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
132.4537 +24.8810 0.0387 12.9 157.4 0.3707 5.0 TRIG_01513316
------------------------------------------
Foreground time interval of the image:
0.484 40.412 (delta_t = 39.928 [sec])
Background time interval of the image:
-179.032 0.484 (delta_t = 179.516 [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 3.072000
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 3.072000
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 3.072000
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 0.484 sec. to 40.412 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60118 ( -0.431517 0.448262 )
Norm@50keV : 6.37812E-04 ( -0.000179879 0.000174385 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.86 using 59 PHA bins.
# Reduced chi-squared = 0.8221 for 57 degrees of freedom
# Null hypothesis probability = 8.287273e-01
Photon flux (15-150 keV) in 39.93 sec: 8.19917E-02 ( -0.0206829 0.0206899 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38142e-07 ( -7.00125e-08 7.30943e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.484 sec. to 40.412 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.51176E-03 ( -5.13142 2.21542 )
Epeak [keV] : 49.3099 ( )
Norm@50keV : 5.77944E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.21 using 59 PHA bins.
# Reduced chi-squared = 0.8251 for 56 degrees of freedom
# Null hypothesis probability = 8.216668e-01
Photon flux (15-150 keV) in 39.93 sec: 7.66801E-02 ( -0.0215908 0.0233399 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8899e-07 ( -6.57691e-08 1.12325e-07 ) ergs/cm2
Band function
Time interval is from 0.484 sec. to 40.412 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.65040 ( -4.6504 -4.6504 )
beta : -2.12903 ( -1.18175 0.685885 )
Epeak [keV] : 31.6201 ( -31.6201 9.84199 )
Norm@50keV : 11.7544 ( -2.89347 445493 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.92 using 59 PHA bins.
# Reduced chi-squared = 0.8166 for 55 degrees of freedom
# Null hypothesis probability = 8.321884e-01
Photon flux (15-150 keV) in 39.93 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19062e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.1003 (-2.48841 3.4883)
R^2/D10^2 : 2.80230E-02 (-0.0179519 0.0430788)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.53 using 59 PHA bins.
# Reduced chi-squared = 0.8164 for 57 degrees of freedom
# Null hypothesis probability = 8.374815e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.886e-08 1.785e-08
25- 50 8.256e-08 3.896e-08
50-150 5.786e-08 3.622e-08
15-150 1.693e-07 8.317e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 155.599 (-100.49 -152.42)
Norm : 0.339773 (-0.0889989 0.142239)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.473e-08 1.992e-08
25- 50 6.472e-08 3.694e-08
50-150 1.297e-07 8.190e-08
15-150 2.291e-07 1.357e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.54962 (-1.83007 2.86986)
R1^2/D10^2 : 4.35637E-02 (-0.0229323 0.0638669)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 9.72565E-06 (-7.31406e-06 3.60322e-05)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.151e-08 1.839e-08
25- 50 7.807e-08 4.726e-08
50-150 1.335e-07 3.704e-08
15-150 2.431e-07 9.681e-08
Peak spectrum fit
Power-law model
Time interval is from 1.104 sec. to 2.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57111 ( -0.394737 0.397131 )
Norm@50keV : 4.63937E-03 ( -0.00117288 0.00114442 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.04 using 59 PHA bins.
# Reduced chi-squared = 1.088 for 57 degrees of freedom
# Null hypothesis probability = 3.011660e-01
Photon flux (15-150 keV) in 1 sec: 0.590968 ( -0.137553 0.137611 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.35483e-08 ( -1.16276e-08 1.19984e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.104 sec. to 2.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34378 ( -4.32939 1.0563 )
Epeak [keV] : 115.130 ( -137.248 -137.248 )
Norm@50keV : 6.37423E-03 ( -0.00581293 3.64613 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.04 using 59 PHA bins.
# Reduced chi-squared = 1.108 for 56 degrees of freedom
# Null hypothesis probability = 2.695090e-01
Photon flux (15-150 keV) in 1 sec: 0.588887 ( -0.144772 0.139078 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.26018e-08 ( -1.77647e-08 1.28215e-08 ) ergs/cm2
Band function
Time interval is from 1.104 sec. to 2.104 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.09165 -5 )
beta : -2.09595 ( -1.09587 0.601294 )
Epeak [keV] : 29.4964 ( -8.79425 14.4812 )
Norm@50keV : 227.365 ( -50.5626 1615.33 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.44 using 59 PHA bins.
# Reduced chi-squared = 1.063 for 55 degrees of freedom
# Null hypothesis probability = 3.501294e-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] : 10.5538 (-2.32858 3.25363)
R^2/D10^2 : 0.243512 (-0.155454 0.367289)
(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 5.614e-09 2.323e-09
25- 50 1.503e-08 6.683e-09
50-150 9.152e-09 4.780e-09
15-150 2.980e-08 1.346e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 164.792 (-100.854 -160.928)
Norm : 2.42389 (-0.592114 0.848988)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.044e-09 3.505e-09
25- 50 1.158e-08 6.460e-09
50-150 2.508e-08 1.469e-08
15-150 4.270e-08 2.459e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.69460 (-2.16764 1.9361)
R1^2/D10^2 : 0.441575 (-0.259467 0.686984)
kT2 [keV] : 199.363 (-167.916 -199.363)
R2^2/D10^2 : 8.40680E-05 (-4.591e-05 0.00309736)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.262e-09 3.732e-09
25- 50 1.380e-08 8.160e-09
50-150 2.653e-08 8.575e-09
15-150 4.659e-08 1.766e-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: 1.60118 ( -0.431517 0.448262 )
Norm@50keV : 6.37812E-04 ( -0.000179879 0.000174385 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.86 using 59 PHA bins.
# Reduced chi-squared = 0.8221 for 57 degrees of freedom
# Null hypothesis probability = 8.287273e-01
Photon flux (15-150 keV) in 39.93 sec: 8.19917E-02 ( -0.0206829 0.0206899 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38142e-07 ( -7.00125e-08 7.30943e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.51176E-03 ( -5.13142 2.21542 )
Epeak [keV] : 49.3099 ( )
Norm@50keV : 5.77944E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.21 using 59 PHA bins.
# Reduced chi-squared = 0.8251 for 56 degrees of freedom
# Null hypothesis probability = 8.216668e-01
Photon flux (15-150 keV) in 39.93 sec: 7.66801E-02 ( -0.0215908 0.0233399 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8899e-07 ( -6.57691e-08 1.12325e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.65040 ( -4.6504 -4.6504 )
beta : -2.12903 ( -1.18175 0.685885 )
Epeak [keV] : 31.6201 ( -31.6201 9.84199 )
Norm@50keV : 11.7544 ( -2.89347 445493 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.92 using 59 PHA bins.
# Reduced chi-squared = 0.8166 for 55 degrees of freedom
# Null hypothesis probability = 8.321884e-01
Photon flux (15-150 keV) in 39.93 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19062e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.18e-08
S(50-100 keV) = 8.14e-08
T90 vs. Hardness ratio plot
T90 = 35.4239999055862 sec.
Hardness ratio (energy fluence ratio) = 1.31715
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.9465
Count Ratio (50-100 keV) / (15-25 keV) = 0.700472
Mask shadow pattern
IMX = -2.113938515478524E-01, IMY = -8.816324261869732E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
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:
-179.032000 0.484000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6276 -40.5037 3.6 52.6 -19.0 2.3576 3.2 5.5 Vela X-1
101.7228 -19.5198 2.9 44.6 28.2 1.9635 4.0 ------ UNKNOWN
188.8621 37.9451 3.0 55.3 -145.3 5.4622 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.484000 40.412000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5139 -40.4888 4.7 52.6 -18.9 -0.5793 -2.4 4.0 Vela X-1
96.0539 -17.6511 2.0 47.6 34.9 1.5865 5.8 ------ UNKNOWN
142.0703 59.1857 2.1 47.6 168.5 0.9725 5.5 ------ UNKNOWN
125.5301 15.4289 2.4 8.7 96.6 0.3468 4.8 ------ UNKNOWN
132.4538 24.8810 2.3 12.9 157.4 0.3706 5.0 ------ UNKNOWN
125.3353 -32.3552 2.4 45.1 -7.1 0.6506 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
93.668590 723.033500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
101.7913 70.0171 2.1 48.5 146.0 18.9890 5.5 ------ UNKNOWN
101.9781 53.8264 2.8 36.7 129.4 8.8330 4.1 ------ UNKNOWN
132.8552 -13.1323 2.9 38.1 -21.1 4.6515 4.0 ------ UNKNOWN
170.0346 40.5205 2.5 34.9 -146.3 5.0584 4.7 ------ UNKNOWN
153.7669 -20.0320 2.7 49.5 -47.1 17.2193 4.2 ------ UNKNOWN
Plot creation:
Sun Sep 27 12:20:48 EDT 2026