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
47.0831 -19.3188 0.0086 19.4986 32.0722 3.8084303 22.326 TRIG_01116221
Foreground time interval of the image:
-47.800 9.853 (delta_t = 57.653 [sec])
Background time interval of the image:
-179.048 -47.800 (delta_t = 131.248 [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 -47.800 sec. to 45.748 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90924 ( -0.0654537 0.0660206 )
Norm@50keV : 5.18304E-03 ( -0.000172178 0.000171299 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.50 using 59 bins.
Reduced chi-squared = 0.798246
# Null hypothesis probability of 8.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 93.55 sec: 0.746802 ( -0.024864 0.02498 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.45896e-06 ( -1.45915e-07 1.46511e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -47.800 sec. to 45.748 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90907 ( -0.0659907 0.0660937 )
Epeak [keV] : 9999.28 ( -9999.35 -9999.36 )
Norm@50keV : 5.18578E-03 ( -0.00142886 0.00110149 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.51 using 59 bins.
Reduced chi-squared = 0.812679
# Null hypothesis probability of 8.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 93.55 sec: 0.751730 ( -0.029813 0.020048 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.49369e-06 ( -1.91362e-07 1.07536e-07 ) ergs/cm2
Band function
Time interval is from -47.800 sec. to 45.748 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] : 11.8391 ( )
R^2/D10^2 : 0.168185 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 319.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.46e-38 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.659e-07 2.849e-08
25- 50 1.443e-06 5.426e-08
50-150 1.205e-06 9.542e-08
15-150 3.114e-06 1.076e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 90.8143 (-10.7687 13.2651)
Norm : 3.24844 (-0.169686 0.187603)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.931e-07 4.626e-08
25- 50 1.344e-06 4.818e-08
50-150 2.058e-06 4.696e-07
15-150 4.195e-06 4.635e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.36379 (-0.530142 0.557338)
R1^2/D10^2 : 1.37717 (-0.377536 0.562823)
kT2 [keV] : 25.1342 (-2.79057 3.63362)
R2^2/D10^2 : 7.97957E-03 (-0.00301172 0.00430892)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.83e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.325e-07 7.919e-08
25- 50 1.314e-06 8.326e-08
50-150 2.274e-06 2.746e-07
15-150 4.420e-06 3.433e-07
Peak spectrum fit
Power-law model
Time interval is from 12.892 sec. to 13.892 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64781 ( -0.11165 0.113563 )
Norm@50keV : 2.94449E-02 ( -0.00196958 0.00195286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.80 using 59 bins.
Reduced chi-squared = 0.715789
# Null hypothesis probability of 9.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.84215 ( -0.23894 0.2391 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.73949e-07 ( -1.95649e-08 1.97483e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 12.892 sec. to 13.892 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44887 ( -0.462165 0.292979 )
Epeak [keV] : 131.456 ( -62.4369 -131.458 )
Norm@50keV : 3.75032E-02 ( -0.00973007 0.0276511 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.16 using 59 bins.
Reduced chi-squared = 0.717143
# Null hypothesis probability of 9.45e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.80617 ( -0.25068 0.25043 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.68955e-07 ( -2.23738e-08 2.21971e-08 ) ergs/cm2
Band function
Time interval is from 12.892 sec. to 13.892 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] : 12.5735 (-0.974992 1.08352)
R^2/D10^2 : 0.783622 (-0.202795 0.267227)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 100.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.60e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.627e-08 2.940e-09
25- 50 8.722e-08 6.130e-09
50-150 8.544e-08 1.223e-08
15-150 1.989e-07 1.545e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 152.561 (-40.8096 -152.179)
Norm : 15.8156 (-1.09711 1.27993)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.52e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.056e-08 3.585e-09
25- 50 7.537e-08 1.024e-08
50-150 1.498e-07 5.952e-08
15-150 2.657e-07 6.185e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.58766 (-1.30152 1.3315)
R1^2/D10^2 : 3.48727 (-1.40539 2.98335)
kT2 [keV] : 29.7359 (-7.02021 13.9471)
R2^2/D10^2 : 2.66163E-02 (-0.0187137 0.0437461)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.851e-08 8.665e-09
25- 50 7.820e-08 1.448e-08
50-150 1.548e-07 6.634e-08
15-150 2.715e-07 8.155e-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: 1.78520 ( -0.0979626 0.0993571 )
Norm@50keV : 3.73653E-03 ( -0.000203904 0.000201953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 57.65 sec: 0.511962 ( -0.0252754 0.0253367 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.98421e-06 ( -1.11236e-07 1.12364e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.78356 ( -0.146263 0.100651 )
Epeak [keV] : 9998.84 ( -9999.34 -9999.35 )
Norm@50keV : 3.74137E-03 ( -0.000205583 0.00147787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 57.65 sec: 0.511744 ( -0.025222 0.025271 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.9833e-06 ( -1.19687e-07 1.10803e-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) = 1.30e-06
S(50-100 keV) = 1.39e-06
T90 vs. Hardness ratio plot
T90 = 49.039999961853 sec.
Hardness ratio (energy fluence ratio) = 1.06923
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.07935
Count Ratio (50-100 keV) / (15-25 keV) = 0.608101
Mask shadow pattern
IMX = 3.000499177724512E-01, IMY = -1.880177922912658E-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:
-179.048000 -47.800000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6967 21.9831 6.1 39.5 -102.2 2.5538 1.9 4.0 Crab
72.4191 -27.8842 3.6 35.2 -12.0 1.5638 3.2 ------ UNKNOWN
58.9584 34.8267 2.1 35.9 -143.5 3.0515 5.5 ------ UNKNOWN
85.2533 -19.6583 3.1 39.7 -34.4 2.4389 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-47.800000 9.852600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6656 21.9975 3.6 39.5 -102.3 1.7127 3.3 2.1 Crab
10.9775 25.2815 3.3 45.4 150.7 1.6612 3.6 ------ UNKNOWN
25.5824 24.3932 2.7 34.0 161.5 0.9060 4.2 ------ UNKNOWN
47.0831 -19.3189 0.5 19.5 32.1 3.8083 22.3 ------ UNKNOWN
92.9719 0.5780 2.5 43.0 -67.0 3.2141 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.052590 178.652590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
7.8703 -6.0722 3.2 40.4 132.8 2.3631 3.7 595.7 UNKNOWN
9.5149 8.4101 2.9 46.3 152.4 2.7262 3.9 ------ UNKNOWN
35.8127 -53.0843 2.3 34.9 40.8 1.7661 5.1 ------ UNKNOWN
52.1352 -47.1919 2.2 28.2 21.7 1.2019 5.2 ------ UNKNOWN
25.6212 29.4226 2.9 53.0 -174.6 2.3236 3.9 ------ UNKNOWN
78.2218 -43.1341 3.2 35.3 -11.8 0.9251 3.6 ------ UNKNOWN
Plot creation:
Mon Oct 24 12:40:37 EDT 2022