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
5.2148 7.8345 0.0047 33.6722 153.7123 2.8816942 40.767 TRIG_01004168
Foreground time interval of the image:
-8.864 0.880 (delta_t = 9.744 [sec])
Background time interval of the image:
-54.003 -8.864 (delta_t = 45.139 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -8.864 sec. to 0.880 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47594 ( -0.0692759 0.0693829 )
Norm@50keV : 1.98277E-02 ( -0.000739104 0.000738696 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.17 using 59 bins.
Reduced chi-squared = 1.07316
# Null hypothesis probability of 3.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.744 sec: 2.45966 ( -0.09793 0.09827 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84047e-06 ( -7.38294e-08 7.40422e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.864 sec. to 0.880 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42588 ( -0.271109 0.0941255 )
Epeak [keV] : 563.601 ( -994.385 -994.385 )
Norm@50keV : 2.09393E-02 ( -0.00129308 0.00666427 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.25 using 59 bins.
Reduced chi-squared = 1.09375
# Null hypothesis probability of 2.93e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.744 sec: 2.45650 ( -0.10621 0.10101 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.83648e-06 ( -7.94182e-08 7.7146e-08 ) ergs/cm2
Band function
Time interval is from -8.864 sec. to 0.880 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] : 16.3038 ( )
R^2/D10^2 : 0.203646 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 233.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.04e-23 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.086e-07 7.941e-09
25- 50 4.643e-07 2.343e-08
50-150 8.686e-07 6.071e-08
15-150 1.442e-06 6.528e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-13.254 -200)
Norm : 10.1117 (-0.376043 0.376043)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.20e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.453e-07 9.695e-09
25- 50 4.720e-07 1.954e-08
50-150 1.035e-06 4.385e-08
15-150 1.752e-06 7.552e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.84317 (-1.10085 1.21959)
R1^2/D10^2 : 1.72962 (-0.623604 1.13325)
kT2 [keV] : 31.2060 (-4.83203 8.11094)
R2^2/D10^2 : 1.74131E-02 (-0.00906675 0.0138818)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.91e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.099e-07 2.582e-08
25- 50 4.703e-07 4.326e-08
50-150 1.146e-06 1.795e-07
15-150 1.827e-06 2.241e-07
Peak spectrum fit
Power-law model
Time interval is from -8.520 sec. to -7.520 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56340 ( -0.126402 0.127552 )
Norm@50keV : 3.23162E-02 ( -0.00240035 0.00238945 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.60 using 59 bins.
Reduced chi-squared = 0.975439
# Null hypothesis probability of 5.28e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.10720 ( -0.30493 0.30549 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.03697e-07 ( -2.42432e-08 2.43983e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.520 sec. to -7.520 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56117 ( -0.444341 0.198917 )
Epeak [keV] : 9984.86 ( -9955.86 -9955.86 )
Norm@50keV : 3.24023E-02 ( -0.0151158 0.0258679 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.60 using 59 bins.
Reduced chi-squared = 0.992857
# Null hypothesis probability of 4.90e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.10436 ( -0.3023 0.30752 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.03235e-07 ( -2.59988e-08 2.46866e-08 ) ergs/cm2
Band function
Time interval is from -8.520 sec. to -7.520 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] : 14.2514 (-1.33877 1.52066)
R^2/D10^2 : 0.543786 (-0.165984 0.232197)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 110.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.92e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.329e-08 3.485e-09
25- 50 8.814e-08 8.625e-09
50-150 1.189e-07 1.798e-08
15-150 2.304e-07 2.135e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.278 (-58.9648 -199.329)
Norm : 16.6862 (-1.20078 1.20172)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.155e-08 3.475e-09
25- 50 7.993e-08 9.270e-09
50-150 1.753e-07 4.722e-08
15-150 2.968e-07 5.500e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.60278 (-1.78734 1.91787)
R1^2/D10^2 : 3.55996 (-1.80186 5.79412)
kT2 [keV] : 31.1076 (-8.21886 20.9345)
R2^2/D10^2 : 2.71679E-02 (-0.0213504 0.0564184)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.37e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.975e-08 9.640e-09
25- 50 8.230e-08 1.801e-08
50-150 1.821e-07 8.786e-08
15-150 3.042e-07 9.530e-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: 1.47594 ( -0.0692759 0.0693829 )
Norm@50keV : 1.98277E-02 ( -0.000739104 0.000738696 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.744 sec: 2.45960 ( -0.0979205 0.0982644 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84023e-06 ( -7.38386e-08 7.41016e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44650 ( -0.266147 0.092738 )
Epeak [keV] : 998.114 ( -999.12 -999.12 )
Norm@50keV : 2.04821E-02 ( -0.00128999 0.00666817 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.96e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.744 sec: 2.45048 ( -0.10096 0.10627 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8346e-06 ( -7.7572e-08 8.02029e-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) = 4.50e-07
S(50-100 keV) = 6.47e-07
T90 vs. Hardness ratio plot
T90 = 8.6599999666214 sec.
Hardness ratio (energy fluence ratio) = 1.43778
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.4201
Count Ratio (50-100 keV) / (15-25 keV) = 1.12652
Mask shadow pattern
IMX = -5.973174420300765E-01, IMY = -2.950537594947298E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-54.003400 -8.864000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2541 38.2983 3.4 34.0 -116.1 0.4812 3.4 4.1 Cyg X-2
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.864000 0.880000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0783 38.3954 6.3 34.1 -115.8 0.1447 1.8 6.2 Cyg X-2
79.9856 38.8368 2.4 51.6 32.1 1.2255 4.8 ------ UNKNOWN
59.2990 34.0046 3.0 38.6 48.3 0.4055 3.8 ------ UNKNOWN
38.8391 22.9962 2.8 29.7 82.8 0.3223 4.1 ------ UNKNOWN
5.2148 7.8345 0.3 33.7 153.7 2.8819 40.8 564.1 UNKNOWN
356.7526 -3.0191 2.2 46.0 163.4 0.6784 5.1 266.0 UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
87.196600 509.896590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2023 38.4097 4.6 46.5 -26.4 1.6218 2.5 5.5 Cyg X-2
42.3986 28.2070 2.8 40.6 71.4 5.6397 4.2 ------ UNKNOWN
352.7095 -41.1477 2.4 50.3 -151.5 4.6019 4.9 ------ UNKNOWN
342.5808 -41.1504 3.1 53.2 -142.5 7.7994 3.7 ------ UNKNOWN
335.6855 -30.9532 2.6 48.0 -129.0 7.5753 4.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:26:36 EDT 2022