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
153.3815 48.2611 0.0340 13.6249 -76.8270 0.2560387 5.646 TRIG_01165948
Foreground time interval of the image:
-0.512 6.448 (delta_t = 6.960 [sec])
Background time interval of the image:
-239.168 -0.512 (delta_t = 238.656 [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 2.048000
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 2.048000
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 2.048000
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 -0.512 sec. to 6.448 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07279 ( -0.478002 0.555557 )
Norm@50keV : 1.96611E-03 ( -0.00073225 0.000701504 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.01 using 59 bins.
Reduced chi-squared = 1.3686
# Null hypothesis probability of 3.38e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 6.96 sec: 0.305256 ( -0.078631 0.078658 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26849e-07 ( -4.09325e-08 4.41675e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.512 sec. to 6.448 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93682 ( )
Epeak [keV] : 17.0736 ( )
Norm@50keV : 2.40071E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.97 using 59 bins.
Reduced chi-squared = 1.39232
# Null hypothesis probability of 2.78e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 6.96 sec: 0.305108 ( -0.078218 0.078862 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23589e-07 ( -4.96147e-08 4.02435e-08 ) ergs/cm2
Band function
Time interval is from -0.512 sec. to 6.448 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] : 7.19066 (-1.91607 2.85117)
R^2/D10^2 : 0.508752 (-0.507649 1.29954)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.08e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.022e-08 1.556e-08
25- 50 4.357e-08 2.805e-08
50-150 7.950e-09 7.034e-09
15-150 8.174e-08 4.889e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.7683 (-28.9626 116.332)
Norm : 1.68542 (-0.627087 1.27327)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.25e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.902e-08 1.452e-08
25- 50 4.247e-08 2.156e-08
50-150 4.335e-08 3.124e-08
15-150 1.148e-07 5.658e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.59022 (-1.79676 2.37679)
R1^2/D10^2 : 1.19541 (-0.903923 4.68412)
kT2 [keV] : 27.7523 (-27.702 -27.8805)
R2^2/D10^2 : 2.12446E-03 (-0.00204409 0.0416587)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.25e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.285e-08 1.941e-08
25- 50 3.752e-08 1.925e-08
50-150 6.398e-08 4.388e-08
15-150 1.343e-07 7.305e-08
Peak spectrum fit
Power-law model
Time interval is from -0.252 sec. to 0.748 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82777 ( -0.513836 0.562772 )
Norm@50keV : 4.87108E-03 ( -0.00185346 0.00179538 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.15 using 59 bins.
Reduced chi-squared = 1.12544
# Null hypothesis probability of 2.40e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.678622 ( -0.213763 0.213766 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.48208e-08 ( -1.64253e-08 1.7524e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.252 sec. to 0.748 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.61081 ( )
Epeak [keV] : 27.8381 ( )
Norm@50keV : 8.46582E+05 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.69 using 59 bins.
Reduced chi-squared = 1.10161
# Null hypothesis probability of 2.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.585599 ( -0.180393 0.207004 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.49086e-08 ( -7.9929e-09 2.66772e-08 ) ergs/cm2
Band function
Time interval is from -0.252 sec. to 0.748 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] : 8.29453 (-2.10254 3.35455)
R^2/D10^2 : 0.694142 (-0.69414 1.47972)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.82e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.859e-09 5.320e-09
25- 50 1.649e-08 1.006e-08
50-150 4.871e-09 3.751e-09
15-150 3.022e-08 1.863e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 74.2880 (-44.5075 -74.288)
Norm : 3.32894 (-1.24969 2.242)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.60e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.590e-09 5.270e-09
25- 50 1.388e-08 8.545e-09
50-150 1.862e-08 1.642e-08
15-150 4.109e-08 2.772e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.17910 (-7.19091 3.05323)
R1^2/D10^2 : 1.06577 (-1.06469 2.91773)
kT2 [keV] : 36.5503 (-36.821 -36.821)
R2^2/D10^2 : 1.72113E-03 (-0.00170694 1.19652)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.82e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.368e-09 5.850e-09
25- 50 1.511e-08 9.555e-09
50-150 2.021e-08 1.175e-08
15-150 4.468e-08 2.203e-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: 2.07279 ( -0.478002 0.555557 )
Norm@50keV : 1.96611E-03 ( -0.00073225 0.000701504 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.38e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 6.96 sec: 0.305231 ( -0.0786262 0.0786528 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26827e-07 ( -4.0925e-08 4.40912e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05910 ( -0.86425 0.567403 )
Epeak [keV] : 9999.35 ( )
Norm@50keV : 1.98812E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.76e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 6.96 sec: 0.303514 ( -0.079606 0.079683 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23617e-07 ( -4.9551e-08 4.66417e-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) = 3.90e-08
S(50-100 keV) = 3.70e-08
T90 vs. Hardness ratio plot
T90 = 6.33599996566772 sec.
Hardness ratio (energy fluence ratio) = 0.948718
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.60429
Count Ratio (50-100 keV) / (15-25 keV) = 0.306578
Mask shadow pattern
IMX = 5.523776989566868E-02, IMY = 2.360075174023397E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.168000 -0.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
193.5468 17.5873 2.3 31.6 84.7 3.7621 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.512000 6.448000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
204.1236 15.0702 2.6 40.7 75.7 0.7325 4.5 ------ UNKNOWN
142.8362 -6.8745 2.3 50.0 172.4 0.5834 5.0 ------ UNKNOWN
153.3814 48.2611 2.0 13.6 -76.8 0.2561 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.332600 962.964500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.1996 29.0176 2.5 31.6 84.7 11.5015 4.6 ------ UNKNOWN
153.3234 14.8083 3.1 33.4 149.4 7.9548 3.7 ------ UNKNOWN
292.9662 70.5628 3.7 57.7 -15.8 15.5190 3.2 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:07:28 EDT 2023