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
335.6935 -7.5269 0.0096 47.0631 -168.2027 1.6086980 20.041 TRIG_00966554
Foreground time interval of the image:
-2.336 4.960 (delta_t = 7.296 [sec])
Background time interval of the image:
-216.851 -2.336 (delta_t = 214.515 [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 -2.336 sec. to 4.960 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76692 ( -0.144546 0.147398 )
Norm@50keV : 1.40791E-02 ( -0.00122581 0.00121254 )
------------------------------------------------------------
Photon flux (15-150 keV) in 7.296 sec: 1.91584 ( -0.15987 0.16023 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.47123e-07 ( -8.43337e-08 8.49605e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.336 sec. to 4.960 sec.
XSPEC: quit
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76479 ( -0.431013 0.149171 )
Epeak [keV] : 9999.21 ( -9999.35 -9999.36 )
Norm@50keV : 1.41110E-02 ( -0.00697438 0.00938523 )
------------------------------------------------------------
Photon flux (15-150 keV) in 7.296 sec: 1.91925 ( -0.1711 0.16444 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.49458e-07 ( -9.16006e-08 8.68166e-08 ) ergs/cm2
Band function
Time interval is from -2.336 sec. to 4.960 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
XSPEC12>exit
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.9530 (-1.30811 1.49638)
R^2/D10^2 : 0.455497 (-0.161824 0.247559)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.004e-07 1.678e-08
25- 50 3.145e-07 3.258e-08
50-150 2.695e-07 5.067e-08
15-150 6.843e-07 7.522e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 112.330 (-29.7767 67.8562)
Norm : 8.30087 (-0.948842 0.965874)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.581e-07 1.974e-08
25- 50 2.795e-07 2.765e-08
50-150 4.824e-07 1.800e-07
15-150 9.200e-07 1.979e-07
Double BB
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.03194 (-1.24339 1.39137)
R1^2/D10^2 : 2.60167 (-1.22622 2.7031)
kT2 [keV] : 33.0019 (-9.27355 22.4858)
R2^2/D10^2 : 8.92793E-03 (-0.00682686 0.0186437)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.619e-07 3.958e-08
25- 50 2.762e-07 6.143e-08
50-150 5.280e-07 2.646e-07
15-150 9.661e-07 3.038e-07
Peak spectrum fit
Power-law model
Time interval is from -0.028 sec. to 0.972 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66542 ( -0.200197 0.206484 )
Norm@50keV : 2.86049E-02 ( -0.00364012 0.00360853 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 sec: 3.75446 ( -0.4715 0.4726 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.65675e-07 ( -3.52445e-08 3.54591e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.028 sec. to 0.972 sec.
XSPEC: quit
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04664 ( -0.975007 0.741105 )
Epeak [keV] : 77.8180 ( -19.7754 -77.818 )
Norm@50keV : 5.88622E-02 ( -0.0324648 0.120783 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 sec: 3.67676 ( -0.48319 0.48374 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.58131e-07 ( -3.72644e-08 3.71531e-08 ) ergs/cm2
Band function
Time interval is from -0.028 sec. to 0.972 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
XSPEC12>exit
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.0564 (-1.96105 2.25948)
R^2/D10^2 : 0.534677 (-0.224064 0.384502)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.231e-08 4.980e-09
25- 50 8.330e-08 1.388e-08
50-150 1.086e-07 2.559e-08
15-150 2.142e-07 3.365e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 153.017 (-60.9817 -151.634)
Norm : 15.5240 (-2.0871 2.67225)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.980e-08 1.375e-08
25- 50 7.399e-08 3.777e-08
50-150 1.472e-07 8.590e-08
15-150 2.610e-07 1.273e-07
Double BB
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.33777 (-2.80812 3.1854)
R1^2/D10^2 : 3.42778 (-2.28175 15.0464)
kT2 [keV] : 24.0503 (-6.98675 22.9827)
R2^2/D10^2 : 5.47295E-02 (-0.0497182 0.102798)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.667e-08 2.038e-08
25- 50 7.771e-08 4.082e-08
50-150 1.435e-07 7.843e-08
15-150 2.579e-07 1.260e-07
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
XSPEC12>exit
XSPEC: quit
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76692 ( -0.144546 0.147398 )
Norm@50keV : 1.40791E-02 ( -0.00122581 0.00121254 )
------------------------------------------------------------
Photon flux (15-150 keV) in 7.296 sec: 1.91574 ( -0.159855 0.160217 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.46984e-07 ( -8.44556e-08 8.49612e-08 ) ergs/cm2
Cutoff power-law model
XSPEC: quit
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76437 ( -0.188537 0.563789 )
Epeak [keV] : 9998.95 ( -9999.34 -9999.35 )
Norm@50keV : 1.41168E-02 ( -0.00696545 0.00938676 )
------------------------------------------------------------
Photon flux (15-150 keV) in 7.296 sec: 1.91483 ( -0.15801 0.16029 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.46685e-07 ( -8.53559e-08 8.43491e-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) = 2.63e-07
S(50-100 keV) = 3.09e-07
T90 vs. Hardness ratio plot
T90 = 6.04799997806549 sec.
Hardness ratio (energy fluence ratio) = 1.1749
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.19289
Count Ratio (50-100 keV) / (15-25 keV) = 0.765201
Mask shadow pattern
IMX = -1.052036859068425E+00, IMY = 2.197308086859326E-01
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:
-216.851410 -2.336000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
88.9907 -34.2591 3.3 58.3 -0.4 4.8892 3.6 ------ UNKNOWN
84.2391 -30.3213 3.1 56.7 -6.9 3.6739 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.336000 4.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
335.6935 -7.5269 0.6 47.1 -168.2 1.6087 20.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
83.748590 780.748600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5634 35.2096 6.2 54.7 163.4 6.7179 1.9 1.4 Cyg X-1
308.1724 41.0616 3.3 54.8 174.3 9.4346 3.5 7.1 Cyg X-3
326.1298 38.4057 4.5 46.8 -170.7 3.8111 2.6 5.4 Cyg X-2
309.1448 -11.7385 2.9 26.5 98.4 4.1604 4.0 ------ UNKNOWN
303.0076 37.7456 2.8 54.6 168.0 13.0934 4.1 ------ UNKNOWN
333.4291 -10.8890 3.7 4.0 53.2 1.8650 3.1 ------ UNKNOWN
Plot creation:
Mon Jun 1 00:11:20 EDT 2020