Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
105.8696 -24.8708 0.0065 16.2839 167.5393 3.2402810 29.156 TRIG_01409824
Foreground time interval of the image:
-52.072 11.341 (delta_t = 63.413 [sec])
Background time interval of the image:
-239.960 -52.072 (delta_t = 187.888 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) 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.
- 4) 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.
- 5) 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)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -52.072 sec. to 92.744 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.79246 ( -0.0756665 0.0763794 )
Norm@50keV : 2.57928E-03 ( -0.000107995 0.000107524 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.17 using 59 bins.
Reduced chi-squared = 1.44158
# Null hypothesis probability of 1.62e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 144.8 sec: 0.354405 ( -0.014863 0.014903 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.43977e-06 ( -1.47095e-07 1.47705e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -52.072 sec. to 92.744 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60407 ( -0.311854 0.242949 )
Epeak [keV] : 102.248 ( -36.644 -102.249 )
Norm@50keV : 3.21801E-03 ( -0.000716765 0.00138771 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.98 using 59 bins.
Reduced chi-squared = 1.44607
# Null hypothesis probability of 1.62e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 144.8 sec: 0.349922 ( -0.01633 0.016363 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.38173e-06 ( -1.72371e-07 1.71869e-07 ) ergs/cm2
Band function
Time interval is from -52.072 sec. to 92.744 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 12.7376 ( )
R^2/D10^2 : 6.51413E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 228.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.50e-22 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.246e-07 2.469e-08
25- 50 1.093e-06 5.408e-08
50-150 1.108e-06 9.839e-08
15-150 2.526e-06 1.093e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 113.278 (-18.2846 21.4775)
Norm : 1.49376 (-0.0827701 0.099494)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.23e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.645e-07 4.243e-08
25- 50 9.996e-07 5.372e-08
50-150 1.733e-06 4.428e-07
15-150 3.297e-06 4.576e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.79150 (-0.867978 0.917604)
R1^2/D10^2 : 0.467654 (-0.164135 0.29646)
kT2 [keV] : 24.4157 (-3.42757 5.09895)
R2^2/D10^2 : 4.44101E-03 (-0.00222629 0.00354425)
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.46e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.532e-07 7.544e-08
25- 50 1.005e-06 1.090e-07
50-150 1.768e-06 3.188e-07
15-150 3.326e-06 3.815e-07
Peak spectrum fit
Power-law model
Time interval is from 2.004 sec. to 3.004 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18295 ( -0.116093 0.11492 )
Norm@50keV : 2.50093E-02 ( -0.00165182 0.00165155 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.18 using 59 bins.
Reduced chi-squared = 0.845263
# Null hypothesis probability of 7.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.92874 ( -0.19997 0.20028 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.54994e-07 ( -1.85382e-08 1.86211e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.004 sec. to 3.004 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09209 ( -0.455808 0.112755 )
Epeak [keV] : 513.875 ( -865.628 -865.628 )
Norm@50keV : 2.75673E-02 ( -0.00290572 0.0158088 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.20 using 59 bins.
Reduced chi-squared = 0.860714
# Null hypothesis probability of 7.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.92281 ( -0.20498 0.19709 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.54314e-07 ( -1.93453e-08 1.72799e-08 ) ergs/cm2
Band function
Time interval is from 2.004 sec. to 3.004 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 20.1022 (-1.76069 1.98505)
R^2/D10^2 : 0.133148 (-0.0353404 0.0469633)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 99.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.80e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.035e-08 1.442e-09
25- 50 5.173e-08 5.145e-09
50-150 1.551e-07 1.880e-08
15-150 2.172e-07 1.890e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-12.5897 -200)
Norm : 12.1188 (-0.81948 0.81948)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.79e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.017e-08 2.395e-09
25- 50 5.804e-08 6.045e-09
50-150 1.273e-07 2.914e-08
15-150 2.155e-07 3.835e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.25268 (-1.31164 1.78688)
R1^2/D10^2 : 3.60030 (-2.07879 5.21872)
kT2 [keV] : 29.0211 (-4.19754 6.83179)
R2^2/D10^2 : 3.56766E-02 (-0.0176839 0.0197789)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.65e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.459e-08 9.838e-09
25- 50 5.075e-08 1.049e-08
50-150 1.781e-07 3.650e-08
15-150 2.534e-07 4.925e-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: 1.66231 ( -0.0901635 0.0908894 )
Norm@50keV : 3.27643E-03 ( -0.000161787 0.000161143 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 63.41 sec: 0.429573 ( -0.0214646 0.0215375 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.92991e-06 ( -1.0079e-07 1.01252e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66390 ( -0.0928526 0.0894214 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 3.27715E-03 ( -0.00120817 0.00124885 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.08e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 63.41 sec: 0.429583 ( -0.021459 0.021327 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.92285e-06 ( -1.02743e-07 1.10695e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 9.66e-07
S(50-100 keV) = 1.11e-06
T90 vs. Hardness ratio plot
T90 = 127.860000014305 sec.
Hardness ratio (energy fluence ratio) = 1.14907
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.18723
Count Ratio (50-100 keV) / (15-25 keV) = 0.684144
Mask shadow pattern
IMX = -2.852350091827213E-01, IMY = -6.303008692623259E-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:
-239.960000 -52.072000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5396 -40.5477 1.8 24.5 -101.9 1.9738 6.3 0.7 Vela X-1
170.2414 -60.7953 13.2 44.4 -61.8 1.1654 0.9 10.6 Cen X-3
68.8408 -26.5170 2.6 31.6 84.7 2.3755 4.5 ------ UNKNOWN
49.6612 -47.3030 2.7 38.0 40.3 2.4216 4.3 ------ UNKNOWN
84.2652 -33.0696 2.6 16.9 90.2 1.4776 4.5 ------ UNKNOWN
100.6564 -72.7150 2.9 31.8 -20.4 1.1885 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-52.072000 11.340590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3577 -40.5369 4.2 24.4 -102.0 0.3858 2.7 7.9 Vela X-1
170.4491 -60.7230 6.4 44.5 -61.9 -0.8327 -1.8 7.2 Cen X-3
77.1591 -5.9784 2.8 41.9 117.8 1.7165 4.1 ------ UNKNOWN
105.8696 -24.8708 0.4 16.3 167.5 3.2402 29.1 ------ UNKNOWN
121.4291 8.4749 2.1 52.3 -178.5 1.7906 5.5 ------ UNKNOWN
143.8817 -2.6690 2.6 53.1 -146.9 1.8276 4.4 ------ UNKNOWN
151.0575 -17.4223 2.1 47.3 -126.9 2.7486 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.140590 962.109500
1082.040000 1282.090000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5473 -40.5031 1.6 29.3 -74.4 13.1705 7.2 3.2 Vela X-1
104.0566 -35.5304 3.4 10.8 -16.1 4.6443 3.4 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:14:20 EST 2026