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
172.3475 31.6280 0.0150 25.8945 -168.5320 1.4837795 12.955 TRIG_01051453
Foreground time interval of the image:
-18.320 65.712 (delta_t = 84.032 [sec])
Background time interval of the image:
-239.000 -18.320 (delta_t = 220.680 [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 96.000000
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 96.000000
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 96.000000
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 -18.320 sec. to 65.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.26796 ( -0.235494 0.25761 )
Norm@50keV : 8.65069E-04 ( -0.000154536 0.000151016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.74 using 59 bins.
Reduced chi-squared = 0.855088
# Null hypothesis probability of 7.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 84.03 sec: 0.148546 ( -0.016927 0.016928 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.90867e-07 ( -9.99117e-08 1.03506e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -18.320 sec. to 65.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86787 ( -1.05511 0.141548 )
Epeak [keV] : 12.7057 ( -12.0102 34.651 )
Norm@50keV : 1.51514E-03 ( -0.000511266 0.00519152 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.16 using 59 bins.
Reduced chi-squared = 0.86
# Null hypothesis probability of 7.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 84.03 sec: 0.148346 ( -0.016755 0.017212 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.61096e-07 ( -1.10828e-07 1.15964e-07 ) ergs/cm2
Band function
Time interval is from -18.320 sec. to 65.712 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] : 8.10914 (-1.20946 1.41015)
R^2/D10^2 : 0.149844 (-0.0698893 0.136605)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.512e-07 2.790e-08
25- 50 2.709e-07 4.857e-08
50-150 7.436e-08 2.830e-08
15-150 4.965e-07 7.769e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 43.5881 (-12.0454 19.2399)
Norm : 0.904683 (-0.179431 0.24992)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.66e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.793e-07 2.542e-08
25- 50 2.446e-07 3.525e-08
50-150 2.073e-07 7.622e-08
15-150 6.312e-07 1.085e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.39704 (-1.25191 1.39467)
R1^2/D10^2 : 1.30786 (-0.878068 4.81429)
kT2 [keV] : 15.0418 (-3.73729 6.40312)
R2^2/D10^2 : 9.38679E-03 (-0.00724592 0.0225073)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.73e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.926e-07 9.889e-08
25- 50 2.216e-07 1.028e-07
50-150 2.309e-07 1.385e-07
15-150 6.451e-07 3.370e-07
Peak spectrum fit
Power-law model
Time interval is from 17.864 sec. to 18.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65442 ( -0.592877 0.648794 )
Norm@50keV : 3.39196E-03 ( -0.00129424 0.00122175 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.57 using 59 bins.
Reduced chi-squared = 0.764386
# Null hypothesis probability of 9.05e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.443572 ( -0.146045 0.146188 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.1537e-08 ( -1.20798e-08 1.27575e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 17.864 sec. to 18.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60175 ( -2.65643 0.982396 )
Epeak [keV] : 315.136 ( -276.653 -276.653 )
Norm@50keV : 3.62663E-03 ( -0.00372858 0.233527 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.56 using 59 bins.
Reduced chi-squared = 0.777857
# Null hypothesis probability of 8.87e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.441298 ( -0.148682 0.145739 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10857e-08 ( -1.35275e-08 1.30897e-08 ) ergs/cm2
Band function
Time interval is from 17.864 sec. to 18.864 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] : 9.83271 (-3.50838 10.5897)
R^2/D10^2 : 0.216418 (-0.212549 0.923764)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.236e-09 2.677e-09
25- 50 1.028e-08 6.535e-09
50-150 5.109e-09 4.037e-09
15-150 1.963e-08 1.258e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.927 (-165.665 -165.665)
Norm : 1.80385 (-0.606742 1.15071)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.487e-09 2.768e-09
25- 50 8.595e-09 5.285e-09
50-150 1.863e-08 1.188e-08
15-150 3.171e-08 1.919e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.64887 (-3.01809 4.49709)
R1^2/D10^2 : 0.723372 (-0.613598 6.58665)
kT2 [keV] : 30.9652 (-17.43 -30.9533)
R2^2/D10^2 : 2.90761E-03 (-0.00289324 0.0196395)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.94e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.282e-09 3.304e-09
25- 50 8.677e-09 4.957e-09
50-150 1.869e-08 1.163e-08
15-150 3.264e-08 1.693e-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: 2.26796 ( -0.235494 0.25761 )
Norm@50keV : 8.65069E-04 ( -0.000154536 0.000151016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 84.03 sec: 0.148530 ( -0.016926 0.0169261 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.90717e-07 ( -9.98335e-08 1.03512e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86671 ( -1.05418 0.141654 )
Epeak [keV] : 12.7835 ( -12.6034 34.3981 )
Norm@50keV : 1.51746E-03 ( -0.000512259 0.00519479 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 84.03 sec: 0.146391 ( -0.017439 0.0088 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.61266e-07 ( -1.10913e-07 1.20728e-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) = 2.22e-07
S(50-100 keV) = 1.84e-07
T90 vs. Hardness ratio plot
T90 = 64.4639999866486 sec.
Hardness ratio (energy fluence ratio) = 0.828829
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.823008
Count Ratio (50-100 keV) / (15-25 keV) = 0.446261
Mask shadow pattern
IMX = -4.757645259286623E-01, IMY = 9.651829944906765E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 96.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 96.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 96.000000
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 -18.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
189.6189 4.0047 2.9 48.4 151.5 3.5344 4.0 ------ UNKNOWN
260.0341 58.3873 2.9 36.6 19.5 1.4271 4.0 ------ UNKNOWN
181.9985 57.1557 2.4 8.4 -83.8 1.0469 4.7 ------ UNKNOWN
150.0746 40.3320 3.3 31.9 -128.4 1.2560 3.5 ------ UNKNOWN
339.6598 68.3360 2.9 56.8 -19.7 4.0209 4.0 ------ UNKNOWN
125.5039 50.0180 3.9 41.3 -98.9 3.6815 3.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-18.320000 65.712000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
202.5974 33.3391 1.9 20.0 124.0 0.8022 6.2 ------ UNKNOWN
172.3476 31.6280 0.9 25.9 -168.5 1.4836 13.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
161.900590 704.200610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4207 35.3138 18.6 15.4 57.2 -0.2836 -0.6 2.5 Her X-1
299.5303 35.2056 2.3 44.0 3.9 3.8328 4.9 3.0 Cyg X-1
308.2336 41.0082 9.1 46.6 -8.2 0.9466 1.3 6.5 Cyg X-3
290.7060 34.4497 2.6 38.5 11.1 2.8805 4.4 ------ UNKNOWN
189.0844 24.4087 3.7 47.3 179.7 2.8394 3.1 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:00:02 EDT 2022