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
64.7393 15.2477 0.0149 32.9350 4.1658 1.7526560 12.999 TRIG_00865036
Foreground time interval of the image:
-28.376 43.624 (delta_t = 72.000 [sec])
Background time interval of the image:
-239.896 -28.376 (delta_t = 211.520 [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 16.384000
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 16.384000
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 16.384000
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 -28.376 sec. to 43.624 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.15346 ( -0.224855 0.243953 )
Norm@50keV : 1.31491E-03 ( -0.000215435 0.000209037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.42 using 59 PHA bins.
# Reduced chi-squared = 0.8319 for 57 degrees of freedom
# Null hypothesis probability = 8.131543e-01
Photon flux (15-150 keV) in 72 sec: 0.212519 ( -0.024619 0.024621 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.84894e-07 ( -1.25019e-07 1.28183e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -28.376 sec. to 43.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83517 ( -1.00152 0.244607 )
Epeak [keV] : 21.3061 ( )
Norm@50keV : 2.01917E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.02 using 59 PHA bins.
# Reduced chi-squared = 0.8396 for 56 degrees of freedom
# Null hypothesis probability = 7.981175e-01
Photon flux (15-150 keV) in 72 sec: 0.210154 ( -0.025389 0.025073 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.58305e-07 ( -1.38222e-07 1.43729e-07 ) ergs/cm2
Band function
Time interval is from -28.376 sec. to 43.624 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] : 9.33126 (-1.34938 1.53271)
R^2/D10^2 : 0.124929 (-0.0554788 0.104637)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.89 using 59 PHA bins.
# Reduced chi-squared = 1.156 for 57 degrees of freedom
# Null hypothesis probability = 1.964038e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.552e-07 3.571e-08
25- 50 3.487e-07 6.120e-08
50-150 1.484e-07 4.846e-08
15-150 6.523e-07 1.063e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 54.0954 (-15.9409 24.6801)
Norm : 1.15073 (-0.208481 0.297865)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.86 using 59 PHA bins.
# Reduced chi-squared = 0.8396 for 57 degrees of freedom
# Null hypothesis probability = 8.005502e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.060e-07 3.384e-08
25- 50 3.040e-07 8.622e-08
50-150 3.173e-07 1.920e-07
15-150 8.273e-07 3.133e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.92354 (-1.31165 1.76221)
R1^2/D10^2 : 2.81582 (-2.1618 6.89965)
kT2 [keV] : 14.4962 (-3.21256 5.74998)
R2^2/D10^2 : 1.78666E-02 (-0.0135287 0.0334614)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.57 using 59 PHA bins.
# Reduced chi-squared = 0.8467 for 55 degrees of freedom
# Null hypothesis probability = 7.836798e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.247e-07 1.132e-07
25- 50 2.762e-07 1.321e-07
50-150 3.087e-07 1.631e-07
15-150 8.096e-07 3.600e-07
Peak spectrum fit
Power-law model
Time interval is from 11.388 sec. to 12.388 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07282 ( -0.586847 0.726946 )
Norm@50keV : 4.13290E-03 ( -0.00184598 0.00168768 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.01 using 59 PHA bins.
# Reduced chi-squared = 1.123 for 57 degrees of freedom
# Null hypothesis probability = 2.439772e-01
Photon flux (15-150 keV) in 1 sec: 0.641678 ( -0.198823 0.198827 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.83116e-08 ( -1.44604e-08 1.53347e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 11.388 sec. to 12.388 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98828 ( )
Epeak [keV] : 11.9811 ( )
Norm@50keV : 4.45372E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.05 using 59 PHA bins.
# Reduced chi-squared = 1.144 for 56 degrees of freedom
# Null hypothesis probability = 2.149296e-01
Photon flux (15-150 keV) in 1 sec: 0.618501 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 11.388 sec. to 12.388 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] : 8.33347 (-2.74583 4.27013)
R^2/D10^2 : 0.592227 (-0.590824 2.31132)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.86 using 59 PHA bins.
# Reduced chi-squared = 1.173 for 57 degrees of freedom
# Null hypothesis probability = 1.745123e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.653e-09 4.734e-09
25- 50 1.436e-08 8.840e-09
50-150 4.306e-09 3.362e-09
15-150 2.632e-08 1.620e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 57.8691 (-35.7049 -57.8867)
Norm : 3.40229 (-1.47254 3.2808)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.54 using 59 PHA bins.
# Reduced chi-squared = 1.132 for 57 degrees of freedom
# Null hypothesis probability = 2.299544e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.499e-09 5.023e-09
25- 50 1.279e-08 7.470e-09
50-150 1.412e-08 1.065e-08
15-150 3.541e-08 2.246e-08
Double BB
# Reduced chi-squared = 1.158 for 55 degrees of freedom
# Reduced chi-squared = 1.157 for 55 degrees of freedom
# Reduced chi-squared = 1.157 for 55 degrees of freedom
# Null hypothesis probability = 1.935470e-01
# Null hypothesis probability = 1.943712e-01
# Null hypothesis probability = 1.949258e-01
# Null hypothesis probability = 1.954266e-01
# Null hypothesis probability = 1.958781e-01
# Null hypothesis probability = 1.962841e-01
# Null hypothesis probability = 1.966481e-01
# Null hypothesis probability = 1.974757e-01
# Null hypothesis probability = 1.984048e-01
# Null hypothesis probability = 1.988944e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.857e-09 5.825e-09
25- 50 1.236e-08 7.465e-09
50-150 1.961e-08 1.208e-08
15-150 4.082e-08 2.055e-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: 2.15346 ( -0.224855 0.243953 )
Norm@50keV : 1.31491E-03 ( -0.000215435 0.000209037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.42 using 59 PHA bins.
# Reduced chi-squared = 0.8319 for 57 degrees of freedom
# Null hypothesis probability = 8.131543e-01
Photon flux (15-150 keV) in 72 sec: 0.212499 ( -0.0246163 0.0246192 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.84736e-07 ( -1.24984e-07 1.28183e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83522 ( -1.00154 0.244601 )
Epeak [keV] : 21.3023 ( )
Norm@50keV : 2.01903E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.02 using 59 PHA bins.
# Reduced chi-squared = 0.8396 for 56 degrees of freedom
# Null hypothesis probability = 7.981175e-01
Photon flux (15-150 keV) in 72 sec: 0.210097 ( -0.024782 0.012703 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.58506e-07 ( -1.38478e-07 1.44252e-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) = 2.77e-07
S(50-100 keV) = 2.49e-07
T90 vs. Hardness ratio plot
T90 = 63.4079999923706 sec.
Hardness ratio (energy fluence ratio) = 0.898917
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.95516
Count Ratio (50-100 keV) / (15-25 keV) = 0.458454
Mask shadow pattern
IMX = 6.460851429346581E-01, IMY = -4.705791420954174E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
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:
-239.896000 -28.376000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6294 22.0193 0.4 38.9 -27.1 8.3626 26.4 0.4 Crab
331.2719 59.7301 2.3 45.7 -179.1 2.2196 5.1 ------ UNKNOWN
119.1817 77.8229 2.9 45.1 -120.1 4.3896 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-28.376000 43.624000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5289 22.1271 115.9 38.8 -27.1 0.0161 0.1 8.9 Crab
64.7394 15.2477 0.9 32.9 4.2 1.7525 13.0 ------ UNKNOWN
100.8703 22.1963 2.1 51.1 -41.8 3.0594 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
124.604600 962.164000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6258 22.0155 0.3 19.1 -107.6 35.0848 44.7 0.4 Crab
52.8147 -39.4648 4.0 55.8 17.1 11.7588 2.9 ------ UNKNOWN
61.4867 -4.8045 2.9 20.3 15.3 2.8569 4.0 ------ UNKNOWN
78.3889 33.8717 2.5 22.4 -143.0 3.0604 4.6 ------ UNKNOWN
Plot creation:
Fri Oct 26 12:20:50 EDT 2018