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
164.3123 50.4873 0.0043 26.7965 -45.3375 4.5626258 45.039 TRIG_00994389
Foreground time interval of the image:
-19.176 10.876 (delta_t = 30.052 [sec])
Background time interval of the image:
-239.000 -19.176 (delta_t = 219.824 [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 -19.176 sec. to 10.876 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55040 ( -0.0624645 0.0626394 )
Norm@50keV : 1.00950E-02 ( -0.000351434 0.000351111 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.65 using 59 bins.
Reduced chi-squared = 1.11667
# Null hypothesis probability of 2.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 30.05 sec: 1.27815 ( -0.04652 0.0466 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.85604e-06 ( -1.06474e-07 1.06772e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.176 sec. to 10.876 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04006 ( -0.271785 0.256043 )
Epeak [keV] : 97.0968 ( -17.3636 45.1216 )
Norm@50keV : 1.78597E-02 ( -0.00434387 0.0061554 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.39 using 59 bins.
Reduced chi-squared = 0.917679
# Null hypothesis probability of 6.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 30.05 sec: 1.23822 ( -0.05015 0.05025 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.74843e-06 ( -1.19286e-07 1.19209e-07 ) ergs/cm2
Band function
Time interval is from -19.176 sec. to 10.876 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] : 15.3499 ( )
R^2/D10^2 : 0.129821 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 195.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.32e-17 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.917e-07 1.247e-08
25- 50 7.777e-07 3.576e-08
50-150 1.260e-06 8.519e-08
15-150 2.229e-06 9.316e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-31.1647 -200)
Norm : 5.19189 (-0.177785 0.177785)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.888e-07 1.442e-08
25- 50 7.479e-07 2.840e-08
50-150 1.640e-06 6.235e-08
15-150 2.777e-06 9.886e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.89682 (-0.865348 0.965303)
R1^2/D10^2 : 1.28560 (-0.45254 0.774895)
kT2 [keV] : 23.9129 (-2.36442 3.19098)
R2^2/D10^2 : 2.16201E-02 (-0.0082008 0.0107433)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.13e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.567e-07 4.746e-08
25- 50 7.527e-07 6.927e-08
50-150 1.621e-06 1.808e-07
15-150 2.730e-06 2.778e-07
Peak spectrum fit
Power-law model
Time interval is from 0.144 sec. to 1.144 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38699 ( -0.115131 0.115986 )
Norm@50keV : 3.07570E-02 ( -0.00221539 0.00221109 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.06 using 59 bins.
Reduced chi-squared = 1.0186
# Null hypothesis probability of 4.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.73478 ( -0.26884 0.269 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.9803e-07 ( -2.36895e-08 2.38396e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.144 sec. to 1.144 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.638475 ( -0.535187 0.477403 )
Epeak [keV] : 94.6219 ( -20.5581 72.8445 )
Norm@50keV : 7.19407E-02 ( -0.0295031 0.0577259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.46 using 59 bins.
Reduced chi-squared = 0.901071
# Null hypothesis probability of 6.84e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.65006 ( -0.27467 0.27458 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.86952e-07 ( -2.50433e-08 2.51309e-08 ) ergs/cm2
Band function
Time interval is from 0.144 sec. to 1.144 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] : 16.4226 (-1.35946 1.49988)
R^2/D10^2 : 0.330576 (-0.0860554 0.114337)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.45e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.832e-08 2.495e-09
25- 50 7.881e-08 7.485e-09
50-150 1.500e-07 1.960e-08
15-150 2.471e-07 2.110e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-25.9316 -200)
Norm : 15.4617 (-1.09643 1.09643)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.95e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.850e-08 3.185e-09
25- 50 7.405e-08 6.925e-09
50-150 1.624e-07 4.228e-08
15-150 2.750e-07 4.440e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.93117 (-1.96341 2.35535)
R1^2/D10^2 : 3.07171 (-1.78728 6.61933)
kT2 [keV] : 23.6080 (-3.79311 6.55797)
R2^2/D10^2 : 7.72518E-02 (-0.0473595 0.0917552)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.82e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.117e-08 1.300e-08
25- 50 7.392e-08 2.583e-08
50-150 1.813e-07 6.098e-08
15-150 2.864e-07 8.950e-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: 1.55040 ( -0.0624645 0.0626394 )
Norm@50keV : 1.00950E-02 ( -0.000351434 0.000351111 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 30.05 sec: 1.27811 ( -0.0465055 0.0465999 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.85565e-06 ( -1.06476e-07 1.06776e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04006 ( -0.271786 0.256042 )
Epeak [keV] : 97.0969 ( -17.3637 45.1215 )
Norm@50keV : 1.78597E-02 ( -0.00434384 0.00615543 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 30.05 sec: 1.23808 ( -0.05014 0.05023 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.74942e-06 ( -1.19368e-07 1.19295e-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) = 7.24e-07
S(50-100 keV) = 9.89e-07
T90 vs. Hardness ratio plot
T90 = 22.9119999408722 sec.
Hardness ratio (energy fluence ratio) = 1.36602
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.43749
Count Ratio (50-100 keV) / (15-25 keV) = 1.0978
Mask shadow pattern
IMX = 3.550219012562849E-01, IMY = 3.592294551720819E-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:
-239.000000 -19.176000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4502 35.2344 3.6 36.9 135.7 1.7203 3.2 6.5 Her X-1
256.5523 22.4676 3.0 47.8 145.9 4.2275 3.8 ------ UNKNOWN
106.7935 58.6393 2.8 51.0 -6.9 2.1534 4.2 ------ UNKNOWN
107.7589 50.4990 3.3 56.3 -14.7 3.3691 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.176000 10.876000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3048 35.4572 3.9 36.6 135.6 0.4979 2.9 10.2 Her X-1
164.3123 50.4873 0.3 26.8 -45.3 4.5614 45.0 ------ UNKNOWN
162.7418 40.3953 1.9 33.2 -61.2 0.8298 5.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
172.100590 853.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9711 -15.6495 0.8 40.1 -52.5 21.3602 15.0 0.7 Sco X-1
255.7963 -37.8590 137.2 22.0 -85.2 0.0685 0.1 9.1 4U 1700-377
256.4561 -36.4257 8.3 21.7 -81.2 1.0910 1.4 1.0 GX 349+2
263.0142 -24.7482 5.6 21.2 -45.3 1.5068 2.1 0.3 GX 1+4
264.7448 -44.4409 169.3 16.2 -108.2 -0.0480 -0.1 0.6 4U 1735-44
268.2468 -1.4484 10.0 37.9 -9.1 1.0961 1.1 7.3 SW J1753.5-0127
270.3409 -25.0996 2.3 16.2 -31.7 3.1925 5.1 3.3 GX 5-1
270.3105 -25.6903 2.3 15.7 -33.2 3.4733 5.5 3.2 GRS 1758-258
274.0300 -14.0873 6.2 24.1 -6.8 1.3215 1.9 3.4 GX 17+2
275.7977 -30.2938 5.5 9.1 -31.3 1.4229 2.1 7.9 H1820-303
284.8310 -24.8200 0.0 11.9 22.0 0.3707 0.6 12.7 HT1900.1-2455
288.7129 10.8787 446.7 47.8 23.2 -0.0440 -0.0 6.4 GRS 1915+105
262.9524 -33.6927 19.8 17.1 -69.7 0.4328 0.6 8.7 GX 354-0
324.1951 -28.2280 4.1 35.0 104.4 4.3900 2.8 ------ UNKNOWN
17.6941 -71.3262 3.0 56.8 173.9 15.9924 3.9 ------ UNKNOWN
260.3880 13.8096 3.8 55.0 -11.5 5.4792 3.0 ------ UNKNOWN
255.0836 -41.5595 2.2 22.5 -95.0 4.3416 5.4 ------ UNKNOWN
Plot creation:
Thu Oct 20 00:51:49 EDT 2022