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
4.8400 -48.0436 0.0044 33.6517 -134.2177 4.8647375 44.050 TRIG_01197311
Foreground time interval of the image:
-6.848 12.701 (delta_t = 19.549 [sec])
Background time interval of the image:
-239.600 -6.848 (delta_t = 232.752 [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 -6.848 sec. to 250.448 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38705 ( -0.0971427 0.0967608 )
Norm@50keV : 1.67784E-03 ( -8.93955e-05 8.93589e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.72 using 59 bins.
Reduced chi-squared = 0.977544
# Null hypothesis probability of 5.23e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 257.3 sec: 0.203741 ( -0.011428 0.011461 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.18311e-06 ( -2.42711e-07 2.43795e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.848 sec. to 250.448 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37320 ( -0.341149 0.099298 )
Epeak [keV] : 9930.27 ( -9999.36 -9999.36 )
Norm@50keV : 1.70310E-03 ( -8.96053e-05 0.000714042 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.87 using 59 bins.
Reduced chi-squared = 0.997679
# Null hypothesis probability of 4.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 257.3 sec: 0.203997 ( -0.012474 0.011665 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.18967e-06 ( -2.72702e-07 2.02307e-07 ) ergs/cm2
Band function
Time interval is from -6.848 sec. to 250.448 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] : 17.0290 ( )
R^2/D10^2 : 1.48640E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 149.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.71e-10 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.258e-07 2.619e-08
25- 50 1.000e-06 8.259e-08
50-150 2.072e-06 2.043e-07
15-150 3.298e-06 2.264e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-15.7392 -200)
Norm : 0.846203 (-0.0452541 0.0452541)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.421e-07 3.023e-08
25- 50 1.043e-06 6.497e-08
50-150 2.287e-06 3.759e-07
15-150 3.872e-06 2.856e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.70173 (-1.30333 1.48159)
R1^2/D10^2 : 0.152699 (-0.0660157 0.13408)
kT2 [keV] : 33.2436 (-6.26878 11.6319)
R2^2/D10^2 : 1.29737E-03 (-0.000775909 0.00131919)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.03e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.632e-07 7.668e-08
25- 50 1.017e-06 1.537e-07
50-150 2.739e-06 7.193e-07
15-150 4.219e-06 1.031e-06
Peak spectrum fit
Power-law model
Time interval is from -0.076 sec. to 0.924 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14325 ( -0.0784511 0.0780846 )
Norm@50keV : 8.25499E-02 ( -0.00379928 0.00379875 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.80 using 59 bins.
Reduced chi-squared = 0.978947
# Null hypothesis probability of 5.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.473115 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.51628e-07 ( -4.30722e-08 4.32009e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.076 sec. to 0.924 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.606252 ( -0.357336 0.330102 )
Epeak [keV] : 145.042 ( -36.884 134.506 )
Norm@50keV : 0.145644 ( -0.0420186 0.0644659 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.75 using 59 bins.
Reduced chi-squared = 0.852679
# Null hypothesis probability of 7.76e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 9.42416 ( -0.47077 0.47071 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90766e-07 ( -2.88387e-08 2.40467e-08 ) ergs/cm2
Band function
Time interval is from -0.076 sec. to 0.924 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] : 19.5176 (-1.12102 1.21352)
R^2/D10^2 : 0.496344 (-0.089104 0.106488)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 107.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.48e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.680e-08 3.335e-09
25- 50 1.803e-07 1.110e-08
50-150 5.073e-07 4.330e-08
15-150 7.244e-07 3.950e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 39.6196 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 124.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.50e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.866e-08 4.935e-09
25- 50 1.898e-07 9.050e-09
50-150 4.162e-07 2.270e-08
15-150 7.047e-07 3.930e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.52586 (-2.44594 2.66304)
R1^2/D10^2 : 2.67729 (-1.19419 3.39903)
kT2 [keV] : 32.2874 (-6.36692 15.2269)
R2^2/D10^2 : 7.57423E-02 (-0.0539508 0.0919651)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.38e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.037e-08 1.183e-08
25- 50 1.875e-07 3.825e-08
50-150 5.849e-07 1.512e-07
15-150 8.327e-07 2.173e-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: 1.40727 ( -0.0588465 0.0588206 )
Norm@50keV : 1.73919E-02 ( -0.000562581 0.000562574 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 19.55 sec: 2.12154 ( -0.0738243 0.0739837 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.28057e-06 ( -1.13556e-07 1.13755e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15479 ( -0.246158 0.233147 )
Epeak [keV] : 183.557 ( -64.2596 1074.57 )
Norm@50keV : 2.27661E-02 ( -0.0048678 0.00662773 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.72e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 19.55 sec: 2.08953 ( -0.079 0.07925 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.23332e-06 ( -1.23282e-07 1.22696e-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) = 9.78e-07
S(50-100 keV) = 1.49e-06
T90 vs. Hardness ratio plot
T90 = 151.488000035286 sec.
Hardness ratio (energy fluence ratio) = 1.52352
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.54262
Count Ratio (50-100 keV) / (15-25 keV) = 1.29454
Mask shadow pattern
IMX = -4.642506576847473E-01, IMY = 4.771047898462376E-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:
-239.600000 -6.848000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
52.6470 -30.1047 2.9 45.7 162.8 3.3520 4.1 ------ UNKNOWN
312.7461 2.2456 2.2 55.2 -32.3 9.2798 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.848000 12.700590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
334.8134 30.1612 2.3 53.7 10.9 1.9574 5.0 ------ UNKNOWN
60.7956 -46.0940 2.9 55.6 -178.9 1.2162 4.0 ------ UNKNOWN
326.8634 14.1058 2.8 48.0 -10.7 0.6643 4.0 ------ UNKNOWN
60.2243 -56.8071 2.2 58.9 -166.8 2.7479 5.3 ------ UNKNOWN
315.7638 16.8041 2.1 58.5 -15.0 2.6172 5.5 ------ UNKNOWN
4.8400 -48.0436 0.3 33.7 -134.2 4.8643 44.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
83.500600 962.531700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
76.2666 -48.5982 3.3 45.7 162.8 10.6251 3.5 ------ UNKNOWN
113.9720 -68.9348 3.5 52.0 -161.5 9.9853 3.3 ------ UNKNOWN
Plot creation:
Tue Dec 26 17:00:33 EST 2023