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
143.5403 -51.4091 0.0064 50.8200 -150.6191 13.2219866 30.268 TRIG_01064421
Foreground time interval of the image:
-14.299 78.568 (delta_t = 92.867 [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
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 -31.360 sec. to 78.568 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65711 ( -0.0630279 0.0632785 )
Norm@50keV : 1.17101E-02 ( -0.000405997 0.000405848 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.18 using 59 bins.
Reduced chi-squared = 1.09088
# Null hypothesis probability of 2.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 109.9 sec: 1.53271 ( -0.05914 0.05938 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.19624e-05 ( -4.28189e-07 4.28357e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.360 sec. to 78.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37034 ( -0.267529 0.252537 )
Epeak [keV] : 118.953 ( -33.0485 376.907 )
Norm@50keV : 1.59428E-02 ( -0.0037114 0.00517238 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.41 using 59 bins.
Reduced chi-squared = 1.04304
# Null hypothesis probability of 3.87e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 109.9 sec: 1.50221 ( -0.0643 0.06463 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17668e-05 ( -4.6419e-07 4.62416e-07 ) ergs/cm2
Band function
Time interval is from -31.360 sec. to 78.568 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] : 15.3481 ( )
R^2/D10^2 : 0.150410 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 236.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.75e-24 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.120e-07 5.616e-08
25- 50 3.294e-06 1.621e-07
50-150 5.334e-06 3.198e-07
15-150 9.441e-06 3.868e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.217 (-26.2472 -166.83)
Norm : 6.19267 (-0.261505 0.285444)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.729e-06 1.094e-07
25- 50 3.256e-06 2.297e-07
50-150 6.726e-06 1.623e-06
15-150 1.171e-05 1.929e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.76890 (-1.0146 1.0574)
R1^2/D10^2 : 1.14860 (-0.389583 0.703793)
kT2 [keV] : 27.4827 (-3.5566 5.20009)
R2^2/D10^2 : 1.38974E-02 (-0.00655684 0.00987445)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.40e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.537e-06 1.951e-07
25- 50 3.368e-06 2.830e-07
50-150 6.736e-06 8.424e-07
15-150 1.164e-05 9.842e-07
Peak spectrum fit
Power-law model
Time interval is from -24.224 sec. to -23.224 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51635 ( -0.276246 0.282851 )
Norm@50keV : 3.25942E-02 ( -0.00521319 0.00519354 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.47 using 59 bins.
Reduced chi-squared = 1.06088
# Null hypothesis probability of 3.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.08729 ( -0.68112 0.68474 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.08432e-07 ( -5.25734e-08 5.27948e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -24.224 sec. to -23.224 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51375 ( -0.952569 2.56651 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 3.26904E-02 ( -0.00523856 -0.0326911 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.48 using 59 bins.
Reduced chi-squared = 1.08
# Null hypothesis probability of 3.17e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.10773 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.08852e-07 ( -5.39343e-08 4.73038e-08 ) ergs/cm2
Band function
Time interval is from -24.224 sec. to -23.224 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] : 17.0837 (-3.36304 4.2535)
R^2/D10^2 : 0.292202 (-0.157799 0.335322)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.34e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.735e-08 5.897e-09
25- 50 7.704e-08 2.212e-08
50-150 1.608e-07 5.115e-08
15-150 2.552e-07 6.430e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-85.349 -199.363)
Norm : 16.7745 (-2.65975 2.66017)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.29e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.177e-08 2.419e-08
25- 50 8.035e-08 4.520e-08
50-150 1.762e-07 9.870e-08
15-150 2.983e-07 1.689e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.22818 (-1.89035 3.86446)
R1^2/D10^2 : 13.6405 (-11.878 49.3164)
kT2 [keV] : 25.5404 (-6.79107 18.9917)
R2^2/D10^2 : 6.21917E-02 (-0.0524894 0.126592)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.649e-08 2.595e-08
25- 50 6.873e-08 3.418e-08
50-150 1.941e-07 1.113e-07
15-150 3.093e-07 1.595e-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: 1.68419 ( -0.0747912 0.0752135 )
Norm@50keV : 9.71381E-03 ( -0.000405162 0.000404475 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.30e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 92.87 sec: 1.28305 ( -0.0580855 0.0582978 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.36346e-06 ( -3.60523e-07 3.61108e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42040 ( -0.316704 0.288963 )
Epeak [keV] : 116.159 ( -36.9135 -116.16 )
Norm@50keV : 1.29940E-02 ( -0.00342434 0.00528425 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.72e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 92.87 sec: 1.26115 ( -0.03141 0.06283 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.2356e-06 ( -3.92896e-07 3.90732e-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) = 3.18e-06
S(50-100 keV) = 4.03e-06
T90 vs. Hardness ratio plot
T90 = 89.9719998836517 sec.
Hardness ratio (energy fluence ratio) = 1.2673
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.47841
Count Ratio (50-100 keV) / (15-25 keV) = 1.12186
Mask shadow pattern
IMX = -1.069176960702829E+00, IMY = 6.019817123666598E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-14.299400 78.568000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.5024 -60.6978 3.8 38.9 -169.0 0.6005 3.0 7.1 Cen X-3
186.2983 -62.8012 5.6 35.2 179.7 0.3816 2.1 10.0 GX 301-2
244.9650 -15.6316 1.0 37.4 58.7 3.8250 11.6 1.0 Sco X-1
256.1088 -37.8268 4.0 40.6 97.4 -1.5234 -2.9 5.9 4U 1700-377
257.1389 -40.5103 2.2 41.3 101.5 2.8998 5.3 ------ UNKNOWN
241.5435 -80.2842 2.1 51.9 156.2 2.9791 5.4 ------ UNKNOWN
202.3189 -60.0677 3.3 30.0 168.2 0.5982 3.5 ------ UNKNOWN
218.0932 17.5754 2.2 49.0 -3.2 1.5167 5.3 ------ UNKNOWN
206.1004 13.2670 3.4 43.6 -18.6 0.7709 3.4 ------ UNKNOWN
141.6244 -56.3441 2.7 51.9 -156.9 1.8700 4.3 ------ UNKNOWN
143.5403 -51.4091 0.4 50.8 -150.6 13.2210 30.3 ------ UNKNOWN
187.9653 17.6718 3.1 51.5 -40.7 2.4557 3.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
166.300630 963.069700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5068 -40.5535 0.7 12.2 -114.5 10.5009 17.1 1.0 Vela X-1
170.3075 -60.6555 1.3 17.4 48.3 6.2429 8.7 2.0 Cen X-3
186.6728 -62.5573 0.0 25.3 48.5 0.8341 1.0 12.8 GX 301-2
58.5518 -55.3616 2.5 47.6 145.9 10.2165 4.5 ------ UNKNOWN
211.9866 -35.0583 2.3 50.4 15.0 8.2846 5.0 ------ UNKNOWN
73.7760 -44.2186 2.7 45.6 166.1 6.8324 4.3 ------ UNKNOWN
156.3716 -19.1304 2.6 33.8 -62.1 4.5580 4.5 ------ UNKNOWN
109.2909 -13.3169 3.3 47.1 -132.6 8.2930 3.5 ------ UNKNOWN
133.8383 -10.9348 2.8 41.3 -98.7 15.8338 4.1 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:50:51 EDT 2022