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
132.4750 +24.9718 0.0231 13.0 157.5 0.1595 8.3 TRIG_01513316
------------------------------------------
Foreground time interval of the image:
0.484 3.160 (delta_t = 2.676 [sec])
Background time interval of the image:
-119.032 -67.744 (delta_t = 51.288 [sec])
-60.032 0.484 (delta_t = 60.516 [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 3.160 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51600 ( -0.2964 0.300298 )
Norm@50keV : 3.83909E-03 ( -0.000732058 0.000719526 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.08 using 59 PHA bins.
# Reduced chi-squared = 1.352 for 57 degrees of freedom
# Null hypothesis probability = 3.941750e-02
Photon flux (15-150 keV) in 2.676 sec: 0.481360 ( -0.0854353 0.085459 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.72089e-08 ( -2.00566e-08 2.05523e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.484 sec. to 3.160 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.05350 ( -1.94309 1.14325 )
Epeak [keV] : 87.7292 ( -44.5659 -88.6225 )
Norm@50keV : 7.11062E-03 ( -0.00386684 0.092302 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.80 using 59 PHA bins.
# Reduced chi-squared = 1.371 for 56 degrees of freedom
# Null hypothesis probability = 3.395881e-02
Photon flux (15-150 keV) in 2.676 sec: 0.475155 ( -0.088636 0.087507 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.18542e-08 ( -2.56703e-08 2.47533e-08 ) ergs/cm2
Band function
Time interval is from 0.484 sec. to 3.160 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5.5955 -5 )
beta : -1.90406 ( -0.607783 0.427798 )
Epeak [keV] : 29.1615 ( -7.64604 5.71116 )
Norm@50keV : 183.970 ( -31.7378 947.645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.89 using 59 PHA bins.
# Reduced chi-squared = 1.325 for 55 degrees of freedom
# Null hypothesis probability = 5.355186e-02
Photon flux (15-150 keV) in 2.676 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] : 11.9285 (-2.26192 2.91593)
R^2/D10^2 : 0.126016 (-0.0693513 0.142829)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.25 using 59 PHA bins.
# Reduced chi-squared = 1.425 for 57 degrees of freedom
# Null hypothesis probability = 1.916051e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.014e-08 3.342e-09
25- 50 3.170e-08 9.235e-09
50-150 2.701e-08 1.124e-08
15-150 6.885e-08 2.016e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.723 (-114.873 -198.723)
Norm : 1.97428 (-0.348763 0.413374)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.316e-08 7.611e-09
25- 50 2.531e-08 1.434e-08
50-150 5.545e-08 3.126e-08
15-150 9.391e-08 5.483e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.43320 (-2.4469 1.86261)
R1^2/D10^2 : 0.257382 (-0.114704 0.385634)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 6.46952E-05 (-3.02461e-05 0.00035975)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.268e-08 6.978e-09
25- 50 2.941e-08 1.463e-08
50-150 5.872e-08 4.037e-08
15-150 1.008e-07 5.343e-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: 1.57113 ( -0.392912 0.395293 )
Norm@50keV : 4.67433E-03 ( -0.00117598 0.0011475 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.13 using 59 PHA bins.
# Reduced chi-squared = 1.090 for 57 degrees of freedom
# Null hypothesis probability = 2.984249e-01
Photon flux (15-150 keV) in 1 sec: 0.595426 ( -0.137916 0.137974 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.38765e-08 ( -1.16611e-08 1.20305e-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: 1.41104 ( )
Epeak [keV] : 148.357 ( )
Norm@50keV : 5.84371E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.13 using 59 PHA bins.
# Reduced chi-squared = 1.109 for 56 degrees of freedom
# Null hypothesis probability = 2.670708e-01
Photon flux (15-150 keV) in 1 sec: 0.593527 ( -0.144756 0.138692 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.30048e-08 ( -1.7834e-08 1.27791e-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 ( -5.9318 -5 )
beta : -2.09330 ( -1.08418 0.598058 )
Epeak [keV] : 29.4724 ( -8.78363 14.4546 )
Norm@50keV : 230.072 ( -50.9114 1633.14 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.53 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 55 degrees of freedom
# Null hypothesis probability = 3.471218e-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] : 10.5543 (-2.32195 3.24065)
R^2/D10^2 : 0.245190 (-0.156192 0.367998)
(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 5.653e-09 2.597e-09
25- 50 1.514e-08 6.029e-09
50-150 9.218e-09 5.297e-09
15-150 3.001e-08 1.210e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 164.233 (-100.968 -161.35)
Norm : 2.44567 (-0.593227 0.850225)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.079e-09 3.670e-09
25- 50 1.166e-08 6.615e-09
50-150 2.535e-08 1.475e-08
15-150 4.309e-08 2.439e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.67432 (-1.9523 2.12505)
R1^2/D10^2 : 0.445983 (-0.261372 0.689057)
kT2 [keV] : 198.135 (-166.628 -198.273)
R2^2/D10^2 : 8.87655E-05 (-4.77538e-05 0.00305054)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.515e-09 3.776e-09
25- 50 1.379e-08 8.045e-09
50-150 2.768e-08 5.170e-09
15-150 4.799e-08 1.794e-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: 1.51600 ( -0.2964 0.300298 )
Norm@50keV : 3.83909E-03 ( -0.000732058 0.000719526 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.08 using 59 PHA bins.
# Reduced chi-squared = 1.352 for 57 degrees of freedom
# Null hypothesis probability = 3.941750e-02
Photon flux (15-150 keV) in 2.676 sec: 0.481360 ( -0.0854353 0.085459 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.72089e-08 ( -2.00566e-08 2.05523e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.05350 ( -1.94309 1.14325 )
Epeak [keV] : 87.7292 ( -44.5659 -88.6225 )
Norm@50keV : 7.11062E-03 ( -0.00386684 0.092302 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.80 using 59 PHA bins.
# Reduced chi-squared = 1.371 for 56 degrees of freedom
# Null hypothesis probability = 3.395881e-02
Photon flux (15-150 keV) in 2.676 sec: 0.475155 ( -0.088636 0.087507 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.18542e-08 ( -2.56703e-08 2.47533e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5.59949 -5 )
beta : -1.90406 ( -0.607783 0.427798 )
Epeak [keV] : 29.1615 ( -7.64604 5.71116 )
Norm@50keV : 183.970 ( -31.7378 947.645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.89 using 59 PHA bins.
# Reduced chi-squared = 1.325 for 55 degrees of freedom
# Null hypothesis probability = 5.355186e-02
Photon flux (15-150 keV) in 2.676 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) = 2.42e-08
S(50-100 keV) = 3.39e-08
T90 vs. Hardness ratio plot
T90 = 2.21200001239777 sec.
Hardness ratio (energy fluence ratio) = 1.40083
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.58691
Count Ratio (50-100 keV) / (15-25 keV) = 0.840197
Mask shadow pattern
IMX = -2.130853109180660E-01, IMY = -8.832058779134017E-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:
-119.032000 -67.743600
-60.032000 0.484000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6355 -40.4994 3.6 52.6 -19.0 1.6315 3.2 5.9 Vela X-1
131.8015 55.7896 2.7 43.8 161.2 1.6155 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.484000 3.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4099 -40.5138 10.4 52.6 -18.8 0.0601 1.1 5.9 Vela X-1
132.4743 24.9713 1.4 13.0 157.5 0.1558 8.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
93.668590 242.989800
356.968000 641.819300
643.968000 651.258000
652.968000 693.622800
697.968000 723.033500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
101.8070 70.0185 2.3 48.5 146.1 13.9310 5.1 ------ UNKNOWN
101.9683 53.8151 2.9 36.7 129.4 6.7886 4.0 ------ UNKNOWN
170.0429 40.5239 2.6 34.9 -146.3 3.9106 4.5 ------ UNKNOWN
153.7159 -20.0684 2.6 49.5 -47.1 14.2239 4.4 ------ UNKNOWN
161.2822 -8.4948 2.5 43.7 -64.2 14.1197 4.6 ------ UNKNOWN
186.8534 29.8493 2.7 48.1 -129.2 12.4551 4.2 ------ UNKNOWN
Plot creation:
Fri Sep 25 19:01:13 EDT 2026