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
326.9859 44.5141 0.0083 16.6532 -87.6777 2.1131267 23.010 TRIG_01167266
Foreground time interval of the image:
0.024 14.749 (delta_t = 14.725 [sec])
Background time interval of the image:
-239.952 0.024 (delta_t = 239.976 [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
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 0.024 sec. to 76.296 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41004 ( -0.112865 0.11228 )
Norm@50keV : 3.95849E-03 ( -0.000236793 0.000236557 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.43 using 59 bins.
Reduced chi-squared = 0.691754
# Null hypothesis probability of 9.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 76.27 sec: 0.483189 ( -0.030355 0.030507 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.91174e-06 ( -1.90775e-07 1.91841e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.024 sec. to 76.296 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41050 ( -0.200775 0.109761 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.96641E-03 ( -0.000236863 0.00127824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.46 using 59 bins.
Reduced chi-squared = 0.704643
# Null hypothesis probability of 9.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 76.27 sec: 0.485381 ( -0.032675 0.028199 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.92465e-06 ( -2.50943e-07 2.25156e-07 ) ergs/cm2
Band function
Time interval is from 0.024 sec. to 76.296 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] : 16.7338 ( )
R^2/D10^2 : 3.65821E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 121.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.50e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.598e-07 1.880e-08
25- 50 6.981e-07 5.991e-08
50-150 1.388e-06 1.537e-07
15-150 2.246e-06 1.747e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-21.5273 -200)
Norm : 1.99662 (-0.119523 0.119523)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.793e-07 2.746e-08
25- 50 7.296e-07 5.312e-08
50-150 1.600e-06 3.150e-07
15-150 2.709e-06 4.248e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.41807 (-1.46136 1.6327)
R1^2/D10^2 : 0.420879 (-0.202677 0.48986)
kT2 [keV] : 33.3554 (-7.07716 14.2305)
R2^2/D10^2 : 3.06541E-03 (-0.00199319 0.00371712)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.38 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 3.382e-07 7.738e-08
25- 50 7.033e-07 1.322e-07
50-150 1.923e-06 5.350e-07
15-150 2.964e-06 7.196e-07
Peak spectrum fit
Power-law model
Time interval is from 10.604 sec. to 11.604 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27607 ( -0.139841 0.139969 )
Norm@50keV : 3.89356E-02 ( -0.00322736 0.00321635 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.76 using 59 bins.
Reduced chi-squared = 0.837895
# Null hypothesis probability of 8.03e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.62530 ( -0.38142 0.38161 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87097e-07 ( -3.64582e-08 3.68289e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 10.604 sec. to 11.604 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.789672 ( -0.647067 0.537227 )
Epeak [keV] : 126.449 ( -46.2396 -126.447 )
Norm@50keV : 6.82252E-02 ( -0.0306082 0.0729005 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.61 using 59 bins.
Reduced chi-squared = 0.814464
# Null hypothesis probability of 8.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.53750 ( -0.39706 0.39498 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.72538e-07 ( -4.09109e-08 4.07093e-08 ) ergs/cm2
Band function
Time interval is from 10.604 sec. to 11.604 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] : 16.5178 (-1.65999 1.90525)
R^2/D10^2 : 0.398173 (-0.122234 0.170655)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.229e-08 3.535e-09
25- 50 9.636e-08 1.115e-08
50-150 1.859e-07 3.135e-08
15-150 3.046e-07 3.420e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-25.0946 -200)
Norm : 18.9117 (-1.56043 1.56043)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.708e-08 4.775e-09
25- 50 9.057e-08 1.330e-08
50-150 1.986e-07 9.054e-08
15-150 3.363e-07 1.073e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.49725 (-2.88224 3.5894)
R1^2/D10^2 : 2.12251 (-1.25626 5.22811)
kT2 [keV] : 29.4361 (-8.24295 46.7016)
R2^2/D10^2 : 4.41179E-02 (-0.0411381 0.103912)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.97e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.493e-08 1.457e-08
25- 50 9.300e-08 3.797e-08
50-150 2.461e-07 1.216e-07
15-150 3.740e-07 1.678e-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: 1.27911 ( -0.123314 0.122258 )
Norm@50keV : 9.26906E-03 ( -0.000632028 0.000632026 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.46e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 14.72 sec: 1.10169 ( -0.0785812 0.0787797 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.35527e-06 ( -1.01271e-07 1.01817e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.894765 ( -0.546417 0.433839 )
Epeak [keV] : 155.172 ( -61.4172 -155.172 )
Norm@50keV : 1.40438E-02 ( -0.00509446 0.0107908 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 14.72 sec: 1.07887 ( -0.082325 0.08374 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32057e-06 ( -1.12121e-07 1.11513e-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) = 6.88e-07
S(50-100 keV) = 1.04e-06
T90 vs. Hardness ratio plot
T90 = 61.539999961853 sec.
Hardness ratio (energy fluence ratio) = 1.51163
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.41991
Count Ratio (50-100 keV) / (15-25 keV) = 1.08498
Mask shadow pattern
IMX = 1.212068208750919E-02, IMY = 2.988785134397000E-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:
-239.952000 0.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4371 35.3663 39.9 40.1 126.3 -0.5644 -0.3 1.8 Her X-1
288.8377 10.9396 9.3 32.4 57.4 -1.0890 -1.2 2.3 GRS 1915+105
299.5911 35.1774 1.3 6.5 72.6 4.7822 9.1 1.5 Cyg X-1
308.1298 41.0187 3.2 2.4 -95.5 1.8530 3.7 4.1 Cyg X-3
326.3499 38.2062 6.1 16.3 -65.3 1.2268 1.9 10.9 Cyg X-2
299.4221 31.0375 2.5 10.0 56.7 2.3356 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.024000 14.748600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5114 35.3919 35.0 40.0 126.3 -0.0632 -0.3 4.0 Her X-1
288.8190 10.8041 8.4 32.5 57.3 0.1605 1.4 8.6 GRS 1915+105
299.4056 35.1640 11.0 6.6 73.4 0.0813 1.1 9.3 Cyg X-1
307.8985 41.0451 4.8 2.3 -98.2 0.1807 2.4 11.1 Cyg X-3
326.0781 38.1546 4.2 16.1 -65.0 0.2453 2.7 11.0 Cyg X-2
326.9859 44.5141 0.5 16.7 -87.7 2.1132 23.0 ------ UNKNOWN
350.5887 58.5514 2.6 34.1 -112.7 0.7540 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.348600 962.200500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5943 35.2086 1.4 22.8 78.3 15.9787 8.2 0.5 Cyg X-1
308.1898 40.9253 3.6 14.2 84.8 5.9732 3.2 4.0 Cyg X-3
326.1363 38.2360 5.9 6.3 8.9 -3.3918 -2.0 5.4 Cyg X-2
288.7819 32.8946 2.6 31.6 84.6 12.9418 4.4 ------ UNKNOWN
320.4158 -9.5274 2.4 54.4 10.9 21.6330 4.9 ------ UNKNOWN
352.8039 -5.6319 3.3 55.3 -29.0 23.7850 3.6 547.7 UNKNOWN
357.6471 4.1314 3.5 48.5 -39.9 16.4013 3.3 285.2 UNKNOWN
Plot creation:
Fri Jun 16 09:06:45 EDT 2023