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
0.5766 -16.4099 0.0151 21.1586 123.7046 2.2697742 12.742 TRIG_01114937
Foreground time interval of the image:
-66.443 29.757 (delta_t = 96.200 [sec])
Background time interval of the image:
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 -71.040 sec. to 36.036 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75727 ( -0.170512 0.175708 )
Norm@50keV : 1.35756E-03 ( -0.000140061 0.000137261 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.57 using 59 bins.
Reduced chi-squared = 0.729298
# Null hypothesis probability of 9.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 107.1 sec: 0.184069 ( -0.01629 0.016303 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.34128e-06 ( -1.42083e-07 1.44827e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -71.040 sec. to 36.036 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75687 ( -0.306485 0.176068 )
Epeak [keV] : 9999.35 ( -9999.35 -9999.36 )
Norm@50keV : 1.35920E-03 ( -0.000916072 0.00120603 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.57 using 59 bins.
Reduced chi-squared = 0.742321
# Null hypothesis probability of 9.25e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 107.1 sec: 0.184749 ( -0.018036 0.017164 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.35931e-06 ( -1.69882e-07 1.23989e-07 ) ergs/cm2
Band function
Time interval is from -71.040 sec. to 36.036 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] : 11.2053 (-1.22237 1.42403)
R^2/D10^2 : 5.51315E-02 (-0.0197183 0.0297165)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.15e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.554e-07 2.378e-08
25- 50 4.500e-07 5.189e-08
50-150 3.237e-07 7.058e-08
15-150 9.291e-07 1.133e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 115.460 (-37.7642 74.9206)
Norm : 0.780768 (-0.0880746 0.112747)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.181e-07 2.677e-08
25- 50 3.876e-07 4.707e-08
50-150 6.784e-07 2.725e-07
15-150 1.284e-06 3.805e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.69126 (-1.82135 1.64778)
R1^2/D10^2 : 0.178828 (-0.0862096 0.299439)
kT2 [keV] : 39.0750 (-16.976 -39.1555)
R2^2/D10^2 : 5.22633E-04 (-0.000477664 0.0028818)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.54e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.099e-07 5.350e-08
25- 50 4.003e-07 1.017e-07
50-150 7.799e-07 3.849e-07
15-150 1.390e-06 5.241e-07
Peak spectrum fit
Power-law model
Time interval is from 3.724 sec. to 4.724 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63229 ( -0.340244 0.351311 )
Norm@50keV : 6.97527E-03 ( -0.00149228 0.00144308 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.89 using 59 bins.
Reduced chi-squared = 1.2086
# Null hypothesis probability of 1.34e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.905586 ( -0.16948 0.169524 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.5001e-08 ( -1.45871e-08 1.5069e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.724 sec. to 4.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64362 ( -0.595479 0.34451 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 6.93325E-03 ( -0.00148624 0.0290993 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.89 using 59 bins.
Reduced chi-squared = 1.23018
# Null hypothesis probability of 1.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.906672 ( -0.170951 0.169008 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.55813e-08 ( -1.11097e-08 9.2839e-09 ) ergs/cm2
Band function
Time interval is from 3.724 sec. to 4.724 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] : 9.63207 (-1.80263 2.52855)
R^2/D10^2 : 0.493140 (-0.288552 0.583894)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.73e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.189e-09 3.370e-09
25- 50 2.165e-08 6.925e-09
50-150 1.012e-08 5.507e-09
15-150 4.096e-08 1.288e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 143.565 (-82.5314 -144.734)
Norm : 3.76460 (-0.767912 1.10517)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.703e-09 5.490e-09
25- 50 1.787e-08 9.940e-09
50-150 3.463e-08 2.194e-08
15-150 6.220e-08 3.609e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.11056 (-1.58592 1.59404)
R1^2/D10^2 : 0.839214 (-0.436112 1.05827)
kT2 [keV] : 197.329 (-160.093 -197.533)
R2^2/D10^2 : 1.41318E-04 (-5.98758e-05 0.00309778)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.026e-08 5.439e-09
25- 50 1.959e-08 1.041e-08
50-150 4.188e-08 1.280e-08
15-150 7.173e-08 2.656e-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: 1.71767 ( -0.1749 0.180183 )
Norm@50keV : 1.42234E-03 ( -0.000147033 0.000144077 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 96.2 sec: 0.190084 ( -0.0171687 0.017193 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26519e-06 ( -1.36508e-07 1.38883e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72456 ( -0.182139 0.175635 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 1.41734E-03 ( -0.0014224 0.000909325 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 96.2 sec: 0.190228 ( -0.017396 0.017019 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25806e-06 ( -1.29764e-07 1.43838e-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) = 3.72e-07
S(50-100 keV) = 4.39e-07
T90 vs. Hardness ratio plot
T90 = 85.9960000514984 sec.
Hardness ratio (energy fluence ratio) = 1.18011
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17299
Count Ratio (50-100 keV) / (15-25 keV) = 0.672616
Mask shadow pattern
IMX = -2.147751411164212E-01, IMY = -3.219851867981682E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-66.443400 29.756600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
0.5767 -16.4099 0.9 21.2 123.7 2.2699 12.7 ------ UNKNOWN
357.7671 27.3931 2.5 54.5 176.0 2.8226 4.7 ------ UNKNOWN
37.1112 -40.5479 3.1 22.6 -7.5 0.5926 3.7 ------ UNKNOWN
83.5318 -64.2880 2.1 58.2 -3.7 4.0965 5.4 ------ UNKNOWN
17.0660 37.5543 3.3 59.5 -161.9 4.3609 3.4 ------ UNKNOWN
45.9774 11.5197 2.2 40.6 -119.8 1.9741 5.2 ------ UNKNOWN
38.2799 27.7386 2.7 51.8 -139.0 3.2406 4.3 ------ UNKNOWN
70.2957 -19.7388 4.1 44.8 -60.5 2.1593 2.8 ------ UNKNOWN
54.7887 5.0056 3.0 41.6 -103.3 2.7844 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
85.756600 962.357100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
354.0971 21.7203 3.2 38.6 -170.8 5.5903 3.6 ------ UNKNOWN
25.2807 -45.0858 4.7 35.4 -11.7 3.4438 2.4 ------ UNKNOWN
11.3175 17.8471 2.5 35.8 -143.5 6.7445 4.6 ------ UNKNOWN
47.2531 -18.5531 2.2 44.4 -61.1 27.2329 5.2 ------ UNKNOWN
Plot creation:
Mon Oct 24 12:42:23 EDT 2022