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
318.0955 -2.3555 0.0093 28.6195 124.2195 4.4661499 20.700 TRIG_00844192
Foreground time interval of the image:
-61.548 49.765 (delta_t = 111.313 [sec])
Background time interval of the image:
-330.635 -315.316 (delta_t = 15.319 [sec])
-239.536 -61.548 (delta_t = 177.988 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -61.548 sec. to 487.604 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87700 ( -0.0961939 0.09772 )
Norm@50keV : 1.09229E-03 ( -6.07281e-05 6.01373e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8029 for 57 degrees of freedom
# Null hypothesis probability = 8.569737e-01
Photon flux (15-150 keV) in 549.2 sec: 0.155256 ( -0.007785 0.007805 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.51556e-06 ( -3.04087e-07 3.06685e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -61.548 sec. to 487.604 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87809 ( -0.0978196 0.0970581 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 1.09197E-03 ( -6.06906e-05 0.000490102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.77 using 59 PHA bins.
# Reduced chi-squared = 0.8173 for 56 degrees of freedom
# Null hypothesis probability = 8.336338e-01
Photon flux (15-150 keV) in 549.2 sec: 0.155515 ( -0.008541 0.007849 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.17846e-06 ( -4.27177e-07 3.46648e-07 ) ergs/cm2
Band function
Time interval is from -61.548 sec. to 487.604 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] : 10.9001 ( )
R^2/D10^2 : 4.98168E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 153.61 using 59 PHA bins.
# Reduced chi-squared = 2.6949 for 57 degrees of freedom
# Null hypothesis probability = 8.346003e-11
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.779e-07 6.371e-08
25- 50 1.894e-06 9.941e-08
50-150 1.263e-06 1.686e-07
15-150 3.835e-06 2.243e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.7912 (-15.7205 21.6632)
Norm : 0.690744 (-0.0535463 0.0604849)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.14 using 59 PHA bins.
# Reduced chi-squared = 0.9323 for 57 degrees of freedom
# Null hypothesis probability = 6.206767e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.898e-07 8.485e-08
25- 50 1.673e-06 8.595e-08
50-150 2.544e-06 7.387e-07
15-150 5.207e-06 7.348e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.13780 (-0.883435 0.900219)
R1^2/D10^2 : 0.198968 (-0.0671094 0.118291)
kT2 [keV] : 31.5772 (-7.60961 15.1724)
R2^2/D10^2 : 7.44963E-04 (-0.000504978 0.00116866)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.38 using 59 PHA bins.
# Reduced chi-squared = 0.8433 for 55 degrees of freedom
# Null hypothesis probability = 7.894446e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.741e-07 1.285e-07
25- 50 1.686e-06 1.977e-07
50-150 2.912e-06 9.627e-07
15-150 5.573e-06 1.332e-06
Peak spectrum fit
Power-law model
Time interval is from 6.016 sec. to 7.016 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87278 ( -0.292862 0.319117 )
Norm@50keV : 9.74355E-03 ( -0.00197756 0.00189443 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.89 using 59 PHA bins.
# Reduced chi-squared = 0.7876 for 57 degrees of freedom
# Null hypothesis probability = 8.774252e-01
Photon flux (15-150 keV) in 1 sec: 1.38250 ( -0.22457 0.22461 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.9588e-08 ( -1.75552e-08 1.79669e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.016 sec. to 7.016 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87513 ( -0.29643 0.318816 )
Epeak [keV] : 9999.33 ( )
Norm@50keV : 9.73387E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.89 using 59 PHA bins.
# Reduced chi-squared = 0.8017 for 56 degrees of freedom
# Null hypothesis probability = 8.563413e-01
Photon flux (15-150 keV) in 1 sec: 1.38332 ( -0.22771 0.2243 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.97594e-08 ( -1.95314e-08 1.50451e-08 ) ergs/cm2
Band function
Time interval is from 6.016 sec. to 7.016 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] : 10.3805 (-2.08362 2.65175)
R^2/D10^2 : 0.555694 (-0.31775 0.727891)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.94 using 59 PHA bins.
# Reduced chi-squared = 0.9990 for 57 degrees of freedom
# Null hypothesis probability = 4.771468e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.234e-08 3.835e-09
25- 50 3.231e-08 8.310e-09
50-150 1.877e-08 7.873e-09
15-150 6.341e-08 1.786e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.1164 (-39.0415 110.224)
Norm : 6.27992 (-1.34879 1.84435)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.68 using 59 PHA bins.
# Reduced chi-squared = 0.8013 for 57 degrees of freedom
# Null hypothesis probability = 8.592101e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.638e-08 3.940e-09
25- 50 2.765e-08 6.225e-09
50-150 4.184e-08 2.645e-08
15-150 8.587e-08 3.501e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.63392 (-2.2908 3.04224)
R1^2/D10^2 : 4.11491 (-3.15365 30.5386)
kT2 [keV] : 22.9539 (-9.25063 43.6549)
R2^2/D10^2 : 2.20034E-02 (-0.0206792 0.135533)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.50 using 59 PHA bins.
# Reduced chi-squared = 0.8272 for 55 degrees of freedom
# Null hypothesis probability = 8.158721e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.787e-08 1.069e-08
25- 50 2.506e-08 1.305e-08
50-150 4.582e-08 2.619e-08
15-150 8.874e-08 4.623e-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: 1.73075 ( -0.124689 0.12678 )
Norm@50keV : 2.50373E-03 ( -0.000174532 0.000172431 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.49 using 59 PHA bins.
# Reduced chi-squared = 1.202 for 57 degrees of freedom
# Null hypothesis probability = 1.416966e-01
Photon flux (15-150 keV) in 111.3 sec: 0.336176 ( -0.0218655 0.0219275 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.57437e-06 ( -1.87226e-07 1.88823e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74086 ( )
Epeak [keV] : 9999.34 ( )
Norm@50keV : 2.48964E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.55 using 59 PHA bins.
# Reduced chi-squared = 1.224 for 56 degrees of freedom
# Null hypothesis probability = 1.211815e-01
Photon flux (15-150 keV) in 111.3 sec: 0.336033 ( -0.02188 0.021899 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.57034e-06 ( -1.80718e-07 1.92972e-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) = 1.60e-06
S(50-100 keV) = 1.74e-06
T90 vs. Hardness ratio plot
T90 = 466.651999950409 sec.
Hardness ratio (energy fluence ratio) = 1.0875
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.14679
Count Ratio (50-100 keV) / (15-25 keV) = 0.615434
Mask shadow pattern
IMX = -3.068594089460298E-01, IMY = -4.511997142804530E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-330.635400 -315.316000
-239.536000 -61.548000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1202 38.4327 3.2 47.5 -172.1 -1.3659 -3.7 7.1 Cyg X-2
341.4981 -46.9783 2.1 42.1 35.0 1.9051 5.5 ------ UNKNOWN
320.3752 47.8340 2.4 57.7 -170.8 5.2113 4.9 ------ UNKNOWN
35.2136 -37.9701 2.3 55.0 -16.4 2.7588 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-61.548000 49.764620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2396 38.3639 8.7 47.4 -172.0 0.3967 1.3 4.1 Cyg X-2
318.0955 -2.3555 0.6 28.6 124.2 4.4663 20.7 ------ UNKNOWN
352.4649 7.8361 2.3 14.2 -126.0 0.7094 5.1 ------ UNKNOWN
34.7022 -26.5013 1.9 50.5 -29.7 2.2985 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
98.964600 656.364590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.0332 -24.8705 14.7 39.0 81.8 -1.3918 -0.8 3.0 HT1900.1-2455
288.8012 10.9171 2.0 32.0 145.0 4.0525 5.9 1.7 GRS 1915+105
299.5930 35.2152 1.8 41.4 -173.1 4.6990 6.4 0.8 Cyg X-1
308.0629 40.9696 2.7 44.3 -160.9 3.6564 4.2 2.4 Cyg X-3
326.2184 38.3489 6.1 41.4 -140.4 -1.5994 -1.9 2.7 Cyg X-2
275.0811 7.1951 2.0 44.0 132.9 10.8427 5.8 ------ UNKNOWN
285.4550 0.6479 2.2 32.8 124.8 3.9372 5.3 ------ UNKNOWN
318.0850 -2.3520 0.9 0.0 59.7 5.5505 12.9 ------ UNKNOWN
2.0139 -39.1319 3.9 54.3 -11.5 4.0324 3.0 ------ UNKNOWN
0.0619 -37.2831 4.8 52.0 -12.5 2.7427 2.4 ------ UNKNOWN
358.5598 -28.1833 2.4 46.4 -22.1 3.9917 4.8 ------ UNKNOWN
338.9659 41.8049 2.4 48.0 -129.1 11.7840 4.8 ------ UNKNOWN
336.3897 44.6758 2.9 49.8 -133.0 9.5286 3.9 ------ UNKNOWN
Plot creation:
Mon Aug 6 22:41:00 EDT 2018