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
129.9475 -39.3091 0.0166 31.3421 -9.8427 0.8137395 11.590 TRIG_01320335
Foreground time interval of the image:
-13.864 11.685 (delta_t = 25.549 [sec])
Background time interval of the image:
-239.816 -13.864 (delta_t = 225.952 [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 -13.864 sec. to 15.800 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.78127 ( -0.297095 0.312215 )
Norm@50keV : 1.31425E-03 ( -0.000263554 0.000256678 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.43 using 59 bins.
Reduced chi-squared = 1.32333
# Null hypothesis probability of 5.16e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 29.66 sec: 0.179812 ( -0.031677 0.031699 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.5918e-07 ( -7.22989e-08 7.38736e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -13.864 sec. to 15.800 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25981 ( -1.80503 0.9564 )
Epeak [keV] : 60.8191 ( -60.5607 -60.8161 )
Norm@50keV : 2.61837E-03 ( -0.00261859 0.0295621 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.90 using 59 bins.
Reduced chi-squared = 1.3375
# Null hypothesis probability of 4.67e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 29.66 sec: 0.177164 ( -0.032388 0.032306 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40627e-07 ( -8.52683e-08 8.47273e-08 ) ergs/cm2
Band function
Time interval is from -13.864 sec. to 15.800 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] : 10.2915 (-1.88537 2.48372)
R^2/D10^2 : 7.81817E-02 (-0.0438033 0.0900452)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.41e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.048e-08 1.675e-08
25- 50 1.306e-07 3.917e-08
50-150 7.406e-08 3.097e-08
15-150 2.552e-07 6.601e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.7887 (-44.1931 -97.7887)
Norm : 0.805567 (-0.165529 0.246292)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.65e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.244e-08 1.541e-08
25- 50 1.075e-07 2.831e-08
50-150 1.720e-07 1.009e-07
15-150 3.419e-07 1.312e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.98303 (-2.22888 2.39756)
R1^2/D10^2 : 0.170610 (-0.104602 0.332999)
kT2 [keV] : 40.1033 (-21.8543 -39.3508)
R2^2/D10^2 : 3.64343E-04 (-0.000405826 0.00663621)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.05e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.046e-08 3.498e-08
25- 50 1.168e-07 6.848e-08
50-150 1.730e-07 1.050e-07
15-150 3.503e-07 1.778e-07
Peak spectrum fit
Power-law model
Time interval is from 0.136 sec. to 1.136 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72620 ( -0.228233 0.237334 )
Norm@50keV : 9.58679E-03 ( -0.00154211 0.00151999 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.71 using 59 bins.
Reduced chi-squared = 0.907193
# Null hypothesis probability of 6.73e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.28516 ( -0.1903 0.19045 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.86074e-08 ( -1.46145e-08 1.48091e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.136 sec. to 1.136 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.467891 ( -1.29974 0.99151 )
Epeak [keV] : 55.3246 ( -12.1811 41.532 )
Norm@50keV : 4.71112E-02 ( -0.0471111 0.201776 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.73 using 59 bins.
Reduced chi-squared = 0.834464
# Null hypothesis probability of 8.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.25554 ( -0.19138 0.19174 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.22129e-08 ( -1.49648e-08 1.55311e-08 ) ergs/cm2
Band function
Time interval is from 0.136 sec. to 1.136 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] : 12.1474 (-1.87267 2.24217)
R^2/D10^2 : 0.319574 (-0.149702 0.272013)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.983e-09 2.625e-09
25- 50 3.187e-08 6.910e-09
50-150 2.850e-08 9.325e-09
15-150 7.036e-08 1.559e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 116.694 (-45.1455 -112.687)
Norm : 5.50856 (-0.961264 1.26724)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.79e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.436e-08 2.805e-09
25- 50 2.557e-08 7.320e-09
50-150 4.500e-08 2.896e-08
15-150 8.493e-08 3.667e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.41594 (-2.81128 3.15947)
R1^2/D10^2 : 1.19980 (-0.770421 3.77724)
kT2 [keV] : 20.9944 (-15.6722 24.7157)
R2^2/D10^2 : 2.71429E-02 (-0.0251306 0.120974)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.18e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.347e-08 7.550e-09
25- 50 2.875e-08 1.538e-08
50-150 4.165e-08 2.442e-08
15-150 8.386e-08 4.295e-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: 1.90177 ( -0.273967 0.292773 )
Norm@50keV : 1.61682E-03 ( -0.000299786 0.00028855 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.84e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 25.55 sec: 0.232205 ( -0.0347736 0.0347872 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.79796e-07 ( -6.7512e-08 6.90376e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.06217 ( -0.912299 1.19955 )
Epeak [keV] : 27.8378 ( -9999.35 -9999.36 )
Norm@50keV : 1.31212E-03 ( -0.000354855 0.00375179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.53e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 25.55 sec: 0.232314 ( -0.03465 0.034625 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78347e-07 ( -6.9634e-08 6.94986e-08 ) 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) = 1.01e-07
S(50-100 keV) = 1.17e-07
T90 vs. Hardness ratio plot
T90 = 15.7120000123978 sec.
Hardness ratio (energy fluence ratio) = 1.15842
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.48127
Count Ratio (50-100 keV) / (15-25 keV) = 0.652513
Mask shadow pattern
IMX = 6.000525167386274E-01, IMY = 1.041072258269904E-01
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:
-239.816000 -13.864000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4898 -40.5527 3.3 33.3 -2.5 1.3447 3.5 1.8 Vela X-1
170.3152 -60.4832 10.9 39.0 47.2 -0.6747 -1.1 8.4 Cen X-3
138.5543 -35.5642 2.5 38.7 -5.1 1.8747 4.5 ------ UNKNOWN
68.2014 -37.1198 2.6 24.8 -127.3 1.4276 4.4 ------ UNKNOWN
35.7999 -27.8724 2.9 47.8 -158.0 2.6258 4.0 ------ UNKNOWN
83.5753 -18.2959 2.7 39.3 -92.0 5.1918 4.2 ------ UNKNOWN
61.7923 -17.8259 2.4 44.7 -122.1 6.5741 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.864000 11.684600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3397 -40.5259 3.9 33.3 -2.6 -0.2142 -3.0 8.8 Vela X-1
170.2277 -60.7098 3.7 38.8 47.5 0.3947 3.2 5.8 Cen X-3
0.6761 -68.6107 2.1 38.2 133.9 0.6738 5.6 ------ UNKNOWN
129.9475 -39.3091 1.0 31.3 -9.8 0.8137 11.6 ------ UNKNOWN
85.9792 -25.6872 2.1 31.7 -89.3 0.5459 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.684600 962.279000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5695 -40.5952 1.8 4.5 71.9 6.1357 6.3 3.1 Vela X-1
169.9923 -60.6899 18.6 32.7 107.3 -1.3177 -0.6 10.3 Cen X-3
186.3176 -62.6887 0.0 40.6 107.1 5.9163 1.2 10.5 GX 301-2
65.1018 -74.4650 3.6 45.7 162.8 11.1065 3.2 ------ UNKNOWN
53.1294 -53.8272 3.5 52.0 -170.2 10.4312 3.3 ------ UNKNOWN
108.7418 -14.9742 2.5 30.6 -80.3 6.9281 4.6 ------ UNKNOWN
111.5309 1.1545 3.0 43.8 -64.1 20.4053 3.8 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:36:46 EDT 2025