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
343.2184 80.4392 0.0074 17.5328 -66.3106 1.2367011 25.809 TRIG_01263718
Foreground time interval of the image:
-0.932 10.333 (delta_t = 11.265 [sec])
Background time interval of the image:
-267.568 -0.932 (delta_t = 266.636 [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 -0.932 sec. to 276.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64886 ( -0.0272164 0.0271686 )
Norm@50keV : 1.03318E-02 ( -0.000145203 0.000145014 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.48 using 59 bins.
Reduced chi-squared = 0.587368
# Null hypothesis probability of 9.95e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 277.4 sec: 1.34862 ( -0.02476 0.0249 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66622e-05 ( -3.63386e-07 3.63452e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.932 sec. to 276.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58780 ( -0.110561 0.0822262 )
Epeak [keV] : 410.240 ( -410.158 -410.208 )
Norm@50keV : 1.09440E-02 ( -0.000785628 0.00117009 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.56 using 59 bins.
Reduced chi-squared = 0.581429
# Null hypothesis probability of 9.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 277.4 sec: 1.33891 ( -0.0297 0.02998 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.65611e-05 ( -4.02416e-07 4.01137e-07 ) ergs/cm2
Band function
Time interval is from -0.932 sec. to 276.496 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] : 18.2327 ( )
R^2/D10^2 : 6.79519E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 1221.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.83e-218 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.249e-06 4.022e-08
25- 50 5.833e-06 1.304e-07
50-150 1.412e-05 3.121e-07
15-150 2.121e-05 3.024e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 197.639 (-14.9825 -197.631)
Norm : 5.27981 (-0.0784151 0.0996548)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.643e-06 6.658e-08
25- 50 7.007e-06 1.221e-07
50-150 1.537e-05 2.927e-07
15-150 2.601e-05 4.688e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.53852 (-0.384318 0.399579)
R1^2/D10^2 : 1.11293 (-0.195091 0.247393)
kT2 [keV] : 28.5813 (-1.25452 1.42422)
R2^2/D10^2 : 1.11112E-02 (-0.00182905 0.00203673)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.21e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.430e-06 1.900e-07
25- 50 7.213e-06 1.900e-07
50-150 1.542e-05 3.481e-07
15-150 2.606e-05 4.674e-07
Peak spectrum fit
Power-law model
Time interval is from 147.452 sec. to 148.452 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17356 ( -0.0513394 0.0512699 )
Norm@50keV : 9.89448E-02 ( -0.00276192 0.00276142 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.99 using 59 bins.
Reduced chi-squared = 0.648947
# Null hypothesis probability of 9.82e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 11.5728 ( -0.3363 0.3366 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0116e-06 ( -3.11849e-08 3.12456e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 147.452 sec. to 148.452 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.05993 ( -0.199282 0.149886 )
Epeak [keV] : 472.468 ( -472.469 -472.469 )
Norm@50keV : 0.111206 ( -0.0139607 0.0244851 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.97 using 59 bins.
Reduced chi-squared = 0.642321
# Null hypothesis probability of 9.83e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 11.5010 ( -0.356 0.3563 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00543e-06 ( -3.30635e-08 3.2911e-08 ) ergs/cm2
Band function
Time interval is from 147.452 sec. to 148.452 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] : 19.9437 ( )
R^2/D10^2 : 0.533810 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 288.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.12e-32 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.098e-08 2.325e-09
25- 50 2.037e-07 8.100e-09
50-150 6.005e-07 2.790e-08
15-150 8.452e-07 2.915e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 48.1029 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 194.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.91e-17 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.198e-07 3.350e-09
25- 50 2.304e-07 6.350e-09
50-150 5.053e-07 1.485e-08
15-150 8.555e-07 2.485e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.42452 (-0.927944 1.00807)
R1^2/D10^2 : 5.20966 (-1.50243 2.34354)
kT2 [keV] : 34.8733 (-3.71857 5.1828)
R2^2/D10^2 : 7.47097E-02 (-0.0262681 0.0332765)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.70e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.219e-08 7.860e-09
25- 50 2.166e-07 1.505e-08
50-150 7.129e-07 6.325e-08
15-150 1.012e-06 6.845e-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: 1.52903 ( -0.106045 0.106677 )
Norm@50keV : 7.05004E-03 ( -0.000417254 0.000415663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 11.26 sec: 0.887171 ( -0.0524488 0.0525502 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.49634e-07 ( -4.85435e-08 4.88354e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52540 ( -0.358072 0.107898 )
Epeak [keV] : 9933.56 ( -9998.88 -9998.88 )
Norm@50keV : 7.07575E-03 ( -0.00151857 0.00348104 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.92e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 11.26 sec: 0.887091 ( -0.027371 0.052261 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.46906e-07 ( -4.98097e-08 5.23027e-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) = 7.07e-06
S(50-100 keV) = 9.02e-06
T90 vs. Hardness ratio plot
T90 = 173.431999921799 sec.
Hardness ratio (energy fluence ratio) = 1.27581
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.19512
Count Ratio (50-100 keV) / (15-25 keV) = 0.829245
Mask shadow pattern
IMX = 1.269330432213816E-01, IMY = 2.893066313359380E-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:
-267.568000 -0.932000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5932 35.1971 1.4 48.7 -146.7 8.2391 8.0 0.3 Cyg X-1
307.9422 41.0560 16.9 40.2 -149.9 0.4258 0.7 9.8 Cyg X-3
326.0236 38.3640 4.6 34.9 -171.5 1.2393 2.5 7.4 Cyg X-2
23.5824 32.5725 2.9 33.3 99.0 2.5902 4.1 ------ UNKNOWN
77.8453 62.6360 2.7 30.4 5.6 1.9947 4.2 ------ UNKNOWN
260.7996 66.0201 2.8 39.3 -92.0 6.5040 4.2 ------ UNKNOWN
286.0358 43.0241 2.8 48.1 -129.2 7.7560 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.932000 10.332600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7418 35.1307 6.4 48.7 -146.9 -0.1932 -1.8 8.6 Cyg X-1
307.9435 40.9978 12.3 40.3 -149.9 0.0625 0.9 8.0 Cyg X-3
326.3389 38.3215 5.6 34.9 -171.9 0.1038 2.1 7.9 Cyg X-2
83.4865 48.5496 2.5 42.4 19.3 0.3326 4.7 ------ UNKNOWN
343.2185 80.4391 0.4 17.5 -66.3 1.2365 25.8 ------ UNKNOWN
313.6625 54.9500 2.1 27.3 -138.2 0.2547 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.932600 934.932600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6170 35.1882 1.6 48.2 -166.7 21.2273 7.1 1.5 Cyg X-1
308.0945 40.9868 4.0 41.5 -174.8 6.0998 2.9 2.2 Cyg X-3
326.2735 38.4258 83.7 42.5 164.0 0.3880 0.1 7.9 Cyg X-2
61.0207 79.2330 2.6 12.8 20.1 4.5941 4.3 ------ UNKNOWN
343.1523 80.4568 0.3 0.0 -4.7 41.5995 33.8 ------ UNKNOWN
189.7828 53.0659 2.9 45.6 -57.8 23.3994 3.9 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:42:52 EST 2024