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
85.8428 +25.4977 0.0317 0.3 -159.1 0.6735 6.1 TRIG_01006917
------------------------------------------
Foreground time interval of the image:
-7.816 15.177 (delta_t = 22.993 [sec])
Background time interval of the image:
-29.824 -7.816 (delta_t = 22.008 [sec])
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
-7.816000 36.926000
38.176000 562.476000
563.176000 705.656000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.60852 ( )
Norm@50keV : 9.26565E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 941.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.93e-160 with 57 degrees of freedom
Photon flux (15-150 keV) in 711.5 sec: 4.09593 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0.000111037 ( 0 0 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-7.816000 36.926000
38.176000 562.476000
563.176000 705.656000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.419396 ( -0.234655 0.226714 )
Epeak [keV] : 20.9453 ( -1.68062 1.5175 )
Norm@50keV : 0.522186 ( -0.127103 0.174613 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 711.5 sec: 2.97520 ( -0.10759 0.10925 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.93032e-05 ( -2.44329e-06 2.46962e-06 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-7.816000 36.926000
38.176000 562.476000
563.176000 705.656000
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.419514 ( -0.212718 0.250268 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 20.9372 ( -1.67126 1.52408 )
Norm@50keV : 0.522378 ( -0.126625 0.175917 )
------------------------------------------------------------
Photon flux (15-150 keV) in 711.5 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] : 7.62404 ( )
R^2/D10^2 : 3.52921 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 229.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.64e-22 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.541e-05 8.076e-07
25- 50 4.083e-05 7.435e-07
50-150 9.127e-06 2.490e-07
15-150 7.536e-05 1.459e-06
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.1657 (-0.342167 0.351897)
Norm : 43.6365 (-1.80616 1.87334)
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.59e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.640e-05 1.380e-06
25- 50 3.930e-05 7.151e-07
50-150 1.095e-05 3.237e-07
15-150 9.665e-05 1.957e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.92091 (-0.405233 0.416004)
R1^2/D10^2 : 16.7074 (-4.41026 7.00985)
kT2 [keV] : 9.25491 (-0.386541 0.499686)
R2^2/D10^2 : 0.872423 (-0.28886 0.328168)
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.761e-05 3.369e-06
25- 50 4.031e-05 2.199e-06
50-150 1.031e-05 7.435e-07
15-150 8.823e-05 5.194e-06
Peak spectrum fit
Power-law model
Time interval is from 585.816 sec. to 586.816 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.73874 ( -0.103582 0.107137 )
Norm@50keV : 2.37384E-02 ( -0.00188706 0.00188389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 107.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.78e-05 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.43666 ( -0.301313 0.301628 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.56055e-07 ( -1.47102e-08 1.47809e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 585.816 sec. to 586.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.149240 ( -0.868982 0.751522 )
Epeak [keV] : 25.9028 ( -3.23857 2.30971 )
Norm@50keV : 1.61779 ( -1.61795 4.3199 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.03e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.07241 ( -0.30907 0.30991 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.25375e-07 ( -1.3681e-08 1.3959e-08 ) ergs/cm2
Band function
Time interval is from 585.816 sec. to 586.816 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.146360 ( -0.707543 3.08769 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 25.8915 ( -3.23118 2.31704 )
Norm@50keV : 1.61101 ( -1.61101 4.33766 )
------------------------------------------------------------
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] : 7.24866 (-0.343385 0.357298)
R^2/D10^2 : 8.89184 (-1.72246 2.14731)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.97e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.771e-08 6.030e-09
25- 50 1.138e-07 6.950e-09
50-150 2.136e-08 3.570e-09
15-150 2.128e-07 1.260e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 26.3052 (-2.43506 2.74922)
Norm : 49.5906 (-5.47547 6.19101)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.42e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.377e-08 6.650e-09
25- 50 9.924e-08 5.715e-09
50-150 4.542e-08 7.400e-09
15-150 2.384e-07 1.400e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.79159 (-1.4037 0.97617)
R1^2/D10^2 : 16.5095 (-5.54883 15.8715)
kT2 [keV] : 11.1181 (-6.97059 6.24338)
R2^2/D10^2 : 0.579421 (-0.461937 2.97536)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.481e-08 2.828e-08
25- 50 1.074e-07 4.415e-08
50-150 3.535e-08 1.902e-08
15-150 2.275e-07 8.594e-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: 3.21668 ( )
Norm@50keV : 9.44913E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 172.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.75e-13 with 57 degrees of freedom
Photon flux (15-150 keV) in 22.99 sec: 3.05556 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.90623e-06 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.233883 ( -0.580525 0.533823 )
Epeak [keV] : 20.1788 ( -3.0692 2.33091 )
Norm@50keV : 0.716173 ( -0.38652 0.954607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 31.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 22.99 sec: 2.60778 ( -0.12611 0.12724 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4531e-06 ( -9.97306e-08 1.00788e-07 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.233691 ( -0.467467 0.768589 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 20.1738 ( -2.84075 2.33082 )
Norm@50keV : 0.716624 ( -0.386836 0.957215 )
------------------------------------------------------------
Photon flux (15-150 keV) in 22.99 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) = 3.36e-05
S(50-100 keV) = 1.10e-05
T90 vs. Hardness ratio plot
T90 = 575.807999968529 sec.
Hardness ratio (energy fluence ratio) = 0.327381
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.779602
Count Ratio (50-100 keV) / (15-25 keV) = 0.110965
Mask shadow pattern
IMX = -4.729703601730605E-03, IMY = 1.802965413192347E-03
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:
-29.824000 -7.816000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5541 21.9216 3.5 3.9 36.9 -0.3753 -3.3 7.1 Crab
45.1337 44.0151 2.3 37.8 135.2 1.3026 5.0 ------ UNKNOWN
57.5135 18.1418 2.7 27.1 85.5 0.6937 4.3 ------ UNKNOWN
84.8719 21.1833 2.1 4.1 16.5 0.6147 5.4 ------ UNKNOWN
85.8659 25.5622 0.2 0.4 -158.8 6.2495 52.3 ------ UNKNOWN
94.4039 71.0128 2.8 46.1 -171.1 0.9842 4.1 ------ UNKNOWN
140.8677 52.1240 2.5 49.2 -133.3 2.4712 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-7.816000 15.176600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7295 21.8812 3.5 3.8 34.5 0.3771 3.3 9.6 Crab
80.6562 1.5462 1.9 24.2 17.5 0.7701 6.2 ------ UNKNOWN
84.0164 7.7556 2.4 17.5 10.7 0.5473 4.9 ------ UNKNOWN
85.8428 25.4977 1.9 0.3 -159.1 0.6738 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
22.876600 36.926000
38.176000 562.476000
563.176000 962.198600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4934 22.1508 4.7 4.0 37.8 -6.4930 -2.5 11.3 Crab
47.5312 25.0065 2.5 34.5 103.0 23.1448 4.5 ------ UNKNOWN
45.9824 40.6319 2.2 36.2 130.1 26.4400 5.2 ------ UNKNOWN
84.8212 21.2348 1.3 4.5 17.7 22.9621 8.8 ------ UNKNOWN
85.8588 25.5731 0.1 0.0 -55.3 247.6662 103.4 ------ UNKNOWN
144.0113 67.7979 2.3 54.6 -151.3 53.1744 5.1 ------ UNKNOWN
Plot creation:
Wed Nov 18 05:14:26 EST 2020