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
148.2718 35.6225 0.0130 37.6289 4.1994 2.3282373 14.730 TRIG_00799669
Foreground time interval of the image:
8.004 89.301 (delta_t = 81.297 [sec])
Background time interval of the image:
-239.000 8.004 (delta_t = 247.004 [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 8.004 sec. to 210.088 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.02276 ( -0.163922 0.170767 )
Norm@50keV : 1.00857E-03 ( -0.000111046 0.000108743 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.87 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 57 degrees of freedom
# Null hypothesis probability = 4.070246e-01
Photon flux (15-150 keV) in 202.1 sec: 0.152902 ( -0.013389 0.013396 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8825e-06 ( -1.91923e-07 1.9502e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.004 sec. to 210.088 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.89265 ( -0.715882 0.232882 )
Epeak [keV] : 34.7480 ( -25.4084 -34.7507 )
Norm@50keV : 1.19898E-03 ( -0.000379441 0.00187923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.74 using 59 PHA bins.
# Reduced chi-squared = 1.049 for 56 degrees of freedom
# Null hypothesis probability = 3.752399e-01
Photon flux (15-150 keV) in 202.1 sec: 0.152118 ( -0.01395 0.013649 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.85633e-06 ( -2.28177e-07 2.12884e-07 ) ergs/cm2
Band function
Time interval is from 8.004 sec. to 210.088 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] : 9.82798 (-1.06181 1.18742)
R^2/D10^2 : 7.38817E-02 (-0.0263441 0.0413731)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 92.69 using 59 PHA bins.
# Reduced chi-squared = 1.626 for 57 degrees of freedom
# Null hypothesis probability = 1.964352e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.919e-07 4.264e-08
25- 50 7.081e-07 8.337e-08
50-150 3.514e-07 8.377e-08
15-150 1.351e-06 1.555e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 65.2415 (-15.9063 24.2987)
Norm : 0.767065 (-0.109959 0.125798)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.55 using 59 PHA bins.
# Reduced chi-squared = 1.062 for 57 degrees of freedom
# Null hypothesis probability = 3.491464e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.944e-07 4.345e-08
25- 50 6.154e-07 6.043e-08
50-150 7.491e-07 1.687e-07
15-150 1.759e-06 1.943e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.03828 (-1.2285 1.69359)
R1^2/D10^2 : 0.703909 (-0.451769 1.51671)
kT2 [keV] : 17.7679 (-4.0767 10.0905)
R2^2/D10^2 : 5.59871E-03 (-0.00456824 0.0107975)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.45 using 59 PHA bins.
# Reduced chi-squared = 1.099 for 55 degrees of freedom
# Null hypothesis probability = 2.855111e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.285e-07 1.899e-07
25- 50 5.662e-07 2.066e-07
50-150 7.611e-07 4.317e-07
15-150 1.756e-06 6.420e-07
Peak spectrum fit
Power-law model
Time interval is from 61.344 sec. to 62.344 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12701 ( -0.582488 0.751566 )
Norm@50keV : 4.19165E-03 ( -0.00193912 0.00176756 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.65 using 59 PHA bins.
# Reduced chi-squared = 0.6957 for 57 degrees of freedom
# Null hypothesis probability = 9.610044e-01
Photon flux (15-150 keV) in 1 sec: 0.668443 ( -0.21774 0.217785 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.90607e-08 ( -1.50425e-08 1.5743e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 61.344 sec. to 62.344 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84669 ( -2.32453 0.209135 )
Epeak [keV] : 23.7728 ( )
Norm@50keV : 6.06269E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.61 using 59 PHA bins.
# Reduced chi-squared = 0.7072 for 56 degrees of freedom
# Null hypothesis probability = 9.523624e-01
Photon flux (15-150 keV) in 1 sec: 0.664582 ( -0.219776 0.216519 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 61.344 sec. to 62.344 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] : 9.39841 (-3.60457 5.90801)
R^2/D10^2 : 0.388872 (-0.383697 2.16905)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.69 using 59 PHA bins.
# Reduced chi-squared = 0.7489 for 57 degrees of freedom
# Null hypothesis probability = 9.205228e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.828e-09 4.321e-09
25- 50 1.551e-08 9.720e-09
50-150 6.744e-09 5.180e-09
15-150 2.908e-08 1.881e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 58.8724 (-35.2114 -58.8721)
Norm : 3.54237 (-1.53844 3.14175)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.75 using 59 PHA bins.
# Reduced chi-squared = 0.6974 for 57 degrees of freedom
# Null hypothesis probability = 9.600174e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.875e-09 5.658e-09
25- 50 1.343e-08 8.309e-09
50-150 1.504e-08 1.231e-08
15-150 3.734e-08 2.434e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.25574 (-4.27798 6.0605)
R1^2/D10^2 : 6.38373 (-5.9222 -6.15674)
kT2 [keV] : 16.6244 (-16.7076 -16.708)
R2^2/D10^2 : 3.35900E-02 (-0.0325602 0.538665)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.59 using 59 PHA bins.
# Reduced chi-squared = 0.7199 for 55 degrees of freedom
# Null hypothesis probability = 9.416431e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.679e-09 5.695e-09
25- 50 1.160e-08 6.410e-09
50-150 1.625e-08 1.224e-08
15-150 3.753e-08 1.947e-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: 1.81150 ( -0.188159 0.193918 )
Norm@50keV : 1.63596E-03 ( -0.000196354 0.000193073 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.29 using 59 PHA bins.
# Reduced chi-squared = 0.9524 for 57 degrees of freedom
# Null hypothesis probability = 5.775420e-01
Photon flux (15-150 keV) in 81.3 sec: 0.226444 ( -0.0247985 0.0248286 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22396e-06 ( -1.47844e-07 1.49428e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57563 ( -0.842169 0.725753 )
Epeak [keV] : 82.4839 ( )
Norm@50keV : 2.20087E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.98 using 59 PHA bins.
# Reduced chi-squared = 0.9640 for 56 degrees of freedom
# Null hypothesis probability = 5.516453e-01
Photon flux (15-150 keV) in 81.3 sec: 0.224519 ( -0.025575 0.025473 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20104e-06 ( -1.6538e-07 1.64137e-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) = 5.70e-07
S(50-100 keV) = 5.62e-07
T90 vs. Hardness ratio plot
T90 = 173.871999979019 sec.
Hardness ratio (energy fluence ratio) = 0.985965
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.95888
Count Ratio (50-100 keV) / (15-25 keV) = 0.484114
Mask shadow pattern
IMX = 7.688365867807131E-01, IMY = -5.645186769244518E-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:
-239.000000 8.004000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.1503 33.0107 3.2 33.0 104.6 1.7261 3.6 ------ UNKNOWN
130.8375 33.6549 2.4 33.1 28.1 1.5938 4.8 ------ UNKNOWN
40.9265 61.4279 0.2 29.1 -174.6 15.5668 56.6 ------ UNKNOWN
347.4721 49.9252 3.2 57.3 -154.0 5.8465 3.6 ------ UNKNOWN
183.6776 29.3441 3.6 58.7 -25.8 6.4191 3.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
8.004000 89.300610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
130.7981 40.7029 2.2 26.6 22.6 0.6754 5.3 ------ UNKNOWN
148.2718 35.6225 0.8 37.6 4.2 2.3282 14.7 ------ UNKNOWN
137.0188 61.9865 2.0 14.4 -32.5 0.6307 5.8 ------ UNKNOWN
167.2717 23.7478 2.9 56.1 -7.4 1.6484 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
158.500600 963.070700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
188.3721 50.7171 2.6 32.4 -132.7 2.9564 4.4 ------ UNKNOWN
234.8476 64.8095 3.7 56.8 -151.8 9.9779 3.1 ------ UNKNOWN
Plot creation:
Sat Jan 20 09:05:09 EST 2018