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
46.4523 -38.8551 0.0042 9.4275 53.9425 2.7331857 45.931 TRIG_01311764
Foreground time interval of the image:
-2.848 15.493 (delta_t = 18.341 [sec])
Background time interval of the image:
-239.208 -2.848 (delta_t = 236.360 [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 -2.848 sec. to 71.464 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54478 ( -0.0768741 0.077158 )
Norm@50keV : 3.48761E-03 ( -0.000146047 0.000145563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.33 using 59 bins.
Reduced chi-squared = 1.00579
# Null hypothesis probability of 4.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 74.31 sec: 0.440859 ( -0.018817 0.018851 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44195e-06 ( -1.10926e-07 1.11496e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.848 sec. to 71.464 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38784 ( -0.306578 0.201806 )
Epeak [keV] : 196.447 ( -98.2328 -196.525 )
Norm@50keV : 4.17499E-03 ( -0.000798757 0.00170632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.47 using 59 bins.
Reduced chi-squared = 1.00839
# Null hypothesis probability of 4.57e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 74.31 sec: 0.436565 ( -0.020338 0.020346 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.408e-06 ( -1.27515e-07 1.26878e-07 ) ergs/cm2
Band function
Time interval is from -2.848 sec. to 71.464 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] : 14.6258 ( )
R^2/D10^2 : 5.22856E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 188.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.17e-16 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.747e-07 1.479e-08
25- 50 6.778e-07 3.641e-08
50-150 9.755e-07 7.988e-08
15-150 1.828e-06 8.992e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-33.793 -200)
Norm : 1.78548 (-0.0728144 0.0728144)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.308e-07 1.382e-08
25- 50 6.363e-07 2.716e-08
50-150 1.396e-06 6.131e-08
15-150 2.363e-06 1.144e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.70283 (-1.01327 1.06716)
R1^2/D10^2 : 0.347517 (-0.118304 0.207961)
kT2 [keV] : 29.9927 (-4.91385 7.9122)
R2^2/D10^2 : 3.30279E-03 (-0.00176745 0.00293194)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.07e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.035e-07 3.879e-08
25- 50 6.535e-07 6.558e-08
50-150 1.456e-06 3.429e-07
15-150 2.413e-06 4.161e-07
Peak spectrum fit
Power-law model
Time interval is from 0.416 sec. to 1.416 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16408 ( -0.148673 0.147119 )
Norm@50keV : 1.64145E-02 ( -0.00140307 0.00140294 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.96 using 59 bins.
Reduced chi-squared = 1.29754
# Null hypothesis probability of 6.49e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.91756 ( -0.16675 0.16691 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68287e-07 ( -1.62077e-08 1.63548e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.416 sec. to 1.416 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.818759 ( -0.606261 0.415722 )
Epeak [keV] : 183.658 ( -183.658 -183.658 )
Norm@50keV : 2.40013E-02 ( -0.0085651 0.0214277 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.77 using 59 bins.
Reduced chi-squared = 1.29946
# Null hypothesis probability of 6.54e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.89199 ( -0.17175 0.17155 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.82159e-08 ( -1.0536e-08 1.31306e-08 ) ergs/cm2
Band function
Time interval is from 0.416 sec. to 1.416 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] : 19.3900 (-2.20499 2.54211)
R^2/D10^2 : 9.87918E-02 (-0.0323899 0.0475074)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 97.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.54e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.246e-09 1.244e-09
25- 50 3.535e-08 4.515e-09
50-150 9.805e-08 1.489e-08
15-150 1.406e-07 1.640e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-20.4301 -200)
Norm : 7.82703 (-0.684693 0.684693)
------------------------------------------------------------
#Fit statistic : Chi-Squared 90.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.91e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.949e-08 2.130e-09
25- 50 3.750e-08 1.292e-08
50-150 8.224e-08 3.727e-08
15-150 1.392e-07 4.298e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.08337 (-1.81678 2.49773)
R1^2/D10^2 : 1.46344 (-0.897572 2.64237)
kT2 [keV] : 29.2555 (-5.63565 11.0778)
R2^2/D10^2 : 2.23127E-02 (-0.014382 0.0237382)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.07e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.497e-08 7.006e-09
25- 50 3.525e-08 1.239e-08
50-150 1.159e-07 5.009e-08
15-150 1.661e-07 6.393e-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: 1.38999 ( -0.0629309 0.0628506 )
Norm@50keV : 9.65665E-03 ( -0.000329769 0.000329698 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.34 sec: 1.17336 ( -0.0420768 0.0421436 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.71482e-06 ( -6.4216e-08 6.44027e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21797 ( -0.247804 0.198568 )
Epeak [keV] : 238.752 ( -110.44 -238.757 )
Norm@50keV : 1.16863E-02 ( -0.00221334 0.00358132 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.34 sec: 1.16157 ( -0.04483 0.04487 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69292e-06 ( -7.17681e-08 7.13426e-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) = 6.17e-07
S(50-100 keV) = 8.47e-07
T90 vs. Hardness ratio plot
T90 = 54.3279999494553 sec.
Hardness ratio (energy fluence ratio) = 1.37277
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36056
Count Ratio (50-100 keV) / (15-25 keV) = 0.88448
Mask shadow pattern
IMX = 9.773204041814562E-02, IMY = -1.342329241330164E-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:
-239.208000 -2.848000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
33.5492 -69.8670 2.4 39.8 82.0 6.6914 4.8 ------ UNKNOWN
101.5557 -34.4284 2.6 50.1 9.1 2.8236 4.4 ------ UNKNOWN
97.5924 -27.8118 3.4 48.5 -0.5 1.9842 3.4 ------ UNKNOWN
101.3767 -26.6342 2.6 52.1 -0.6 3.0666 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.848000 15.492600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
46.4523 -38.8551 0.3 9.4 53.9 2.7333 45.9 ------ UNKNOWN
351.7870 -4.2994 2.5 53.6 -173.5 0.8282 4.7 555.8 UNKNOWN
89.4780 -8.0041 2.4 49.9 -28.6 0.6971 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
58.492600 677.592600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
338.8346 -40.8304 2.4 50.6 154.3 13.6907 4.7 ------ UNKNOWN
1.5031 -6.0878 1.8 52.1 -153.5 15.1801 6.4 376.2 UNKNOWN
Plot creation:
Fri Jun 20 01:40:16 EDT 2025