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
84.3756 3.5793 0.0063 13.6316 -6.7139 2.2884759 30.629 TRIG_01347179
Foreground time interval of the image:
-19.204 20.173 (delta_t = 39.377 [sec])
Background time interval of the image:
-239.328 -19.204 (delta_t = 220.124 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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 1.024000
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 1.024000
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 -19.204 sec. to 56.588 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38340 ( -0.105536 0.105241 )
Norm@50keV : 2.40365E-03 ( -0.00013571 0.000135577 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.55 using 59 bins.
Reduced chi-squared = 0.904386
# Null hypothesis probability of 6.79e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 75.79 sec: 0.291642 ( -0.01717 0.017232 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76657e-06 ( -1.10072e-07 1.10632e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.204 sec. to 56.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38434 ( -0.110152 0.102117 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.40804E-03 ( -0.000135657 0.000596835 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.59 using 59 bins.
Reduced chi-squared = 0.92125
# Null hypothesis probability of 6.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 75.79 sec: 0.293232 ( -0.018828 0.015578 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76609e-06 ( -1.10235e-07 1.10555e-07 ) ergs/cm2
Band function
Time interval is from -19.204 sec. to 56.588 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] : 17.8154 ( )
R^2/D10^2 : 1.80432E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 154.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.36e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.718e-08 1.066e-08
25- 50 4.001e-07 3.160e-08
50-150 9.193e-07 9.701e-08
15-150 1.407e-06 9.663e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-17.0278 -200)
Norm : 1.20622 (-0.068276 0.068276)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.42e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.276e-07 1.417e-08
25- 50 4.379e-07 3.403e-08
50-150 9.603e-07 1.793e-07
15-150 1.626e-06 1.811e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.51761 (-0.974444 1.12744)
R1^2/D10^2 : 0.399401 (-0.175315 0.340614)
kT2 [keV] : 31.2116 (-4.63586 6.98071)
R2^2/D10^2 : 2.43196E-03 (-0.00112845 0.00168502)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.180e-07 3.918e-08
25- 50 3.982e-07 6.609e-08
50-150 1.191e-06 2.323e-07
15-150 1.808e-06 2.827e-07
Peak spectrum fit
Power-law model
Time interval is from 5.108 sec. to 6.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08907 ( -0.242043 0.23447 )
Norm@50keV : 9.39388E-03 ( -0.00126546 0.00126335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.46 using 59 bins.
Reduced chi-squared = 1.16596
# Null hypothesis probability of 1.83e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.08850 ( -0.150541 0.15105 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.85712e-08 ( -1.44975e-08 1.46037e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.108 sec. to 6.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.941272 ( -1.08149 0.363409 )
Epeak [keV] : 401.749 ( -401.755 -401.755 )
Norm@50keV : 1.09847E-02 ( -0.00436226 0.0215733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.39 using 59 bins.
Reduced chi-squared = 1.18554
# Null hypothesis probability of 1.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.08225 ( -0.15606 0.14964 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4494e-08 ( -1.02602e-08 5.08476e-09 ) ergs/cm2
Band function
Time interval is from 5.108 sec. to 6.108 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] : 20.8296 (-3.40641 4.42552)
R^2/D10^2 : 4.52843E-02 (-0.0208106 0.0355543)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.05e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.725e-09 1.090e-09
25- 50 1.905e-08 4.355e-09
50-150 6.156e-08 1.440e-08
15-150 8.433e-08 1.723e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-36.7084 -200)
Norm : 4.46869 (-0.620239 0.620239)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.03e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.112e-08 6.255e-09
25- 50 2.140e-08 1.189e-08
50-150 4.693e-08 2.620e-08
15-150 7.946e-08 4.349e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.21807 (-2.48927 10.5357)
R1^2/D10^2 : 2.12972 (-1.98681 41.3452)
kT2 [keV] : 26.2834 (-5.83781 -26.2834)
R2^2/D10^2 : 1.98072E-02 (-0.0193835 0.0176409)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.30e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.439e-09 4.678e-09
25- 50 1.789e-08 7.535e-09
50-150 6.853e-08 3.100e-08
15-150 9.486e-08 3.985e-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: 1.31729 ( -0.0973132 0.0968368 )
Norm@50keV : 3.75841E-03 ( -0.000194141 0.000194133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 39.38 sec: 0.449848 ( -0.0244709 0.0245674 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4565e-06 ( -8.28532e-08 8.31564e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31743 ( -0.106037 0.0940802 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.76819E-03 ( -0.000194741 0.000866314 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.14e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 39.38 sec: 0.449689 ( -0.012204 0.024501 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45521e-06 ( -8.15048e-08 8.47655e-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) = 4.12e-07
S(50-100 keV) = 6.31e-07
T90 vs. Hardness ratio plot
T90 = 46.7479999065399 sec.
Hardness ratio (energy fluence ratio) = 1.53155
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.25438
Count Ratio (50-100 keV) / (15-25 keV) = 1.07229
Mask shadow pattern
IMX = 2.408471398172416E-01, IMY = 2.835244323493349E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.328000 -19.204000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6107 22.0192 0.4 6.2 -140.1 8.6601 26.2 1.3 Crab
40.1457 16.4832 2.2 38.5 106.4 5.5873 5.2 ------ UNKNOWN
98.8820 -37.3924 2.8 56.8 -7.0 4.5296 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.204000 20.172600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6329 22.1660 6.4 6.4 -140.7 0.1443 1.8 9.1 Crab
84.3756 3.5793 0.4 13.6 -6.7 2.2885 30.6 ------ UNKNOWN
114.5113 -16.8612 2.0 47.5 -36.2 1.1876 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
65.572600 442.172620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6251 22.0073 0.4 18.4 -175.6 14.8498 27.9 0.6 Crab
82.0301 -48.6949 3.3 52.3 8.5 4.6437 3.5 ------ UNKNOWN
95.1071 58.6064 2.2 55.7 -166.7 9.1611 5.1 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:27:36 EST 2026