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
139.9009 +12.6444 0.0093 17.2 -42.5 1.2046 20.7 TRIG_01519536
------------------------------------------
Foreground time interval of the image:
-0.704 18.973 (delta_t = 19.677 [sec])
Background time interval of the image:
-179.128 -0.704 (delta_t = 178.424 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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 1.024000
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 1.024000
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 -0.704 sec. to 93.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08604 ( -0.167236 0.161961 )
Norm@50keV : 1.46421E-03 ( -0.000122337 0.0001217 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.57 using 59 PHA bins.
# Reduced chi-squared = 1.115 for 57 degrees of freedom
# Null hypothesis probability = 2.561990e-01
Photon flux (15-150 keV) in 93.81 sec: 0.169619 ( -0.014803 0.0148837 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44256e-06 ( -1.28379e-07 1.28913e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.704 sec. to 93.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08173 ( -0.186584 0.147117 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.47218E-03 ( -0.000122728 0.000120063 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.66 using 59 PHA bins.
# Reduced chi-squared = 1.137 for 56 degrees of freedom
# Null hypothesis probability = 2.248783e-01
Photon flux (15-150 keV) in 93.81 sec: 0.169560 ( -0.014841 0.014844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44658e-06 ( -1.32385e-07 1.23276e-07 ) ergs/cm2
Band function
Time interval is from -0.704 sec. to 93.108 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.912950 ( 0.91295 5.91292 )
beta : -1.08601 ( -0.161901 0.167408 )
Epeak [keV] : 41.8445 ( -41.8444 -41.8444 )
Norm@50keV : 2.46752E-03 ( -0.00112359 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.57 using 59 PHA bins.
# Reduced chi-squared = 1.156 for 55 degrees of freedom
# Null hypothesis probability = 2.001680e-01
Photon flux (15-150 keV) in 93.81 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] : 23.2936 ( )
R^2/D10^2 : 4.68510E-03 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 118.32 using 59 PHA bins.
# Reduced chi-squared = 2.0758 for 57 degrees of freedom
# Null hypothesis probability = 3.467328e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.295e-08 7.641e-09
25- 50 2.347e-07 3.602e-08
50-150 9.507e-07 1.352e-07
15-150 1.228e-06 1.463e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-16.8517 -200)
Norm : 0.712018 (-0.0602238 0.0602238)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.663e-07 1.825e-08
25- 50 3.199e-07 6.895e-08
50-150 7.015e-07 2.678e-07
15-150 1.188e-06 4.503e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.30377 (-2.06564 1.81106)
R1^2/D10^2 : 6.89513E-02 (-0.0309404 0.0894889)
kT2 [keV] : 87.6220 (-41.7892 -87.4867)
R2^2/D10^2 : 1.39095E-04 (-0.000106424 0.000447411)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.251e-07 7.196e-08
25- 50 2.744e-07 1.207e-07
50-150 1.037e-06 5.599e-07
15-150 1.436e-06 6.687e-07
Peak spectrum fit
Power-law model
Time interval is from -0.216 sec. to 0.784 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.468427 ( -0.312752 0.279919 )
Norm@50keV : 1.05404E-02 ( -0.00177098 0.00165143 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.42 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 57 degrees of freedom
# Null hypothesis probability = 2.076431e-01
Photon flux (15-150 keV) in 1 sec: 1.25504 ( -0.169481 0.170239 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.43917e-07 ( -1.95071e-08 1.95577e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.216 sec. to 0.784 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.459566 ( -0.337562 0.263227 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.06368E-02 ( -0.00178235 0.00134194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.50 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.805038e-01
Photon flux (15-150 keV) in 1 sec: 1.26082 1.25473 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.43501e-07 ( -1.9105e-08 2.0078e-08 ) ergs/cm2
Band function
Time interval is from -0.216 sec. to 0.784 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.759541 ( 0.759303 0.759303 )
beta : -0.468401 ( -0.280168 0.312745 )
Epeak [keV] : 16.3682 ( -16.373 -16.373 )
Norm@50keV : 1.52941E-02 ( -0.0062631 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.42 using 59 PHA bins.
# Reduced chi-squared = 1.189 for 55 degrees of freedom
# Null hypothesis probability = 1.587445e-01
Photon flux (15-150 keV) in 1 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] : 43.3024 (-11.1447 20.8843)
R^2/D10^2 : 7.65878E-03 (-0.00443303 0.00847066)
(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 1.749e-09 5.486e-10
25- 50 1.220e-08 3.439e-09
50-150 1.281e-07 3.501e-08
15-150 1.420e-07 3.948e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-24.6798 -200)
Norm : 4.80225 (-0.703272 0.703272)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.195e-08 6.740e-09
25- 50 2.299e-08 1.295e-08
50-150 5.043e-08 2.847e-08
15-150 8.537e-08 4.745e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.4496 (-3.1092 4.30195)
R1^2/D10^2 : 0.261946 (-0.206408 0.548144)
kT2 [keV] : 199.177 (-143.813 -199.177)
R2^2/D10^2 : 4.28935E-04 (-9.09197e-05 0.00121761)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.627e-09 4.099e-09
25- 50 1.923e-08 1.082e-08
50-150 1.194e-07 8.450e-08
15-150 1.453e-07 1.146e-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: 0.557751 ( -0.16043 0.151787 )
Norm@50keV : 3.65239E-03 ( -0.000332392 0.000322233 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.78 using 59 PHA bins.
# Reduced chi-squared = 1.417 for 57 degrees of freedom
# Null hypothesis probability = 2.083588e-02
Photon flux (15-150 keV) in 19.68 sec: 0.428792 ( -0.0334062 0.0335753 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.3824e-07 ( -6.93104e-08 6.94791e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.548338 ( -0.177366 0.14072 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 3.68290E-03 ( -0.000333689 0.000260509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.89 using 59 PHA bins.
# Reduced chi-squared = 1.445 for 56 degrees of freedom
# Null hypothesis probability = 1.641606e-02
Photon flux (15-150 keV) in 19.68 sec: 0.429946 ( -0.034865 0.032376 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.38575e-07 ( -6.937e-08 6.86399e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.712785 ( 0.712785 0.712785 )
beta : -0.557730 ( -0.151942 0.160543 )
Epeak [keV] : 16.3704 ( -16.3704 -16.3704 )
Norm@50keV : 5.37419E-03 ( -0.00203295 46606.7 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.78 using 59 PHA bins.
# Reduced chi-squared = 1.469 for 55 degrees of freedom
# Null hypothesis probability = 1.337601e-02
Photon flux (15-150 keV) in 19.68 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) = 2.82e-07
S(50-100 keV) = 5.32e-07
T90 vs. Hardness ratio plot
T90 = 89.3639999628067 sec.
Hardness ratio (energy fluence ratio) = 1.88652
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.37079
Count Ratio (50-100 keV) / (15-25 keV) = 1.15927
Mask shadow pattern
IMX = 2.280825908753507E-01, IMY = 2.088212299842881E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-179.128000 -0.704000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
208.2690 62.7142 2.7 59.5 -161.8 9.0177 4.3 ------ UNKNOWN
188.0136 36.9183 2.1 48.0 -129.0 6.7246 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.704000 18.972680
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
86.1110 27.5485 2.2 39.8 87.5 1.3529 5.3 ------ UNKNOWN
91.8252 9.4855 2.4 41.4 58.5 1.0132 4.7 ------ UNKNOWN
152.7596 76.8951 2.2 50.1 173.2 0.7769 5.1 ------ UNKNOWN
139.9009 12.6444 0.6 17.2 -42.5 1.2050 20.7 ------ UNKNOWN
189.1137 61.1538 2.2 50.5 -161.1 0.6999 5.2 ------ UNKNOWN
149.1567 -24.8622 2.5 55.4 -32.7 1.4895 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
68.772600 652.943600
660.872000 717.394600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4986 -40.5700 3.1 53.4 -12.1 7.7618 3.7 1.6 Vela X-1
133.5794 -12.2400 3.0 25.7 -1.9 3.6553 3.8 ------ UNKNOWN
129.3837 -39.3425 2.3 52.9 -6.1 9.6654 5.0 ------ UNKNOWN
163.9743 -31.7402 2.4 50.0 -43.2 16.5652 4.8 ------ UNKNOWN
Plot creation:
Sun Oct 18 15:24:21 EDT 2026