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
162.4131 31.4929 0.0200 9.7303 -153.8313 0.8448659 9.581 TRIG_01081113
Foreground time interval of the image:
31.784 72.701 (delta_t = 40.917 [sec])
Background time interval of the image:
-239.000 31.784 (delta_t = 270.784 [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 64.000000
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 64.000000
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 64.000000
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 31.784 sec. to 139.704 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98602 ( -0.27755 0.303658 )
Norm@50keV : 7.27572E-04 ( -0.000144285 0.000138419 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.79 using 59 bins.
Reduced chi-squared = 0.69807
# Null hypothesis probability of 9.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 107.9 sec: 0.108448 ( -0.0147658 0.01477 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.23588e-07 ( -1.3058e-07 1.36477e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 31.784 sec. to 139.704 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.19018 ( -0.946129 0.103227 )
Epeak [keV] : 78.5456 ( )
Norm@50keV : 5.63432E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.58 using 59 bins.
Reduced chi-squared = 0.706786
# Null hypothesis probability of 9.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 107.9 sec: 9.82474E-02 ( -0.0274693 0.0250096 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.72313e-07 ( -1.5301e-07 1.5976e-07 ) ergs/cm2
Band function
Time interval is from 31.784 sec. to 139.704 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] : 8.85598 (-1.68067 2.11498)
R^2/D10^2 : 7.65990E-02 (-0.0762124 0.0958039)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.251e-07 2.967e-08
25- 50 2.593e-07 5.222e-08
50-150 9.412e-08 4.199e-08
15-150 4.785e-07 1.016e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.1834 (-27.2545 62.3404)
Norm : 0.530966 (-0.108454 0.152381)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.468e-07 2.644e-08
25- 50 2.328e-07 3.917e-08
50-150 2.964e-07 1.444e-07
15-150 6.760e-07 1.812e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.82966 (-1.45003 1.76193)
R1^2/D10^2 : 0.645767 (-0.454379 2.47679)
kT2 [keV] : 21.6783 (-7.46341 17.1379)
R2^2/D10^2 : 2.13450E-03 (-0.00181286 0.00581118)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.44e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.674e-07 9.247e-08
25- 50 1.939e-07 9.319e-08
50-150 3.740e-07 2.264e-07
15-150 7.352e-07 3.646e-07
Peak spectrum fit
Power-law model
Time interval is from 51.660 sec. to 52.660 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26425 ( -0.655677 0.636173 )
Norm@50keV : 3.96298E-03 ( -0.00126607 0.00123852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.38 using 59 bins.
Reduced chi-squared = 0.813684
# Null hypothesis probability of 8.41e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.469820 ( -0.147034 0.147512 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.95212e-08 ( -1.4389e-08 1.49228e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 51.660 sec. to 52.660 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28419 ( -0.68265 0.617443 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.94029E-03 ( -0.00126932 0.0181074 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.39 using 59 bins.
Reduced chi-squared = 0.828393
# Null hypothesis probability of 8.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.469777 ( -0.147337 0.147403 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.95039e-08 ( -1.86239e-08 1.93547e-08 ) ergs/cm2
Band function
Time interval is from 51.660 sec. to 52.660 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] : 16.7742 (-7.07504 20.8219)
R^2/D10^2 : 3.56522E-02 (-0.0343663 0.186412)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.94e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.050e-09 1.317e-09
25- 50 8.975e-09 5.685e-09
50-150 1.795e-08 1.235e-08
15-150 2.898e-08 1.825e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-126.538 -199.363)
Norm : 1.90758 (-0.601213 0.601225)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.750e-09 2.929e-09
25- 50 9.137e-09 5.890e-09
50-150 2.004e-08 1.231e-08
15-150 3.393e-08 2.066e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.29583 (-6.78416 7.89436)
R1^2/D10^2 : 0.297470 (-0.253802 875.432)
kT2 [keV] : 72.2058 (-80.8615 -80.8616)
R2^2/D10^2 : 5.29418E-04 (-0.000367126 0.0377261)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.95e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.021e-09 2.372e-09
25- 50 8.801e-09 5.615e-09
50-150 3.047e-08 1.805e-08
15-150 4.329e-08 2.130e-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: 2.01106 ( -0.286227 0.315261 )
Norm@50keV : 1.13508E-03 ( -0.000234704 0.000225358 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.49e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 40.92 sec: 0.171134 ( -0.0239551 0.0239607 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.28592e-07 ( -7.95444e-08 8.34768e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.18273 ( -1.10688 0.104893 )
Epeak [keV] : 77.1406 ( )
Norm@50keV : 9.11968E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 40.92 sec: 0.171023 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.26816e-07 ( -8.63265e-08 8.52405e-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) = 2.17e-07
S(50-100 keV) = 2.19e-07
T90 vs. Hardness ratio plot
T90 = 95.2640000581741 sec.
Hardness ratio (energy fluence ratio) = 1.00922
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.892132
Count Ratio (50-100 keV) / (15-25 keV) = 0.467153
Mask shadow pattern
IMX = -1.539010018946463E-01, IMY = 7.562433797807978E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-239.000000 31.784000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
108.1638 37.1498 2.3 41.4 102.4 5.2772 5.0 ------ UNKNOWN
175.1416 65.5345 3.0 43.0 175.6 2.1495 3.8 ------ UNKNOWN
200.6602 72.6407 3.3 54.2 178.7 3.8520 3.5 ------ UNKNOWN
212.1650 64.1429 2.9 54.0 -169.6 3.4114 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
31.784000 72.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
196.9254 77.7072 2.4 56.7 173.2 2.5673 4.7 ------ UNKNOWN
162.4131 31.4929 1.2 9.7 -153.8 0.8450 9.6 ------ UNKNOWN
173.1120 -22.9629 1.9 50.8 -38.7 2.0407 6.0 ------ UNKNOWN
181.3300 -14.4890 1.8 46.9 -53.1 2.4373 6.4 ------ UNKNOWN
214.4061 38.2832 2.8 51.9 -137.1 1.9781 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
111.300600 720.554000
721.000000 943.300610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
155.6534 78.7415 2.8 47.3 142.3 10.2734 4.2 ------ UNKNOWN
123.2831 -9.6193 3.1 55.6 12.9 19.6828 3.8 ------ UNKNOWN
150.7860 5.2214 3.0 28.5 -11.2 2.7860 3.8 ------ UNKNOWN
145.5574 -16.1265 2.9 50.3 -14.8 6.3449 4.0 ------ UNKNOWN
191.1748 22.6671 2.4 27.0 -113.9 4.5888 4.8 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:16:10 EDT 2022