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
15.6091 -59.0991 0.0168 23.6809 52.2535 2.0913793 11.444 TRIG_01340561
Foreground time interval of the image:
-17.299 72.501 (delta_t = 89.800 [sec])
Background time interval of the image:
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 -50.996 sec. to 84.520 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73299 ( -0.119989 0.121951 )
Norm@50keV : 1.99217E-03 ( -0.000141782 0.000140473 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.08 using 59 bins.
Reduced chi-squared = 1.31719
# Null hypothesis probability of 5.45e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 135.5 sec: 0.267718 ( -0.01792 0.017954 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.49378e-06 ( -1.84169e-07 1.85752e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -50.996 sec. to 84.520 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59958 ( -0.461324 0.224614 )
Epeak [keV] : 143.344 ( -78.8086 -143.344 )
Norm@50keV : 2.34066E-03 ( -0.00081486 0.00168519 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.80 using 59 bins.
Reduced chi-squared = 1.33571
# Null hypothesis probability of 4.74e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 135.5 sec: 0.265925 ( -0.018795 0.018782 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.46512e-06 ( -2.05484e-07 2.04188e-07 ) ergs/cm2
Band function
Time interval is from -50.996 sec. to 84.520 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] : 12.9621 ( )
R^2/D10^2 : 4.73123E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 143.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.38e-09 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.285e-07 2.771e-08
25- 50 7.844e-07 7.229e-08
50-150 8.317e-07 1.241e-07
15-150 1.845e-06 1.497e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 135.043 (-37.1198 50.2153)
Norm : 1.09107 (-0.0870142 0.118209)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.38e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.827e-07 3.774e-08
25- 50 6.982e-07 7.175e-08
50-150 1.317e-06 4.520e-07
15-150 2.398e-06 5.176e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.78593 (-0.97295 1.10704)
R1^2/D10^2 : 0.637081 (-0.305131 0.686075)
kT2 [keV] : 22.8123 (-3.51152 5.1753)
R2^2/D10^2 : 4.88122E-03 (-0.00256638 0.00429399)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.84e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.264e-07 9.837e-08
25- 50 6.730e-07 1.278e-07
50-150 1.341e-06 3.786e-07
15-150 2.441e-06 6.119e-07
Peak spectrum fit
Power-law model
Time interval is from -48.592 sec. to -47.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12077 ( -0.496954 0.647289 )
Norm@50keV : 5.56155E-03 ( -0.00243307 0.00231449 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.58 using 59 bins.
Reduced chi-squared = 1.06281
# Null hypothesis probability of 3.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.884230 ( -0.315349 0.31603 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.17619e-08 ( -2.01399e-08 2.06917e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -48.592 sec. to -47.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.15250 ( -7.44362 2.85843 )
Epeak [keV] : 46.7124 ( -14.6362 19.077 )
Norm@50keV : 0.276156 ( -0.349135 2027.19 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.48 using 59 bins.
Reduced chi-squared = 1.00857
# Null hypothesis probability of 4.57e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.826297 ( -0.323402 0.328193 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.11493e-08 ( -1.88093e-08 2.06632e-08 ) ergs/cm2
Band function
Time interval is from -48.592 sec. to -47.592 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] : 12.0614 (-3.13792 3.96122)
R^2/D10^2 : 0.237528 (-0.237528 0.484095)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.311e-09 4.646e-09
25- 50 2.315e-08 1.365e-08
50-150 2.032e-08 1.492e-08
15-150 5.078e-08 3.191e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 60.5612 (-31.4524 89.3885)
Norm : 4.87999 (-2.01917 3.03052)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.20e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.228e-08 7.795e-09
25- 50 1.875e-08 1.193e-08
50-150 2.150e-08 1.816e-08
15-150 5.253e-08 3.444e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.77437 (-1.7874 13.1986)
R1^2/D10^2 : 1061.17 (-945.402 -945.402)
kT2 [keV] : 12.6712 (-3.33264 -12.6965)
R2^2/D10^2 : 0.188897 (-0.186907 0.397014)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.649e-09 4.665e-09
25- 50 2.159e-08 1.340e-08
50-150 2.153e-08 1.535e-08
15-150 5.277e-08 3.331e-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: 1.77879 ( -0.158636 0.163465 )
Norm@50keV : 1.51177E-03 ( -0.000159676 0.000157435 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 89.8 sec: 0.206631 ( -0.0191461 0.0191536 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25085e-06 ( -1.34583e-07 1.36514e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.993118 ( -0.791295 0.665428 )
Epeak [keV] : 55.9811 ( -11.9357 64.6737 )
Norm@50keV : 4.17104E-03 ( -0.00237034 0.00741901 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.17e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 89.8 sec: 0.200935 ( -0.019703 0.019716 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16142e-06 ( -1.48673e-07 1.54294e-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) = 6.84e-07
S(50-100 keV) = 8.24e-07
T90 vs. Hardness ratio plot
T90 = 102.683999896049 sec.
Hardness ratio (energy fluence ratio) = 1.20468
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.07985
Count Ratio (50-100 keV) / (15-25 keV) = 0.780218
Mask shadow pattern
IMX = 2.684805557516891E-01, IMY = -3.467912886804919E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-17.299400 72.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
334.5285 -62.7183 2.3 43.2 44.5 2.1014 5.1 ------ UNKNOWN
24.9415 -11.0896 2.3 43.0 143.8 1.8933 5.1 ------ UNKNOWN
15.6091 -59.0991 1.0 23.7 52.3 2.0912 11.5 ------ UNKNOWN
329.8941 -83.1745 2.8 41.5 14.0 1.0605 4.1 ------ UNKNOWN
17.8154 -75.8862 2.8 31.2 18.9 0.8348 4.2 ------ UNKNOWN
100.0310 -78.4150 2.6 35.3 -11.3 0.8022 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
132.500600 340.300640
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6573 -62.7704 33.9 57.9 -24.7 -0.4962 -0.3 0.0 GX 301-2
296.5070 -46.9259 2.5 46.1 48.6 3.8235 4.5 ------ UNKNOWN
320.7858 -47.8565 2.3 33.4 65.0 2.7322 5.0 ------ UNKNOWN
344.4906 -69.2372 2.7 16.6 19.9 1.0526 4.2 ------ UNKNOWN
59.3241 -19.6143 2.2 50.4 -142.2 4.5083 5.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:32:58 EST 2026