.06e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.895e-09 2.961e-09
25- 50 1.639e-08 9.872e-09
50-150 1.637e-08 1.047e-08
15-150 3.765e-08 2.384e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-199.363 -199.363)
Norm : 2.84808 (-0.769815 0.770468)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.92e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.092e-09 4.323e-09
25- 50 1.364e-08 8.250e-09
50-150 2.992e-08 1.803e-08
15-150 5.065e-08 3.034e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.18582 (-4.95977 3.67598)
R1^2/D10^2 : 0.365840 (-0.15933 1.70393)
kT2 [keV] : 54.3673 (-116.36 -126.836)
R2^2/D10^2 : 9.14223E-04 (-0.000152797 0.0599469)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.68e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.348e-09 3.794e-09
25- 50 1.535e-08 9.305e-09
50-150 3.227e-08 1.779e-08
15-150 5.397e-08 2.526e-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: 1.52876 ( -0.259621 0.266231 )
Norm@50keV : 2.18810E-03 ( -0.000359829 0.000354413 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 20.03 sec: 0.275327 ( -0.0421564 0.0421765 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.1389e-07 ( -7.38328e-08 7.5559e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.842213 ( -1.3414 0.870285 )
Epeak [keV] : 77.7993 ( -28.2658 -77.7986 )
Norm@50keV : 5.14131E-03 ( -0.00321049 0.0224365 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.79e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 20.03 sec: 0.268287 ( -0.04354 0.043484 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87404e-07 ( -8.26778e-08 8.53358e-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) = 1.04e-07
S(50-100 keV) = 1.44e-07
T90 vs. Hardness ratio plot
T90 = 16.8319998979568 sec.
Hardness ratio (energy fluence ratio) = 1.38462
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50532
Count Ratio (50-100 keV) / (15-25 keV) = 0.980954
Mask shadow pattern
IMX = 7.111350310776945E-02, IMY = 2.411941707005720E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.896000 1.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5477 -40.5396 2.7 39.1 -160.4 2.6444 4.3 1.3 Vela X-1
53.9413 -12.5821 2.2 40.6 53.9 4.2202 5.4 ------ UNKNOWN
12.1782 -26.8815 3.6 56.9 1.5 5.0635 3.2 ------ UNKNOWN
10.1126 -32.2107 3.2 55.1 -4.9 3.2858 3.6 ------ UNKNOWN
358.1209 -57.3477 2.9 49.5 -37.8 5.3603 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
1.064000 21.096000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4790 -40.4093 5.2 39.1 -160.6 0.2193 2.2 9.0 Vela X-1
76.9551 -59.8160 1.2 14.1 -73.6 0.6633 9.3 ------ UNKNOWN
150.3985 -30.0980 2.0 54.9 -163.6 1.4559 5.7 ------ UNKNOWN
48.5006 -72.9672 2.5 30.9 -64.5 0.4817 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.804640 638.804000
640.104000 654.156000
655.104000 873.653000
875.104000 879.434300
880.104000 962.184000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5616 -40.5714 3.0 40.4 -173.7 7.1334 3.9 1.8 Vela X-1
170.3698 -60.6460 7.6 42.3 -128.8 3.9746 1.5 2.1 Cen X-3
356.4454 -35.6223 3.0 55.3 -4.8 10.0509 3.9 ------ UNKNOWN
Plot creation:
Wed Jun 14 13:54:47 EDT 2023