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
166.9628 -19.7859 0.0076 33.0407 49.1241 10.7445818 25.255 TRIG_01321323
Foreground time interval of the image:
-94.507 14.293 (delta_t = 108.800 [sec])
Background time interval of the image:
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 -100.284 sec. to 116.504 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.79818 ( -0.0500969 0.0502721 )
Norm@50keV : 5.77844E-03 ( -0.000152588 0.000152443 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.92 using 59 bins.
Reduced chi-squared = 1.36702
# Null hypothesis probability of 3.43e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 216.8 sec: 0.795737 ( -0.023533 0.023632 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.15356e-05 ( -3.08955e-07 3.09261e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -100.284 sec. to 116.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48745 ( -0.218308 0.207802 )
Epeak [keV] : 84.5258 ( -15.801 64.2285 )
Norm@50keV : 8.17179E-03 ( -0.00165344 0.00220133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.30 using 59 bins.
Reduced chi-squared = 1.27321
# Null hypothesis probability of 8.18e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 216.8 sec: 0.775883 ( -0.026628 0.026764 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12484e-05 ( -3.62591e-07 3.61289e-07 ) ergs/cm2
Band function
Time interval is from -100.284 sec. to 116.504 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] : 13.7306 ( )
R^2/D10^2 : 0.109873 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 355.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.12e-45 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.502e-07 5.008e-08
25- 50 3.466e-06 1.041e-07
50-150 4.259e-06 2.168e-07
15-150 8.675e-06 2.537e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 121.007 (-16.8958 12.8314)
Norm : 3.25670 (-0.111971 0.17857)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.45e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.838e-06 1.092e-07
25- 50 3.294e-06 1.474e-07
50-150 5.902e-06 1.319e-06
15-150 1.103e-05 1.382e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.41829 (-0.802315 0.848799)
R1^2/D10^2 : 0.736398 (-0.218571 0.354279)
kT2 [keV] : 25.1724 (-2.98707 4.34125)
R2^2/D10^2 : 8.51917E-03 (-0.00384956 0.00556996)
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.02e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.696e-06 1.437e-07
25- 50 3.436e-06 1.897e-07
50-150 5.878e-06 6.135e-07
15-150 1.101e-05 7.252e-07
Peak spectrum fit
Power-law model
Time interval is from -0.004 sec. to 0.996 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25111 ( -0.122523 0.122081 )
Norm@50keV : 5.13301E-02 ( -0.00355076 0.00355032 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.36 using 59 bins.
Reduced chi-squared = 0.988772
# Null hypothesis probability of 4.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.07211 ( -0.43318 0.43406 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.13618e-07 ( -3.94634e-08 3.96429e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.004 sec. to 0.996 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24700 ( -0.323464 0.164423 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.15632E-02 ( -0.00356581 0.0222606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.38 using 59 bins.
Reduced chi-squared = 1.00679
# Null hypothesis probability of 4.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.09513 ( -0.62592 0.57954 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.61024e-07 ( -3.95957e-08 1.88465e-08 ) ergs/cm2
Band function
Time interval is from -0.004 sec. to 0.996 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] : 19.3786 ( )
R^2/D10^2 : 0.303445 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 116.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.42e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.224e-08 3.240e-09
25- 50 1.084e-07 1.149e-08
50-150 3.004e-07 3.755e-08
15-150 4.310e-07 4.055e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-15.8061 -200)
Norm : 25.1192 (-1.76764 1.76764)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.87e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.254e-08 4.850e-09
25- 50 1.203e-07 1.490e-08
50-150 2.638e-07 8.175e-08
15-150 4.467e-07 8.055e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.55593 (-1.42001 1.80708)
R1^2/D10^2 : 7.09480 (-3.99167 10.5832)
kT2 [keV] : 31.0817 (-5.32504 9.34215)
R2^2/D10^2 : 5.65717E-02 (-0.0317739 0.0490848)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.03e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.389e-08 1.942e-08
25- 50 1.071e-07 2.435e-08
50-150 3.590e-07 8.445e-08
15-150 5.200e-07 1.128e-07
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: 1.66665 ( -0.0680141 0.0681999 )
Norm@50keV : 6.31420E-03 ( -0.000234704 0.000234267 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 108.8 sec: 0.829063 ( -0.0331413 0.0332435 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.37893e-06 ( -2.46882e-07 2.47376e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50679 ( -0.280497 0.19846 )
Epeak [keV] : 158.353 ( -69.9788 -158.426 )
Norm@50keV : 7.56292E-03 ( -0.00141666 0.00273723 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.37e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 108.8 sec: 0.820353 ( -0.035915 0.036001 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.30621e-06 ( -2.77995e-07 2.75732e-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) = 3.25e-06
S(50-100 keV) = 3.73e-06
T90 vs. Hardness ratio plot
T90 = 175.784000039101 sec.
Hardness ratio (energy fluence ratio) = 1.14769
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.23728
Count Ratio (50-100 keV) / (15-25 keV) = 0.773934
Mask shadow pattern
IMX = 4.256489236012435E-01, IMY = -4.918003610058224E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-94.507400 14.292600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5375 -40.5654 0.8 9.2 137.4 3.0775 14.6 0.8 Vela X-1
170.3154 -60.4939 12.6 38.0 122.4 0.6114 0.9 7.7 Cen X-3
166.9628 -19.7860 0.5 33.0 49.1 10.7456 25.2 ------ UNKNOWN
134.9309 -20.9889 2.4 10.9 -16.3 1.0037 4.9 ------ UNKNOWN
128.6678 -19.4046 2.3 12.7 -45.0 1.0472 5.1 ------ UNKNOWN
130.4119 1.3416 2.4 33.0 -32.2 1.1874 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
85.692600 207.169500
208.992000 251.492590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5419 -40.5679 1.2 33.9 -155.1 3.1769 9.6 1.0 Vela X-1
170.3601 -60.5785 2.6 40.9 157.1 2.2617 4.4 3.0 Cen X-3
186.7973 -62.6783 3.1 45.0 146.9 3.4852 3.8 6.7 GX 301-2
166.9276 -19.7879 1.6 0.1 -107.0 1.8671 7.2 ------ UNKNOWN
115.7801 -25.4554 3.9 47.3 -127.2 3.8048 3.0 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:35:55 EDT 2025