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
5.6678 -0.2639 0.0123 24.8303 170.5365 0.1881012 15.644 TRIG_00973628
Foreground time interval of the image:
-0.016 0.672 (delta_t = 0.688 [sec])
Background time interval of the image:
-239.104 -0.016 (delta_t = 239.088 [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 -0.016 sec. to 0.672 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45184 ( -0.168983 0.171227 )
Norm@50keV : 1.68135E-02 ( -0.00183456 0.00182433 )
------------------------------------------------------------
Photon flux (15-150 keV) in 0.688 sec: 2.07303 ( -0.2197 0.21981 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10672e-07 ( -1.32635e-08 1.34009e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.016 sec. to 0.672 sec.
XSPEC: quit
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.534902 ( -0.829632 0.694607 )
Epeak [keV] : 77.7636 ( -18.3751 86.7387 )
Norm@50keV : 5.04322E-02 ( -0.028031 0.0833924 )
------------------------------------------------------------
Photon flux (15-150 keV) in 0.688 sec: 2.01902 ( -0.22365 0.22368 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03896e-07 ( -1.42005e-08 1.44054e-08 ) ergs/cm2
Band function
Time interval is from -0.016 sec. to 0.672 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] : 14.6810 (-1.7851 2.07274)
R^2/D10^2 : 0.266314 (-0.098652 0.15246)
(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 8.295e-09 1.687e-09
25- 50 3.231e-08 4.376e-09
50-150 4.693e-08 9.911e-09
15-150 8.753e-08 1.190e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-62.9333 -200)
Norm : 8.56088 (-0.895777 0.895777)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.467e-08 7.066e-09
25- 50 2.822e-08 1.548e-08
50-150 6.188e-08 3.409e-08
15-150 1.048e-07 5.752e-08
Double BB
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.70454 (-2.48788 2.99551)
R1^2/D10^2 : 1.39907 (-0.847405 2.42811)
kT2 [keV] : 24.0885 (-6.13673 15.4738)
R2^2/D10^2 : 3.47547E-02 (-0.0291933 0.0770485)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.249e-08 6.712e-09
25- 50 3.010e-08 1.572e-08
50-150 6.290e-08 3.523e-08
15-150 1.055e-07 5.377e-08
Peak spectrum fit
Power-law model
Time interval is from -0.170 sec. to 0.830 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41246 ( -0.182888 0.183848 )
Norm@50keV : 1.21961E-02 ( -0.00142297 0.00141713 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 sec: 1.48954 ( -0.1715 0.17164 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17566e-07 ( -1.50811e-08 1.52315e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.170 sec. to 0.830 sec.
XSPEC: quit
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.602359 ( -0.855772 0.742177 )
Epeak [keV] : 84.0885 ( -23.1773 204.322 )
Norm@50keV : 3.22326E-02 ( -0.0181839 0.0563063 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 sec: 1.45644 ( -0.17401 0.17413 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10958e-07 ( -1.62929e-08 1.64216e-08 ) ergs/cm2
Band function
Time interval is from -0.170 sec. to 0.830 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] : 14.8246 (-2.04908 2.44738)
R^2/D10^2 : 0.184673 (-0.0763249 0.125729)
(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 8.513e-09 1.954e-09
25- 50 3.346e-08 5.920e-09
50-150 4.978e-08 1.155e-08
15-150 9.175e-08 1.529e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-59.3801 -200)
Norm : 6.16447 (-0.699984 0.699984)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.535e-08 5.211e-09
25- 50 2.953e-08 1.611e-08
50-150 6.476e-08 3.554e-08
15-150 1.097e-07 6.045e-08
Double BB
XSPEC12>/*
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.16785 (-2.15986 2.63919)
R1^2/D10^2 : 0.909362 (-0.508834 1.49413)
kT2 [keV] : 27.6958 (-7.68994 20.559)
R2^2/D10^2 : 1.52605E-02 (-0.013207 0.0383754)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.306e-08 6.953e-09
25- 50 3.165e-08 1.557e-08
50-150 6.939e-08 3.694e-08
15-150 1.141e-07 5.752e-08
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: 1.45184 ( -0.168983 0.171227 )
Norm@50keV : 1.68135E-02 ( -0.00183456 0.00182433 )
------------------------------------------------------------
Photon flux (15-150 keV) in 0.688 sec: 2.07299 ( -0.219698 0.2198 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10659e-07 ( -1.32613e-08 1.34042e-08 ) ergs/cm2
Cutoff power-law model
XSPEC: quit
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.534902 ( -0.829632 0.694608 )
Epeak [keV] : 77.7636 ( -18.3751 86.7387 )
Norm@50keV : 5.04323E-02 ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 0.688 sec: 2.01885 ( -0.22362 0.22364 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03934e-07 ( -1.42044e-08 1.44177e-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) = 2.67e-08
S(50-100 keV) = 3.91e-08
T90 vs. Hardness ratio plot
T90 = 0.615999937057495 sec.
Hardness ratio (energy fluence ratio) = 1.46442
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.52769
Count Ratio (50-100 keV) / (15-25 keV) = 1.1371
Mask shadow pattern
IMX = -4.564087144354455E-01, IMY = -7.607749107181289E-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:
-239.104000 -0.016000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
76.7383 -50.4005 2.8 54.0 8.1 3.1733 4.1 ------ UNKNOWN
19.4080 36.8170 4.0 52.2 -140.7 3.3170 2.9 ------ UNKNOWN
26.8063 34.0545 3.1 49.1 -133.1 4.0978 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.016000 0.672000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
5.6678 -0.2638 0.7 24.8 170.5 0.1881 15.6 340.4 UNKNOWN
1.1358 32.6606 2.2 53.2 -160.2 0.1835 5.2 ------ UNKNOWN
81.0879 -22.1319 2.1 52.6 -27.6 0.1803 5.5 ------ UNKNOWN
50.8027 8.8444 2.0 34.4 -86.6 0.1271 5.7 ------ UNKNOWN
49.1078 18.8011 2.4 40.9 -99.3 0.2245 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.196590 648.796630
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1844 38.3653 66.4 53.0 166.5 -0.3494 -0.2 2.7 Cyg X-2
339.6336 -29.7038 3.0 38.5 63.0 4.7819 3.8 ------ UNKNOWN
351.4667 -32.1571 4.1 34.6 46.7 2.2911 2.8 ------ UNKNOWN
332.3911 45.2501 2.2 54.2 176.7 11.0852 5.3 ------ UNKNOWN
4.0307 -3.6480 2.5 3.7 51.2 2.0404 4.7 326.1 UNKNOWN
347.3648 30.4812 2.7 35.4 177.3 2.7433 4.3 ------ UNKNOWN
Plot creation:
Wed Jul 1 20:10:18 EDT 2020