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
301.3985 49.4075 0.0267 41.3484 -21.8456 0.5387006 7.213 TRIG_01094950
Foreground time interval of the image:
-1.864 5.384 (delta_t = 7.248 [sec])
Background time interval of the image:
-239.192 -1.864 (delta_t = 237.328 [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 4.096000
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 4.096000
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 4.096000
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 -1.864 sec. to 5.384 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40921 ( -0.361643 0.360645 )
Norm@50keV : 5.21334E-03 ( -0.00103793 0.00103505 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.18 using 59 bins.
Reduced chi-squared = 0.862807
# Null hypothesis probability of 7.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 7.248 sec: 0.636239 ( -0.131284 0.132025 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64484e-07 ( -7.89032e-08 7.96439e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.864 sec. to 5.384 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40635 ( -1.40669 3.01609 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 5.23176E-03 ( -0.00104327 -0.00523179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.18 using 59 bins.
Reduced chi-squared = 0.878214
# Null hypothesis probability of 7.29e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 7.248 sec: 0.639194 ( -0.145695 0.136288 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.65038e-07 ( -7.58054e-08 6.75136e-08 ) ergs/cm2
Band function
Time interval is from -1.864 sec. to 5.384 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] : 18.6667 (-4.4121 6.11636)
R^2/D10^2 : 3.43288E-02 (-0.0211376 0.0519243)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.91e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.715e-08 7.375e-09
25- 50 8.145e-08 3.565e-08
50-150 2.078e-07 8.194e-08
15-150 3.064e-07 1.218e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-91.2608 -199.363)
Norm : 2.63435 (-0.524113 0.524083)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.31e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.755e-08 2.856e-08
25- 50 9.146e-08 5.309e-08
50-150 2.006e-07 1.156e-07
15-150 3.396e-07 1.967e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.48453 (-1.7684 3.55164)
R1^2/D10^2 : 3.77008 (-3.42326 41.7059)
kT2 [keV] : 24.7604 (-6.78913 14.6746)
R2^2/D10^2 : 1.19411E-02 (-0.00926862 0.0238573)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.48e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.138e-08 3.008e-08
25- 50 7.313e-08 3.860e-08
50-150 2.386e-07 1.422e-07
15-150 3.631e-07 1.984e-07
Peak spectrum fit
Power-law model
Time interval is from 0.364 sec. to 1.364 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32240 ( -0.484881 0.461171 )
Norm@50keV : 1.08146E-02 ( -0.00282423 0.00282662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.13 using 59 bins.
Reduced chi-squared = 0.774211
# Null hypothesis probability of 8.94e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.29570 ( -0.361279 0.36386 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.06309e-07 ( -2.94048e-08 2.95536e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.364 sec. to 1.364 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32582 ( -0.493864 0.458369 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 1.08375E-02 ( -0.00283563 0.00283616 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.14 using 59 bins.
Reduced chi-squared = 0.788214
# Null hypothesis probability of 8.74e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.30568 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.06574e-07 ( -3.08524e-08 2.55312e-08 ) ergs/cm2
Band function
Time interval is from 0.364 sec. to 1.364 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] : 18.6409 (-4.90218 8.11215)
R^2/D10^2 : 7.36803E-02 (-0.0524938 0.13737)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.02e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.067e-09 3.146e-09
25- 50 2.404e-08 1.235e-08
50-150 6.115e-08 3.767e-08
15-150 9.026e-08 4.932e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-101.688 -199.363)
Norm : 5.45889 (-1.44561 1.44567)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.359e-08 8.410e-09
25- 50 2.615e-08 1.604e-08
50-150 5.735e-08 3.438e-08
15-150 9.709e-08 5.770e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.17938 (-2.67014 14.8912)
R1^2/D10^2 : 9.14050 (-9.04342 4313.04)
kT2 [keV] : 23.1925 (-7.36799 -23.1947)
R2^2/D10^2 : 3.16789E-02 (-0.0296399 0.0717967)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.50e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.332e-08 7.625e-09
25- 50 2.095e-08 1.130e-08
50-150 6.740e-08 4.241e-08
15-150 1.017e-07 5.640e-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: 1.40921 ( -0.361643 0.360645 )
Norm@50keV : 5.21334E-03 ( -0.00103793 0.00103505 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 7.248 sec: 0.636228 ( -0.131277 0.132016 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64437e-07 ( -7.88909e-08 7.97164e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41871 ( -1.28428 0.650235 )
Epeak [keV] : 9998.82 ( -9999.34 -9999.34 )
Norm@50keV : 5.15677E-03 ( -0.00103841 0.0164133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.28e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 7.248 sec: 0.636882 ( -0.134974 0.130276 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64191e-07 ( -8.05028e-08 7.96751e-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) = 8.63e-08
S(50-100 keV) = 1.30e-07
T90 vs. Hardness ratio plot
T90 = 6.59200000762939 sec.
Hardness ratio (energy fluence ratio) = 1.50637
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.870759
Count Ratio (50-100 keV) / (15-25 keV) = 1.035
Mask shadow pattern
IMX = 8.168240404729624E-01, IMY = 3.274607089242439E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.192000 -1.864000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5900 35.1928 1.5 53.3 -32.4 13.0518 7.6 0.5 Cyg X-1
308.1752 40.8870 5.1 44.8 -35.3 1.6849 2.3 4.9 Cyg X-3
326.3636 38.1659 0.0 38.6 -54.7 -0.6885 -1.0 13.0 Cyg X-2
105.7542 59.6679 2.5 39.9 102.1 4.4357 4.5 ------ UNKNOWN
144.4215 73.1973 3.8 40.1 70.9 3.5548 3.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.864000 5.384000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5327 35.1982 4.3 53.4 -32.4 -0.5719 -2.6 2.8 Cyg X-1
308.1377 40.8638 6.0 44.8 -35.2 -0.1799 -1.9 5.5 Cyg X-3
326.0590 38.3661 2.9 38.5 -54.2 0.3172 4.1 5.9 Cyg X-2
301.3990 49.4077 1.6 41.3 -21.8 0.5382 7.2 ------ UNKNOWN
342.2822 37.9208 2.3 32.1 -73.3 0.3430 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
621.108630 962.876000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6418 22.0035 0.8 36.0 126.6 11.5168 13.7 0.8 Crab
348.1361 42.0443 2.5 43.4 -50.4 5.1995 4.6 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:07:20 EDT 2022