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
121.7209 -32.8937 0.0035 31.3072 -15.3239 5.9106283 54.961 TRIG_01061284
Foreground time interval of the image:
-4.588 15.565 (delta_t = 20.153 [sec])
Background time interval of the image:
-239.336 -4.588 (delta_t = 234.748 [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 -4.588 sec. to 612.796 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64963 ( -0.0983616 0.0994708 )
Norm@50keV : 1.07438E-03 ( -5.99789e-05 5.9693e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.31 using 59 bins.
Reduced chi-squared = 1.1107
# Null hypothesis probability of 2.64e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 617.4 sec: 0.140275 ( -0.007725 0.00774 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.17016e-06 ( -3.65635e-07 3.68317e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.588 sec. to 612.796 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26114 ( -0.423607 0.387055 )
Epeak [keV] : 94.8909 ( -26.4307 2079.13 )
Norm@50keV : 1.68193E-03 ( -0.000592364 0.001028 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.37 using 59 bins.
Reduced chi-squared = 1.07804
# Null hypothesis probability of 3.21e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 617.4 sec: 0.137011 ( -0.008358 0.008363 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.97801e-06 ( -4.11713e-07 4.13397e-07 ) ergs/cm2
Band function
Time interval is from -4.588 sec. to 612.796 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] : 14.3682 ( )
R^2/D10^2 : 1.75646E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 129.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.52e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.716e-07 4.918e-08
25- 50 1.799e-06 1.269e-07
50-150 2.478e-06 2.544e-07
15-150 4.749e-06 3.031e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 158.048 (-38.4266 -157.457)
Norm : 0.572853 (-0.0344269 0.0413732)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.50e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.042e-07 6.977e-08
25- 50 1.688e-06 1.818e-07
50-150 3.404e-06 1.097e-06
15-150 5.997e-06 1.420e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.12213 (-0.989327 1.18099)
R1^2/D10^2 : 0.442185 (-0.245219 0.682732)
kT2 [keV] : 19.9690 (-2.17956 2.9575)
R2^2/D10^2 : 4.61291E-03 (-0.00191049 0.00259778)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.54e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.496e-07 2.878e-07
25- 50 1.596e-06 2.294e-07
50-150 3.245e-06 4.519e-07
15-150 5.791e-06 8.532e-07
Peak spectrum fit
Power-law model
Time interval is from 2.684 sec. to 3.684 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14438 ( -0.138675 0.136796 )
Norm@50keV : 2.45922E-02 ( -0.00215661 0.00215625 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.82 using 59 bins.
Reduced chi-squared = 1.11965
# Null hypothesis probability of 2.49e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.86605 ( -0.25714 0.25745 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.53618e-07 ( -2.41141e-08 2.42573e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.684 sec. to 3.684 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.172854 ( -0.690651 0.591316 )
Epeak [keV] : 101.476 ( -22.5747 72.3258 )
Norm@50keV : 7.14862E-02 ( -0.0334326 0.0763619 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.24 using 59 bins.
Reduced chi-squared = 0.986429
# Null hypothesis probability of 5.04e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.79812 ( -0.26151 0.26148 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.42633e-07 ( -2.59823e-08 2.58396e-08 ) ergs/cm2
Band function
Time interval is from 2.684 sec. to 3.684 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] : 18.8891 (-1.93234 2.20551)
R^2/D10^2 : 0.168876 (-0.0517268 0.07245)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.65e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.187e-08 1.991e-09
25- 50 5.685e-08 7.515e-09
50-150 1.489e-07 2.200e-08
15-150 2.176e-07 2.440e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-18.3434 -200)
Norm : 11.7883 (-1.06165 1.06165)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.51e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.935e-08 2.930e-09
25- 50 5.645e-08 1.518e-08
50-150 1.238e-07 5.486e-08
15-150 2.096e-07 8.068e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.48413 (-3.0948 4.6236)
R1^2/D10^2 : 0.801426 (-0.478748 1.53709)
kT2 [keV] : 29.1091 (-7.06424 40.0025)
R2^2/D10^2 : 3.09103E-02 (-0.0289173 0.0579057)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.31e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.856e-08 8.855e-09
25- 50 5.854e-08 2.983e-08
50-150 1.687e-07 8.644e-08
15-150 2.458e-07 1.154e-07
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: 1.25990 ( -0.0476731 0.0475778 )
Norm@50keV : 2.00257E-02 ( -0.000534932 0.000534713 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 20.15 sec: 2.37235 ( -0.068203 0.0683479 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02794e-06 ( -1.12791e-07 1.12919e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.627665 ( -0.223946 0.213528 )
Epeak [keV] : 127.493 ( -18.6364 34.7042 )
Norm@50keV : 3.74414E-02 ( -0.00695739 0.00896613 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 20.15 sec: 2.28171 ( -0.07331 0.07358 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.91958e-06 ( -1.20557e-07 1.20255e-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) = 1.64e-06
S(50-100 keV) = 2.09e-06
T90 vs. Hardness ratio plot
T90 = 55.0639998912811 sec.
Hardness ratio (energy fluence ratio) = 1.27439
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28405
Count Ratio (50-100 keV) / (15-25 keV) = 0.937418
Mask shadow pattern
IMX = 5.865584203005796E-01, IMY = 1.607272149705196E-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:
-239.336000 -4.588000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6056 22.0157 0.6 41.6 -147.2 10.4168 19.7 1.5 Crab
135.3912 -40.6232 8.9 44.0 -8.5 0.6430 1.3 7.5 Vela X-1
67.5005 14.5693 3.1 40.4 -173.2 1.6521 3.7 ------ UNKNOWN
149.8326 -33.2996 4.3 54.6 -20.0 2.5869 2.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.588000 15.564600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6287 22.0225 369.4 41.6 -147.2 -0.0050 -0.0 0.5 Crab
135.5550 -40.4425 4.2 44.1 -8.8 0.4431 2.8 6.8 Vela X-1
67.5607 -26.6406 2.6 22.2 108.0 0.4924 4.4 ------ UNKNOWN
121.7209 -32.8937 0.2 31.3 -15.3 5.9107 55.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
78.164590 962.716300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5179 -40.5792 1.2 13.4 37.4 6.9872 9.6 1.5 Vela X-1
170.1161 -60.6306 5.7 41.7 55.0 4.0549 2.0 5.9 Cen X-3
119.7678 -0.9425 2.6 32.0 -95.3 5.6908 4.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:55:07 EDT 2022