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
38.9954 55.2191 0.0178 46.9568 -41.1652 3.2013722 10.855 TRIG_01110821
Foreground time interval of the image:
-11.440 23.237 (delta_t = 34.677 [sec])
Background time interval of the image:
-62.763 -11.440 (delta_t = 51.323 [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 -11.440 sec. to 136.976 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58917 ( -0.153745 0.155793 )
Norm@50keV : 2.19642E-03 ( -0.000216384 0.000215638 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.90 using 59 bins.
Reduced chi-squared = 1.05088
# Null hypothesis probability of 3.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 148.4 sec: 0.281318 ( -0.027924 0.027992 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.05284e-06 ( -3.17296e-07 3.19131e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -11.440 sec. to 136.976 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.258573 ( -0.849729 0.716323 )
Epeak [keV] : 65.8238 ( -10.2078 21.7398 )
Norm@50keV : 1.01878E-02 ( -0.00563827 0.0162795 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.55 using 59 bins.
Reduced chi-squared = 0.866964
# Null hypothesis probability of 7.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 148.4 sec: 0.267571 ( -0.028754 0.028859 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.84823e-06 ( -3.30004e-07 3.36147e-07 ) ergs/cm2
Band function
Time interval is from -11.440 sec. to 136.976 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] : 14.6994 (-1.46478 1.6407)
R^2/D10^2 : 3.54016E-02 (-0.011345 0.016389)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.25e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.384e-07 4.274e-08
25- 50 9.295e-07 1.109e-07
50-150 1.354e-06 2.504e-07
15-150 2.522e-06 2.894e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 162.623 (-53.924 -163.544)
Norm : 1.17303 (-0.123245 0.139651)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.77e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.438e-07 7.665e-08
25- 50 8.320e-07 3.015e-07
50-150 1.696e-06 9.439e-07
15-150 2.972e-06 1.141e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.39061 (-2.74783 3.3528)
R1^2/D10^2 : 0.190015 (-0.122109 0.513587)
kT2 [keV] : 20.2809 (-4.09587 9.35755)
R2^2/D10^2 : 8.47663E-03 (-0.0068699 0.0138846)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.50e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.601e-07 1.940e-07
25- 50 8.946e-07 4.111e-07
50-150 1.603e-06 8.956e-07
15-150 2.857e-06 1.491e-06
Peak spectrum fit
Power-law model
Time interval is from 0.164 sec. to 1.164 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.93654 ( -0.390674 0.452846 )
Norm@50keV : 4.29545E-03 ( -0.00171262 0.00168007 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 88.69 using 59 bins.
Reduced chi-squared = 1.55596
# Null hypothesis probability of 4.56e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.12840 ( -0.464459 0.46694 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.01718e-08 ( -1.92026e-08 1.91963e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.164 sec. to 1.164 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.78960 ( 5.81476 3.42894 )
Epeak [keV] : 54.0048 ( -8.06338 8.99196 )
Norm@50keV : 39.3406 ( -40.7605 1244.45 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.62 using 59 bins.
Reduced chi-squared = 1.15393
# Null hypothesis probability of 2.01e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.41439 ( -0.453142 0.49429 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07651e-07 ( -2.71391e-08 2.70963e-08 ) ergs/cm2
Band function
Time interval is from 0.164 sec. to 1.164 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] : 11.6445 (-1.22139 1.11842)
R^2/D10^2 : 0.547324 (-0.232788 0.347647)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.39e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.565e-08 5.941e-09
25- 50 4.751e-08 1.506e-08
50-150 3.795e-08 1.377e-08
15-150 1.011e-07 3.256e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.8016 (-7.78469 9.53911)
Norm : 11.1602 (-4.54273 5.31304)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.06e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.403e-08 9.105e-09
25- 50 2.923e-08 9.820e-09
50-150 1.861e-08 8.259e-09
15-150 7.187e-08 2.615e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.138670 (13.1599 -0.13867)
R1^2/D10^2 : 85.3171 (-85.3172 -85.3172)
kT2 [keV] : 11.6457 (-1.22177 1.11804)
R2^2/D10^2 : 0.547081 (-0.232662 0.347774)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.03e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.44659 ( -0.141592 0.141378 )
Norm@50keV : 7.24280E-03 ( -0.0006659 0.000665578 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 34.68 sec: 0.891835 ( -0.0855755 0.0858345 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4051e-06 ( -2.33278e-07 2.34167e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.41491E-02 ( -0.795874 0.676833 )
Epeak [keV] : 71.9162 ( -9.74187 17.6145 )
Norm@50keV : 3.97372E-02 ( -0.0204381 0.0520319 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.77e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 34.68 sec: 0.846503 ( -0.087342 0.087767 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.26445e-06 ( -2.39961e-07 2.42861e-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) = 7.88e-07
S(50-100 keV) = 1.05e-06
T90 vs. Hardness ratio plot
T90 = 106.368000030518 sec.
Hardness ratio (energy fluence ratio) = 1.33249
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.93224
Count Ratio (50-100 keV) / (15-25 keV) = 1.55745
Mask shadow pattern
IMX = 8.060750188929401E-01, IMY = 7.048003004474200E-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:
-62.763400 -11.440000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
190.1226 31.4297 2.4 43.0 143.8 1.5817 4.9 ------ UNKNOWN
167.4409 15.4530 2.8 56.4 173.5 2.3103 4.1 ------ UNKNOWN
120.6038 29.0763 2.4 48.2 -129.3 2.3425 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-11.440000 23.236590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
242.0685 51.0539 1.9 39.4 77.0 2.2687 6.0 ------ UNKNOWN
38.9954 55.2191 1.1 47.0 -41.2 3.2011 10.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
130.636590 648.936600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.5595 17.2693 3.3 49.7 35.5 6.1608 3.5 ------ UNKNOWN
32.0556 8.1828 2.5 47.3 -12.8 5.0651 4.6 ------ UNKNOWN
127.9007 49.7459 2.8 50.7 -145.5 8.4614 4.2 ------ UNKNOWN
81.6598 27.8292 1.9 41.0 -88.1 18.4145 6.1 ------ UNKNOWN
Plot creation:
Mon Oct 24 12:44:34 EDT 2022