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
42.6676 -22.9900 0.0076 22.5 168.5 1.3938 25.2 TRIG_01400467
------------------------------------------
Foreground time interval of the image:
-9.976 16.709 (delta_t = 26.685 [sec])
Background time interval of the image:
-239.992 -9.976 (delta_t = 230.016 [sec])
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 -9.976 sec. to 91.720 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48658 ( -0.14372 0.144775 )
Norm@50keV : 1.14184E-03 ( -0.000100693 0.000100308 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.67 using 59 PHA bins.
# Reduced chi-squared = 1.012 for 57 degrees of freedom
# Null hypothesis probability = 4.503479e-01
Photon flux (15-150 keV) in 101.7 sec: 0.142038 ( -0.012415 0.0124295 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10409e-06 ( -1.06089e-07 1.0694e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -9.976 sec. to 91.720 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.640313 ( -0.702886 0.607049 )
Epeak [keV] : 80.3574 ( -17.2373 73.9358 )
Norm@50keV : 3.05185E-03 ( -0.00151641 0.00366043 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.72 using 59 PHA bins.
# Reduced chi-squared = 0.9235 for 56 degrees of freedom
# Null hypothesis probability = 6.376674e-01
Photon flux (15-150 keV) in 101.7 sec: 0.137237 ( -0.012927 0.012905 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04271e-06 ( -1.13451e-07 1.15328e-07 ) ergs/cm2
Band function
Time interval is from -9.976 sec. to 91.720 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.640206 ( -0.243949 0.689043 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 80.3396 ( -14.4119 73.7426 )
Norm@50keV : 3.05223E-03 ( -0.00151696 0.00366236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.72 using 59 PHA bins.
# Reduced chi-squared = 0.9403 for 55 degrees of freedom
# Null hypothesis probability = 6.009071e-01
Photon flux (15-150 keV) in 101.7 sec: 0.138347 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.05153e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.4558 (-1.49154 1.67062)
R^2/D10^2 : 1.49205E-02 (-0.00454423 0.00643525)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.51 using 59 PHA bins.
# Reduced chi-squared = 1.219 for 57 degrees of freedom
# Null hypothesis probability = 1.237364e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.549e-08 1.265e-08
25- 50 3.082e-07 3.615e-08
50-150 5.075e-07 8.955e-08
15-150 8.912e-07 9.590e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-57.1008 -200)
Norm : 0.585107 (-0.0499242 0.0499242)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.482e-07 1.592e-08
25- 50 2.851e-07 4.526e-08
50-150 6.252e-07 2.082e-07
15-150 1.058e-06 4.074e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.50481 (-1.69807 2.33705)
R1^2/D10^2 : 0.261783 (-0.1842 0.768398)
kT2 [keV] : 20.0067 (-2.95188 4.76044)
R2^2/D10^2 : 5.20088E-03 (-0.00297323 0.00441611)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.345e-07 6.635e-08
25- 50 2.803e-07 9.458e-08
50-150 6.082e-07 2.254e-07
15-150 1.023e-06 3.144e-07
Peak spectrum fit
Power-law model
Time interval is from 2.292 sec. to 3.292 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26786 ( -0.244717 0.242871 )
Norm@50keV : 7.12192E-03 ( -0.0011044 0.00110399 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.70 using 59 PHA bins.
# Reduced chi-squared = 1.083 for 57 degrees of freedom
# Null hypothesis probability = 3.116836e-01
Photon flux (15-150 keV) in 1 sec: 0.844849 ( -0.133748 0.134075 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.0944e-08 ( -1.1964e-08 1.20803e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.292 sec. to 3.292 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.155340 ( -1.48891 1.10755 )
Epeak [keV] : 82.0487 ( -18.5603 90.7854 )
Norm@50keV : 3.32284E-02 ( -0.0332249 0.10964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.60 using 59 PHA bins.
# Reduced chi-squared = 1.011 for 56 degrees of freedom
# Null hypothesis probability = 4.525558e-01
Photon flux (15-150 keV) in 1 sec: 0.807486 ( -0.138094 0.137901 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.69216e-08 ( -1.2226e-08 1.25478e-08 ) ergs/cm2
Band function
Time interval is from 2.292 sec. to 3.292 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.136265 ( -1.0208 1.29879 )
beta : -9.37167 ( 9.37167 19.3717 )
Epeak [keV] : 82.6679 ( -17.1155 48.8624 )
Norm@50keV : 3.24499E-02 ( -0.0324406 70.6365 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.60 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 55 degrees of freedom
# Null hypothesis probability = 4.151033e-01
Photon flux (15-150 keV) in 1 sec: 0.808468 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.82925e-08 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 18.3421 (-2.77738 3.34502)
R^2/D10^2 : 5.44633E-02 (-0.023721 0.0401996)
(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 3.646e-09 1.096e-09
25- 50 1.710e-08 3.760e-09
50-150 4.195e-08 1.132e-08
15-150 6.270e-08 1.480e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-56.5868 -200)
Norm : 3.52003 (-0.549898 0.549898)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.765e-09 5.030e-09
25- 50 1.686e-08 9.385e-09
50-150 3.698e-08 2.103e-08
15-150 6.261e-08 3.535e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.59332 (-2.97597 4.31494)
R1^2/D10^2 : 0.947947 (-0.912403 7.0268)
kT2 [keV] : 20.9538 (-3.93263 7.86021)
R2^2/D10^2 : 3.16860E-02 (-0.0245195 0.0297198)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.168e-09 3.524e-09
25- 50 1.652e-08 8.565e-09
50-150 4.439e-08 2.639e-08
15-150 6.708e-08 3.662e-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: 1.38159 ( -0.102954 0.102606 )
Norm@50keV : 3.39997E-03 ( -0.000211362 0.000211212 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.63 using 59 PHA bins.
# Reduced chi-squared = 1.292 for 57 degrees of freedom
# Null hypothesis probability = 6.824411e-02
Photon flux (15-150 keV) in 26.68 sec: 0.412356 ( -0.0262107 0.0262432 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.79877e-07 ( -5.98107e-08 6.00914e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.545326 ( -0.517151 0.45939 )
Epeak [keV] : 87.4452 ( -16.4851 45.7639 )
Norm@50keV : 8.94969E-03 ( -0.00362499 0.00706666 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.13 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 56 degrees of freedom
# Null hypothesis probability = 2.390143e-01
Photon flux (15-150 keV) in 26.68 sec: 0.398895 ( -0.027312 0.027285 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.28342e-07 ( -6.64999e-08 6.67187e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.230804 ( -0.628246 5.22636 )
beta : -1.94201 ( 1.93931 0.452665 )
Epeak [keV] : 71.5908 ( -38.8222 37.1647 )
Norm@50keV : 1.36535E-02 ( -0.00741622 38.2593 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.41 using 59 PHA bins.
# Reduced chi-squared = 1.117 for 55 degrees of freedom
# Null hypothesis probability = 2.572811e-01
Photon flux (15-150 keV) in 26.68 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.33302e-07 ( -8.33115e-07 -6.37118e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.71e-07
S(50-100 keV) = 3.87e-07
T90 vs. Hardness ratio plot
T90 = 75.3279999494553 sec.
Hardness ratio (energy fluence ratio) = 1.42804
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.35054
Count Ratio (50-100 keV) / (15-25 keV) = 1.17496
Mask shadow pattern
IMX = -4.050497680243674E-01, IMY = -8.243610342977839E-02
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:
-239.992000 -9.976000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
26.7625 7.0457 3.4 41.5 111.8 4.6718 3.4 ------ UNKNOWN
351.1504 -33.8256 3.1 24.1 4.3 1.0900 3.7 ------ UNKNOWN
52.7251 -51.0182 3.1 28.9 -122.1 1.3252 3.8 ------ UNKNOWN
82.5113 -50.8719 2.9 47.3 -127.3 5.6370 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-9.976000 16.708600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
42.6676 -22.9900 0.5 22.5 168.5 1.3937 25.2 ------ UNKNOWN
89.2120 -33.0085 2.1 56.3 -148.1 1.6913 5.6 ------ UNKNOWN
88.7997 -34.8936 2.0 55.3 -146.1 1.5548 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
98.208600 607.838000
609.008000 704.328000
705.008000 962.121600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
348.2968 -67.3529 3.4 55.4 -11.0 10.8519 3.4 ------ UNKNOWN
91.3839 -12.5641 3.0 47.3 -127.3 19.3592 3.9 ------ UNKNOWN
Plot creation:
Thu Oct 2 15:10:04 EDT 2025