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
272.2841 67.8871 0.0106 8.4086 111.9310 1.6516508 18.122 TRIG_00994856
Foreground time interval of the image:
-8.704 28.837 (delta_t = 37.541 [sec])
Background time interval of the image:
-239.664 -8.704 (delta_t = 230.960 [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 -8.704 sec. to 90.012 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.01588 ( -0.0892416 0.0909078 )
Norm@50keV : 3.06982E-03 ( -0.00015711 0.000155569 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.45 using 59 bins.
Reduced chi-squared = 1.1307
# Null hypothesis probability of 2.32e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 98.72 sec: 0.463903 ( -0.02047 0.020524 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.79772e-06 ( -1.33964e-07 1.35161e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.704 sec. to 90.012 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80067 ( -0.372335 0.340125 )
Epeak [keV] : 40.9927 ( -35.9387 -40.9927 )
Norm@50keV : 4.01712E-03 ( -0.00138091 0.00233215 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.32 using 59 bins.
Reduced chi-squared = 1.13071
# Null hypothesis probability of 2.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 98.72 sec: 0.456592 ( -0.023395 0.023426 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.72719e-06 ( -1.71871e-07 1.73459e-07 ) ergs/cm2
Band function
Time interval is from -8.704 sec. to 90.012 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] : 10.4866 ( )
R^2/D10^2 : 0.166706 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 174.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.57e-14 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.739e-07 2.927e-08
25- 50 9.928e-07 4.847e-08
50-150 5.936e-07 6.826e-08
15-150 1.960e-06 9.724e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.5078 (-9.63191 12.2007)
Norm : 2.21968 (-0.169743 0.189223)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.55e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.618e-07 3.485e-08
25- 50 8.921e-07 3.993e-08
50-150 1.140e-06 1.239e-07
15-150 2.594e-06 1.387e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.82979 (-0.995301 1.03187)
R1^2/D10^2 : 1.13774 (-0.402417 0.839529)
kT2 [keV] : 19.8578 (-3.40867 5.02604)
R2^2/D10^2 : 1.03923E-02 (-0.00493181 0.00936082)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.29e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.643e-07 1.552e-07
25- 50 8.427e-07 1.688e-07
50-150 1.169e-06 3.306e-07
15-150 2.576e-06 6.476e-07
Peak spectrum fit
Power-law model
Time interval is from 50.964 sec. to 51.964 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77392 ( -0.148034 0.153426 )
Norm@50keV : 1.83741E-02 ( -0.00174945 0.00171936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.46 using 59 bins.
Reduced chi-squared = 0.990526
# Null hypothesis probability of 4.95e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.50689 ( -0.2039 0.20395 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6936e-07 ( -1.64732e-08 1.67201e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 50.964 sec. to 51.964 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47093 ( -0.578566 0.291179 )
Epeak [keV] : 81.7905 ( -29.915 -81.7954 )
Norm@50keV : 2.66761E-02 ( -0.00967686 0.0266895 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.49 using 59 bins.
Reduced chi-squared = 0.990893
# Null hypothesis probability of 4.94e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.16463 ( -0.31997 0.30415 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6523e-07 ( -1.7785e-08 1.80732e-08 ) ergs/cm2
Band function
Time interval is from 50.964 sec. to 51.964 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] : 12.5302 (-1.36201 1.52699)
R^2/D10^2 : 0.508591 (-0.171566 0.261787)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 98.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.76e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.693e-08 2.535e-09
25- 50 5.600e-08 5.400e-09
50-150 5.436e-08 9.940e-09
15-150 1.273e-07 1.425e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 115.556 (-33.3527 52.138)
Norm : 10.6187 (-1.06763 1.35854)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.770e-08 3.135e-09
25- 50 4.922e-08 5.245e-09
50-150 8.620e-08 3.239e-08
15-150 1.631e-07 4.015e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.69593 (-1.07875 1.30625)
R1^2/D10^2 : 13.0189 (-8.17431 29.5948)
kT2 [keV] : 19.4776 (-3.00798 4.14371)
R2^2/D10^2 : 8.58823E-02 (-0.0447328 0.0771022)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.05e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.081e-08 1.380e-08
25- 50 4.469e-08 1.110e-08
50-150 8.738e-08 2.403e-08
15-150 1.629e-07 4.220e-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: 1.98020 ( -0.149413 0.155555 )
Norm@50keV : 2.34779E-03 ( -0.000239411 0.00023577 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 37.54 sec: 0.349001 ( -0.0271464 0.0271495 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.12005e-07 ( -7.78929e-08 7.96107e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.934900 ( -0.986284 0.772215 )
Epeak [keV] : 39.9618 ( -8.0602 12.124 )
Norm@50keV : 9.83426E-03 ( -0.00983912 0.0292691 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 37.54 sec: 0.332701 ( -0.029239 0.029372 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.14968e-07 ( -9.10533e-08 1.01407e-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) = 8.46e-07
S(50-100 keV) = 8.37e-07
T90 vs. Hardness ratio plot
T90 = 70.8999999761581 sec.
Hardness ratio (energy fluence ratio) = 0.989362
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.96921
Count Ratio (50-100 keV) / (15-25 keV) = 0.490964
Mask shadow pattern
IMX = -5.520936979141938E-02, IMY = -1.371229878208657E-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:
-239.664000 -8.704000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5943 35.1929 43.0 37.2 175.9 -0.1222 -0.3 11.2 Her X-1
180.9041 78.3669 2.4 17.5 -38.5 1.3093 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.704000 28.836600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3063 35.2777 8.4 37.1 176.3 0.1704 1.4 8.4 Her X-1
343.6835 73.6398 2.5 24.5 43.5 0.4409 4.5 ------ UNKNOWN
272.2841 67.8872 0.6 8.4 111.9 1.6530 18.1 ------ UNKNOWN
212.1647 29.8510 2.9 47.2 -131.4 1.2942 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
56.036590 962.456000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6064 35.1829 0.0 34.2 -171.3 -0.9292 -1.0 12.0 Her X-1
299.6737 35.0693 4.2 36.3 123.0 5.2934 2.7 8.9 Cyg X-1
308.0082 40.9917 4.5 33.0 108.5 3.6159 2.6 5.2 Cyg X-3
3.8037 48.5177 3.8 46.6 48.2 8.1696 3.0 ------ UNKNOWN
252.3376 11.2809 2.2 58.1 -174.3 20.5034 5.2 ------ UNKNOWN
248.8190 18.2527 2.3 51.8 -168.8 12.4492 5.0 ------ UNKNOWN
207.4460 44.6825 4.7 40.1 -108.9 6.5067 2.5 ------ UNKNOWN
Plot creation:
Thu Oct 20 00:51:16 EDT 2022