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
193.3326 19.2107 0.0238 2.1128 -13.4780 0.0777405 7.985 TRIG_01061687
Foreground time interval of the image:
-0.004 0.424 (delta_t = 0.428 [sec])
Background time interval of the image:
-26.835 -0.004 (delta_t = 26.831 [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 0.512000
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 0.512000
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 0.512000
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 -0.004 sec. to 0.424 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51578 ( -0.335594 0.352783 )
Norm@50keV : 1.06356E-02 ( -0.00242175 0.00237018 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.23 using 59 bins.
Reduced chi-squared = 1.00404
# Null hypothesis probability of 4.67e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.428 sec: 1.33349 ( -0.28158 0.28163 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.30799e-08 ( -1.05552e-08 1.07426e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.004 sec. to 0.424 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.906373 ( -1.68604 0.915172 )
Epeak [keV] : 85.7934 ( -38.1719 -85.7934 )
Norm@50keV : 2.25489E-02 ( -0.0140209 0.154614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.61 using 59 bins.
Reduced chi-squared = 1.01089
# Null hypothesis probability of 4.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.428 sec: 1.32056 ( -0.28403 0.28346 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.147e-08 ( -1.11769e-08 1.13568e-08 ) ergs/cm2
Band function
Time interval is from -0.004 sec. to 0.424 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] : 14.0066 (-3.49696 4.51305)
R^2/D10^2 : 0.200635 (-0.12491 0.340573)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.21e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.559e-09 1.418e-09
25- 50 1.324e-08 4.267e-09
50-150 1.711e-08 8.712e-09
15-150 3.391e-08 1.285e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.338 (-117.553 -199.349)
Norm : 5.49265 (-1.15358 1.15452)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.83e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.854e-09 3.510e-09
25- 50 1.126e-08 6.559e-09
50-150 2.470e-08 1.432e-08
15-150 4.181e-08 2.437e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.93181 (-3.78323 5.35211)
R1^2/D10^2 : 1.40331 (-1.15978 26.3722)
kT2 [keV] : 23.7745 (-20.5799 -23.6617)
R2^2/D10^2 : 2.31140E-02 (-0.0232699 0.125866)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.32e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.586e-09 3.266e-09
25- 50 1.167e-08 6.165e-09
50-150 2.420e-08 1.510e-08
15-150 4.146e-08 2.159e-08
Peak spectrum fit
Power-law model
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68200 ( -0.442646 0.491058 )
Norm@50keV : 4.86992E-03 ( -0.0015699 0.00149984 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.31 using 59 bins.
Reduced chi-squared = 0.882632
# Null hypothesis probability of 7.22e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.642790 ( -0.172965 0.172974 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.51627e-08 ( -1.47139e-08 1.54174e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.840585 ( -3.29753 1.35379 )
Epeak [keV] : 57.7464 ( -57.7449 -57.7449 )
Norm@50keV : 1.50966E-02 ( -0.0150978 1.75554 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.80 using 59 bins.
Reduced chi-squared = 0.889286
# Null hypothesis probability of 7.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.630264 ( -0.175298 0.17579 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.12715e-08 ( -1.56208e-08 1.77486e-08 ) ergs/cm2
Band function
Time interval is from -0.288 sec. to 0.712 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] : 10.8549 (-3.00353 4.39842)
R^2/D10^2 : 0.235626 (-0.167582 0.521307)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.785e-09 3.541e-09
25- 50 1.608e-08 7.668e-09
50-150 1.059e-08 7.611e-09
15-150 3.246e-08 1.785e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 121.197 (-74.2999 -119.483)
Norm : 2.76145 (-0.805192 1.22885)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.36e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.190e-09 4.263e-09
25- 50 1.288e-08 7.485e-09
50-150 2.311e-08 1.664e-08
15-150 4.318e-08 2.822e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.20369 (-7.56291 5.45373)
R1^2/D10^2 : 0.714816 (-0.646959 -0.646959)
kT2 [keV] : 22.4016 (-26.2854 -26.2854)
R2^2/D10^2 : 9.69041E-03 (-0.00571901 0.35058)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.89e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.026e-09 4.458e-09
25- 50 1.364e-08 7.900e-09
50-150 1.952e-08 1.236e-08
15-150 4.018e-08 2.299e-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: 1.51578 ( -0.335594 0.352783 )
Norm@50keV : 1.06356E-02 ( -0.00242175 0.00237018 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.67e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.428 sec: 1.33346 ( -0.281572 0.281616 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.30743e-08 ( -1.05498e-08 1.076e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.906371 ( -1.68604 0.915173 )
Epeak [keV] : 85.7933 ( -38.1718 -85.7933 )
Norm@50keV : 2.25489E-02 ( -0.0140209 0.154614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.428 sec: 1.32042 ( -0.28075 0.28341 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.14857e-08 ( -1.11781e-08 1.13621e-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) = 1.07e-08
S(50-100 keV) = 1.50e-08
T90 vs. Hardness ratio plot
T90 = 0.383999943733215 sec.
Hardness ratio (energy fluence ratio) = 1.40187
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.94039
Count Ratio (50-100 keV) / (15-25 keV) = 1.42941
Mask shadow pattern
IMX = 3.587654926147974E-02, IMY = 8.598641932710489E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-26.835400 -0.004000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
241.8080 55.4600 2.4 53.2 8.1 1.1855 4.9 ------ UNKNOWN
161.8745 -12.7998 2.3 42.9 -156.4 0.5670 5.0 ------ UNKNOWN
156.9122 58.8761 2.3 49.3 -47.7 1.7872 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.004000 0.424000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
199.0303 11.9725 2.2 7.8 106.2 0.0506 5.2 ------ UNKNOWN
193.3326 19.2107 1.4 2.1 -13.5 0.0777 8.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
40.364610 962.915500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
215.5306 24.2845 2.8 21.2 60.0 4.3589 4.2 ------ UNKNOWN
242.4043 64.1502 3.2 55.5 11.4 19.9818 3.6 ------ UNKNOWN
166.5720 -32.3904 2.9 57.6 -165.4 21.1502 3.9 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:53:02 EDT 2022