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
128.1616 +21.8102 0.0110 13.7 106.5 0.7158 17.5 TRIG_01402466
------------------------------------------
Foreground time interval of the image:
-0.036 9.873 (delta_t = 9.909 [sec])
Background time interval of the image:
-108.227 -0.036 (delta_t = 108.191 [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 0.512000
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 0.512000
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 0.512000
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 -0.036 sec. to 103.432 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32151 ( -0.0331435 0.0330468 )
Norm@50keV : 1.02534E-02 ( -0.000178301 0.000177987 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.43 using 59 PHA bins.
# Reduced chi-squared = 0.7269 for 57 degrees of freedom
# Null hypothesis probability = 9.397494e-01
Photon flux (15-150 keV) in 103.5 sec: 1.22825 ( -0.0244775 0.0246039 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04329e-05 ( -1.78964e-07 1.79046e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.036 sec. to 103.432 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31671 ( -0.0328662 0.0339792 )
Epeak [keV] : 9893.11 ( -9833.33 -9833.33 )
Norm@50keV : 1.03042E-02 ( -0.000176277 0.00162344 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.41 using 59 PHA bins.
# Reduced chi-squared = 0.7394 for 56 degrees of freedom
# Null hypothesis probability = 9.273845e-01
Photon flux (15-150 keV) in 103.5 sec: 1.22120 ( -0.01811 0.03085 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04061e-05 ( -1.80473e-07 1.92407e-07 ) ergs/cm2
Band function
Time interval is from -0.036 sec. to 103.432 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.267837 ( 0.675741 5.6495 )
beta : -1.33787 ( -0.0460601 0.0400869 )
Epeak [keV] : 48.0901 ( -48.0629 144.028 )
Norm@50keV : 5.25199E-02 ( -0.0527047 312.616 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.26 using 59 PHA bins.
# Reduced chi-squared = 0.7138 for 55 degrees of freedom
# Null hypothesis probability = 9.461741e-01
Photon flux (15-150 keV) in 103.5 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] : 20.4895 ( )
R^2/D10^2 : 4.83134E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 733.53 using 59 PHA bins.
# Reduced chi-squared = 12.869 for 57 degrees of freedom
# Null hypothesis probability = 3.253013e-118
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.007e-07 1.527e-08
25- 50 2.028e-06 5.537e-08
50-150 6.331e-06 1.527e-07
15-150 8.759e-06 1.615e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 5.29253 ( )
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.364e-06 2.743e-08
25- 50 2.624e-06 5.175e-08
50-150 5.755e-06 1.087e-07
15-150 9.742e-06 2.023e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.35222 (-0.549517 0.578876)
R1^2/D10^2 : 0.626137 (-0.125399 0.16504)
kT2 [keV] : 34.0721 (-2.19314 2.66304)
R2^2/D10^2 : 7.51990E-03 (-0.00164328 0.00188072)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.728e-07 6.924e-08
25- 50 2.431e-06 8.642e-08
50-150 6.991e-06 2.277e-07
15-150 1.039e-05 2.976e-07
Peak spectrum fit
Power-law model
Time interval is from 56.140 sec. to 57.140 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02715 ( -0.0567447 0.0565168 )
Norm@50keV : 8.21952E-02 ( -0.00260071 0.00259855 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.44 using 59 PHA bins.
# Reduced chi-squared = 0.8849 for 57 degrees of freedom
# Null hypothesis probability = 7.179342e-01
Photon flux (15-150 keV) in 1 sec: 9.47810 ( -0.305845 0.305992 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.80412e-07 ( -3.08169e-08 3.09535e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 56.140 sec. to 57.140 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.800247 ( -0.229711 0.195545 )
Epeak [keV] : 307.473 ( -124.823 3236.83 )
Norm@50keV : 0.103444 ( -0.0177181 0.0261766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.28 using 59 PHA bins.
# Reduced chi-squared = 0.8443 for 56 degrees of freedom
# Null hypothesis probability = 7.901423e-01
Photon flux (15-150 keV) in 1 sec: 9.38206 ( -0.31853 0.31863 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.71734e-07 ( -3.2478e-08 3.2343e-08 ) ergs/cm2
Band function
Time interval is from 56.140 sec. to 57.140 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.800240 ( -0.151614 0.14731 )
beta : -9.35683 ( 9.36583 19.3658 )
Epeak [keV] : 307.440 ( -63.6619 3227.58 )
Norm@50keV : 0.103439 ( -0.0222212 0.0254908 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.28 using 59 PHA bins.
# Reduced chi-squared = 0.8597 for 55 degrees of freedom
# Null hypothesis probability = 7.608328e-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] : 21.8726 ( )
R^2/D10^2 : 0.343188 ( )
(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 3.047e-08 1.880e-09
25- 50 1.605e-07 7.450e-09
50-150 5.738e-07 3.275e-08
15-150 7.648e-07 3.040e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 38.4478 ( )
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.574e-08 3.390e-09
25- 50 1.842e-07 6.300e-09
50-150 4.039e-07 1.385e-08
15-150 6.838e-07 2.170e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.00735 (-1.18024 1.39392)
R1^2/D10^2 : 4.20097 (-1.58935 2.82604)
kT2 [keV] : 33.3150 (-3.47099 5.09724)
R2^2/D10^2 : 8.00140E-02 (-0.0293156 0.0347405)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.174e-08 8.130e-09
25- 50 1.689e-07 1.445e-08
50-150 6.462e-07 6.015e-08
15-150 8.769e-07 6.390e-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: 1.86843 ( -0.147086 0.152446 )
Norm@50keV : 4.03752E-03 ( -0.000406718 0.000400952 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.54 using 59 PHA bins.
# Reduced chi-squared = 1.027 for 57 degrees of freedom
# Null hypothesis probability = 4.187227e-01
Photon flux (15-150 keV) in 9.909 sec: 0.571816 ( -0.0486829 0.0486981 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.67804e-07 ( -3.66449e-08 3.71764e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.791725 ( -0.805875 0.678062 )
Epeak [keV] : 48.0257 ( -7.77584 15.1714 )
Norm@50keV : 1.64482E-02 ( -0.00955133 0.0307901 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.55 using 59 PHA bins.
# Reduced chi-squared = 0.9027 for 56 degrees of freedom
# Null hypothesis probability = 6.804380e-01
Photon flux (15-150 keV) in 9.909 sec: 0.550795 ( -0.05014 0.050215 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.3441e-07 ( -3.90831e-08 4.12165e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.791613 ( -0.457553 0.932351 )
beta : -10.00000 ( 10 1.91529e-08 )
Epeak [keV] : 48.0156 ( -7.74941 15.1689 )
Norm@50keV : 1.64505E-02 ( -0.00137916 0.0307885 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.55 using 59 PHA bins.
# Reduced chi-squared = 0.9191 for 55 degrees of freedom
# Null hypothesis probability = 6.450719e-01
Photon flux (15-150 keV) in 9.909 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.28182e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.35e-06
S(50-100 keV) = 3.76e-06
T90 vs. Hardness ratio plot
T90 = 64.1879999637604 sec.
Hardness ratio (energy fluence ratio) = 1.6
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.51483
Count Ratio (50-100 keV) / (15-25 keV) = 1.26424
Mask shadow pattern
IMX = -6.935331641332819E-02, IMY = -2.341736403797344E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-108.227390 -0.036000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5118 -40.5355 5.9 56.1 -8.7 1.1569 2.0 1.4 Vela X-1
115.3093 -28.7789 2.4 50.6 15.7 1.9186 4.9 ------ UNKNOWN
132.4826 49.6857 2.8 35.1 156.8 1.0866 4.1 ------ UNKNOWN
140.0093 -14.5748 3.2 29.9 -11.9 0.6385 3.6 ------ UNKNOWN
168.6873 1.8505 3.0 30.5 -80.2 0.8782 3.8 ------ UNKNOWN
158.3720 -27.8122 2.7 46.3 -35.2 1.3495 4.3 ------ UNKNOWN
197.0745 42.5993 2.3 55.0 -145.4 4.3337 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.036000 9.872590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3930 -40.5815 3.7 56.1 -8.6 -0.4632 -3.1 6.4 Vela X-1
128.1617 21.8102 0.7 13.7 106.5 0.7159 17.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
57.372590 302.604000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
127.4261 58.1050 2.1 36.3 164.2 2.7280 5.6 ------ UNKNOWN
163.4398 70.4784 2.7 52.9 178.9 4.7820 4.2 ------ UNKNOWN
128.1520 21.8221 0.4 0.0 103.6 10.1978 31.9 ------ UNKNOWN
128.8036 -15.1346 2.6 37.0 -16.2 2.1473 4.5 ------ UNKNOWN
142.7101 23.0336 3.1 13.5 -113.0 1.3547 3.8 ------ UNKNOWN
140.6118 -34.4191 2.3 57.5 -27.3 9.3558 5.0 ------ UNKNOWN
Plot creation:
Wed Oct 8 19:08:16 EDT 2025