Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
83.4662 +22.2880 0.0114 15.3 53.7 2.6195 16.8 TRIG_01209403
------------------------------------------
Foreground time interval of the image:
0.000 72.000 (delta_t = 72.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from 0.000 sec. to 72.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.16617 ( -0.137784 0.143344 )
Norm@50keV : 1.97731E-03 ( -0.000179985 0.000177001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.68 using 59 PHA bins.
# Reduced chi-squared = 0.7839 for 57 degrees of freedom
# Null hypothesis probability = 8.821225e-01
Photon flux (15-150 keV) in 72 sec: 0.321639 ( -0.0214776 0.0214959 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33252e-06 ( -1.04705e-07 1.06455e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 72.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93196 ( -0.596135 0.0672994 )
Epeak [keV] : 11.8384 ( -10.0633 -11.8439 )
Norm@50keV : 2.70564E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.11 using 59 PHA bins.
# Reduced chi-squared = 0.7876 for 56 degrees of freedom
# Null hypothesis probability = 8.750855e-01
Photon flux (15-150 keV) in 72 sec: 0.317547 ( -0.023197 0.023023 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.29615e-06 ( -1.29614e-07 1.30226e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 72.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.06147 ( 1.06056 1.06056 )
beta : -2.26185 ( 2.26031 0.196695 )
Epeak [keV] : 24.0542 ( -23.6965 12.4564 )
Norm@50keV : 1.17348E-02 ( -0.0135903 1859.23 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.49 using 59 PHA bins.
# Reduced chi-squared = 0.7907 for 55 degrees of freedom
# Null hypothesis probability = 8.686728e-01
Photon flux (15-150 keV) in 72 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] : 8.92304 (-0.739019 0.810262)
R^2/D10^2 : 0.218432 (-0.0637445 0.0902864)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 92.43 using 59 PHA bins.
# Reduced chi-squared = 1.622 for 57 degrees of freedom
# Null hypothesis probability = 2.078920e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.427e-07 2.729e-08
25- 50 5.090e-07 3.852e-08
50-150 1.891e-07 4.014e-08
15-150 9.408e-07 7.524e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.8723 (-9.5454 13.3012)
Norm : 1.75356 (-0.20788 0.257972)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.112e-07 3.056e-08
25- 50 4.528e-07 3.280e-08
50-150 4.549e-07 8.086e-08
15-150 1.219e-06 1.048e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.31501 (-0.942322 1.01297)
R1^2/D10^2 : 1.28549 (-0.619044 1.52731)
kT2 [keV] : 18.3355 (-3.79071 6.25383)
R2^2/D10^2 : 9.04798E-03 (-0.00618137 0.0146766)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.292e-07 8.928e-08
25- 50 4.206e-07 1.027e-07
50-150 5.127e-07 2.720e-07
15-150 1.263e-06 3.626e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 72.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.16617 ( -0.137784 0.143344 )
Norm@50keV : 1.97731E-03 ( -0.000179985 0.000177001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.68 using 59 PHA bins.
# Reduced chi-squared = 0.7839 for 57 degrees of freedom
# Null hypothesis probability = 8.821225e-01
Photon flux (15-150 keV) in 72 sec: 0.321639 ( -0.0214776 0.0214959 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33252e-06 ( -1.04705e-07 1.06455e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 72.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93196 ( -0.596135 0.0672994 )
Epeak [keV] : 11.8384 ( -10.0633 -11.8439 )
Norm@50keV : 2.70564E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.11 using 59 PHA bins.
# Reduced chi-squared = 0.7876 for 56 degrees of freedom
# Null hypothesis probability = 8.750855e-01
Photon flux (15-150 keV) in 72 sec: 0.317547 ( -0.023197 0.023023 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.29615e-06 ( -1.29614e-07 1.30147e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 72.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.06147 ( 1.06056 1.06056 )
beta : -2.26185 ( 2.26031 0.196695 )
Epeak [keV] : 24.0542 ( -23.6965 12.4564 )
Norm@50keV : 1.17348E-02 ( -0.0135903 2354.6 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.49 using 59 PHA bins.
# Reduced chi-squared = 0.7907 for 55 degrees of freedom
# Null hypothesis probability = 8.686728e-01
Photon flux (15-150 keV) in 72 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.92304 (-0.739019 0.810262)
R^2/D10^2 : 0.218432 (-0.0637445 0.0902864)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.427e-07 2.815e-08
25- 50 5.090e-07 4.208e-08
50-150 1.891e-07 3.946e-08
15-150 9.408e-07 7.704e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.8723 (-9.5454 13.3012)
Norm : 1.75356 (-0.20788 0.257972)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.112e-07 2.801e-08
25- 50 4.528e-07 3.085e-08
50-150 4.549e-07 7.970e-08
15-150 1.219e-06 1.076e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.31501 (-0.942322 1.01297)
R1^2/D10^2 : 1.28549 (-0.619044 1.52731)
kT2 [keV] : 18.3355 (-3.79071 6.25383)
R2^2/D10^2 : 9.04798E-03 (-0.00618137 0.0146766)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.292e-07 8.100e-08
25- 50 4.206e-07 9.454e-08
50-150 5.127e-07 2.317e-07
15-150 1.263e-06 3.934e-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: 2.16617 ( -0.137784 0.143344 )
Norm@50keV : 1.97731E-03 ( -0.000179985 0.000177001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.68 using 59 PHA bins.
# Reduced chi-squared = 0.7839 for 57 degrees of freedom
# Null hypothesis probability = 8.821225e-01
Photon flux (15-150 keV) in 72 sec: 0.321639 ( -0.0214776 0.0214959 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33252e-06 ( -1.04705e-07 1.06455e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93196 ( -0.596135 0.0672994 )
Epeak [keV] : 11.8384 ( -10.0633 -11.8439 )
Norm@50keV : 2.70564E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.11 using 59 PHA bins.
# Reduced chi-squared = 0.7876 for 56 degrees of freedom
# Null hypothesis probability = 8.750855e-01
Photon flux (15-150 keV) in 72 sec: 0.317547 ( -0.023197 0.023023 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.29615e-06 ( -1.29614e-07 1.30147e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.06147 ( 1.06056 1.06056 )
beta : -2.26185 ( 2.26031 0.196695 )
Epeak [keV] : 24.0542 ( -23.6965 12.4564 )
Norm@50keV : 1.17348E-02 ( -0.0135903 1859.23 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.49 using 59 PHA bins.
# Reduced chi-squared = 0.7907 for 55 degrees of freedom
# Null hypothesis probability = 8.686728e-01
Photon flux (15-150 keV) in 72 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) = 4.19e-07
S(50-100 keV) = 3.73e-07
T90 vs. Hardness ratio plot
T90 = 72 sec.
Hardness ratio (energy fluence ratio) = 0.890215
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.935585
Count Ratio (50-100 keV) / (15-25 keV) = 0.429969
Mask shadow pattern
IMX = 1.621066919308871E-01, IMY = -2.203243405290099E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 72.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4690 22.1448 1.1 15.2 54.1 1.6462 10.6 12.0 Crab
104.1466 21.8208 2.6 32.2 77.6 1.4122 4.4 ------ UNKNOWN
44.6887 42.4187 2.2 39.2 -22.0 1.0390 5.1 ------ UNKNOWN
23.4048 58.3276 2.5 59.6 -16.6 3.6940 4.5 ------ UNKNOWN
36.9717 2.9685 3.1 36.0 -90.1 1.1194 3.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
127.800640 243.062800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4884 22.1548 1.0 0.1 172.6 2.4885 11.8 11.6 Crab
84.1323 -1.4021 2.3 23.7 -177.3 1.0403 5.1 ------ UNKNOWN
64.0097 -22.3966 2.8 48.5 -151.4 1.7994 4.1 ------ UNKNOWN
50.1893 11.4650 2.2 33.5 -99.0 1.6864 5.2 ------ UNKNOWN
49.8446 -12.7437 2.8 48.1 -129.2 3.9041 4.1 ------ UNKNOWN
Plot creation:
Thu Jan 18 10:00:04 EST 2024