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
344.5701 1.0189 0.0027 24.7406 101.9320 31.9669591 71.707 TRIG_01250617
Foreground time interval of the image:
0.112 10.413 (delta_t = 10.301 [sec])
Background time interval of the image:
-50.987 0.112 (delta_t = 51.099 [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 0.512000
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 0.512000
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 0.512000
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 0.112 sec. to 832.112 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26106 ( -0.0362383 0.0360976 )
Norm@50keV : 3.07059E-03 ( -5.82766e-05 5.81383e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.51 using 59 bins.
Reduced chi-squared = 0.745789
# Null hypothesis probability of 9.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 832 sec: 0.363834 ( -0.007782 0.007821 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.54966e-05 ( -4.75717e-07 4.76432e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.112 sec. to 832.112 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25740 ( -0.0372815 0.0356016 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.08427E-03 ( -5.78037e-05 0.000205532 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.65 using 59 bins.
Reduced chi-squared = 0.761607
# Null hypothesis probability of 9.06e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 832 sec: 0.366778 ( -0.010857 0.004733 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.5602e-05 ( -5.77591e-07 3.64523e-07 ) ergs/cm2
Band function
Time interval is from 0.112 sec. to 832.112 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] : 21.1851 ( )
R^2/D10^2 : 1.30651E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 667.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.11e-105 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.182e-07 3.536e-08
25- 50 4.746e-06 1.414e-07
50-150 1.589e-05 4.368e-07
15-150 2.155e-05 4.368e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 1.58039 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 303.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.61e-35 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.274e-06 7.072e-08
25- 50 6.298e-06 1.394e-07
50-150 1.381e-05 2.829e-07
15-150 2.339e-05 4.950e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.60233 (-0.618289 0.65515)
R1^2/D10^2 : 0.168334 (-0.0359307 0.0482459)
kT2 [keV] : 37.1005 (-2.88685 3.67227)
R2^2/D10^2 : 1.80544E-03 (-0.000456872 0.000534875)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.249e-06 1.652e-07
25- 50 5.766e-06 1.876e-07
50-150 1.757e-05 7.446e-07
15-150 2.559e-05 9.818e-07
Peak spectrum fit
Power-law model
Time interval is from 7.612 sec. to 8.612 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61789 ( -0.157303 0.162092 )
Norm@50keV : 2.27496E-02 ( -0.00232276 0.00229471 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.58 using 59 bins.
Reduced chi-squared = 0.887368
# Null hypothesis probability of 7.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.93997 ( -0.27555 0.27563 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.12339e-07 ( -2.31831e-08 2.34318e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.612 sec. to 8.612 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01543 ( -0.729881 0.6296 )
Epeak [keV] : 78.0515 ( -21.5705 -78.0515 )
Norm@50keV : 4.73711E-02 ( -0.0249297 0.0656865 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.92 using 59 bins.
Reduced chi-squared = 0.855714
# Null hypothesis probability of 7.70e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.88324 ( -0.2828 0.28227 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03395e-07 ( -2.50463e-08 2.5307e-08 ) ergs/cm2
Band function
Time interval is from 7.612 sec. to 8.612 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] : 13.6645 (-1.53743 1.70469)
R^2/D10^2 : 0.465148 (-0.158669 0.243886)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.21e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.838e-08 3.075e-09
25- 50 6.672e-08 8.270e-09
50-150 8.099e-08 1.602e-08
15-150 1.661e-07 2.045e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 162.968 (-59.4213 -161.844)
Norm : 12.1361 (-1.19208 1.44803)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.85e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.093e-08 7.545e-09
25- 50 5.801e-08 2.186e-08
50-150 1.184e-07 6.425e-08
15-150 2.073e-07 9.868e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.29003 (-1.51579 2.18481)
R1^2/D10^2 : 7.59556 (-5.27753 15.9035)
kT2 [keV] : 19.3577 (-3.33495 5.98074)
R2^2/D10^2 : 0.110996 (-0.0732555 0.108555)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.114e-08 1.405e-08
25- 50 5.680e-08 1.913e-08
50-150 1.102e-07 4.815e-08
15-150 1.982e-07 7.555e-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: 1.11705 ( -0.024899 0.0247995 )
Norm@50keV : 0.205385 ( -0.00294213 0.00293218 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.18e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.3 sec: 23.8642 ( -0.371092 0.37245 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19988e-05 ( -2.87214e-07 2.87256e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11244 ( -0.0289124 0.0239206 )
Epeak [keV] : 9951.00 ( -9945.33 -9945.33 )
Norm@50keV : 0.206546 ( -0.00284576 0.022595 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.03e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.3 sec: 23.8501 ( -0.352 0.3725 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19718e-05 ( 0 0 ) 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) = 5.55e-06
S(50-100 keV) = 9.24e-06
T90 vs. Hardness ratio plot
T90 = 416 sec.
Hardness ratio (energy fluence ratio) = 1.66486
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.51371
Count Ratio (50-100 keV) / (15-25 keV) = 1.3586
Mask shadow pattern
IMX = -9.527226604463888E-02, IMY = -4.508503657237785E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-50.987400 0.112000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0343 40.9537 5.5 52.3 -179.0 -0.6414 -2.1 3.4 Cyg X-3
326.1696 38.3220 53.4 38.2 -177.2 -0.0299 -0.2 0.1 Cyg X-2
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.112000 10.412600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1066 40.9067 3.3 52.2 -179.1 -3.3631 -3.5 2.8 Cyg X-3
326.4046 38.3847 0.0 38.0 -177.0 0.8360 1.9 11.6 Cyg X-2
344.5701 1.0189 0.2 24.7 101.9 31.9717 71.7 ------ UNKNOWN
302.6414 31.4723 2.9 56.0 168.9 8.2787 3.9 ------ UNKNOWN
338.6862 15.6547 2.9 23.5 141.0 1.5511 4.0 ------ UNKNOWN
35.1727 19.7372 2.9 30.4 -46.4 1.5444 4.0 ------ UNKNOWN
49.1317 30.9243 3.3 43.6 -64.0 4.9963 3.5 ------ UNKNOWN
45.5824 36.7366 2.1 41.8 -73.2 5.0297 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
71.412600 962.117000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5482 35.2105 1.7 54.0 -175.2 27.3072 6.9 2.1 Cyg X-1
308.1056 40.9118 13.1 51.7 -164.5 3.0765 0.9 2.5 Cyg X-3
326.4414 38.3553 0.0 40.9 -151.5 -2.7598 -1.4 12.9 Cyg X-2
328.7661 -27.3425 3.3 32.2 77.4 7.4658 3.4 ------ UNKNOWN
9.2017 -27.5913 2.5 37.1 12.6 7.0619 4.6 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:17:33 EDT 2024