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
33.2144 38.1112 0.0065 32.6971 75.0753 9.7042926 29.238 TRIG_00882747
Foreground time interval of the image:
5.868 105.701 (delta_t = 99.833 [sec])
Background time interval of the image:
-239.000 5.868 (delta_t = 244.868 [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 5.868 sec. to 206.680 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86377 ( -0.0777441 0.0789212 )
Norm@50keV : 3.33414E-03 ( -0.000160588 0.000159786 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 88.84 using 59 PHA bins.
# Reduced chi-squared = 1.559 for 57 degrees of freedom
# Null hypothesis probability = 4.421823e-03
Photon flux (15-150 keV) in 200.8 sec: 0.471319 ( -0.021483 0.021519 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.15607e-06 ( -2.96389e-07 2.97857e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.868 sec. to 206.680 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.329152 ( -0.501856 0.451168 )
Epeak [keV] : 49.5010 ( -3.45164 4.3706 )
Norm@50keV : 2.19279E-02 ( -0.0092747 0.0187229 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.11 using 59 PHA bins.
# Reduced chi-squared = 0.8234 for 56 degrees of freedom
# Null hypothesis probability = 8.243563e-01
Photon flux (15-150 keV) in 200.8 sec: 0.435178 ( -0.023269 0.023359 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.45272e-06 ( -3.30675e-07 3.38944e-07 ) ergs/cm2
Band function
Time interval is from 5.868 sec. to 206.680 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] : 11.8437 (-0.529047 0.555814)
R^2/D10^2 : 0.119359 (-0.0192333 0.0227509)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.43 using 59 PHA bins.
# Reduced chi-squared = 1.323 for 57 degrees of freedom
# Null hypothesis probability = 5.153661e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.102e-07 5.271e-08
25- 50 2.201e-06 1.014e-07
50-150 1.840e-06 2.011e-07
15-150 4.751e-06 2.309e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 86.0631 (-11.5476 14.6537)
Norm : 2.16956 (-0.143345 0.155199)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.23 using 59 PHA bins.
# Reduced chi-squared = 1.057 for 57 degrees of freedom
# Null hypothesis probability = 3.596638e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.135e-06 8.032e-08
25- 50 1.900e-06 8.564e-08
50-150 2.814e-06 3.012e-07
15-150 5.849e-06 5.371e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.24100 (-2.16526 1.34305)
R1^2/D10^2 : 0.229869 (-0.0660862 0.172582)
kT2 [keV] : 24.5951 (-9.14761 34.3291)
R2^2/D10^2 : 3.37056E-03 (-0.00264408 0.0199925)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.64 using 59 PHA bins.
# Reduced chi-squared = 0.8479 for 55 degrees of freedom
# Null hypothesis probability = 7.815662e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.493e-07 1.195e-07
25- 50 2.125e-06 3.179e-07
50-150 2.526e-06 9.102e-07
15-150 5.500e-06 1.223e-06
Peak spectrum fit
Power-law model
Time interval is from 38.828 sec. to 39.828 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66823 ( -0.299432 0.316979 )
Norm@50keV : 1.41677E-02 ( -0.00285587 0.00279874 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.63 using 59 PHA bins.
# Reduced chi-squared = 1.151 for 57 degrees of freedom
# Null hypothesis probability = 2.026216e-01
Photon flux (15-150 keV) in 1 sec: 1.86130 ( -0.35172 0.35208 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.31553e-07 ( -2.75035e-08 2.77926e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 38.828 sec. to 39.828 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.912667 ( -1.57242 1.29019 )
Epeak [keV] : 72.6505 ( -46.5543 -72.6503 )
Norm@50keV : 3.44005E-02 ( -0.0344017 0.165804 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.50 using 59 PHA bins.
# Reduced chi-squared = 1.152 for 56 degrees of freedom
# Null hypothesis probability = 2.036946e-01
Photon flux (15-150 keV) in 1 sec: 1.82764 ( -0.36021 0.35795 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.43865e-08 ( -3.1676e-08 2.08075e-08 ) ergs/cm2
Band function
Time interval is from 38.828 sec. to 39.828 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] : 14.7130 (-2.84503 3.49294)
R^2/D10^2 : 0.230715 (-0.124628 0.266214)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.58 using 59 PHA bins.
# Reduced chi-squared = 1.221 for 57 degrees of freedom
# Null hypothesis probability = 1.224821e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.049e-08 3.991e-09
25- 50 4.093e-08 1.307e-08
50-150 5.977e-08 2.312e-08
15-150 1.112e-07 3.506e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 151.488 (-76.4519 -149.209)
Norm : 7.75252 (-1.54934 2.07587)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.78 using 59 PHA bins.
# Reduced chi-squared = 1.136 for 57 degrees of freedom
# Null hypothesis probability = 2.237244e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.990e-08 1.145e-08
25- 50 3.693e-08 2.074e-08
50-150 7.319e-08 4.436e-08
15-150 1.300e-07 7.615e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.51313 (-1.73257 3.42655)
R1^2/D10^2 : 29.5053 (-27.9774 2073.44)
kT2 [keV] : 17.7924 (-3.86832 6.05245)
R2^2/D10^2 : 0.104875 (-0.0715777 0.161051)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.42 using 59 PHA bins.
# Reduced chi-squared = 1.135 for 55 degrees of freedom
# Null hypothesis probability = 2.292816e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.047e-08 1.203e-08
25- 50 3.397e-08 1.774e-08
50-150 7.009e-08 4.290e-08
15-150 1.245e-07 5.712e-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: 1.74202 ( -0.0724203 0.0731255 )
Norm@50keV : 6.25821E-03 ( -0.00027474 0.000273893 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 92.05 using 59 PHA bins.
# Reduced chi-squared = 1.615 for 57 degrees of freedom
# Null hypothesis probability = 2.254798e-03
Photon flux (15-150 keV) in 99.83 sec: 0.843742 ( -0.0367813 0.0368478 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.76757e-06 ( -2.61321e-07 2.62262e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.387002 ( -0.445159 0.404246 )
Epeak [keV] : 56.3565 ( -4.32116 6.02523 )
Norm@50keV : 3.15649E-02 ( -0.011976 0.0220461 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.87 using 59 PHA bins.
# Reduced chi-squared = 0.9263 for 56 degrees of freedom
# Null hypothesis probability = 6.318452e-01
Photon flux (15-150 keV) in 99.83 sec: 0.786513 ( -0.03964 0.03976 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.20437e-06 ( -2.96176e-07 3.00748e-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) = 1.77e-06
S(50-100 keV) = 1.95e-06
T90 vs. Hardness ratio plot
T90 = 115.007999897003 sec.
Hardness ratio (energy fluence ratio) = 1.10169
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.45881
Count Ratio (50-100 keV) / (15-25 keV) = 0.748845
Mask shadow pattern
IMX = 1.653252734593688E-01, IMY = -6.202629123611765E-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:
-239.000000 5.868000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0959 40.9137 3.2 49.6 -27.7 2.0539 3.6 2.4 Cyg X-3
326.3993 38.3017 0.0 35.3 -26.3 0.4438 1.4 10.8 Cyg X-2
30.0973 15.8777 2.4 27.5 119.5 1.5027 4.8 ------ UNKNOWN
13.4795 36.2126 2.5 19.1 55.8 1.1385 4.6 ------ UNKNOWN
28.4048 -24.3842 2.7 51.7 173.5 3.1030 4.2 ------ UNKNOWN
327.0795 50.4806 2.7 40.6 -8.4 1.4210 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
5.868000 105.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0456 40.8425 6.7 49.6 -27.8 -0.5601 -1.7 7.2 Cyg X-3
326.1583 38.1848 6.6 35.4 -26.6 0.3478 1.7 8.2 Cyg X-2
33.2144 38.1113 0.4 32.7 75.1 9.7035 29.2 ------ UNKNOWN
345.2162 63.8784 2.1 45.0 15.1 1.6219 5.5 ------ UNKNOWN
18.5578 18.1042 2.4 16.2 119.7 0.8024 4.8 ------ UNKNOWN
15.6440 -26.9911 2.4 49.1 -171.5 1.6885 4.8 ------ UNKNOWN
6.6721 -16.1770 2.1 36.7 -163.1 1.0400 5.4 ------ UNKNOWN
295.2937 50.0896 2.0 59.5 -17.8 5.2771 5.8 ------ UNKNOWN
307.8753 32.8062 3.1 49.1 -38.4 1.6334 3.8 ------ UNKNOWN
310.7987 21.7621 2.3 47.2 -53.4 3.3137 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
158.300590 963.082300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
212.0899 86.0079 4.1 55.9 10.8 8.0669 2.8 ------ UNKNOWN
40.9445 61.4402 0.4 23.8 19.9 19.1308 30.3 ------ UNKNOWN
357.9866 67.6430 2.8 35.4 -11.5 2.9164 4.1 ------ UNKNOWN
309.9905 72.4478 2.8 51.9 -11.6 5.5958 4.1 ------ UNKNOWN
Plot creation:
Thu Mar 21 14:32:21 EDT 2019