Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
85.7836 +25.2357 0.0065 36.8 86.5 27.0590 29.5 TRIG_01006906
------------------------------------------
Foreground time interval of the image:
-18.799 69.701 (delta_t = 88.500 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
-122.908000 209.820000
211.000000 294.172000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.49604 ( )
Norm@50keV : 1.09442E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 531.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.16e-78 with 57 degrees of freedom
Photon flux (15-150 keV) in 415.9 sec: 4.41228 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.14495e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-122.908000 209.820000
211.000000 294.172000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.373403 ( -0.313013 0.299835 )
Epeak [keV] : 20.6521 ( -2.05766 1.78054 )
Norm@50keV : 0.660221 ( -0.212805 0.331342 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.73e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 415.9 sec: 3.33782 ( -0.13298 0.13527 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.80002e-05 ( -1.76508e-06 1.78587e-06 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-122.908000 209.820000
211.000000 294.172000
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.69201 ( )
beta : -8.53835 ( )
Epeak [keV] : 6.95840 ( )
Norm@50keV : 0.113516 ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 415.9 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] : 7.23905 ( )
R^2/D10^2 : 5.09027 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 148.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.97e-10 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.843e-05 6.738e-07
25- 50 2.691e-05 5.240e-07
50-150 5.028e-06 2.163e-07
15-150 5.037e-05 1.144e-06
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.0127 (-0.46112 0.478072)
Norm : 48.7430 (-2.45322 2.57653)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.51e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.008e-05 9.919e-07
25- 50 2.531e-05 5.095e-07
50-150 6.954e-06 2.807e-07
15-150 6.235e-05 1.352e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.72745 (-0.555192 0.57711)
R1^2/D10^2 : 21.3869 (-7.10926 13.7861)
kT2 [keV] : 8.85189 (-0.513172 0.760294)
R2^2/D10^2 : 1.25242 (-0.579035 0.661082)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.94e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.507e-05 2.805e-06
25- 50 2.606e-05 2.107e-06
50-150 6.212e-06 7.050e-07
15-150 5.734e-05 5.469e-06
Peak spectrum fit
Power-law model
Time interval is from 227.124 sec. to 228.124 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.88550 ( )
Norm@50keV : 2.97979E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 120.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.69e-06 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 7.54991 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40439e-07 ( 0 0 ) ergs/cm2
Cutoff power-law model
Time interval is from 227.124 sec. to 228.124 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.236386 ( -0.791857 0.706238 )
Epeak [keV] : 25.7085 ( -3.0795 2.27551 )
Norm@50keV : 2.57747 ( -1.64199 5.52794 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.81e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.82106 ( -0.40705 0.40923 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.00671e-07 ( -1.6377e-08 1.6595e-08 ) ergs/cm2
Band function
Time interval is from 227.124 sec. to 228.124 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.287733 ( -0.715983 0.901402 )
beta : -6.49474 ( 6.50099 2.19998 )
Epeak [keV] : 25.7996 ( -3.11149 2.20634 )
Norm@50keV : 2.78964 ( -1.4999 7.6471 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 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] : 7.31138 (-0.306273 0.315383)
R^2/D10^2 : 11.4356 (-2.00568 2.45836)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.025e-07 7.605e-09
25- 50 1.525e-07 7.850e-09
50-150 2.951e-08 4.725e-09
15-150 2.845e-07 1.400e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 24.4098 (-1.92756 2.12934)
Norm : 73.0072 (-7.52969 8.44227)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.316e-07 8.650e-09
25- 50 1.328e-07 6.850e-09
50-150 5.453e-08 8.830e-09
15-150 3.190e-07 1.625e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.73274 (-1.74677 7.42377)
R1^2/D10^2 : 66.5088 (-51.2831 2165.35)
kT2 [keV] : 8.14190 (-0.713842 3.00501)
R2^2/D10^2 : 6.08508 (-5.49776 4.15945)
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.167e-07 5.064e-08
25- 50 1.459e-07 4.714e-08
50-150 3.717e-08 1.289e-08
15-150 2.998e-07 9.235e-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: 3.06979 ( )
Norm@50keV : 1.13963E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 207.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.98e-19 with 57 degrees of freedom
Photon flux (15-150 keV) in 88.5 sec: 3.29884 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25236e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.121765 ( -0.565447 0.520713 )
Epeak [keV] : 22.5947 ( -2.82091 2.16744 )
Norm@50keV : 0.749625 ( -0.392543 0.937387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 88.5 sec: 2.82150 ( -0.13647 0.13791 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.06104e-05 ( -4.34447e-07 4.39934e-07 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.50093 ( )
beta : -9.06137 ( )
Epeak [keV] : 14.8195 ( )
Norm@50keV : 7.25368E-02 ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 88.5 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) = 2.22e-05
S(50-100 keV) = 7.87e-06
T90 vs. Hardness ratio plot
T90 = 358.479999899864 sec.
Hardness ratio (energy fluence ratio) = 0.354505
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.796077
Count Ratio (50-100 keV) / (15-25 keV) = 0.113804
Mask shadow pattern
IMX = 4.508308154667406E-02, IMY = -7.466551194411509E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-18.799400 69.700590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7274 21.8868 5.6 38.8 81.2 -2.7651 -2.1 9.3 Crab
85.7836 25.2357 0.4 36.8 86.5 27.0599 29.5 ------ UNKNOWN
132.2267 72.7912 2.5 53.5 162.7 5.4062 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
128.700590 209.820000
211.000000 303.054400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4792 21.9397 5.4 3.9 38.3 -1.3616 -2.1 9.7 Crab
47.5159 25.0229 2.5 34.5 103.0 6.0104 4.7 ------ UNKNOWN
46.2186 40.6813 2.4 36.2 130.1 6.2153 4.9 ------ UNKNOWN
84.7084 20.9057 1.1 4.4 18.2 6.6593 10.6 ------ UNKNOWN
85.7555 25.2391 0.1 0.0 116.2 62.5018 104.5 ------ UNKNOWN
113.9382 15.0451 2.2 28.2 -69.4 4.4746 5.3 ------ UNKNOWN
111.9043 -7.3551 2.7 41.3 -36.4 4.7198 4.3 ------ UNKNOWN
123.5930 53.2395 2.4 39.7 -140.0 4.8462 4.8 ------ UNKNOWN
115.9002 -11.3951 2.8 46.9 -37.4 6.0522 4.1 ------ UNKNOWN
137.0798 42.3244 2.7 45.1 -120.6 11.4936 4.4 ------ UNKNOWN
Plot creation:
Tue Nov 17 19:24:06 EST 2020