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
21.5128 63.0640 0.0178 22.2992 -167.6158 0.6665924 10.784 TRIG_00992099
Foreground time interval of the image:
-0.712 25.533 (delta_t = 26.245 [sec])
Background time interval of the image:
-239.368 -0.712 (delta_t = 238.656 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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 -0.712 sec. to 30.328 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05410 ( -0.279909 0.308037 )
Norm@50keV : 1.15468E-03 ( -0.000243188 0.000235258 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.38 using 59 bins.
Reduced chi-squared = 0.954035
# Null hypothesis probability of 5.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 31.04 sec: 0.177668 ( -0.026269 0.026271 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.31743e-07 ( -6.23653e-08 6.49382e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.712 sec. to 30.328 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72796 ( -1.32712 0.388281 )
Epeak [keV] : 32.6571 ( -30.893 -32.6571 )
Norm@50keV : 1.82089E-03 ( -0.000974299 0.0105457 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.09 using 59 bins.
Reduced chi-squared = 0.965893
# Null hypothesis probability of 5.48e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 31.04 sec: 0.175761 ( -0.026837 0.026891 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.18495e-07 ( -7.1555e-08 6.99697e-08 ) ergs/cm2
Band function
Time interval is from -0.712 sec. to 30.328 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] : 8.23197 (-1.42772 1.80875)
R^2/D10^2 : 0.172750 (-0.0927145 0.192684)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.54e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.706e-08 1.858e-08
25- 50 1.233e-07 3.099e-08
50-150 3.553e-08 1.644e-08
15-150 2.259e-07 5.466e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 57.4936 (-21.3461 43.5342)
Norm : 0.950136 (-0.218632 0.300287)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.359e-08 1.471e-08
25- 50 1.105e-07 2.036e-08
50-150 1.213e-07 5.373e-08
15-150 3.054e-07 7.063e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.74645 (-1.51524 1.69778)
R1^2/D10^2 : 0.560888 (-0.348918 1.26564)
kT2 [keV] : 22.5125 (-8.68603 25.284)
R2^2/D10^2 : 2.44530E-03 (-0.00226228 0.0142226)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.86e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.865e-08 4.426e-08
25- 50 1.027e-07 4.793e-08
50-150 1.479e-07 8.739e-08
15-150 3.292e-07 1.662e-07
Peak spectrum fit
Power-law model
Time interval is from 0.292 sec. to 1.292 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07005 ( -0.415157 0.393538 )
Norm@50keV : 5.35172E-03 ( -0.00124593 0.00124176 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.82 using 59 bins.
Reduced chi-squared = 1.06702
# Null hypothesis probability of 3.40e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.619089 ( -0.147095 0.14792 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.65067e-08 ( -1.41444e-08 1.43319e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.292 sec. to 1.292 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.388637 ( -2.09991 2.08468 )
Epeak [keV] : 133.399 ( -133.393 -133.393 )
Norm@50keV : 1.08718E-02 ( -0.00656608 0.064855 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.23 using 59 bins.
Reduced chi-squared = 1.07554
# Null hypothesis probability of 3.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.601722 ( -0.152666 0.15281 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.45519e-08 ( -1.49743e-08 1.50707e-08 ) ergs/cm2
Band function
Time interval is from 0.292 sec. to 1.292 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] : 21.6018 (-5.54143 8.2558)
R^2/D10^2 : 2.33259E-02 (-0.014877 0.0371598)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.031e-09 1.029e-09
25- 50 1.062e-08 4.865e-09
50-150 3.701e-08 2.047e-08
15-150 4.967e-08 2.675e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-76.5166 -200)
Norm : 2.54341 (-0.609464 0.609464)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.31e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.333e-09 3.800e-09
25- 50 1.218e-08 7.160e-09
50-150 2.672e-08 1.576e-08
15-150 4.523e-08 2.719e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.85838 (-7.09369 21.5448)
R1^2/D10^2 : 0.434319 (-0.416989 83.8209)
kT2 [keV] : 28.1504 (-26.7151 -28.3164)
R2^2/D10^2 : 8.85324E-03 (-0.00437987 0.0164075)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.22e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.352e-09 2.625e-09
25- 50 1.107e-08 6.085e-09
50-150 3.983e-08 2.419e-08
15-150 5.525e-08 3.060e-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: 1.97885 ( -0.277774 0.303617 )
Norm@50keV : 1.31306E-03 ( -0.000263944 0.000254207 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.27e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.24 sec: 0.195068 ( -0.0286939 0.028694 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.17415e-07 ( -5.87865e-08 6.09802e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.78024 ( -1.2274 0.383449 )
Epeak [keV] : 45.5732 ( -45.2549 -45.5732 )
Norm@50keV : 1.71790E-03 ( -0.0017179 0.00747318 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.94e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.24 sec: 0.193675 ( -0.029134 0.029431 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10322e-07 ( -6.71508e-08 3.51537e-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) = 1.02e-07
S(50-100 keV) = 9.78e-08
T90 vs. Hardness ratio plot
T90 = 26.9439998865128 sec.
Hardness ratio (energy fluence ratio) = 0.958824
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.974237
Count Ratio (50-100 keV) / (15-25 keV) = 0.520128
Mask shadow pattern
IMX = -4.005701245528479E-01, IMY = 8.795511655533213E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.368000 -0.712000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6145 22.0082 0.7 44.7 -49.1 9.9860 15.5 1.1 Crab
356.1080 18.7787 2.3 40.8 96.4 4.9701 5.1 ------ UNKNOWN
18.6218 6.7705 2.4 38.6 57.0 2.6128 4.7 ------ UNKNOWN
51.0199 -5.5505 3.3 49.9 9.1 2.1389 3.4 ------ UNKNOWN
23.5766 37.6858 2.1 10.3 96.5 1.3160 5.6 ------ UNKNOWN
13.0712 53.5854 2.7 18.7 164.0 0.9869 4.3 ------ UNKNOWN
78.4117 36.4747 2.7 33.2 -65.1 1.8446 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.712000 25.532600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6777 22.0665 16.2 44.7 -49.2 -0.1161 -0.7 4.0 Crab
21.5127 63.0640 1.1 22.3 -167.6 0.6666 10.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
68.932590 604.232600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0043 40.9533 14.8 47.0 137.9 1.6911 0.8 4.8 Cyg X-3
326.1592 38.3409 30.1 40.9 119.3 -0.6639 -0.4 1.3 Cyg X-2
286.8774 43.8813 3.5 53.7 156.6 8.6149 3.3 ------ UNKNOWN
33.4038 26.2964 2.7 37.6 21.8 3.1686 4.2 ------ UNKNOWN
266.9617 48.8197 2.2 56.8 173.9 13.3591 5.3 ------ UNKNOWN
223.6385 67.7275 3.0 48.3 -151.5 4.1470 3.8 ------ UNKNOWN
84.9630 32.5345 2.7 49.5 -43.5 7.3317 4.2 ------ UNKNOWN
Plot creation:
Sun Nov 15 21:51:37 EST 2020