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
196.0117 29.6377 0.0049 33.9022 161.3656 3.9504168 39.518 TRIG_00982707
Foreground time interval of the image:
-0.420 17.381 (delta_t = 17.801 [sec])
Background time interval of the image:
-239.720 -0.420 (delta_t = 239.300 [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 0.256000
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 0.256000
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 0.256000
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 -0.420 sec. to 112.632 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62401 ( -0.0861124 0.0866432 )
Norm@50keV : 3.34883E-03 ( -0.000159514 0.000158961 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.11 using 59 bins.
Reduced chi-squared = 0.598421
# Null hypothesis probability of 9.93e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 113.1 sec: 0.433617 ( -0.020792 0.020851 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.53275e-06 ( -1.79676e-07 1.80661e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.420 sec. to 112.632 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57159 ( -0.329995 0.131591 )
Epeak [keV] : 374.703 ( -420.529 -420.529 )
Norm@50keV : 3.55972E-03 ( -0.00035084 0.00160576 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.07 using 59 bins.
Reduced chi-squared = 0.608393
# Null hypothesis probability of 9.91e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 113.1 sec: 0.432321 ( -0.022138 0.0167 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.51716e-06 ( -2.04077e-07 1.924e-07 ) ergs/cm2
Band function
Time interval is from -0.420 sec. to 112.632 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] : 13.8693 ( )
R^2/D10^2 : 6.07782E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 158.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.97e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.795e-07 2.550e-08
25- 50 1.030e-06 6.057e-08
50-150 1.298e-06 1.250e-07
15-150 2.608e-06 1.566e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 172.511 (-38.242 -172.386)
Norm : 1.75619 (-0.0913656 0.100843)
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.85e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.033e-07 3.540e-08
25- 50 9.510e-07 1.042e-07
50-150 1.983e-06 6.046e-07
15-150 3.437e-06 7.272e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.16117 (-0.969486 1.03942)
R1^2/D10^2 : 0.465912 (-0.171359 0.311957)
kT2 [keV] : 28.8052 (-4.75933 7.55355)
R2^2/D10^2 : 3.57998E-03 (-0.00192468 0.0032455)
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.85e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.981e-07 7.137e-08
25- 50 9.622e-07 9.642e-08
50-150 2.057e-06 4.411e-07
15-150 3.518e-06 5.084e-07
Peak spectrum fit
Power-law model
Time interval is from -0.180 sec. to 0.820 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.976735 ( -0.0749161 0.0741708 )
Norm@50keV : 9.34696E-02 ( -0.00401031 0.00400198 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.52 using 59 bins.
Reduced chi-squared = 1.00912
# Null hypothesis probability of 4.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.480692 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01932e-06 ( -4.76026e-08 4.77183e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.180 sec. to 0.820 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.816047 ( -0.291802 0.215316 )
Epeak [keV] : 428.292 ( -428.292 -428.292 )
Norm@50keV : 0.110176 ( -0.0193031 0.0368469 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.54 using 59 bins.
Reduced chi-squared = 1.00964
# Null hypothesis probability of 4.55e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 10.6894 ( -0.4778 0.4779 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01284e-06 ( -4.93438e-08 4.9149e-08 ) ergs/cm2
Band function
Time interval is from -0.180 sec. to 0.820 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] : 22.7549 ( )
R^2/D10^2 : 0.349369 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 153.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.48e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.295e-08 2.975e-09
25- 50 1.777e-07 1.150e-08
50-150 6.875e-07 4.615e-08
15-150 8.982e-07 4.925e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 43.1032 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 214.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.05e-20 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.073e-07 5.300e-09
25- 50 2.065e-07 9.650e-09
50-150 4.528e-07 2.450e-08
15-150 7.666e-07 3.940e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.46885 (-1.401 1.6935)
R1^2/D10^2 : 4.14902 (-1.70135 3.14895)
kT2 [keV] : 36.9354 (-5.22642 8.7485)
R2^2/D10^2 : 6.83028E-02 (-0.0319775 0.041987)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.867e-08 1.214e-08
25- 50 1.925e-07 2.760e-08
50-150 7.646e-07 1.281e-07
15-150 1.026e-06 1.450e-07
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: 1.28317 ( -0.0691434 0.0687631 )
Norm@50keV : 1.48640E-02 ( -0.000564161 0.000564108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.30e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.8 sec: 1.76793 ( -0.071177 0.0713027 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.62541e-06 ( -1.07765e-07 1.08018e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16343 ( -0.268058 0.15905 )
Epeak [keV] : 380.923 ( -381.831 -381.831 )
Norm@50keV : 1.69113E-02 ( -0.00246679 0.00546777 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.17e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.8 sec: 1.75672 ( -0.07478 0.07473 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.60693e-06 ( -1.16465e-07 1.1513e-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) = 9.25e-07
S(50-100 keV) = 1.20e-06
T90 vs. Hardness ratio plot
T90 = 86.5719999074936 sec.
Hardness ratio (energy fluence ratio) = 1.2973
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31537
Count Ratio (50-100 keV) / (15-25 keV) = 0.907145
Mask shadow pattern
IMX = -6.367983277053566E-01, IMY = -2.147321580813681E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.720000 -0.420000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
291.4881 62.0342 3.0 46.5 46.0 4.0323 3.9 ------ UNKNOWN
323.4578 72.1868 3.1 44.2 24.1 1.8650 3.8 ------ UNKNOWN
123.0469 45.3536 2.4 35.3 -81.6 3.0183 4.8 ------ UNKNOWN
62.3918 53.7926 2.8 54.2 -31.4 6.0072 4.2 ------ UNKNOWN
144.1225 22.2499 2.2 45.7 -123.8 6.1336 5.3 ------ UNKNOWN
102.9108 46.9453 2.9 43.6 -63.8 4.6314 3.9 ------ UNKNOWN
99.0528 47.6366 2.5 44.9 -60.3 6.0301 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.420000 17.380600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
304.2602 61.6525 2.5 50.2 39.6 1.5856 4.6 ------ UNKNOWN
196.0117 29.6377 0.3 33.9 161.4 3.9505 39.5 ------ UNKNOWN
189.8459 30.5745 2.7 31.8 170.6 0.3608 4.2 ------ UNKNOWN
12.7054 62.7089 2.7 55.3 1.6 1.2121 4.3 ------ UNKNOWN
140.1057 43.6767 2.7 28.6 -101.2 0.4691 4.3 ------ UNKNOWN
94.2878 48.7931 2.4 46.1 -55.9 1.4045 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
71.980590 962.413500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
238.8816 27.6339 3.0 37.5 68.5 6.2237 3.9 ------ UNKNOWN
160.6311 69.5664 3.3 44.7 -30.4 4.9619 3.5 ------ UNKNOWN
163.1568 1.3278 3.1 42.2 -139.8 5.5827 3.7 ------ UNKNOWN
161.2461 24.3754 3.9 31.3 -105.0 5.0908 4.2 ------ UNKNOWN
160.9311 24.4137 4.0 31.6 -104.7 5.7013 4.7 ------ UNKNOWN
153.3352 9.0991 3.5 44.8 -122.0 10.5208 3.3 ------ UNKNOWN
152.0554 13.1332 2.4 43.8 -116.2 17.0777 4.7 ------ UNKNOWN
153.7654 3.0919 2.9 48.0 -129.1 16.0100 4.0 ------ UNKNOWN
142.3368 50.5503 3.5 44.8 -60.3 12.4663 3.3 ------ UNKNOWN
Plot creation:
Mon Nov 16 12:40:51 EST 2020