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
108.3372 -39.7784 0.0091 21.6201 156.9337 1.4409948 21.058 TRIG_00874475
Foreground time interval of the image:
-1.796 15.852 (delta_t = 17.648 [sec])
Background time interval of the image:
-298.187 -277.496 (delta_t = 20.691 [sec])
-239.888 -1.796 (delta_t = 238.092 [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 -1.796 sec. to 15.852 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81411 ( -0.143235 0.147382 )
Norm@50keV : 4.74708E-03 ( -0.000428446 0.000421681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.00 using 59 PHA bins.
# Reduced chi-squared = 0.9825 for 57 degrees of freedom
# Null hypothesis probability = 5.126057e-01
Photon flux (15-150 keV) in 17.65 sec: 0.657787 ( -0.051072 0.0511 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.71107e-07 ( -7.0145e-08 7.11498e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.796 sec. to 15.852 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62861 ( -0.611539 0.562442 )
Epeak [keV] : 89.3582 ( )
Norm@50keV : 6.01123E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.67 using 59 PHA bins.
# Reduced chi-squared = 0.9941 for 56 degrees of freedom
# Null hypothesis probability = 4.873852e-01
Photon flux (15-150 keV) in 17.65 sec: 0.652226 ( -0.053692 0.05351 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.56214e-07 ( -8.25016e-08 8.12662e-08 ) ergs/cm2
Band function
Time interval is from -1.796 sec. to 15.852 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] : 11.0556 (-1.0343 1.16739)
R^2/D10^2 : 0.209447 (-0.0656458 0.0934127)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 93.59 using 59 PHA bins.
# Reduced chi-squared = 1.642 for 57 degrees of freedom
# Null hypothesis probability = 1.615763e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.450e-08 1.302e-08
25- 50 2.690e-07 2.453e-08
50-150 1.864e-07 4.058e-08
15-150 5.499e-07 5.313e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.7381 (-25.2988 42.4819)
Norm : 2.90688 (-0.312833 0.370062)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.50 using 59 PHA bins.
# Reduced chi-squared = 0.9913 for 57 degrees of freedom
# Null hypothesis probability = 4.937133e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.341e-07 1.594e-08
25- 50 2.308e-07 2.162e-08
50-150 3.691e-07 1.341e-07
15-150 7.340e-07 1.446e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.99065 (-1.71697 1.60364)
R1^2/D10^2 : 0.860126 (-0.421062 1.38354)
kT2 [keV] : 26.7315 (-8.35672 20.9213)
R2^2/D10^2 : 5.68440E-03 (-0.00471038 0.0181058)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.60 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 55 degrees of freedom
# Null hypothesis probability = 3.793749e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.310e-07 3.377e-08
25- 50 2.330e-07 5.922e-08
50-150 3.951e-07 1.981e-07
15-150 7.591e-07 2.589e-07
Peak spectrum fit
Power-law model
Time interval is from 1.024 sec. to 2.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20429 ( -0.383372 0.365754 )
Norm@50keV : 9.05344E-03 ( -0.00165752 0.00165735 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.84 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 57 degrees of freedom
# Null hypothesis probability = 4.439689e-01
Photon flux (15-150 keV) in 1 sec: 1.06333 ( -0.20264 0.20346 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.17508e-08 ( -1.90097e-08 1.92203e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.024 sec. to 2.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20155 ( -0.412172 0.344458 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 9.09559E-03 ( -0.00166515 -0.00909559 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.86 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 56 degrees of freedom
# Null hypothesis probability = 4.063147e-01
Photon flux (15-150 keV) in 1 sec: 1.06976 ( -0.218146 0.20498 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.09829e-08 ( -1.82887e-08 1.99116e-08 ) ergs/cm2
Band function
Time interval is from 1.024 sec. to 2.024 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] : 24.5068 (-8.54227 13.3491)
R^2/D10^2 : 2.40969E-02 (-0.0168094 0.0688951)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.85 using 59 PHA bins.
# Reduced chi-squared = 1.278 for 57 degrees of freedom
# Null hypothesis probability = 7.683074e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.541e-09 1.308e-09
25- 50 1.427e-08 6.148e-09
50-150 6.370e-08 2.807e-08
15-150 8.050e-08 2.699e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-70.2313 -200)
Norm : 4.38443 (-0.823258 0.823258)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.79 using 59 PHA bins.
# Reduced chi-squared = 1.084 for 57 degrees of freedom
# Null hypothesis probability = 3.091358e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.092e-08 6.335e-09
25- 50 2.101e-08 1.215e-08
50-150 4.608e-08 2.635e-08
15-150 7.802e-08 4.503e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.11320 (-2.28181 2.82818)
R1^2/D10^2 : 1.17496 (-0.833849 3.27326)
kT2 [keV] : 57.4742 (-26.1665 -57.4692)
R2^2/D10^2 : 2.09050E-03 (-0.00175471 0.00800197)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.01 using 59 PHA bins.
# Reduced chi-squared = 0.9821 for 55 degrees of freedom
# Null hypothesis probability = 5.122963e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.038e-08 5.900e-09
25- 50 1.874e-08 1.022e-08
50-150 7.206e-08 3.882e-08
15-150 1.012e-07 5.230e-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: 1.81411 ( -0.143235 0.147382 )
Norm@50keV : 4.74708E-03 ( -0.000428446 0.000421681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.00 using 59 PHA bins.
# Reduced chi-squared = 0.9825 for 57 degrees of freedom
# Null hypothesis probability = 5.126057e-01
Photon flux (15-150 keV) in 17.65 sec: 0.657752 ( -0.0510675 0.0510961 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.70987e-07 ( -7.02253e-08 7.11556e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62860 ( -0.611538 0.562544 )
Epeak [keV] : 89.3568 ( )
Norm@50keV : 6.01127E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.67 using 59 PHA bins.
# Reduced chi-squared = 0.9941 for 56 degrees of freedom
# Null hypothesis probability = 4.873852e-01
Photon flux (15-150 keV) in 17.65 sec: 0.652096 ( -0.05367 0.026751 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.56415e-07 ( -8.26179e-08 8.11759e-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) = 2.19e-07
S(50-100 keV) = 2.49e-07
T90 vs. Hardness ratio plot
T90 = 15.0599999427795 sec.
Hardness ratio (energy fluence ratio) = 1.13699
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17674
Count Ratio (50-100 keV) / (15-25 keV) = 0.692999
Mask shadow pattern
IMX = -3.646480396765555E-01, IMY = -1.552817912817654E-01
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:
-298.187400 -277.496100
-239.888000 -1.796000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4639 -40.5188 11.5 35.4 -169.6 0.3349 1.0 3.7 Vela X-1
170.0526 -60.7291 0.0 41.7 -122.8 -1.1338 -1.7 10.0 Cen X-3
38.3144 -27.1524 2.5 44.3 34.0 2.8592 4.6 ------ UNKNOWN
53.0195 -29.0431 2.2 35.3 49.0 2.9732 5.3 ------ UNKNOWN
156.7354 -37.4734 3.0 49.5 -156.0 2.5124 3.9 ------ UNKNOWN
159.6455 -38.9094 3.0 50.1 -152.5 2.6223 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.796000 15.852000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5094 -40.6794 5.6 35.4 -169.4 0.1787 2.1 7.5 Vela X-1
170.1437 -60.4841 9.3 41.8 -123.1 0.1908 1.2 9.8 Cen X-3
108.3372 -39.7784 0.5 21.6 156.9 1.4411 21.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
60.012590 962.201700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4888 -40.6407 5.5 20.7 -131.1 1.7595 2.1 5.5 Vela X-1
102.5984 0.0856 3.6 40.2 118.8 9.0329 3.3 ------ UNKNOWN
121.8017 6.1901 3.7 47.6 146.0 8.2856 3.1 ------ UNKNOWN
75.0653 -75.7406 3.6 38.9 -39.8 3.4552 3.2 ------ UNKNOWN
Plot creation:
Mon Dec 17 21:02:58 EST 2018