Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
299.5149 +35.0608 0.0373 31.8 -15.1 0.9012 5.2 TRIG_01148770
------------------------------------------
Foreground time interval of the image:
-27.240 41.505 (delta_t = 68.745 [sec])
Background time interval of the image:
-239.096 -27.240 (delta_t = 211.856 [sec])
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
-27.240000 174.474000
175.904000 470.432000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42928 ( -0.184226 0.197718 )
Norm@50keV : 6.75222E-04 ( -9.9586e-05 9.90495e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.82 using 59 PHA bins.
# Reduced chi-squared = 0.9091 for 57 degrees of freedom
# Null hypothesis probability = 6.692375e-01
Photon flux (15-150 keV) in 496.2 sec: 0.127107 ( -0.0118545 0.0118545 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.29059e-06 ( -3.75149e-07 3.85763e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-27.240000 174.474000
175.904000 470.432000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.590789 ( -1.45289 1.06049 )
Epeak [keV] : 26.5009 ( -11.4362 5.00048 )
Norm@50keV : 1.02666E-02 ( -0.0102676 0.0867553 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.05 using 59 PHA bins.
# Reduced chi-squared = 0.7330 for 56 degrees of freedom
# Null hypothesis probability = 9.329601e-01
Photon flux (15-150 keV) in 496.2 sec: 0.121892 ( -0.011927 0.011997 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.85396e-06 ( -3.56664e-07 3.99585e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-27.240000 174.474000
175.904000 470.432000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.384893 ( -0.987505 0.663078 )
beta : -3.36395 ( 9.37167 19.3714 )
Epeak [keV] : 26.6991 ( -5.7617 5.13093 )
Norm@50keV : 5.21071E-02 ( -0.0506627 85.8886 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.43 using 59 PHA bins.
# Reduced chi-squared = 0.7350 for 55 degrees of freedom
# Null hypothesis probability = 9.292930e-01
Photon flux (15-150 keV) in 496.2 sec: 0.122100 ( 6.8779 -0.012165 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.84991e-06 ( -2.84644e-06 -3.51726e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.43409 (-0.696592 0.768845)
R^2/D10^2 : 0.191003 (-0.0637827 0.0962891)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.79 using 59 PHA bins.
# Reduced chi-squared = 0.8208 for 57 degrees of freedom
# Null hypothesis probability = 8.307033e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.919e-07 1.404e-07
25- 50 1.369e-06 1.868e-07
50-150 2.806e-07 9.157e-08
15-150 2.541e-06 3.166e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.6015 (-6.58737 8.77596)
Norm : 0.941173 (-0.163825 0.206778)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.003e-06 1.109e-07
25- 50 1.216e-06 1.414e-07
50-150 7.690e-07 2.609e-07
15-150 2.988e-06 3.667e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.85938 (-2.27141 1.32386)
R1^2/D10^2 : 0.390065 (-0.191149 1.25784)
kT2 [keV] : 14.5785 (-10.7944 15.2427)
R2^2/D10^2 : 5.26017E-03 (-0.00505087 0.0412114)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.693e-07 4.390e-07
25- 50 1.258e-06 5.824e-07
50-150 7.112e-07 4.230e-07
15-150 2.939e-06 1.353e-06
Peak spectrum fit
Power-law model
Time interval is from 117.596 sec. to 118.596 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.92609 ( -2.45588 -1.92655 )
Norm@50keV : 5.38514E-03 ( -0.00538379 0.00535961 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.92 using 59 PHA bins.
# Reduced chi-squared = 0.5951 for 57 degrees of freedom
# Null hypothesis probability = 9.935372e-01
Photon flux (15-150 keV) in 1 sec: 0.781518 ( -0.532002 0.532772 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.95173e-08 ( -4.43324e-08 8.79951e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 117.596 sec. to 118.596 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83977 ( -1.89053 6.14007 )
Epeak [keV] : 89.0316 ( )
Norm@50keV : 5.89947E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.93 using 59 PHA bins.
# Reduced chi-squared = 0.6058 for 56 degrees of freedom
# Null hypothesis probability = 9.913952e-01
Photon flux (15-150 keV) in 1 sec: 0.781051 ( -0.781051 0.531709 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.86832e-08 ( -4.86832e-08 8.75268e-08 ) ergs/cm2
Band function
Time interval is from 117.596 sec. to 118.596 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.43100 ( 1.46976 1.46976 )
beta : -1.83315 ( 1.91683 1.91683 )
Epeak [keV] : 20.4847 ( -15.0912 -15.0912 )
Norm@50keV : 1.36927E-02 ( -0.0151652 1.44596 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.93 using 59 PHA bins.
# Reduced chi-squared = 0.6169 for 55 degrees of freedom
# Null hypothesis probability = 9.886655e-01
Photon flux (15-150 keV) in 1 sec: 1.25688 ( 5.74312 -0.12885 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.97648 (-7.97648 -7.97648)
R^2/D10^2 : 0.849941 (-0.849938 -0.849938)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.757e-09 6.690e-09
25- 50 1.699e-08 1.286e-08
50-150 4.418e-09 4.216e-09
15-150 3.117e-08 2.398e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.5009 (-69.637 -69.637)
Norm : 3.72956 (-3.72612 172.511)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.561e-09 6.640e-09
25- 50 1.518e-08 1.109e-08
50-150 1.940e-08 1.697e-08
15-150 4.414e-08 3.464e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.19149 (-1.34076 9.2164)
R1^2/D10^2 : 2.80168E+05 (-279295 4.399e+07)
kT2 [keV] : 20.5615 (-15.9515 -20.6598)
R2^2/D10^2 : 2.56463E-02 (-0.0252377 0.419735)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.142e-08 6.620e-09
25- 50 9.910e-09 5.830e-09
50-150 3.713e-08 2.948e-08
15-150 5.846e-08 3.744e-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: 2.37851 ( -0.144787 0.15194 )
Norm@50keV : 2.41037E-03 ( -0.00024933 0.000246274 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.45 using 59 PHA bins.
# Reduced chi-squared = 1.026 for 57 degrees of freedom
# Null hypothesis probability = 4.217356e-01
Photon flux (15-150 keV) in 68.74 sec: 0.440434 ( -0.031571 0.0315937 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.60853e-06 ( -1.31674e-07 1.33683e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52056 ( -0.809952 0.406164 )
Epeak [keV] : 21.1476 ( )
Norm@50keV : 8.01139E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.41 using 59 PHA bins.
# Reduced chi-squared = 0.9538 for 56 degrees of freedom
# Null hypothesis probability = 5.733304e-01
Photon flux (15-150 keV) in 68.74 sec: 0.425195 ( -0.033416 0.033515 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47979e-06 ( -1.48733e-07 1.6004e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.15547 ( -0.718816 1.15896 )
beta : -2.88541 ( 2.88708 0.463657 )
Epeak [keV] : 24.0351 ( -12.8468 6.2901 )
Norm@50keV : 1.43381E-02 ( -0.00484324 628.707 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.81 using 59 PHA bins.
# Reduced chi-squared = 0.9603 for 55 degrees of freedom
# Null hypothesis probability = 5.585930e-01
Photon flux (15-150 keV) in 68.74 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50639e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.08e-06
S(50-100 keV) = 8.04e-07
T90 vs. Hardness ratio plot
T90 = 234.299999952316 sec.
Hardness ratio (energy fluence ratio) = 0.744444
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.921705
Count Ratio (50-100 keV) / (15-25 keV) = 0.270667
Mask shadow pattern
IMX = 5.993148535282942E-01, IMY = 1.619439026318902E-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:
-239.096000 -27.240000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.8809 11.0113 4.9 46.8 -49.4 3.1966 2.4 6.3 GRS 1915+105
299.5451 35.1274 0.6 31.8 -15.0 8.3607 20.0 5.0 Cyg X-1
308.0964 40.9421 3.7 26.6 -0.2 1.2766 3.1 0.9 Cyg X-3
326.2377 38.4622 7.0 13.9 18.8 0.5888 1.6 9.0 Cyg X-2
23.7854 32.0231 3.5 41.8 122.6 7.5556 3.3 ------ UNKNOWN
316.4551 70.2401 2.5 44.5 42.2 3.0080 4.6 ------ UNKNOWN
21.3957 18.0551 3.0 42.9 143.6 5.7486 3.9 ------ UNKNOWN
21.1051 -0.8248 2.8 51.8 166.4 9.0876 4.1 ------ UNKNOWN
267.4212 54.6633 2.8 55.8 10.8 5.8061 4.0 ------ UNKNOWN
18.2231 1.4118 3.8 48.1 166.3 5.1436 3.1 ------ UNKNOWN
265.0336 50.1161 3.3 57.4 5.4 6.5794 3.5 ------ UNKNOWN
12.2369 -4.6832 2.8 47.5 177.8 4.6909 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-27.240000 41.504600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7068 11.1305 15.9 46.9 -49.1 -0.4845 -0.7 12.3 GRS 1915+105
299.5230 35.0846 2.3 31.8 -15.1 0.8876 5.1 7.8 Cyg X-1
308.3602 41.0184 54.7 26.4 0.2 0.0341 0.2 12.0 Cyg X-3
326.2864 38.2510 6.1 13.7 18.4 0.2584 1.9 6.9 Cyg X-2
334.0592 59.0993 2.4 32.0 49.7 0.9213 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
210.204590 339.504590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
359.9578 -16.9245 3.8 43.7 3.8 1.0461 3.0 ------ UNKNOWN
348.8792 -63.0177 2.7 3.1 179.8 0.9475 4.3 ------ UNKNOWN
Plot creation:
Sat Jan 14 04:23:42 EST 2023