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
356.9044 19.6523 0.0039 30.7910 -13.2289 5.0352379 50.086 TRIG_00725036
Foreground time interval of the image:
-24.851 11.149 (delta_t = 36.000 [sec])
Background time interval of the image:
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 -63.412 sec. to 65.792 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57103 ( -0.0538573 0.0540108 )
Norm@50keV : 7.15327E-03 ( -0.000201658 0.000201523 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.99 using 59 PHA bins.
# Reduced chi-squared = 0.9297 for 57 degrees of freedom
# Null hypothesis probability = 6.261940e-01
Photon flux (15-150 keV) in 129.2 sec: 0.911200 ( -0.027524 0.027599 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.67646e-06 ( -2.61108e-07 2.61785e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -63.412 sec. to 65.792 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32242 ( -0.222112 0.211058 )
Epeak [keV] : 142.578 ( -43.7112 413.978 )
Norm@50keV : 9.39952E-03 ( -0.00189864 0.00252775 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.92 using 59 PHA bins.
# Reduced chi-squared = 0.8735 for 56 degrees of freedom
# Null hypothesis probability = 7.376292e-01
Photon flux (15-150 keV) in 129.2 sec: 0.894393 ( -0.030699 0.03079 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.50007e-06 ( -3.01792e-07 3.00334e-07 ) ergs/cm2
Band function
Time interval is from -63.412 sec. to 65.792 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] : 15.1594 ( )
R^2/D10^2 : 9.39076E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 294.48 using 59 PHA bins.
# Reduced chi-squared = 5.1662 for 57 degrees of freedom
# Null hypothesis probability = 1.014713e-33
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.827e-07 3.249e-08
25- 50 2.338e-06 8.850e-08
50-150 3.674e-06 2.119e-07
15-150 6.594e-06 2.183e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-27.6305 -200)
Norm : 3.66637 (-0.102203 0.102203)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.99 using 59 PHA bins.
# Reduced chi-squared = 0.8594 for 57 degrees of freedom
# Null hypothesis probability = 7.659716e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.181e-06 3.534e-08
25- 50 2.272e-06 7.558e-08
50-150 4.980e-06 1.550e-07
15-150 8.433e-06 2.435e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.83998 (-0.769916 0.801876)
R1^2/D10^2 : 0.651179 (-0.175564 0.268388)
kT2 [keV] : 28.8384 (-3.31673 4.54527)
R2^2/D10^2 : 7.53609E-03 (-0.00300366 0.00423452)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.79 using 59 PHA bins.
# Reduced chi-squared = 0.9053 for 55 degrees of freedom
# Null hypothesis probability = 6.733399e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.051e-06 9.341e-08
25- 50 2.343e-06 1.499e-07
50-150 5.073e-06 5.420e-07
15-150 8.467e-06 6.764e-07
Peak spectrum fit
Power-law model
Time interval is from 2.092 sec. to 3.092 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18837 ( -0.0786508 0.0784471 )
Norm@50keV : 4.98614E-02 ( -0.00229695 0.00229695 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.01 using 59 PHA bins.
# Reduced chi-squared = 0.8773 for 57 degrees of freedom
# Null hypothesis probability = 7.326547e-01
Photon flux (15-150 keV) in 1 sec: 5.84334 ( -0.27645 0.27668 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.07598e-07 ( -2.59165e-08 2.60071e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.092 sec. to 3.092 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.562212 ( -0.362369 0.334206 )
Epeak [keV] : 126.951 ( -27.5593 79.1503 )
Norm@50keV : 9.71171E-02 ( -0.0284202 0.0439106 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.10 using 59 PHA bins.
# Reduced chi-squared = 0.6982 for 56 degrees of freedom
# Null hypothesis probability = 9.580796e-01
Photon flux (15-150 keV) in 1 sec: 5.69569 ( -0.28731 0.28717 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14594e-07 ( -1.68478e-08 2.82658e-08 ) ergs/cm2
Band function
Time interval is from 2.092 sec. to 3.092 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] : 19.0924 (-1.08173 1.16408)
R^2/D10^2 : 0.321021 (-0.0567772 0.0679965)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 94.77 using 59 PHA bins.
# Reduced chi-squared = 1.663 for 57 degrees of freedom
# Null hypothesis probability = 1.245959e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.296e-08 2.170e-09
25- 50 1.108e-07 7.050e-09
50-150 2.971e-07 2.325e-08
15-150 4.309e-07 2.520e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-6.95021 -200)
Norm : 24.1169 (-1.13439 1.13439)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 101.62 using 59 PHA bins.
# Reduced chi-squared = 1.7827 for 57 degrees of freedom
# Null hypothesis probability = 2.563669e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.004e-08 2.995e-09
25- 50 1.155e-07 6.250e-09
50-150 2.533e-07 1.340e-08
15-150 4.288e-07 2.785e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.42210 (-1.96163 2.60739)
R1^2/D10^2 : 3.20561 (-1.81627 5.75607)
kT2 [keV] : 26.4201 (-3.49012 6.74397)
R2^2/D10^2 : 9.34993E-02 (-0.0534013 0.0723865)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.07 using 59 PHA bins.
# Reduced chi-squared = 0.7468 for 55 degrees of freedom
# Null hypothesis probability = 9.185219e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.103e-08 1.039e-08
25- 50 1.101e-07 1.968e-08
50-150 3.381e-07 5.130e-08
15-150 4.892e-07 7.275e-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: 1.49258 ( -0.0587336 0.0588506 )
Norm@50keV : 9.47490E-03 ( -0.000297065 0.000296921 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.55 using 59 PHA bins.
# Reduced chi-squared = 0.9044 for 57 degrees of freedom
# Null hypothesis probability = 6.789835e-01
Photon flux (15-150 keV) in 36 sec: 1.18050 ( -0.0392006 0.0392902 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.23977e-06 ( -1.09904e-07 1.10223e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08106 ( -0.250331 0.236755 )
Epeak [keV] : 118.171 ( -25.8785 84.3826 )
Norm@50keV : 1.48264E-02 ( -0.00328399 0.00450079 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.39 using 59 PHA bins.
# Reduced chi-squared = 0.7569 for 56 degrees of freedom
# Null hypothesis probability = 9.105516e-01
Photon flux (15-150 keV) in 36 sec: 1.14686 ( -0.04318 0.04328 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.13944e-06 ( -1.24715e-07 1.24459e-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) = 2.22e-06
S(50-100 keV) = 2.98e-06
T90 vs. Hardness ratio plot
T90 = 118.495999932289 sec.
Hardness ratio (energy fluence ratio) = 1.34234
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.46315
Count Ratio (50-100 keV) / (15-25 keV) = 1.0605
Mask shadow pattern
IMX = 5.800932083954842E-01, IMY = 1.363683258125580E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-24.851400 11.148590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.9044 19.6523 0.2 30.8 -13.2 5.0342 50.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.148670 423.748600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0723 40.9103 34.6 46.5 -35.0 0.2678 0.3 3.1 Cyg X-3
326.2805 38.4466 4.9 32.5 -31.3 0.9640 2.4 9.1 Cyg X-2
299.8092 65.3728 2.6 58.7 -7.5 11.7652 4.5 ------ UNKNOWN
327.3029 -15.1803 2.4 45.4 -121.3 6.6984 4.8 ------ UNKNOWN
Plot creation:
Mon Dec 19 18:44:20 EST 2016