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
229.7032 -57.3604 0.0229 29.3 -157.3 1.4489 8.3 TRIG_01218696
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [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
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42256 ( -0.306633 0.343856 )
Norm@50keV : 9.67765E-04 ( -0.000227652 0.000221281 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.34 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 57 degrees of freedom
# Null hypothesis probability = 3.903853e-01
Photon flux (15-150 keV) in 64 sec: 0.181453 ( -0.0245431 0.0245432 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.07343e-07 ( -1.04719e-07 1.09349e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.88517 ( -1.9883 -1.9883 )
Epeak [keV] : 290.338 ( -99.0297 -302.052 )
Norm@50keV : 5.63028E-04 ( -0.000292242 0.00056188 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.68 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.128623e-01
Photon flux (15-150 keV) in 64 sec: 0.181375 ( -0.024534 0.024534 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.03652e-07 ( -1.01204e-07 1.12828e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.62461 ( 9.62461 9.62461 )
beta : -2.42256 ( -0.34383 0.306293 )
Epeak [keV] : 9.51213 ( -9.51213 -9.51213 )
Norm@50keV : 0.131533 ( -0.0309409 0.0300755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.34 using 59 PHA bins.
# Reduced chi-squared = 1.079 for 55 degrees of freedom
# Null hypothesis probability = 3.204613e-01
Photon flux (15-150 keV) in 64 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] : 6.32082 (-0.949446 1.13876)
R^2/D10^2 : 0.505082 (-0.256281 0.522704)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.12 using 59 PHA bins.
# Reduced chi-squared = 1.283 for 57 degrees of freedom
# Null hypothesis probability = 7.381954e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.842e-07 4.205e-08
25- 50 2.054e-07 4.944e-08
50-150 2.317e-08 1.215e-08
15-150 4.128e-07 8.883e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 32.2781 (-10.7776 19.4616)
Norm : 1.34263 (-0.400362 0.642017)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.812e-07 3.075e-08
25- 50 2.153e-07 4.106e-08
50-150 1.295e-07 6.119e-08
15-150 5.261e-07 1.192e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.37736 (-0.493715 1.07383)
R1^2/D10^2 : 0.933029 (-0.503541 0.723973)
kT2 [keV] : 42.4188 (-21.6264 -42.4289)
R2^2/D10^2 : 3.18450E-04 (-0.000299422 0.00148604)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.971e-07 7.130e-08
25- 50 1.813e-07 6.758e-08
50-150 3.310e-07 1.977e-07
15-150 7.095e-07 2.628e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42256 ( -0.306633 0.343856 )
Norm@50keV : 9.67765E-04 ( -0.000227652 0.000221281 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.34 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 57 degrees of freedom
# Null hypothesis probability = 3.903853e-01
Photon flux (15-150 keV) in 64 sec: 0.181453 ( -0.0245431 0.0245432 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.07343e-07 ( -1.04719e-07 1.09349e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.88517 ( -1.9883 -1.9883 )
Epeak [keV] : 290.338 ( -99.0297 -302.052 )
Norm@50keV : 5.63028E-04 ( -0.000292242 0.00056188 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.68 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.128623e-01
Photon flux (15-150 keV) in 64 sec: 0.181375 ( -0.024534 0.024534 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.03652e-07 ( -1.01204e-07 1.12828e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.62461 ( 9.62461 9.62461 )
beta : -2.42256 ( -0.34383 0.306293 )
Epeak [keV] : 9.51213 ( -9.51213 -9.51213 )
Norm@50keV : 0.131533 ( -0.0309409 0.0300755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.34 using 59 PHA bins.
# Reduced chi-squared = 1.079 for 55 degrees of freedom
# Null hypothesis probability = 3.204613e-01
Photon flux (15-150 keV) in 64 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] : 6.32082 (-0.949446 1.13876)
R^2/D10^2 : 0.505082 (-0.256281 0.522704)
(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 1.842e-07 4.333e-08
25- 50 2.054e-07 5.219e-08
50-150 2.317e-08 1.337e-08
15-150 4.128e-07 9.306e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 32.2781 (-10.7776 19.4616)
Norm : 1.34263 (-0.400362 0.642017)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.812e-07 3.408e-08
25- 50 2.153e-07 4.666e-08
50-150 1.295e-07 6.293e-08
15-150 5.261e-07 1.081e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.37736 (-0.493715 1.07383)
R1^2/D10^2 : 0.933029 (-0.503541 0.723973)
kT2 [keV] : 42.4188 (-21.6264 -42.4289)
R2^2/D10^2 : 3.18450E-04 (-0.000299422 0.00148604)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.971e-07 6.195e-08
25- 50 1.813e-07 6.611e-08
50-150 3.310e-07 1.992e-07
15-150 7.095e-07 2.676e-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: 2.42256 ( -0.306633 0.343856 )
Norm@50keV : 9.67765E-04 ( -0.000227652 0.000221281 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.34 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 57 degrees of freedom
# Null hypothesis probability = 3.903853e-01
Photon flux (15-150 keV) in 64 sec: 0.181453 ( -0.0245431 0.0245432 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.07343e-07 ( -1.04719e-07 1.09349e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.88517 ( -1.9883 -1.9883 )
Epeak [keV] : 290.338 ( -99.0297 -302.052 )
Norm@50keV : 5.63028E-04 ( -0.000292242 0.00056188 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.68 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.128623e-01
Photon flux (15-150 keV) in 64 sec: 0.181375 ( -0.024534 0.024534 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.03652e-07 ( -1.01204e-07 1.12828e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.62461 ( 9.62461 9.62461 )
beta : -2.42256 ( -0.34383 0.306293 )
Epeak [keV] : 9.51213 ( -9.51213 -9.51213 )
Norm@50keV : 0.131533 ( -0.0309409 0.0300755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.34 using 59 PHA bins.
# Reduced chi-squared = 1.079 for 55 degrees of freedom
# Null hypothesis probability = 3.204613e-01
Photon flux (15-150 keV) in 64 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) = 2.00e-07
S(50-100 keV) = 1.49e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.745
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.704042
Count Ratio (50-100 keV) / (15-25 keV) = 0.350671
Mask shadow pattern
IMX = -5.173340099402849E-01, IMY = 2.168167138738900E-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 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3046 -40.6391 17.3 29.9 33.8 0.1176 0.7 11.4 Vela X-1
170.3551 -60.7719 16.2 1.2 97.4 0.0974 0.7 9.0 Cen X-3
186.5990 -62.7531 0.8 7.6 -162.8 1.8142 14.1 1.9 GX 301-2
255.9002 -37.8723 5.7 55.2 -158.9 -1.0735 -2.0 4.4 4U 1700-377
256.3289 -36.3717 3.5 56.7 -159.5 2.0000 3.3 6.0 GX 349+2
264.8521 -44.3923 3.9 53.8 -147.5 -1.8784 -3.0 5.8 4U 1735-44
229.7033 -57.3604 1.4 29.3 -157.3 1.4492 8.3 ------ UNKNOWN
91.8592 -49.6893 2.7 42.7 -16.5 0.8578 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Tue Mar 5 19:50:47 EST 2024