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
350.3678 6.6468 0.0102 23.0035 -167.3340 0.8672042 18.747 TRIG_01047531
Foreground time interval of the image:
-4.688 7.664 (delta_t = 12.352 [sec])
Background time interval of the image:
-239.424 -4.688 (delta_t = 234.736 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -4.688 sec. to 7.664 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12031 ( -0.16559 0.174419 )
Norm@50keV : 3.61394E-03 ( -0.000436793 0.000429941 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.72 using 59 bins.
Reduced chi-squared = 1.01263
# Null hypothesis probability of 4.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.35 sec: 0.574385 ( -0.051001 0.051006 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.15611e-07 ( -4.45826e-08 4.56079e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.688 sec. to 7.664 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.806357 ( -0.992605 0.824142 )
Epeak [keV] : 35.2855 ( -9.4787 7.05829 )
Norm@50keV : 2.22484E-02 ( -0.0222484 0.0674802 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.59 using 59 bins.
Reduced chi-squared = 0.885536
# Null hypothesis probability of 7.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.35 sec: 0.549856 ( -0.052245 0.05255 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.67508e-07 ( -4.51507e-08 5.01756e-08 ) ergs/cm2
Band function
Time interval is from -4.688 sec. to 7.664 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] : 9.17726 (-0.877929 0.966148)
R^2/D10^2 : 0.374564 (-0.121618 0.181)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.660e-08 1.157e-08
25- 50 1.678e-07 1.748e-08
50-150 6.793e-08 1.933e-08
15-150 3.123e-07 3.637e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.4920 (-11.0257 16.0561)
Norm : 3.22598 (-0.452188 0.566655)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.806e-08 1.184e-08
25- 50 1.423e-07 1.439e-08
50-150 1.420e-07 3.987e-08
15-150 3.824e-07 5.014e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.23024 (-1.66166 1.8666)
R1^2/D10^2 : 1.91464 (-1.18378 6.12175)
kT2 [keV] : 13.7887 (-2.95597 6.38991)
R2^2/D10^2 : 5.29659E-02 (-0.0443069 0.111697)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.11e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.493e-08 4.656e-08
25- 50 1.464e-07 7.416e-08
50-150 1.222e-07 6.875e-08
15-150 3.635e-07 1.831e-07
Peak spectrum fit
Power-law model
Time interval is from 3.252 sec. to 4.252 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82517 ( -0.239395 0.256173 )
Norm@50keV : 8.39898E-03 ( -0.00151116 0.00148262 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.62 using 59 bins.
Reduced chi-squared = 1.01088
# Null hypothesis probability of 4.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.16892 ( -0.178257 0.17828 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.72681e-08 ( -1.3811e-08 1.41432e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.252 sec. to 4.252 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.206960 ( -1.52084 1.19473 )
Epeak [keV] : 48.2699 ( -8.32959 12.7054 )
Norm@50keV : 0.111190 ( -0.111818 0.623876 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.98 using 59 bins.
Reduced chi-squared = 0.856786
# Null hypothesis probability of 7.68e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.12059 ( -0.177783 0.17874 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.95537e-08 ( -1.2595e-08 1.36955e-08 ) ergs/cm2
Band function
Time interval is from 3.252 sec. to 4.252 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] : 12.1233 (-1.72634 1.94521)
R^2/D10^2 : 0.297242 (-0.126313 0.223176)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.247e-09 2.384e-09
25- 50 2.945e-08 5.930e-09
50-150 2.620e-08 8.480e-09
15-150 6.490e-08 1.316e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 84.1564 (-29.4855 62.4774)
Norm : 5.55397 (-1.00391 1.28986)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.42e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.445e-08 3.040e-09
25- 50 2.408e-08 4.985e-09
50-150 3.515e-08 2.159e-08
15-150 7.368e-08 2.589e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.61198 (-3.16022 4.86834)
R1^2/D10^2 : 3.58239 (-3.3944 2544.02)
kT2 [keV] : 14.1176 (-2.63538 4.31755)
R2^2/D10^2 : 0.147813 (-0.110682 0.200023)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.85e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.245e-08 6.485e-09
25- 50 2.664e-08 1.411e-08
50-150 3.082e-08 1.894e-08
15-150 6.991e-08 3.721e-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: 2.12031 ( -0.16559 0.174419 )
Norm@50keV : 3.61394E-03 ( -0.000436793 0.000429941 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.35 sec: 0.574334 ( -0.0509954 0.0510013 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.15533e-07 ( -4.46382e-08 4.5627e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.806357 ( -0.992606 0.824142 )
Epeak [keV] : 35.2855 ( -9.4787 7.05829 )
Norm@50keV : 2.22484E-02 ( -0.0222484 0.0674803 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.35 sec: 0.549747 ( -0.052225 0.052527 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.67583e-07 ( -4.51788e-08 5.01941e-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) = 1.30e-07
S(50-100 keV) = 1.19e-07
T90 vs. Hardness ratio plot
T90 = 10.8159999847412 sec.
Hardness ratio (energy fluence ratio) = 0.915385
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.00097
Count Ratio (50-100 keV) / (15-25 keV) = 0.419832
Mask shadow pattern
IMX = -4.142163713626277E-01, IMY = 9.308937244723164E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-239.424000 -4.688000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
315.3025 0.1834 2.6 47.9 145.2 4.3176 4.4 ------ UNKNOWN
25.3640 -40.6478 2.6 34.2 9.6 1.3894 4.5 ------ UNKNOWN
54.0112 -40.8601 4.2 53.0 -6.1 1.6753 2.8 ------ UNKNOWN
57.5569 -39.7481 3.2 55.4 -8.2 2.8788 3.6 ------ UNKNOWN
59.1265 -34.2457 3.3 55.7 -15.0 3.3844 3.5 ------ UNKNOWN
23.2752 1.8202 3.5 26.3 -81.3 1.0607 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.688000 7.664000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
333.0582 -42.6233 2.2 38.2 77.2 0.8037 5.2 ------ UNKNOWN
336.8321 3.2410 2.2 29.7 164.9 0.2881 5.2 ------ UNKNOWN
350.3678 6.6468 0.6 23.0 -167.3 0.8671 18.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
200.876600 308.476600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6561 -40.5827 6.3 42.3 156.5 0.5901 1.8 6.1 Vela X-1
167.7489 6.8593 3.2 35.0 59.8 1.1012 3.6 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:02:15 EDT 2022