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
33.5367 -22.0515 0.0126 42.6071 -5.2734 1.8097747 15.220 TRIG_01230423
Foreground time interval of the image:
-6.368 36.693 (delta_t = 43.061 [sec])
Background time interval of the image:
-239.408 -6.368 (delta_t = 233.040 [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 -6.368 sec. to 46.300 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07199 ( -0.19118 0.203974 )
Norm@50keV : 2.29059E-03 ( -0.000297467 0.000289584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.84 using 59 bins.
Reduced chi-squared = 1.12
# Null hypothesis probability of 2.49e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52.67 sec: 0.355495 ( -0.036831 0.036872 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11829e-06 ( -1.31775e-07 1.33592e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.368 sec. to 46.300 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58030 ( -0.896187 0.504552 )
Epeak [keV] : 38.5577 ( -20.1288 -38.5571 )
Norm@50keV : 4.25578E-03 ( -0.00227765 0.00869283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.65 using 59 bins.
Reduced chi-squared = 1.11875
# Null hypothesis probability of 2.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52.67 sec: 0.348216 ( -0.038673 0.038554 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08077e-06 ( -1.40804e-07 1.44925e-07 ) ergs/cm2
Band function
Time interval is from -6.368 sec. to 46.300 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] : 11.0538 (-1.28699 1.41872)
R^2/D10^2 : 0.110919 (-0.041065 0.0668454)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.30e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.493e-07 2.736e-08
25- 50 4.248e-07 5.615e-08
50-150 2.943e-07 8.069e-08
15-150 8.684e-07 1.085e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 65.1266 (-16.9309 26.331)
Norm : 1.78255 (-0.285861 0.333941)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.72e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.388e-07 3.368e-08
25- 50 3.724e-07 4.495e-08
50-150 4.527e-07 1.321e-07
15-150 1.064e-06 1.604e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.11813 (-0.882492 1.26373)
R1^2/D10^2 : 14.3637 (-11.8609 99.8276)
kT2 [keV] : 14.0992 (-2.03592 2.73775)
R2^2/D10^2 : 3.81135E-02 (-0.019862 0.0335037)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.51e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.633e-07 1.105e-07
25- 50 3.453e-07 8.551e-08
50-150 4.145e-07 1.225e-07
15-150 1.023e-06 2.436e-07
Peak spectrum fit
Power-law model
Time interval is from 0.184 sec. to 1.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84743 ( -0.462978 0.525137 )
Norm@50keV : 7.10883E-03 ( -0.00217072 0.00200764 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.41 using 59 bins.
Reduced chi-squared = 0.656316
# Null hypothesis probability of 9.79e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.998237 ( -0.259189 0.259333 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.53762e-08 ( -1.90091e-08 1.91906e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.184 sec. to 1.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.75864 ( -1.85107 0.257004 )
Epeak [keV] : 247.690 ( )
Norm@50keV : 2.56696E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.84 using 59 bins.
Reduced chi-squared = 0.657857
# Null hypothesis probability of 9.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.840004 ( -0.419309 0.407806 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.68683e-08 ( -2.8179e-08 2.10662e-08 ) ergs/cm2
Band function
Time interval is from 0.184 sec. to 1.184 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] : 9.82183 (-3.79495 11.7056)
R^2/D10^2 : 0.468959 (-0.448651 2.55498)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.15e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.155e-09 5.673e-09
25- 50 2.219e-08 1.226e-08
50-150 1.099e-08 7.785e-09
15-150 4.233e-08 2.531e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 119.804 (-73.6728 -119.163)
Norm : 4.16015 (-1.24877 2.10633)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.084e-08 6.515e-09
25- 50 1.938e-08 1.126e-08
50-150 3.456e-08 2.327e-08
15-150 6.478e-08 4.090e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.26875 (-2.42934 3.05835)
R1^2/D10^2 : 4.29778 (-3.62048 79.4134)
kT2 [keV] : 28.4881 (-11.4809 57.4788)
R2^2/D10^2 : 8.29335E-03 (-0.00787328 0.0275786)
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.75e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.391e-08 7.675e-09
25- 50 1.607e-08 8.975e-09
50-150 3.878e-08 2.461e-08
15-150 6.876e-08 3.525e-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: 2.01862 ( -0.178679 0.18933 )
Norm@50keV : 2.62246E-03 ( -0.000322048 0.000315348 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.93e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.06 sec: 0.396775 ( -0.0404707 0.0405149 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04247e-06 ( -1.19606e-07 1.21159e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.918060 ( -0.995425 0.826442 )
Epeak [keV] : 44.4521 ( -12.7913 13.0224 )
Norm@50keV : 1.04037E-02 ( -0.00662936 0.0252237 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.06 sec: 0.379904 ( -0.04239 0.042365 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.73905e-07 ( -1.23048e-07 1.28676e-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) = 3.43e-07
S(50-100 keV) = 3.27e-07
T90 vs. Hardness ratio plot
T90 = 41.9319999217987 sec.
Hardness ratio (energy fluence ratio) = 0.953353
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.982136
Count Ratio (50-100 keV) / (15-25 keV) = 0.574128
Mask shadow pattern
IMX = 9.158820703909174E-01, IMY = 8.453446961476060E-02
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:
-239.408000 -6.368000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0528 38.3766 4.2 46.2 156.5 -2.8386 -2.7 6.5 Cyg X-2
23.3337 46.5308 2.3 33.8 -138.1 1.9228 5.1 ------ UNKNOWN
52.8454 1.5870 2.1 43.3 -50.3 3.8556 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.368000 36.692600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0549 38.2558 7.9 46.2 156.3 0.3085 1.5 6.8 Cyg X-2
326.9220 28.3310 2.3 43.0 142.9 1.0183 5.1 ------ UNKNOWN
4.6341 15.6406 2.1 6.2 129.5 0.3860 5.5 ------ UNKNOWN
33.5367 -22.0515 0.8 42.6 -5.3 1.8105 15.2 ------ UNKNOWN
355.5328 48.9598 3.6 36.9 -170.4 0.2911 3.2 ------ UNKNOWN
28.2578 19.3063 2.4 17.3 -82.6 0.4002 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
130.492640 962.728000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
99.1114 -34.3732 2.8 58.1 -5.9 14.8658 4.2 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:25:48 EDT 2024