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
104.2255 39.3104 0.0129 29.4210 -8.7127 2.8004309 14.841 TRIG_00853882
Foreground time interval of the image:
-77.099 62.744 (delta_t = 139.843 [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 -93.580 sec. to 62.744 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77161 ( -0.118759 0.121149 )
Norm@50keV : 1.60322E-03 ( -0.000119899 0.000118771 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.26 using 59 PHA bins.
# Reduced chi-squared = 0.8642 for 57 degrees of freedom
# Null hypothesis probability = 7.572781e-01
Photon flux (15-150 keV) in 156.3 sec: 0.218547 ( -0.014892 0.014905 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.30999e-06 ( -1.76999e-07 1.78748e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -93.580 sec. to 62.744 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04361 ( -0.598274 0.519354 )
Epeak [keV] : 59.1297 ( -10.6492 37.4506 )
Norm@50keV : 4.00174E-03 ( -0.00188928 0.00444593 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.26 using 59 PHA bins.
# Reduced chi-squared = 0.7724 for 56 degrees of freedom
# Null hypothesis probability = 8.935343e-01
Photon flux (15-150 keV) in 156.3 sec: 0.211574 ( -0.015679 0.015669 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.1576e-06 ( -2.02946e-07 2.06683e-07 ) ergs/cm2
Band function
Time interval is from -93.580 sec. to 62.744 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] : 11.7307 (-0.902485 0.992486)
R^2/D10^2 : 5.74146E-02 (-0.0150594 0.0200661)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.54 using 59 PHA bins.
# Reduced chi-squared = 1.325 for 57 degrees of freedom
# Null hypothesis probability = 5.065869e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.606e-07 3.165e-08
25- 50 7.983e-07 6.549e-08
50-150 6.504e-07 9.573e-08
15-150 1.709e-06 1.436e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8430 (-19.9173 39.76)
Norm : 0.969659 (-0.0967825 0.092158)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.79 using 59 PHA bins.
# Reduced chi-squared = 0.7683 for 57 degrees of freedom
# Null hypothesis probability = 9.004442e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.961e-07 4.611e-08
25- 50 6.848e-07 5.064e-08
50-150 1.109e-06 3.521e-07
15-150 2.190e-06 3.822e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.64171 (-1.68351 1.59226)
R1^2/D10^2 : 0.197123 (-0.0855671 0.22287)
kT2 [keV] : 24.5351 (-6.69955 16.18)
R2^2/D10^2 : 2.38913E-03 (-0.00198216 0.00653884)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.52 using 59 PHA bins.
# Reduced chi-squared = 0.7731 for 55 degrees of freedom
# Null hypothesis probability = 8.904826e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.532e-07 8.940e-08
25- 50 7.280e-07 1.862e-07
50-150 1.106e-06 5.163e-07
15-150 2.187e-06 7.378e-07
Peak spectrum fit
Power-law model
Time interval is from -82.112 sec. to -81.112 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73154 ( -0.284623 0.294612 )
Norm@50keV : 8.62467E-03 ( -0.00162044 0.00157474 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.11 using 59 PHA bins.
# Reduced chi-squared = 1.125 for 57 degrees of freedom
# Null hypothesis probability = 2.413325e-01
Photon flux (15-150 keV) in 1 sec: 1.15842 ( -0.188337 0.18838 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.96856e-08 ( -1.52835e-08 1.56533e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -82.112 sec. to -81.112 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.00705 ( -1.2838 -2.00705 )
Epeak [keV] : 2.99380 ( )
Norm@50keV : 6.02231E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.01 using 59 PHA bins.
# Reduced chi-squared = 1.143 for 56 degrees of freedom
# Null hypothesis probability = 2.159988e-01
Photon flux (15-150 keV) in 1 sec: 1.15906 ( -0.18907 0.18803 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.00958e-08 ( -1.94864e-08 1.12776e-08 ) ergs/cm2
Band function
Time interval is from -82.112 sec. to -81.112 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] : 9.12194 (-1.39371 1.77107)
R^2/D10^2 : 0.794330 (-0.396035 0.708705)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.22 using 59 PHA bins.
# Reduced chi-squared = 1.214 for 57 degrees of freedom
# Null hypothesis probability = 1.286217e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.296e-08 3.483e-09
25- 50 2.812e-08 7.610e-09
50-150 1.118e-08 5.223e-09
15-150 5.225e-08 1.296e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 104.675 (-49.3827 -105.386)
Norm : 5.14103 (-1.04595 1.45389)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.87 using 59 PHA bins.
# Reduced chi-squared = 1.138 for 57 degrees of freedom
# Null hypothesis probability = 2.214374e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.343e-08 2.951e-09
25- 50 2.344e-08 5.975e-09
50-150 3.897e-08 2.375e-08
15-150 7.585e-08 2.757e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.92606 (-1.19627 1.53826)
R1^2/D10^2 : 1.23764 (-0.668731 1.56776)
kT2 [keV] : 200.000 (-161.711 -200)
R2^2/D10^2 : 1.50814E-04 (-5.84057e-05 0.000592647)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.32 using 59 PHA bins.
#Fit statistic : Chi-Squared = 53.11 using 59 PHA bins.
# Reduced chi-squared = 0.9694 for 55 degrees of freedom
# Reduced chi-squared = 0.9656 for 55 degrees of freedom
# Null hypothesis probability = 5.391909e-01
# Null hypothesis probability = 5.472904e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.427e-08 5.852e-09
25- 50 2.541e-08 1.041e-08
50-150 4.731e-08 3.880e-08
15-150 8.699e-08 4.971e-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: 1.85527 ( -0.156226 0.161962 )
Norm@50keV : 1.21470E-03 ( -0.000126848 0.000124885 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.78 using 59 PHA bins.
# Reduced chi-squared = 0.8032 for 57 degrees of freedom
# Null hypothesis probability = 8.565630e-01
Photon flux (15-150 keV) in 139.8 sec: 0.171106 ( -0.0152459 0.0152529 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56133e-06 ( -1.61862e-07 1.64254e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.991055 ( -0.835139 0.689963 )
Epeak [keV] : 50.5758 ( -9.94902 33.6625 )
Norm@50keV : 3.71530E-03 ( -0.00216573 0.0072771 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.04 using 59 PHA bins.
# Reduced chi-squared = 0.7328 for 56 degrees of freedom
# Null hypothesis probability = 9.331440e-01
Photon flux (15-150 keV) in 139.8 sec: 0.165486 ( -0.01585 0.015858 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44103e-06 ( -1.79425e-07 1.87234e-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) = 6.44e-07
S(50-100 keV) = 7.53e-07
T90 vs. Hardness ratio plot
T90 = 137.459999918938 sec.
Hardness ratio (energy fluence ratio) = 1.16925
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36914
Count Ratio (50-100 keV) / (15-25 keV) = 0.720723
Mask shadow pattern
IMX = 5.574473002885124E-01, IMY = 8.542741209734461E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-77.099400 62.744000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6046 22.0135 1.0 53.4 0.3 5.4893 11.5 1.6 Crab
259.0004 66.7174 2.7 46.0 139.2 2.7336 4.2 ------ UNKNOWN
104.2255 39.3103 0.8 29.4 -8.7 2.8001 14.8 ------ UNKNOWN
88.9502 21.4470 2.2 51.5 -5.5 2.1671 5.3 ------ UNKNOWN
190.1023 23.0934 2.3 51.8 -137.1 4.6773 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
192.900600 963.088400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6207 22.0174 0.3 24.7 29.5 31.5076 44.9 0.7 Crab
58.4701 37.0031 2.8 35.7 79.2 6.2993 4.1 ------ UNKNOWN
86.9088 -15.2887 2.7 56.9 -1.9 11.9748 4.3 ------ UNKNOWN
203.1833 67.6172 2.7 57.3 -175.4 15.9752 4.2 ------ UNKNOWN
125.2390 48.6750 2.8 17.7 -150.8 2.6951 4.1 ------ UNKNOWN
91.9843 -14.6474 2.6 55.2 -7.5 8.5101 4.5 ------ UNKNOWN
186.9567 55.1449 3.0 54.8 -158.1 12.7864 3.8 ------ UNKNOWN
156.2611 41.7389 3.5 39.0 -132.9 4.1794 3.3 ------ UNKNOWN
Plot creation:
Fri Oct 26 12:35:57 EDT 2018