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
227.1696 -26.8804 0.0073 33.2996 -82.3585 3.2216431 26.279 TRIG_01090656
Foreground time interval of the image:
-3.560 9.056 (delta_t = 12.616 [sec])
Background time interval of the image:
-239.008 -3.560 (delta_t = 235.448 [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 1.024000
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 1.024000
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 1.024000
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 -3.560 sec. to 9.056 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14370 ( -0.0847821 0.0839039 )
Norm@50keV : 1.69302E-02 ( -0.00082139 0.00082012 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.46 using 59 bins.
Reduced chi-squared = 0.937895
# Null hypothesis probability of 6.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.62 sec: 1.97295 ( -0.09998 0.10015 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.20394e-06 ( -1.13641e-07 1.13874e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.560 sec. to 9.056 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.865645 ( -0.360868 0.307959 )
Epeak [keV] : 231.483 ( -99.3116 -231.49 )
Norm@50keV : 2.26250E-02 ( -0.00604496 0.00995063 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.46 using 59 bins.
Reduced chi-squared = 0.918929
# Null hypothesis probability of 6.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.62 sec: 1.94990 ( -0.10367 0.10376 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.176e-06 ( -1.20069e-07 1.19402e-07 ) ergs/cm2
Band function
Time interval is from -3.560 sec. to 9.056 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] : 20.1636 ( )
R^2/D10^2 : 9.00987E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 120.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.88e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.883e-08 8.922e-09
25- 50 4.449e-07 3.067e-08
50-150 1.342e-06 1.059e-07
15-150 1.876e-06 1.111e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.359 ( )
Norm : 8.28053 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 118.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.95e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.602e-07 1.413e-08
25- 50 5.006e-07 2.707e-08
50-150 1.098e-06 6.947e-08
15-150 1.859e-06 1.382e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.0916 (-2.48209 2.66924)
R1^2/D10^2 : 0.516360 (-0.229427 0.617534)
kT2 [keV] : 39.1475 (-10.0141 33.5822)
R2^2/D10^2 : 8.49482E-03 (-0.00682205 0.0143074)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.571e-07 3.045e-08
25- 50 4.873e-07 1.030e-07
50-150 1.541e-06 5.854e-07
15-150 2.185e-06 6.534e-07
Peak spectrum fit
Power-law model
Time interval is from 0.300 sec. to 1.300 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13331 ( -0.196817 0.193656 )
Norm@50keV : 2.75246E-02 ( -0.00319808 0.00319634 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.77 using 59 bins.
Reduced chi-squared = 1.22404
# Null hypothesis probability of 1.19e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.20377 ( -0.38118 0.3817 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.8482e-07 ( -3.63809e-08 3.65757e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.300 sec. to 1.300 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.869470 ( -0.871465 0.43288 )
Epeak [keV] : 234.502 ( -234.516 -234.516 )
Norm@50keV : 3.67427E-02 ( -0.014785 0.0556096 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.42 using 59 bins.
Reduced chi-squared = 1.23964
# Null hypothesis probability of 1.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.18184 ( -0.38669 0.38675 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.81443e-07 ( -3.85919e-08 3.79387e-08 ) ergs/cm2
Band function
Time interval is from 0.300 sec. to 1.300 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] : 19.1680 (-2.77321 3.41698)
R^2/D10^2 : 0.175415 (-0.0726824 0.117179)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.40e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.263e-08 2.919e-09
25- 50 6.111e-08 1.019e-08
50-150 1.653e-07 3.280e-08
15-150 2.390e-07 4.005e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-30.2258 -200)
Norm : 13.1136 (-1.56904 1.56904)
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.77e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.266e-08 1.831e-08
25- 50 6.282e-08 3.511e-08
50-150 1.378e-07 7.605e-08
15-150 2.333e-07 1.284e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.5155 (-4.69279 4.2898)
R1^2/D10^2 : 0.665481 (-0.409868 0.676875)
kT2 [keV] : 62.8124 (-34.2406 -60.0127)
R2^2/D10^2 : 3.76220E-03 (-0.0033047 0.0527499)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.03e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.025e-08 8.775e-09
25- 50 6.553e-08 3.140e-08
50-150 1.961e-07 1.008e-07
15-150 2.819e-07 1.373e-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: 1.14370 ( -0.0847821 0.0839039 )
Norm@50keV : 1.69302E-02 ( -0.00082139 0.00082012 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.62 sec: 1.97295 ( -0.0999714 0.100138 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.20368e-06 ( -1.13652e-07 1.139e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.865640 ( -0.360867 0.307988 )
Epeak [keV] : 231.480 ( -99.3749 -231.49 )
Norm@50keV : 2.26251E-02 ( -0.00604495 0.00995063 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.62 sec: 1.94978 ( -0.10365 0.10373 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.17699e-06 ( -1.20218e-07 1.19436e-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) = 4.47e-07
S(50-100 keV) = 8.10e-07
T90 vs. Hardness ratio plot
T90 = 11.0759998559952 sec.
Hardness ratio (energy fluence ratio) = 1.81208
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.66778
Count Ratio (50-100 keV) / (15-25 keV) = 1.72325
Mask shadow pattern
IMX = 8.734597730554834E-02, IMY = 6.510334254058794E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.008000 -3.560000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3153 -60.6227 14.0 53.7 -10.5 0.5629 0.8 0.0 Cen X-3
186.3062 -62.8432 59.1 52.8 -20.3 -0.1594 -0.2 10.6 GX 301-2
213.3802 39.6967 2.7 52.7 170.4 3.8408 4.4 ------ UNKNOWN
225.7944 19.6856 2.6 41.9 -162.2 1.8869 4.4 ------ UNKNOWN
238.2034 -18.7713 3.0 41.2 -99.5 4.4935 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.560000 9.056000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3371 -60.6221 9.3 53.7 -10.5 -0.1911 -1.2 0.6 Cen X-3
186.4472 -62.7552 6.6 52.7 -20.4 -0.3188 -1.8 5.8 GX 301-2
189.7591 34.6022 3.0 45.6 146.3 0.6057 3.8 ------ UNKNOWN
151.2239 -39.8315 2.4 49.5 19.7 0.6119 4.8 ------ UNKNOWN
166.3104 -59.3483 2.3 53.8 -7.6 0.7697 5.0 ------ UNKNOWN
227.1696 -26.8804 0.4 33.3 -82.4 3.2218 26.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
774.092610 963.122000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9757 -15.6413 0.4 34.9 -88.0 18.8103 29.0 0.2 Sco X-1
254.5368 35.2599 50.1 48.1 -168.3 -0.1312 -0.2 6.3 Her X-1
167.3040 -11.6461 4.5 50.2 39.6 3.7069 2.6 ------ UNKNOWN
239.8314 40.3599 4.0 42.9 175.5 1.3876 2.9 ------ UNKNOWN
263.9380 43.6188 3.3 58.6 -172.6 5.5565 3.5 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:12:19 EDT 2022