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
352.0924 51.6206 0.0215 2.9025 -74.2657 1.5119953 8.958 TRIG_01205744
Foreground time interval of the image:
-54.584 73.069 (delta_t = 127.653 [sec])
Background time interval of the image:
-239.032 -54.584 (delta_t = 184.448 [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 16.384000
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 16.384000
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 16.384000
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 -54.584 sec. to 107.528 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56026 ( -0.266988 0.275619 )
Norm@50keV : 5.56837E-04 ( -9.40919e-05 9.24274e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.53 using 59 bins.
Reduced chi-squared = 1.0093
# Null hypothesis probability of 4.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 162.1 sec: 7.07055E-02 ( -0.011023 0.0110286 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.48639e-07 ( -1.54425e-07 1.57859e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -54.584 sec. to 107.528 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.885980 ( -1.43802 0.876441 )
Epeak [keV] : 77.8317 ( -30.8904 -77.8303 )
Norm@50keV : 1.26955E-03 ( -0.000784587 0.00589663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.45 using 59 bins.
Reduced chi-squared = 1.00804
# Null hypothesis probability of 4.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 162.1 sec: 6.88549E-02 ( -0.0115095 0.0114482 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.99951e-07 ( -1.68597e-07 1.75831e-07 ) ergs/cm2
Band function
Time interval is from -54.584 sec. to 107.528 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] : 13.6826 (-2.28198 2.85898)
R^2/D10^2 : 1.11684E-02 (-0.00550241 0.0101972)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.92e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.173e-08 2.246e-08
25- 50 2.607e-07 6.144e-08
50-150 3.175e-07 1.050e-07
15-150 6.499e-07 1.423e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 180.279 (-92.2394 -180.371)
Norm : 0.290316 (-0.0459096 0.0537894)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.84e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.187e-07 6.838e-08
25- 50 2.255e-07 1.236e-07
50-150 4.777e-07 2.718e-07
15-150 8.218e-07 4.592e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.77394 (-2.68188 71.1156)
R1^2/D10^2 : 0.617221 (-0.603908 1966.46)
kT2 [keV] : 16.7151 (-3.79373 58.3214)
R2^2/D10^2 : 4.97153E-03 (-0.00494066 0.0048232)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.17e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.142e-07 5.705e-08
25- 50 2.218e-07 1.082e-07
50-150 3.990e-07 2.381e-07
15-150 7.351e-07 3.493e-07
Peak spectrum fit
Power-law model
Time interval is from 10.292 sec. to 11.292 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67362 ( -0.540827 0.598564 )
Norm@50keV : 3.63079E-03 ( -0.00128986 0.00121586 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.07 using 59 bins.
Reduced chi-squared = 1.10649
# Null hypothesis probability of 2.70e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.477869 ( -0.14495 0.145051 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.36969e-08 ( -1.19974e-08 1.25849e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 10.292 sec. to 11.292 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.881650 ( -5.52682 1.3525 )
Epeak [keV] : 64.8266 ( -50.9479 -64.6615 )
Norm@50keV : 9.71273E-03 ( -0.00982107 4.8984 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.86 using 59 bins.
Reduced chi-squared = 1.1225
# Null hypothesis probability of 2.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.462695 ( -0.164159 0.154076 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.14e-08 ( -1.21474e-08 1.37586e-08 ) ergs/cm2
Band function
Time interval is from 10.292 sec. to 11.292 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] : 13.1927 (-3.50396 5.07722)
R^2/D10^2 : 8.61228E-02 (-0.0861228 0.17393)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.54e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.178e-09 2.007e-09
25- 50 1.112e-08 6.740e-09
50-150 1.234e-08 8.955e-09
15-150 2.664e-08 1.659e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 148.440 (-98.9431 -143.419)
Norm : 1.95258 (-0.627566 1.04662)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.876e-09 2.914e-09
25- 50 9.290e-09 5.435e-09
50-150 1.983e-08 1.185e-08
15-150 3.399e-08 2.045e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.85997 (-1.85556 5.41342)
R1^2/D10^2 : 448.188 (-464.123 -464.242)
kT2 [keV] : 14.5730 (-4.05357 7.08316)
R2^2/D10^2 : 5.64494E-02 (-0.0270436 0.0533178)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.652e-09 2.109e-09
25- 50 9.788e-09 5.880e-09
50-150 1.390e-08 9.520e-09
15-150 2.835e-08 1.744e-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: 1.51365 ( -0.2377 0.242588 )
Norm@50keV : 6.96941E-04 ( -0.000104818 0.000103584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 127.7 sec: 8.73287E-02 ( -0.0124049 0.0124125 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.42452e-07 ( -1.3787e-07 1.40613e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.654429 ( -1.28922 0.947367 )
Epeak [keV] : 73.7539 ( -20.1855 -73.7539 )
Norm@50keV : 1.98948E-03 ( -0.00198948 0.00738107 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 127.7 sec: 8.45100E-02 ( -0.0128935 0.0128467 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.81837e-07 ( -1.49765e-07 1.56573e-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) = 2.16e-07
S(50-100 keV) = 2.93e-07
T90 vs. Hardness ratio plot
T90 = 134.015999913216 sec.
Hardness ratio (energy fluence ratio) = 1.35648
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.51198
Count Ratio (50-100 keV) / (15-25 keV) = 1.0195
Mask shadow pattern
IMX = 1.374898082235024E-02, IMY = 4.880133904148388E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
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:
-239.032000 -54.584000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1060 40.9718 3.1 34.5 -72.5 1.8954 3.7 1.2 Cyg X-3
326.0938 38.4462 7.2 25.1 -93.8 0.5852 1.6 8.3 Cyg X-2
39.2080 18.0883 2.2 47.3 135.2 7.4700 5.3 ------ UNKNOWN
208.7426 69.2488 2.9 56.8 3.1 5.1057 4.0 ------ UNKNOWN
341.6547 73.6838 3.2 22.9 5.1 1.0646 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-54.584000 73.068590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0687 41.1115 3.6 34.5 -72.3 0.9916 3.2 9.7 Cyg X-3
326.2894 38.3976 4.0 25.0 -94.1 0.6546 2.9 7.2 Cyg X-2
16.1719 60.8074 1.9 14.0 58.1 0.9977 6.0 ------ UNKNOWN
214.3395 76.3957 2.2 49.6 5.2 2.4672 5.3 ------ UNKNOWN
352.0924 51.6207 1.3 2.9 -74.3 1.5118 9.0 ------ UNKNOWN
293.5263 40.2801 2.2 43.9 -63.1 3.4301 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
108.668590 963.118000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5960 35.1459 4.0 40.5 -63.4 8.0929 2.9 3.4 Cyg X-1
308.1808 40.9624 2.6 31.6 -62.7 6.6128 4.4 3.2 Cyg X-3
326.4003 38.3615 12.7 22.3 -87.0 1.2283 0.9 11.0 Cyg X-2
228.6406 63.3949 4.0 56.8 3.0 11.4828 2.9 ------ UNKNOWN
277.5090 53.5209 2.3 43.2 -27.3 9.4969 4.9 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:18:32 EST 2024