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
16.5535 -47.7114 0.0136 25.1025 -17.1819 0.8424297 14.143 TRIG_01161127
Foreground time interval of the image:
-3.072 11.320 (delta_t = 14.392 [sec])
Background time interval of the image:
-239.864 -3.072 (delta_t = 236.792 [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 -3.072 sec. to 11.320 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.10335 ( -0.251012 0.272778 )
Norm@50keV : 2.82832E-03 ( -0.000495423 0.000475503 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.32 using 59 bins.
Reduced chi-squared = 0.865263
# Null hypothesis probability of 7.55e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 14.39 sec: 0.445744 ( -0.054118 0.054129 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.7833e-07 ( -5.75256e-08 5.92429e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.072 sec. to 11.320 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.22170 ( -0.512639 0.0260408 )
Epeak [keV] : 94.7499 ( )
Norm@50keV : 2.35289E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.76 using 59 bins.
Reduced chi-squared = 0.870714
# Null hypothesis probability of 7.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 14.39 sec: 0.392704 ( -0.11046 0.097471 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.8295e-07 ( -6.19454e-08 6.39818e-08 ) ergs/cm2
Band function
Time interval is from -3.072 sec. to 11.320 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] : 8.44933 (-1.28353 1.54658)
R^2/D10^2 : 0.377296 (-0.181944 0.349717)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.74e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.277e-08 1.531e-08
25- 50 1.397e-07 2.748e-08
50-150 4.378e-08 1.651e-08
15-150 2.563e-07 4.605e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 58.0613 (-19.6805 37.1719)
Norm : 2.33061 (-0.489128 0.655323)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.382e-08 1.276e-08
25- 50 1.263e-07 1.883e-08
50-150 1.398e-07 5.057e-08
15-150 3.499e-07 6.404e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.81375 (-1.66628 1.59072)
R1^2/D10^2 : 1.39657 (-0.842044 1.65839)
kT2 [keV] : 29.0863 (-12.4984 52.0038)
R2^2/D10^2 : 2.69270E-03 (-0.0024913 0.0177987)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.46e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.136e-08 3.870e-08
25- 50 1.120e-07 3.949e-08
50-150 1.988e-07 1.149e-07
15-150 4.021e-07 1.703e-07
Peak spectrum fit
Power-law model
Time interval is from 0.020 sec. to 1.020 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.14401 ( -0.339978 0.388553 )
Norm@50keV : 6.63864E-03 ( -0.00179891 0.00174122 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.46 using 59 bins.
Reduced chi-squared = 1.28877
# Null hypothesis probability of 7.01e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.06780 ( -0.208043 0.20804 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.19812e-08 ( -1.45461e-08 1.51464e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.020 sec. to 1.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.457600 ( -2.24824 1.54763 )
Epeak [keV] : 36.7594 ( -32.4586 16.3248 )
Norm@50keV : 6.58539E-02 ( -0.0658794 1.31726 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.38 using 59 bins.
Reduced chi-squared = 1.25679
# Null hypothesis probability of 9.36e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.03042 ( -0.208087 0.20947 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57905e-08 ( -1.30066e-08 1.52474e-08 ) ergs/cm2
Band function
Time interval is from 0.020 sec. to 1.020 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] : 9.88548 (-1.85853 2.12843)
R^2/D10^2 : 0.544995 (-0.290709 0.661963)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.00e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.080e-08 3.722e-09
25- 50 2.642e-08 1.000e-08
50-150 1.334e-08 6.722e-09
15-150 5.056e-08 1.644e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 50.9835 (-19.2916 40.1648)
Norm : 6.11119 (-1.67773 2.44436)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.99e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.501e-08 3.903e-09
25- 50 2.170e-08 6.375e-09
50-150 2.146e-08 1.168e-08
15-150 5.817e-08 1.762e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.230837 (-0.351128 1.84256)
R1^2/D10^2 : 5.81763E+22 (-6.62217e+22 -6.62359e+22)
kT2 [keV] : 10.3486 (-1.8978 2.22987)
R2^2/D10^2 : 0.444633 (-0.237614 0.520137)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.13e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.426e-08 7.200e-09
25- 50 2.305e-08 1.278e-08
50-150 1.794e-08 1.187e-08
15-150 5.525e-08 2.947e-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: 2.10335 ( -0.251012 0.272778 )
Norm@50keV : 2.82832E-03 ( -0.000495423 0.000475503 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.55e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 14.39 sec: 0.445705 ( -0.0541127 0.0541241 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78258e-07 ( -5.75157e-08 5.92441e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.49882 ( -0.749111 0.238376 )
Epeak [keV] : 180.594 ( )
Norm@50keV : 1.78319E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.64e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 14.39 sec: 0.445796 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.77468e-07 ( -5.68707e-08 5.9989e-08 ) 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) = 1.17e-07
S(50-100 keV) = 1.09e-07
T90 vs. Hardness ratio plot
T90 = 11.7999999523163 sec.
Hardness ratio (energy fluence ratio) = 0.931624
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.890497
Count Ratio (50-100 keV) / (15-25 keV) = 0.440829
Mask shadow pattern
IMX = 4.475793670390039E-01, IMY = 1.383939603464624E-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:
-239.864000 -3.072000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.0974 -24.8729 6.0 48.5 146.1 4.4416 1.9 4.4 HT1900.1-2455
297.5562 -65.3667 2.2 31.6 84.6 3.3533 5.3 ------ UNKNOWN
352.8010 -5.6289 3.4 40.0 -109.0 3.9520 3.4 547.8 UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.072000 11.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
284.9192 -25.0299 3.7 48.5 145.8 0.7853 3.1 9.1 HT1900.1-2455
16.5535 -47.7115 0.8 25.1 -17.2 0.8425 14.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
96.036590 962.270700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
61.5099 -71.7626 2.6 31.6 84.6 9.2889 4.4 ------ UNKNOWN
54.7385 -5.6128 3.6 53.2 -20.3 10.0316 3.2 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:12:25 EDT 2023