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
9.7298 57.6337 0.0091 57.1930 -174.1937 14.3297439 20.988 TRIG_01202522
Foreground time interval of the image:
-7.040 21.120 (delta_t = 28.160 [sec])
Background time interval of the image:
-239.824 -7.040 (delta_t = 232.784 [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 2.048000
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 2.048000
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 2.048000
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 -7.040 sec. to 21.120 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03128 ( -0.0917248 0.0898922 )
Norm@50keV : 3.44510E-02 ( -0.00187769 0.0018622 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.81 using 59 bins.
Reduced chi-squared = 0.979123
# Null hypothesis probability of 5.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 28.16 sec: 3.97370 ( -0.2258 0.22679 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03777e-05 ( -5.24426e-07 5.24666e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -7.040 sec. to 21.120 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02503 ( -0.367008 0.106016 )
Epeak [keV] : 9999.99 ( -9999.99 -9999.99 )
Norm@50keV : 3.46515E-02 ( -0.00187888 0.00172177 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.81 using 59 bins.
Reduced chi-squared = 0.996607
# Null hypothesis probability of 4.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 28.16 sec: 3.97132 ( -0.23369 0.2282 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03818e-05 ( -5.19856e-07 5.12078e-07 ) ergs/cm2
Band function
Time interval is from -7.040 sec. to 21.120 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] : 24.9465 ( )
R^2/D10^2 : 9.48969E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 129.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.38e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.892e-07 3.110e-08
25- 50 1.639e-06 1.488e-07
50-150 7.566e-06 5.294e-07
15-150 9.494e-06 5.688e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 17.4997 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 163.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.31e-12 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.227e-06 7.124e-08
25- 50 2.360e-06 1.433e-07
50-150 5.177e-06 3.520e-07
15-150 8.765e-06 5.350e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.58521 (-2.00402 2.36911)
R1^2/D10^2 : 1.13195 (-0.533201 1.24978)
kT2 [keV] : 42.1176 (-7.79057 16.6284)
R2^2/D10^2 : 1.62114E-02 (-0.00983631 0.0145557)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.877e-07 1.721e-07
25- 50 2.070e-06 4.000e-07
50-150 7.718e-06 1.954e-06
15-150 1.048e-05 2.291e-06
Peak spectrum fit
Power-law model
Time interval is from 0.180 sec. to 1.180 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.919778 ( -0.219477 0.210331 )
Norm@50keV : 8.63562E-02 ( -0.01208 0.0119194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.97 using 59 bins.
Reduced chi-squared = 1.17491
# Null hypothesis probability of 1.72e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.102950 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.619e-07 ( -1.2818e-07 1.28284e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.180 sec. to 1.180 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.220065 ( -1.25958 0.9826 )
Epeak [keV] : 124.516 ( -34.5802 320.669 )
Norm@50keV : 0.244962 ( -0.143571 0.460534 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.97 using 59 bins.
Reduced chi-squared = 1.12446
# Null hypothesis probability of 2.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.35713E-02 ( -0.0235713 -0.0235713 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.54113e-07 ( -1.33591e-07 1.32238e-07 ) ergs/cm2
Band function
Time interval is from 0.180 sec. to 1.180 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] : 24.7798 (-3.51578 4.41618)
R^2/D10^2 : 0.265191 (-0.106902 0.165183)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.842e-08 7.885e-09
25- 50 1.605e-07 3.595e-08
50-150 7.317e-07 1.499e-07
15-150 9.206e-07 1.696e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-24.9424 -200)
Norm : 41.4686 (-5.81595 5.81595)
------------------------------------------------------------
#Fit statistic : Chi-Squared 90.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.15e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.033e-07 5.780e-08
25- 50 1.987e-07 1.128e-07
50-150 4.358e-07 2.425e-07
15-150 7.378e-07 4.135e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.1302 (-10.1557 -10.1557)
R1^2/D10^2 : 1.30184 (-1.29764 -1.29764)
kT2 [keV] : 30.6070 (-7.57052 -30.6235)
R2^2/D10^2 : 0.118771 (-0.118503 0.201726)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.20e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.452e-08 2.527e-08
25- 50 1.761e-07 9.370e-08
50-150 7.393e-07 3.962e-07
15-150 9.599e-07 4.878e-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: 1.03128 ( -0.0917248 0.0898922 )
Norm@50keV : 3.44510E-02 ( -0.00187769 0.0018622 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 28.16 sec: 3.97363 ( -0.225744 0.226832 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03767e-05 ( -5.24559e-07 5.24598e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02472 ( -0.366661 0.0908835 )
Epeak [keV] : 9809.35 ( -9690.91 -9690.91 )
Norm@50keV : 3.46524E-02 ( -0.00177866 0.0134864 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 28.16 sec: 3.96808 ( -0.23063 0.22998 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03864e-05 ( -5.16145e-07 5.19355e-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) = 1.96e-06
S(50-100 keV) = 3.83e-06
T90 vs. Hardness ratio plot
T90 = 22.0960000753403 sec.
Hardness ratio (energy fluence ratio) = 1.95408
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.86124
Count Ratio (50-100 keV) / (15-25 keV) = 2.32832
Mask shadow pattern
IMX = -1.543322842016900E+00, IMY = 1.569353617951765E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.824000 -7.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
98.9896 26.0216 2.1 31.6 84.7 3.6983 5.5 ------ UNKNOWN
44.9802 72.5856 2.0 37.4 -166.9 2.7386 5.7 ------ UNKNOWN
187.7312 41.3832 2.8 44.4 -61.2 6.9021 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-7.040000 21.120000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
88.8185 21.5761 3.4 40.1 94.8 1.2125 3.4 ------ UNKNOWN
78.1280 45.9002 2.1 29.2 137.1 0.6467 5.4 ------ UNKNOWN
9.7298 57.6337 0.6 57.2 -174.2 14.3340 20.8 ------ UNKNOWN
9.3605 76.8847 2.9 44.3 -155.6 0.6977 4.0 ------ UNKNOWN
173.4315 55.1581 3.7 29.7 -74.4 0.4385 3.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
217.476590 664.076600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3945 -60.5898 4.2 54.3 -8.0 3.3557 2.7 3.1 Cen X-3
186.7995 -62.7886 9.8 52.4 -17.8 1.8559 1.2 4.1 GX 301-2
244.9889 -15.6126 1.1 41.8 -106.0 32.9606 10.3 1.7 Sco X-1
171.0281 -2.6884 4.3 32.1 77.1 2.9885 2.7 ------ UNKNOWN
163.5477 -25.7401 2.9 39.0 36.6 4.2599 4.0 ------ UNKNOWN
226.0558 17.4344 1.8 37.4 -167.0 5.2388 6.4 ------ UNKNOWN
Plot creation:
Tue Dec 26 16:57:39 EST 2023