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
354.3098 53.4458 0.0283 32.2843 -86.2549 0.5139592 6.789 TRIG_01000452
Foreground time interval of the image:
0.016 10.352 (delta_t = 10.336 [sec])
Background time interval of the image:
-239.040 0.016 (delta_t = 239.056 [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 0.016 sec. to 10.352 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.02547 ( -0.587506 0.775984 )
Norm@50keV : 1.56535E-03 ( -0.000827564 0.000947945 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.94 using 59 bins.
Reduced chi-squared = 0.770877
# Null hypothesis probability of 8.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.34 sec: 0.438650 ( -0.10051 0.100955 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.96852e-07 ( -5.90609e-08 6.70488e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.016 sec. to 10.352 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.95609 ( )
Epeak [keV] : 1.10253 ( )
Norm@50keV : 9.57122E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.38 using 59 bins.
Reduced chi-squared = 0.7925
# Null hypothesis probability of 8.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.34 sec: 0.422401 ( -0.137427 0.116648 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76718e-07 ( -5.44138e-08 6.57648e-08 ) ergs/cm2
Band function
Time interval is from 0.016 sec. to 10.352 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] : 4.69772 (-1.06461 1.40003)
R^2/D10^2 : 4.84633 (-4.84733 12.4351)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.432e-08 5.304e-08
25- 50 5.265e-08 3.410e-08
50-150 1.568e-09 1.509e-09
15-150 1.485e-07 8.727e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.8909 (-6.64636 13.4104)
Norm : 7.05647 (-3.6052 9.1853)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.83e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.052e-08 4.122e-08
25- 50 6.520e-08 3.441e-08
50-150 1.288e-08 1.160e-08
15-150 1.686e-07 7.602e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.18735 (-4.18721 1.54458)
R1^2/D10^2 : 7.76149 (-7.76274 -7.76274)
kT2 [keV] : 20.9937 (-20.9871 -20.9871)
R2^2/D10^2 : 4.09617E-03 (-0.00410074 5.87421)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.74e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.424e-08 5.335e-08
25- 50 5.538e-08 2.940e-08
50-150 6.014e-08 4.390e-08
15-150 2.098e-07 1.153e-07
Peak spectrum fit
Power-law model
Time interval is from 0.084 sec. to 1.084 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.12683 ( -0.548316 0.704803 )
Norm@50keV : 6.06878E-03 ( -0.00299047 0.00338436 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.11 using 59 bins.
Reduced chi-squared = 0.844035
# Null hypothesis probability of 7.93e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.83344 ( -0.37416 0.37482 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.75336e-08 ( -2.05539e-08 2.26323e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.084 sec. to 1.084 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96770 ( -0.0509479 0.0229113 )
Epeak [keV] : 0.635505 ( -0.418462 19.7474 )
Norm@50keV : 5.16659E-02 ( -0.0299143 0.0722902 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.62 using 59 bins.
Reduced chi-squared = 0.886071
# Null hypothesis probability of 7.14e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.77393 ( -0.36939 0.36749 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.82072e-08 ( -1.84873e-08 2.28973e-08 ) ergs/cm2
Band function
Time interval is from 0.084 sec. to 1.084 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] : 4.24963 (-0.794118 0.99334)
R^2/D10^2 : 33.3656 (-21.479 64.2737)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.038e-08 2.121e-08
25- 50 1.727e-08 9.567e-09
50-150 2.993e-10 2.761e-10
15-150 5.795e-08 3.324e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.1109 (-4.8345 10.4214)
Norm : 37.5289 (-19.7764 49.2826)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.34e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.823e-08 1.548e-08
25- 50 2.283e-08 1.056e-08
50-150 3.048e-09 2.500e-09
15-150 6.410e-08 2.781e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.84111 (-0.809882 0.92985)
R1^2/D10^2 : 51.2687 (-33.9262 128.375)
kT2 [keV] : 21.6428 (-10.0406 44.9216)
R2^2/D10^2 : 1.79059E-02 (-0.0171523 0.105853)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.49e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.975e-08 2.247e-08
25- 50 2.045e-08 1.099e-08
50-150 2.876e-08 2.275e-08
15-150 8.895e-08 4.723e-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: 3.02547 ( -0.587506 0.775984 )
Norm@50keV : 1.56535E-03 ( -0.000827564 0.000947945 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.34 sec: 0.438547 ( -0.1005 0.100947 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.96786e-07 ( -5.90524e-08 6.71135e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96097 ( )
Epeak [keV] : 0.982126 ( )
Norm@50keV : 9.52997E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.34 sec: 0.438010 ( -0.100976 0.101216 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95968e-07 ( -6.92356e-08 6.72865e-08 ) 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) = 6.55e-08
S(50-100 keV) = 3.22e-08
T90 vs. Hardness ratio plot
T90 = 9.77600002288818 sec.
Hardness ratio (energy fluence ratio) = 0.491603
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.470518
Count Ratio (50-100 keV) / (15-25 keV) = 0.109159
Mask shadow pattern
IMX = 4.126676935346126E-02, IMY = 6.304410812636503E-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:
-239.040000 0.016000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
16.3759 2.0048 2.7 26.1 133.8 1.3797 4.3 ------ UNKNOWN
80.3104 38.5405 2.5 50.1 5.1 2.5590 4.7 ------ UNKNOWN
0.2254 11.5634 3.4 25.2 177.8 0.9562 3.5 ------ UNKNOWN
48.2507 40.3318 2.3 25.8 -2.7 1.3213 5.0 ------ UNKNOWN
43.9214 40.7669 3.6 23.0 -6.9 0.7898 3.2 ------ UNKNOWN
51.4835 57.9814 2.4 37.0 -29.7 1.7693 4.8 ------ UNKNOWN
327.7237 5.4222 2.6 55.0 -160.1 4.8155 4.5 ------ UNKNOWN
6.8515 54.8109 3.3 28.9 -73.1 1.1997 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.016000 10.352000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
6.7091 -17.1099 2.0 46.9 142.3 0.8963 5.7 ------ UNKNOWN
347.6495 -14.7348 2.2 53.3 165.0 0.9965 5.3 ------ UNKNOWN
354.3098 53.4458 1.7 32.3 -86.3 0.5139 6.8 ------ UNKNOWN
331.7255 24.6982 2.1 43.9 -138.7 0.4994 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
539.360610 963.002000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
106.1462 30.0320 2.8 45.6 49.0 5.9717 4.2 ------ UNKNOWN
277.7578 79.8317 3.4 49.0 151.6 5.9567 3.4 ------ UNKNOWN
127.6900 35.6323 2.3 27.6 39.3 2.5256 5.1 ------ UNKNOWN
238.9970 46.2336 2.3 51.2 -160.5 6.0284 5.0 ------ UNKNOWN
161.9930 -6.3755 2.5 52.5 -40.8 8.4400 4.6 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:31:01 EDT 2022