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
83.5338 +21.5938 0.0102 11.6 131.8 2.2443 18.7 TRIG_01186908
------------------------------------------
Foreground time interval of the image:
0.000 12.420 (delta_t = 12.420 [sec])
14.000 64.000 (delta_t = 50.000 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 64.000000
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 64.000000
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
Multiple GTIs in the spectrum
tstart tstop
0.000000 12.420000
14.000000 64.000000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99107 ( -0.126588 0.130359 )
Norm@50keV : 1.94577E-03 ( -0.000157287 0.000154956 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.87 using 59 PHA bins.
# Reduced chi-squared = 1.103 for 57 degrees of freedom
# Null hypothesis probability = 2.763941e-01
Photon flux (15-150 keV) in 62.42 sec: 0.290674 ( -0.0190758 0.0190913 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11953e-06 ( -8.52626e-08 8.63936e-08 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 12.420000
14.000000 64.000000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67243 ( -0.569626 0.486519 )
Epeak [keV] : 43.5615 ( )
Norm@50keV : 2.95245E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.71 using 59 PHA bins.
# Reduced chi-squared = 1.102 for 56 degrees of freedom
# Null hypothesis probability = 2.792888e-01
Photon flux (15-150 keV) in 62.42 sec: 0.285934 ( -0.020447 0.020379 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07983e-06 ( -1.03892e-07 1.05796e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 12.420000
14.000000 64.000000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.74262 ( -0.284475 -0.284475 )
beta : -2.07029 ( 2.07394 0.167131 )
Epeak [keV] : 23.1071 ( -25.0041 75.6475 )
Norm@50keV : 1.55651 ( -1.5586 296.292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.91 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 55 degrees of freedom
# Null hypothesis probability = 2.718100e-01
Photon flux (15-150 keV) in 62.42 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08483e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.0891 (-0.801242 0.87573)
R^2/D10^2 : 0.126549 (-0.0347799 0.0478931)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 109.26 using 59 PHA bins.
# Reduced chi-squared = 1.9168 for 57 degrees of freedom
# Null hypothesis probability = 3.849622e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.642e-07 1.851e-08
25- 50 4.135e-07 3.246e-08
50-150 2.214e-07 4.095e-08
15-150 7.992e-07 5.836e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 68.4525 (-13.3457 18.8206)
Norm : 1.42508 (-0.15494 0.18002)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.277e-07 2.026e-08
25- 50 3.600e-07 2.316e-08
50-150 4.547e-07 8.395e-08
15-150 1.042e-06 9.738e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.68543 (-1.24403 1.41877)
R1^2/D10^2 : 0.808913 (-0.42855 1.24486)
kT2 [keV] : 19.1331 (-4.23979 8.7237)
R2^2/D10^2 : 7.78298E-03 (-0.00587117 0.00818655)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.347e-07 5.743e-08
25- 50 3.454e-07 7.537e-08
50-150 4.670e-07 1.884e-07
15-150 1.047e-06 3.097e-07
Peak spectrum fit
Power-law model
Time interval is from 14.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99107 ( -0.126588 0.130359 )
Norm@50keV : 1.94577E-03 ( -0.000157287 0.000154956 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.87 using 59 PHA bins.
# Reduced chi-squared = 1.103 for 57 degrees of freedom
# Null hypothesis probability = 2.763941e-01
Photon flux (15-150 keV) in 62.42 sec: 0.290674 ( -0.0190758 0.0190913 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11953e-06 ( -8.52626e-08 8.63936e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 14.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67243 ( -0.569626 0.486519 )
Epeak [keV] : 43.5615 ( )
Norm@50keV : 2.95245E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.71 using 59 PHA bins.
# Reduced chi-squared = 1.102 for 56 degrees of freedom
# Null hypothesis probability = 2.792888e-01
Photon flux (15-150 keV) in 62.42 sec: 0.285934 ( -0.020447 0.020379 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07983e-06 ( -1.03892e-07 1.05796e-07 ) ergs/cm2
Band function
Time interval is from 14.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.74262 ( -0.284475 -0.284475 )
beta : -2.07029 ( 2.07394 0.167131 )
Epeak [keV] : 23.1071 ( -25.0041 75.6475 )
Norm@50keV : 1.55651 ( -1.5586 296.283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.91 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 55 degrees of freedom
# Null hypothesis probability = 2.718100e-01
Photon flux (15-150 keV) in 62.42 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08483e-06 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.0891 (-0.801242 0.87573)
R^2/D10^2 : 0.126549 (-0.0347799 0.0478931)
(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 1.642e-07 1.919e-08
25- 50 4.135e-07 3.386e-08
50-150 2.214e-07 3.758e-08
15-150 7.992e-07 5.930e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 68.4525 (-13.3457 18.8206)
Norm : 1.42508 (-0.15494 0.18002)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.277e-07 2.041e-08
25- 50 3.600e-07 2.400e-08
50-150 4.547e-07 7.522e-08
15-150 1.042e-06 9.145e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.68543 (-1.24403 1.41877)
R1^2/D10^2 : 0.808913 (-0.42855 1.24486)
kT2 [keV] : 19.1331 (-4.23979 8.7237)
R2^2/D10^2 : 7.78298E-03 (-0.00587117 0.00818655)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.347e-07 6.816e-08
25- 50 3.454e-07 9.070e-08
50-150 4.670e-07 2.062e-07
15-150 1.047e-06 2.681e-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: 1.99107 ( -0.126588 0.130359 )
Norm@50keV : 1.94577E-03 ( -0.000157287 0.000154956 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.87 using 59 PHA bins.
# Reduced chi-squared = 1.103 for 57 degrees of freedom
# Null hypothesis probability = 2.763941e-01
Photon flux (15-150 keV) in 62.42 sec: 0.290674 ( -0.0190758 0.0190913 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11953e-06 ( -8.52626e-08 8.63936e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67243 ( -0.569626 0.486519 )
Epeak [keV] : 43.5615 ( )
Norm@50keV : 2.95245E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.71 using 59 PHA bins.
# Reduced chi-squared = 1.102 for 56 degrees of freedom
# Null hypothesis probability = 2.792888e-01
Photon flux (15-150 keV) in 62.42 sec: 0.285934 ( -0.020447 0.020379 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07983e-06 ( -1.03892e-07 1.05796e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.74262 ( -0.284475 -0.284475 )
beta : -2.07029 ( 2.07394 0.167131 )
Epeak [keV] : 23.1071 ( -25.0041 75.6475 )
Norm@50keV : 1.55651 ( -1.5586 296.295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.91 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 55 degrees of freedom
# Null hypothesis probability = 2.718100e-01
Photon flux (15-150 keV) in 62.42 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08483e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.36e-07
S(50-100 keV) = 3.38e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.00595
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.940734
Count Ratio (50-100 keV) / (15-25 keV) = 0.465192
Mask shadow pattern
IMX = -1.366781061899295E-01, IMY = -1.526540725336933E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 12.420000
14.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5156 21.8325 0.0 11.7 132.8 0.5928 4.9 12.7 Crab
79.1565 32.0939 2.7 21.2 153.3 0.5352 4.2 ------ UNKNOWN
91.2572 -13.3436 3.0 29.4 16.4 0.5522 3.9 ------ UNKNOWN
133.3774 17.3631 2.0 37.5 -87.3 1.8215 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
120.000590 296.060000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5344 21.8587 3.2 0.3 -175.7 0.9451 3.6 10.8 Crab
76.3264 -21.2541 2.7 43.4 13.3 2.2206 4.3 ------ UNKNOWN
98.6026 9.0076 2.3 19.2 -47.8 1.4739 5.1 ------ UNKNOWN
99.9071 -19.2409 2.4 43.9 -19.1 2.2465 4.8 ------ UNKNOWN
110.4517 -21.5266 2.7 50.5 -29.6 3.0566 4.2 ------ UNKNOWN
Plot creation:
Fri Aug 25 04:08:04 EDT 2023