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
52.9344 37.0784 0.0042 38.5153 -24.7701 2.7592286 45.547 TRIG_00987016
Foreground time interval of the image:
-0.132 9.973 (delta_t = 10.105 [sec])
Background time interval of the image:
-239.328 -0.132 (delta_t = 239.196 [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 0.512000
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 0.512000
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 0.512000
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 -0.132 sec. to 61.308 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20924 ( -0.0252933 0.0252002 )
Norm@50keV : 2.64435E-02 ( -0.00039428 0.00039364 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.25 using 59 bins.
Reduced chi-squared = 1.56579
# Null hypothesis probability of 4.06e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 61.44 sec: 3.10804 ( -0.05144 0.05155 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64423e-05 ( -2.30093e-07 2.30253e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.132 sec. to 61.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.748813 ( -0.114273 0.111717 )
Epeak [keV] : 173.320 ( -21.7893 34.3288 )
Norm@50keV : 4.01955E-02 ( -0.00379233 0.00426817 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.81 using 59 bins.
Reduced chi-squared = 0.657321
# Null hypothesis probability of 9.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 61.44 sec: 3.01090 ( -0.055 0.05528 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62578e-05 ( -2.35965e-07 2.35677e-07 ) ergs/cm2
Band function
Time interval is from -0.132 sec. to 61.308 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] : 22.2999 ( )
R^2/D10^2 : 0.100405 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 693.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.91e-110 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.642e-07 1.705e-08
25- 50 3.007e-06 6.636e-08
50-150 1.118e-05 2.028e-07
15-150 1.475e-05 2.181e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 13.8342 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 732.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.38e-118 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.116e-06 3.318e-08
25- 50 4.071e-06 6.390e-08
50-150 8.929e-06 1.444e-07
15-150 1.512e-05 2.396e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.56873 (-0.689541 0.729781)
R1^2/D10^2 : 0.843128 (-0.160632 0.212776)
kT2 [keV] : 33.5990 (-1.89278 2.32848)
R2^2/D10^2 : 2.12330E-02 (-0.004476 0.00492153)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.98e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.164e-06 6.881e-08
25- 50 3.597e-06 1.017e-07
50-150 1.146e-05 3.072e-07
15-150 1.622e-05 3.901e-07
Peak spectrum fit
Power-law model
Time interval is from 22.244 sec. to 23.244 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.755694 ( -0.0508801 0.0503831 )
Norm@50keV : 0.122785 ( -0.00375056 0.00373701 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.50 using 59 bins.
Reduced chi-squared = 0.868421
# Null hypothesis probability of 7.49e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.409140 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46241e-06 ( -4.45609e-08 4.46134e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 22.244 sec. to 23.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.469360 ( -0.212216 0.202146 )
Epeak [keV] : 339.457 ( -116.109 595.312 )
Norm@50keV : 0.160214 ( -0.0268736 0.0336098 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.56 using 59 bins.
Reduced chi-squared = 0.777857
# Null hypothesis probability of 8.87e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 14.0274 ( -0.4247 0.4251 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4566e-06 ( -4.53304e-08 4.52619e-08 ) ergs/cm2
Band function
Time interval is from 22.244 sec. to 23.244 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] : 27.4435 ( )
R^2/D10^2 : 0.281226 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 177.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.57e-14 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.494e-08 2.110e-09
25- 50 2.074e-07 9.850e-09
50-150 1.136e-06 4.400e-08
15-150 1.379e-06 4.500e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 54.6587 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 693.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.17e-110 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.361e-07 4.100e-09
25- 50 2.618e-07 8.600e-09
50-150 5.742e-07 1.765e-08
15-150 9.721e-07 3.130e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.95133 (-1.60926 1.90115)
R1^2/D10^2 : 2.55550 (-0.919616 1.64383)
kT2 [keV] : 41.6129 (-4.81424 7.82363)
R2^2/D10^2 : 7.33915E-02 (-0.0290911 0.0334615)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.76e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.739e-08 9.780e-09
25- 50 2.370e-07 2.230e-08
50-150 1.168e-06 9.820e-08
15-150 1.472e-06 1.265e-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: 0.953539 ( -0.0637794 0.0629758 )
Norm@50keV : 1.81496E-02 ( -0.000682986 0.000680547 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.94e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.1 sec: 2.08543 ( -0.0797105 0.0798819 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01588e-06 ( -7.52451e-08 7.53158e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.542411 ( -0.283597 0.265991 )
Epeak [keV] : 216.372 ( -63.469 264.303 )
Norm@50keV : 2.69666E-02 ( -0.00596629 0.00814967 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.1 sec: 2.05050 ( -0.08243 0.08261 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.99311e-06 ( -7.81538e-08 7.78407e-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) = 3.47e-06
S(50-100 keV) = 6.01e-06
T90 vs. Hardness ratio plot
T90 = 38.6879999637604 sec.
Hardness ratio (energy fluence ratio) = 1.73199
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.81396
Count Ratio (50-100 keV) / (15-25 keV) = 1.82937
Mask shadow pattern
IMX = 7.226485954659663E-01, IMY = 3.334527808191839E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.328000 -0.132000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0359 40.9904 4.9 40.4 127.0 1.5567 2.4 4.1 Cyg X-3
326.1272 38.3523 3.3 35.1 105.5 1.7409 3.4 2.8 Cyg X-2
33.4307 11.5096 3.6 55.9 10.9 3.5168 3.2 ------ UNKNOWN
262.2670 50.7917 2.5 51.0 171.1 3.4325 4.7 ------ UNKNOWN
62.7175 37.2966 3.3 42.4 -35.2 1.3741 3.5 ------ UNKNOWN
78.2807 45.8289 2.8 42.2 -56.7 2.4730 4.1 ------ UNKNOWN
197.9542 61.5333 2.2 54.0 -143.5 7.1009 5.3 ------ UNKNOWN
173.1012 67.0405 3.4 48.4 -129.8 3.7034 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.132000 9.972590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0996 41.0121 2.9 40.3 127.0 0.4855 3.9 3.6 Cyg X-3
326.2923 38.4481 18.1 34.9 105.3 0.0553 0.6 9.5 Cyg X-2
284.2317 45.5726 3.1 46.9 151.3 0.4524 3.7 ------ UNKNOWN
52.9344 37.0784 0.3 38.5 -24.8 2.7592 45.5 ------ UNKNOWN
65.6971 40.8750 2.2 40.7 -41.1 0.4281 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
66.772600 962.828800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6244 22.0067 0.3 30.5 -58.9 36.1131 36.9 0.7 Crab
19.4800 8.5632 3.7 41.6 65.3 9.4175 3.1 ------ UNKNOWN
36.8697 -12.9876 3.3 52.3 30.0 15.3503 3.5 ------ UNKNOWN
52.3799 -18.8074 3.0 55.9 10.7 16.5616 3.9 ------ UNKNOWN
Plot creation:
Mon Nov 16 12:38:49 EST 2020