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
181.0271 53.1921 0.0229 20.4094 130.6616 0.8835266 8.370 TRIG_01164180
Foreground time interval of the image:
-0.520 35.224 (delta_t = 35.744 [sec])
Background time interval of the image:
-239.352 -0.520 (delta_t = 238.832 [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 8.192000
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 8.192000
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 8.192000
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 -0.520 sec. to 35.224 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60371 ( -0.333233 0.340591 )
Norm@50keV : 1.41373E-03 ( -0.000298027 0.000290366 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.16 using 59 bins.
Reduced chi-squared = 1.17825
# Null hypothesis probability of 1.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 35.74 sec: 0.181886 ( -0.034614 0.034627 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.72383e-07 ( -1.05274e-07 1.08308e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.520 sec. to 35.224 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60199 ( -1.57673 1.11981 )
Epeak [keV] : 9998.81 ( -9999.18 -9999.18 )
Norm@50keV : 1.41703E-03 ( -0.000300072 0.0139895 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.16 using 59 bins.
Reduced chi-squared = 1.19929
# Null hypothesis probability of 1.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 35.74 sec: 0.181945 ( -0.034777 0.034569 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.73626e-07 ( -1.35379e-07 8.47724e-08 ) ergs/cm2
Band function
Time interval is from -0.520 sec. to 35.224 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] : 10.2915 (-2.13978 3.06151)
R^2/D10^2 : 7.81238E-02 (-0.0482982 0.108046)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.34e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.078e-08 2.124e-08
25- 50 1.573e-07 5.273e-08
50-150 8.917e-08 4.509e-08
15-150 3.073e-07 9.553e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 153.940 (-92.1638 -158.27)
Norm : 0.747755 (-0.150359 0.214087)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.63e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.848e-08 3.935e-08
25- 50 1.274e-07 7.039e-08
50-150 2.542e-07 1.558e-07
15-150 4.501e-07 2.607e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.27709 (-1.82286 2.28496)
R1^2/D10^2 : 0.156678 (-0.0817646 0.140411)
kT2 [keV] : 200.000 (-172.074 -200)
R2^2/D10^2 : 2.64328E-05 (-1.17362e-05 0.000125308)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.47e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.300e-08 4.044e-08
25- 50 1.407e-07 7.510e-08
50-150 2.943e-07 1.723e-07
15-150 5.080e-07 2.339e-07
Peak spectrum fit
Power-law model
Time interval is from 9.304 sec. to 10.304 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.26395 ( -0.476328 0.6252 )
Norm@50keV : 3.69730E-03 ( -0.00168637 0.00165098 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.95 using 59 bins.
Reduced chi-squared = 0.999123
# Null hypothesis probability of 4.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.633270 ( -0.203646 0.204315 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.50332e-08 ( -1.33776e-08 1.42433e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 9.304 sec. to 10.304 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.33650E-02 ( -4.50003 2.02906 )
Epeak [keV] : 34.3059 ( -34.3409 18.3305 )
Norm@50keV : 9.42711E-02 ( -0.0941262 166.324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.69 using 59 bins.
Reduced chi-squared = 0.95875
# Null hypothesis probability of 5.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.648766 ( -0.198458 0.200815 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 9.304 sec. to 10.304 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] : 8.75081 (-2.70401 3.5214)
R^2/D10^2 : 0.556663 (-0.555902 1.74177)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.174e-09 5.010e-09
25- 50 1.662e-08 9.890e-09
50-150 5.813e-09 4.626e-09
15-150 3.061e-08 1.932e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 43.7740 (-21.7359 52.2317)
Norm : 4.13295 (-1.62367 2.8934)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.67e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.763e-09 4.948e-09
25- 50 1.333e-08 8.307e-09
50-150 1.135e-08 9.105e-09
15-150 3.445e-08 2.118e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.25354 (-5.25339 7.00371)
R1^2/D10^2 : 2.12163 (-2.12147 -2.12147)
kT2 [keV] : 12.5187 (-12.5175 -12.5175)
R2^2/D10^2 : 9.26554E-02 (-0.0927003 1.57274)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.38e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.342e-09 7.135e-09
25- 50 1.478e-08 9.635e-09
50-150 1.009e-08 6.695e-09
15-150 3.421e-08 2.065e-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: 1.60371 ( -0.333233 0.340591 )
Norm@50keV : 1.41373E-03 ( -0.000298027 0.000290366 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 35.74 sec: 0.181880 ( -0.0346119 0.0346251 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.72318e-07 ( -1.05215e-07 1.08393e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60874 ( -0.340222 0.338016 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.41194E-03 ( -0.000298013 0.0118906 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 35.74 sec: 0.181916 ( -0.035856 0.034536 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.73626e-07 ( -1.33792e-07 1.05608e-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) = 1.23e-07
S(50-100 keV) = 1.62e-07
T90 vs. Hardness ratio plot
T90 = 29.0599999427795 sec.
Hardness ratio (energy fluence ratio) = 1.31707
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.70745
Count Ratio (50-100 keV) / (15-25 keV) = 0.769353
Mask shadow pattern
IMX = -2.424463437888354E-01, IMY = -2.822522106552625E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.352000 -0.520000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4565 35.3494 4.1 42.2 17.6 1.3375 2.8 0.4 Her X-1
204.3499 37.8068 2.4 31.6 84.7 3.2460 4.7 ------ UNKNOWN
215.6170 59.7869 2.7 10.0 57.1 1.5057 4.3 ------ UNKNOWN
282.4145 37.3379 2.5 49.9 -12.1 2.9838 4.6 ------ UNKNOWN
251.3616 84.0397 2.3 16.8 -87.0 2.1626 4.9 ------ UNKNOWN
291.4232 44.2870 2.7 46.9 -24.4 3.0628 4.3 ------ UNKNOWN
32.5872 72.1868 3.4 38.5 -103.3 4.3240 3.4 ------ UNKNOWN
79.4618 54.1716 2.6 51.0 -137.1 8.0364 4.4 ------ UNKNOWN
335.9958 63.0035 2.9 42.7 -69.2 5.7650 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.520000 35.224000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4728 35.2907 10.5 42.3 17.6 0.1754 1.1 3.2 Her X-1
154.9408 30.0857 2.3 49.3 145.0 2.0783 4.9 ------ UNKNOWN
181.0271 53.1921 1.4 20.4 130.7 0.8837 8.4 ------ UNKNOWN
291.5811 49.6258 2.3 42.3 -28.4 0.7708 5.1 ------ UNKNOWN
314.7229 63.2811 2.3 37.8 -56.5 0.9214 5.0 ------ UNKNOWN
65.8581 63.6389 2.0 44.5 -124.0 2.1315 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
111.148630 962.768000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4665 35.2940 3.6 53.0 12.2 6.7177 3.2 2.9 Her X-1
234.2373 22.6373 2.9 50.2 39.8 12.1938 4.0 ------ UNKNOWN
197.2696 24.0234 2.8 31.6 84.7 8.9850 4.1 ------ UNKNOWN
193.4065 46.9192 2.6 10.0 57.1 5.1528 4.5 ------ UNKNOWN
67.0887 81.0806 3.8 41.2 -78.7 13.7538 3.1 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:09:20 EDT 2023