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
5.3801 71.3846 0.0119 18.2925 124.7735 1.0419499 16.193 TRIG_01095288
Foreground time interval of the image:
-1.816 11.656 (delta_t = 13.472 [sec])
Background time interval of the image:
-232.507 -1.816 (delta_t = 230.691 [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 -1.816 sec. to 11.656 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30133 ( -0.200356 0.198993 )
Norm@50keV : 4.48879E-03 ( -0.000493797 0.000492733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.32 using 59 bins.
Reduced chi-squared = 1.21614
# Null hypothesis probability of 1.27e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.47 sec: 0.535662 ( -0.059559 0.05966 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.97376e-07 ( -7.45612e-08 7.53804e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.816 sec. to 11.656 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29782 ( -0.600457 0.238405 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 4.50740E-03 ( -0.000496706 0.000491106 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.32 using 59 bins.
Reduced chi-squared = 1.23786
# Null hypothesis probability of 1.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.47 sec: 0.538714 ( -0.078657 0.072283 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.02805e-07 ( -1.06684e-07 7.37877e-08 ) ergs/cm2
Band function
Time interval is from -1.816 sec. to 11.656 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] : 17.0481 (-2.46788 3.05044)
R^2/D10^2 : 3.98681E-02 (-0.0168564 0.0278554)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 91.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.68e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.176e-08 7.341e-09
25- 50 1.409e-07 2.764e-08
50-150 2.925e-07 6.883e-08
15-150 4.652e-07 7.395e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-41.4013 -200)
Norm : 2.20143 (-0.242604 0.242604)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.12e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.384e-08 4.106e-08
25- 50 1.420e-07 7.777e-08
50-150 3.115e-07 1.713e-07
15-150 5.274e-07 2.852e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.71604 (-2.1932 7.08145)
R1^2/D10^2 : 0.993394 (-0.88593 6.29994)
kT2 [keV] : 26.1820 (-6.75354 -26.31)
R2^2/D10^2 : 8.41588E-03 (-0.00801187 0.0147732)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.07e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.717e-08 3.633e-08
25- 50 1.248e-07 4.830e-08
50-150 3.890e-07 2.111e-07
15-150 5.809e-07 2.417e-07
Peak spectrum fit
Power-law model
Time interval is from -0.052 sec. to 0.948 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18657 ( -0.185605 0.184056 )
Norm@50keV : 2.00161E-02 ( -0.00211317 0.00211225 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.32 using 59 bins.
Reduced chi-squared = 0.98807
# Null hypothesis probability of 5.01e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.34514 ( -0.25174 0.25209 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03873e-07 ( -2.43459e-08 2.45396e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.052 sec. to 0.948 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01396 ( -0.808795 0.338782 )
Epeak [keV] : 309.735 ( -309.734 -309.734 )
Norm@50keV : 2.41819E-02 ( -0.00893565 0.0324906 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.15 using 59 bins.
Reduced chi-squared = 1.00268
# Null hypothesis probability of 4.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.33005 ( -0.25977 0.25923 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01865e-07 ( -2.6105e-08 2.54248e-08 ) ergs/cm2
Band function
Time interval is from -0.052 sec. to 0.948 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] : 18.8864 (-2.48668 3.00496)
R^2/D10^2 : 0.131322 (-0.0502001 0.0774137)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.46e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.227e-09 1.930e-09
25- 50 4.419e-08 7.000e-09
50-150 1.157e-07 2.326e-08
15-150 1.691e-07 2.330e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-29.844 -200)
Norm : 9.57883 (-1.03262 1.03262)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.77e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.385e-08 1.321e-08
25- 50 4.587e-08 2.476e-08
50-150 1.006e-07 5.465e-08
15-150 1.703e-07 9.315e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.57799 (-2.00513 7.6372)
R1^2/D10^2 : 8.08694 (-7.68247 136.741)
kT2 [keV] : 23.6794 (-4.25328 34.0454)
R2^2/D10^2 : 5.78621E-02 (-0.0458116 0.0560414)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.81e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.943e-08 9.422e-09
25- 50 3.907e-08 1.060e-08
50-150 1.338e-07 4.035e-08
15-150 1.923e-07 4.880e-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: 1.30133 ( -0.200356 0.198993 )
Norm@50keV : 4.48879E-03 ( -0.000493797 0.000492733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.27e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.47 sec: 0.535655 ( -0.0595559 0.059658 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.97299e-07 ( -7.45435e-08 7.53948e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29781 ( -0.599519 0.239991 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 4.50740E-03 ( -0.000496706 0.000491106 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.47 sec: 0.535525 ( -0.059586 0.059545 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.96776e-07 ( -7.56664e-08 7.49026e-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) = 1.33e-07
S(50-100 keV) = 2.16e-07
T90 vs. Hardness ratio plot
T90 = 12.336000084877 sec.
Hardness ratio (energy fluence ratio) = 1.62406
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31245
Count Ratio (50-100 keV) / (15-25 keV) = 1.21261
Mask shadow pattern
IMX = -1.885367209634014E-01, IMY = -2.715366784012588E-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:
-232.507400 -1.816000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5890 35.1984 0.6 33.4 -18.7 8.2840 19.8 0.2 Cyg X-1
308.0707 40.9556 4.2 24.8 -22.2 0.9884 2.7 1.8 Cyg X-3
326.2978 38.4956 0.0 20.1 -58.0 0.1684 0.4 12.0 Cyg X-2
173.5864 82.0627 2.5 40.4 92.8 5.7883 4.6 ------ UNKNOWN
245.4231 52.1944 2.2 49.2 42.1 6.8454 5.2 ------ UNKNOWN
290.8798 67.6654 3.1 23.1 51.7 1.3802 3.8 ------ UNKNOWN
308.0113 37.6772 1.9 27.5 -26.6 2.3220 6.2 ------ UNKNOWN
7.5825 27.8744 2.9 36.3 -132.7 2.3250 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.816000 11.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.3888 35.1740 7.3 33.6 -18.5 -0.1255 -1.6 10.0 Cyg X-1
307.9904 40.8150 9.2 25.0 -22.3 -0.0772 -1.2 9.9 Cyg X-3
326.3777 38.2786 5.7 20.3 -58.4 0.1281 2.0 10.0 Cyg X-2
5.3801 71.3846 0.7 18.3 124.8 1.0418 16.2 ------ UNKNOWN
49.2576 26.4593 2.1 58.3 -174.3 1.8250 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
68.892600 962.922000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5694 35.2032 1.4 49.2 -28.4 25.6398 8.2 1.0 Cyg X-1
308.0969 40.9533 16.0 41.3 -33.9 1.4070 0.7 0.6 Cyg X-3
326.0756 38.1671 0.0 38.7 -55.5 -0.7879 -0.4 10.3 Cyg X-2
134.3752 71.5634 3.0 33.4 98.3 5.9224 3.8 ------ UNKNOWN
69.9009 26.2280 2.3 57.2 177.2 26.0838 4.9 ------ UNKNOWN
65.0519 39.8252 3.1 43.1 175.5 6.8616 3.8 ------ UNKNOWN
33.5127 39.9383 3.8 34.5 -148.0 3.9416 3.1 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:06:09 EDT 2022