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
85.5833 14.0101 0.0122 12.6026 -69.3460 4.1774770 15.843 TRIG_01104842
Foreground time interval of the image:
-1.208 224.200 (delta_t = 225.408 [sec])
Background time interval of the image:
-239.288 -1.208 (delta_t = 238.080 [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 -1.208 sec. to 224.200 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54212 ( -0.129692 0.131272 )
Norm@50keV : 1.09259E-03 ( -8.63192e-05 8.5814e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.34 using 59 bins.
Reduced chi-squared = 0.918246
# Null hypothesis probability of 6.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 225.4 sec: 0.138006 ( -0.010475 0.010483 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32137e-06 ( -1.99623e-07 2.01841e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.208 sec. to 224.200 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.637833 ( -0.659982 0.575051 )
Epeak [keV] : 72.3096 ( -13.5687 43.548 )
Norm@50keV : 3.21493E-03 ( -0.00157032 0.00374097 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.64 using 59 bins.
Reduced chi-squared = 0.797143
# Null hypothesis probability of 8.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 225.4 sec: 0.132342 ( -0.011049 0.011049 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.14894e-06 ( -2.20242e-07 2.25954e-07 ) ergs/cm2
Band function
Time interval is from -1.208 sec. to 224.200 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] : 14.1687 (-1.21599 1.34978)
R^2/D10^2 : 1.92541E-02 (-0.00533905 0.00726282)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.10e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.838e-07 2.759e-08
25- 50 6.918e-07 6.897e-08
50-150 9.200e-07 1.365e-07
15-150 1.796e-06 1.739e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 187.477 (-62.1342 -189.703)
Norm : 0.565549 (-0.0432278 0.0474471)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.175e-07 5.804e-08
25- 50 6.103e-07 1.732e-07
50-150 1.336e-06 6.311e-07
15-150 2.264e-06 8.572e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.23059 (-2.26071 2.77252)
R1^2/D10^2 : 0.166132 (-0.109854 0.73041)
kT2 [keV] : 19.6369 (-3.45217 7.18573)
R2^2/D10^2 : 4.93062E-03 (-0.00358706 0.00591495)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.39e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.867e-07 1.329e-07
25- 50 6.295e-07 2.378e-07
50-150 1.191e-06 4.503e-07
15-150 2.107e-06 8.215e-07
Peak spectrum fit
Power-law model
Time interval is from 4.276 sec. to 5.276 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.742282 ( -0.233725 0.220316 )
Norm@50keV : 1.06849E-02 ( -0.00150641 0.00148203 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.05 using 59 bins.
Reduced chi-squared = 1.10614
# Null hypothesis probability of 2.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.23142 ( -0.16577 0.16654 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28009e-07 ( -1.74205e-08 1.74866e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 4.276 sec. to 5.276 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.668976 ( -1.71753 1.20363 )
Epeak [keV] : 117.054 ( -32.5497 282.742 )
Norm@50keV : 3.95915E-02 ( -0.0395939 0.134366 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.91 using 59 bins.
Reduced chi-squared = 1.05196
# Null hypothesis probability of 3.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.16766 ( -0.177146 0.17648 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21719e-07 ( -1.96086e-08 1.90477e-08 ) ergs/cm2
Band function
Time interval is from 4.276 sec. to 5.276 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] : 25.3575 (-3.77262 5.00302)
R^2/D10^2 : 3.12850E-02 (-0.0130149 0.0199225)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.83e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.468e-09 9.345e-10
25- 50 1.982e-08 4.480e-09
50-150 9.429e-08 2.091e-08
15-150 1.176e-07 2.418e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-23.8168 -200)
Norm : 4.79335 (-0.694179 0.694179)
------------------------------------------------------------
#Fit statistic : Chi-Squared 96.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.60e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.194e-08 6.720e-09
25- 50 2.296e-08 1.312e-08
50-150 5.036e-08 2.801e-08
15-150 8.527e-08 4.853e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.33953 (-2.33302 6.44999)
R1^2/D10^2 : 67.7658 (-68.7801 -68.7801)
kT2 [keV] : 26.2554 (-4.0742 5.5601)
R2^2/D10^2 : 2.78242E-02 (-0.0121507 0.018859)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.79e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.826e-09 1.227e-09
25- 50 2.331e-08 5.035e-09
50-150 7.730e-08 1.802e-08
15-150 1.054e-07 2.204e-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: 1.54212 ( -0.129692 0.131272 )
Norm@50keV : 1.09259E-03 ( -8.63192e-05 8.5814e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 225.4 sec: 0.138002 ( -0.0104738 0.0104826 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32103e-06 ( -1.99806e-07 2.01879e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.637832 ( -0.659981 0.575052 )
Epeak [keV] : 72.3096 ( -13.5687 43.5481 )
Norm@50keV : 3.21493E-03 ( -0.00157033 0.00374097 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 225.4 sec: 0.132329 ( -0.011046 0.011046 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.1497e-06 ( -2.20439e-07 2.26155e-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) = 5.86e-07
S(50-100 keV) = 8.05e-07
T90 vs. Hardness ratio plot
T90 = 202.239999890327 sec.
Hardness ratio (energy fluence ratio) = 1.37372
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.57617
Count Ratio (50-100 keV) / (15-25 keV) = 1.04205
Mask shadow pattern
IMX = 7.885979576074158E-02, IMY = 2.092046966218329E-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:
-239.288000 -1.208000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6429 22.0295 0.5 18.3 -46.6 9.5155 23.7 1.1 Crab
104.6144 53.6492 2.2 44.4 4.9 3.2986 5.3 ------ UNKNOWN
95.9713 66.5758 2.8 57.0 -1.7 5.3451 4.1 ------ UNKNOWN
79.0586 44.3165 3.1 38.3 -22.6 1.9587 3.7 ------ UNKNOWN
75.5600 -18.8239 2.7 35.8 -143.5 2.0755 4.3 ------ UNKNOWN
70.8724 -19.0891 3.0 39.0 -138.4 2.1619 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.208000 224.200000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6026 22.1032 5.3 18.4 -46.5 -0.5526 -2.2 5.6 Crab
85.5833 14.0101 0.7 12.6 -69.3 4.1776 15.8 ------ UNKNOWN
67.1342 14.6940 2.1 30.2 -78.2 2.0125 5.5 ------ UNKNOWN
57.9159 58.6228 2.0 57.5 -24.2 8.6855 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Mon Oct 24 04:59:34 EDT 2022