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
21.0795 42.1028 0.0186 27.3287 -104.1974 1.2080288 10.350 TRIG_01044678
Foreground time interval of the image:
-34.408 7.592 (delta_t = 42.000 [sec])
Background time interval of the image:
-239.408 -34.408 (delta_t = 205.000 [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 -34.408 sec. to 7.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73567 ( -0.222609 0.233251 )
Norm@50keV : 1.85101E-03 ( -0.000279706 0.000274257 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.32 using 59 bins.
Reduced chi-squared = 0.935439
# Null hypothesis probability of 6.14e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 42 sec: 0.248989 ( -0.032752 0.032762 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.18091e-07 ( -1.11286e-07 1.13672e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -34.408 sec. to 7.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.726749 ( -1.13377 0.913906 )
Epeak [keV] : 57.3002 ( -13.6941 93.5556 )
Norm@50keV : 6.56178E-03 ( -0.00656158 0.0199127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.68 using 59 bins.
Reduced chi-squared = 0.887143
# Null hypothesis probability of 7.11e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 42 sec: 0.240547 ( -0.033525 0.03357 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.63512e-07 ( -1.13655e-07 1.21144e-07 ) ergs/cm2
Band function
Time interval is from -34.408 sec. to 7.592 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] : 12.6367 (-1.83927 2.13237)
R^2/D10^2 : 5.15548E-02 (-0.0223555 0.0397201)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.36e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.333e-08 1.945e-08
25- 50 2.448e-07 4.452e-08
50-150 2.430e-07 7.134e-08
15-150 5.612e-07 1.046e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 106.317 (-39.0107 -106.958)
Norm : 1.09936 (-0.175781 0.211906)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.10e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.206e-07 2.411e-08
25- 50 2.111e-07 3.824e-08
50-150 3.540e-07 1.799e-07
15-150 6.857e-07 2.329e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.71000 (-1.88574 2.92961)
R1^2/D10^2 : 0.990000 (-0.816342 4.14814)
kT2 [keV] : 16.7482 (-3.41924 6.10232)
R2^2/D10^2 : 1.55537E-02 (-0.0113501 0.0229548)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.166e-07 6.680e-08
25- 50 2.083e-07 1.090e-07
50-150 3.278e-07 1.869e-07
15-150 6.526e-07 3.102e-07
Peak spectrum fit
Power-law model
Time interval is from 0.592 sec. to 1.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59729 ( -0.328147 0.348497 )
Norm@50keV : 1.01119E-02 ( -0.00202496 0.00196787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.76 using 59 bins.
Reduced chi-squared = 0.855439
# Null hypothesis probability of 7.73e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.29837 ( -0.24037 0.24083 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.46106e-08 ( -2.01528e-08 2.04482e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.592 sec. to 1.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59524 ( -1.24772 2.68721 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.01366E-02 ( -0.00204126 -0.0101368 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.77 using 59 bins.
Reduced chi-squared = 0.870893
# Null hypothesis probability of 7.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.30191 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.48702e-08 ( -2.13037e-08 2.14138e-08 ) ergs/cm2
Band function
Time interval is from 0.592 sec. to 1.592 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] : 15.2908 (-3.15566 4.09458)
R^2/D10^2 : 0.136017 (-0.0771034 0.16885)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.636e-09 2.670e-09
25- 50 2.683e-08 9.280e-09
50-150 4.306e-08 1.794e-08
15-150 7.653e-08 2.483e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.906 (-115.342 -198.906)
Norm : 5.26229 (-0.965149 1.19682)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.60e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.311e-08 7.635e-09
25- 50 2.521e-08 1.415e-08
50-150 5.524e-08 3.206e-08
15-150 9.356e-08 5.320e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.27902 (-1.42214 2.08007)
R1^2/D10^2 : 36.6029 (-33.2667 208.653)
kT2 [keV] : 19.5705 (-4.65139 7.98003)
R2^2/D10^2 : 5.14283E-02 (-0.0358599 0.064666)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.89e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.548e-08 7.737e-09
25- 50 2.109e-08 9.847e-09
50-150 5.321e-08 3.184e-08
15-150 8.977e-08 4.475e-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: 1.73567 ( -0.222609 0.233251 )
Norm@50keV : 1.85101E-03 ( -0.000279706 0.000274257 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.14e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 42 sec: 0.248978 ( -0.0327504 0.0327597 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.17982e-07 ( -1.11218e-07 1.13725e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.726598 ( -1.13382 0.913856 )
Epeak [keV] : 57.2918 ( -13.6939 93.565 )
Norm@50keV : 6.56359E-03 ( -0.00656157 0.0199127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.11e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 42 sec: 0.240516 ( -0.033514 0.033557 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.63718e-07 ( -1.13711e-07 1.21309e-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) = 1.97e-07
S(50-100 keV) = 2.37e-07
T90 vs. Hardness ratio plot
T90 = 39 sec.
Hardness ratio (energy fluence ratio) = 1.20305
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.25799
Count Ratio (50-100 keV) / (15-25 keV) = 0.906446
Mask shadow pattern
IMX = -1.267459649226316E-01, IMY = 5.009892620903551E-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:
-239.408000 -34.408000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7420 35.1902 19.9 40.2 28.6 -0.2553 -0.6 7.5 Cyg X-1
308.2051 40.9983 2.9 31.6 25.1 1.3609 4.1 5.1 Cyg X-3
326.1205 38.3857 3.3 26.8 -2.2 0.8425 3.5 4.5 Cyg X-2
215.7474 74.3911 2.2 40.8 118.7 4.1356 5.2 ------ UNKNOWN
294.6469 33.5396 3.5 43.9 32.5 1.5264 3.3 ------ UNKNOWN
303.8047 15.6409 3.4 55.6 11.5 3.8802 3.4 ------ UNKNOWN
356.1278 78.7302 3.5 17.6 141.2 0.8119 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-34.408000 7.592000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6877 35.2013 5.2 40.2 28.7 0.3481 2.2 4.8 Cyg X-1
308.1021 40.8588 5.9 31.7 25.0 -0.2372 -1.9 5.6 Cyg X-3
326.2012 38.3237 10.6 26.8 -2.4 -0.1020 -1.1 1.4 Cyg X-2
311.5036 21.7433 2.4 47.0 6.1 0.8270 4.9 ------ UNKNOWN
330.9860 44.4235 2.3 19.8 -4.2 0.4186 4.9 ------ UNKNOWN
21.0795 42.1029 1.1 27.3 -104.2 1.2082 10.4 ------ UNKNOWN
61.8460 35.7238 2.2 51.4 -139.3 1.8631 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
374.492590 622.292590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7159 35.1139 5.2 50.2 21.5 1.9980 2.2 8.1 Cyg X-1
308.0420 40.9751 3.3 41.7 18.7 1.5967 3.5 3.4 Cyg X-3
326.1566 38.3111 5.9 36.0 -2.2 0.7439 1.9 1.0 Cyg X-2
222.1636 74.0436 3.2 40.9 98.0 3.6679 3.6 ------ UNKNOWN
116.6790 54.4124 3.6 49.4 158.2 2.6599 3.2 ------ UNKNOWN
301.0727 29.7824 2.8 54.2 16.7 4.9604 4.1 ------ UNKNOWN
319.6897 22.0589 2.7 53.0 -6.2 2.7523 4.3 ------ UNKNOWN
81.7084 27.5632 3.5 57.6 -156.4 4.8994 3.3 ------ UNKNOWN
350.3753 14.6755 2.6 50.6 -44.5 5.4139 4.5 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:03:48 EDT 2022