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
299.5585 +35.0831 0.0167 37.3 -171.0 5.8591 11.6 TRIG_01143281
------------------------------------------
Foreground time interval of the image:
-143.999 70.201 (delta_t = 214.200 [sec])
Background time interval of the image:
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
Time interval is from -148.692 sec. to 345.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.29216 ( -0.135057 0.140435 )
Norm@50keV : 1.10299E-03 ( -9.81406e-05 9.65568e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.51 using 59 PHA bins.
# Reduced chi-squared = 0.5880 for 57 degrees of freedom
# Null hypothesis probability = 9.944561e-01
Photon flux (15-150 keV) in 494.6 sec: 0.191920 ( -0.012459 0.0124887 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.20576e-06 ( -3.7821e-07 3.83077e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -148.692 sec. to 345.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98827 ( -1.98827 -1.98827 )
Epeak [keV] : 1.57907 ( -0.528476 23.2031 )
Norm@50keV : 1.65168E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.17 using 59 PHA bins.
# Reduced chi-squared = 0.6101 for 56 degrees of freedom
# Null hypothesis probability = 9.906304e-01
Photon flux (15-150 keV) in 494.6 sec: 0.191450 ( -0.013447 0.012836 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.18168e-06 ( -4.82903e-07 4.02456e-07 ) ergs/cm2
Band function
Time interval is from -148.692 sec. to 345.864 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.425276 ( 1.30619 1.30619 )
beta : -2.37307 ( 2.37773 0.19113 )
Epeak [keV] : 21.1945 ( -19.9347 7.7303 )
Norm@50keV : 2.70228E-02 ( -0.0267541 449.31 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 32.36 using 59 PHA bins.
# Reduced chi-squared = 0.5884 for 55 degrees of freedom
# Null hypothesis probability = 9.935976e-01
Photon flux (15-150 keV) in 494.6 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] : 8.36150 (-0.66179 0.720146)
R^2/D10^2 : 0.165292 (-0.0474775 0.0671274)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 88.50 using 59 PHA bins.
# Reduced chi-squared = 1.553 for 57 degrees of freedom
# Null hypothesis probability = 4.740117e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.066e-06 1.222e-07
25- 50 2.012e-06 1.669e-07
50-150 6.096e-07 1.305e-07
15-150 3.687e-06 2.787e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 44.0135 (-7.40857 9.60996)
Norm : 1.13747 (-0.148583 0.177445)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.331e-06 1.222e-07
25- 50 1.822e-06 1.286e-07
50-150 1.560e-06 3.099e-07
15-150 4.713e-06 3.722e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.51928 (-0.955808 1.02248)
R1^2/D10^2 : 0.729124 (-0.339682 0.776843)
kT2 [keV] : 20.0777 (-5.23545 11.02)
R2^2/D10^2 : 3.26040E-03 (-0.00250292 0.00781613)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.407e-06 2.649e-07
25- 50 1.685e-06 3.569e-07
50-150 1.936e-06 1.026e-06
15-150 5.028e-06 1.394e-06
Peak spectrum fit
Power-law model
Time interval is from 54.888 sec. to 55.888 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52033 ( -0.945828 0.980233 )
Norm@50keV : 5.30487E-03 ( -0.0023289 0.00200278 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.34 using 59 PHA bins.
# Reduced chi-squared = 0.8656 for 57 degrees of freedom
# Null hypothesis probability = 7.546846e-01
Photon flux (15-150 keV) in 1 sec: 0.666032 ( -0.256934 0.262234 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.01449e-08 ( -2.17795e-08 2.15152e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 54.888 sec. to 55.888 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.00543 ( -2.99396 0.538617 )
Epeak [keV] : 473.627 ( )
Norm@50keV : 4.49608E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.45 using 59 PHA bins.
# Reduced chi-squared = 0.8474 for 56 degrees of freedom
# Null hypothesis probability = 7.849495e-01
Photon flux (15-150 keV) in 1 sec: 0.679353 0.666736 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.87468e-08 ( -2.01069e-08 2.30576e-08 ) ergs/cm2
Band function
Time interval is from 54.888 sec. to 55.888 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.22558 ( 1.22596 1.22596 )
beta : -1.51916 ( 1.52124 0.945721 )
Epeak [keV] : 26.9054 ( -26.9718 -26.9718 )
Norm@50keV : 1.13482E-02 ( -0.0113655 0.257867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.34 using 59 PHA bins.
# Reduced chi-squared = 0.8971 for 55 degrees of freedom
# Null hypothesis probability = 6.898294e-01
Photon flux (15-150 keV) in 1 sec: ( ) 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] : 22.8318 (-18.7333 -23.1865)
R^2/D10^2 : 1.62298E-02 (-0.0149291 24.2106)
(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 1.085e-08 6.850e-09
25- 50 6.387e-09 4.077e-09
50-150 2.115e-10 2.745e-10
15-150 1.745e-08 1.081e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-199.362 -199.362)
Norm : 2.67625 (-1.0138 1.0157)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.664e-09 4.250e-09
25- 50 1.282e-08 8.135e-09
50-150 2.812e-08 1.747e-08
15-150 4.760e-08 3.047e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.10863 (-1.80191 2.02839)
R1^2/D10^2 : 10.2971 (-9.70773 253.971)
kT2 [keV] : 83.8990 (-65.0978 -86.1306)
R2^2/D10^2 : 5.51279E-04 (-0.000450719 0.0184798)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.092e-08 6.935e-09
25- 50 6.327e-09 3.623e-09
50-150 3.923e-08 2.485e-08
15-150 5.648e-08 3.058e-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: 2.25448 ( -0.202135 0.215436 )
Norm@50keV : 1.07477E-03 ( -0.000161628 0.000158745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.63 using 59 PHA bins.
# Reduced chi-squared = 0.8004 for 57 degrees of freedom
# Null hypothesis probability = 8.604183e-01
Photon flux (15-150 keV) in 214.2 sec: 0.183186 ( -0.0187 0.0187011 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.18259e-06 ( -2.71959e-07 2.79343e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.89653 ( -1.18335 0.0916398 )
Epeak [keV] : 10.4963 ( )
Norm@50keV : 1.81106E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.19 using 59 PHA bins.
# Reduced chi-squared = 0.8070 for 56 degrees of freedom
# Null hypothesis probability = 8.487963e-01
Photon flux (15-150 keV) in 214.2 sec: 0.180955 ( -0.019543 0.019488 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.08255e-06 ( -3.57774e-07 3.56266e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99320 ( -5.55512 -4.9932 )
beta : -2.55746 ( -0.421384 0.29204 )
Epeak [keV] : 22.2860 ( -3.7247 2.80993 )
Norm@50keV : 486.581 ( -49.0242 1214.88 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.09 using 59 PHA bins.
# Reduced chi-squared = 0.7108 for 55 degrees of freedom
# Null hypothesis probability = 9.483126e-01
Photon flux (15-150 keV) in 214.2 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) = 1.68e-06
S(50-100 keV) = 1.37e-06
T90 vs. Hardness ratio plot
T90 = 458.452000021935 sec.
Hardness ratio (energy fluence ratio) = 0.815476
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.940387
Count Ratio (50-100 keV) / (15-25 keV) = 0.391681
Mask shadow pattern
IMX = -7.536063648928708E-01, IMY = 1.199777000842203E-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:
-143.999410 70.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6099 35.3278 3.8 12.4 -93.6 1.2142 3.1 7.5 Her X-1
288.7932 10.8183 14.4 48.1 -135.3 1.0531 0.8 7.6 GRS 1915+105
299.5594 35.0851 1.0 37.3 -171.0 5.8634 11.6 7.2 Cyg X-1
308.1030 40.9329 23.2 40.0 175.4 0.2837 0.5 1.2 Cyg X-3
326.0732 38.3020 4.5 53.1 168.3 4.3829 2.6 4.8 Cyg X-2
193.3536 56.5416 2.8 35.8 44.1 2.6666 4.2 ------ UNKNOWN
311.6318 27.8913 2.2 49.9 -171.8 5.4608 5.2 ------ UNKNOWN
229.4236 26.0306 2.2 27.8 -35.5 2.4140 5.3 ------ UNKNOWN
228.2939 11.8192 2.2 40.8 -46.0 3.5521 5.3 ------ UNKNOWN
300.4013 13.7271 2.5 52.5 -149.4 5.0573 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
155.800600 693.090000
722.000000 785.250000
786.000000 786.890000
788.000000 788.130000
811.000000 811.260000
812.000000 872.840000
883.000000 899.390000
901.000000 902.280000
903.000000 924.000580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6083 35.2494 35.0 36.4 -32.8 0.4783 0.3 9.3 Her X-1
288.6698 11.0123 13.9 26.1 -111.4 0.9582 0.8 8.6 GRS 1915+105
299.5945 35.2098 0.6 0.1 44.5 20.9571 19.3 0.5 Cyg X-1
308.0523 40.9557 1.9 8.9 89.7 6.6075 6.1 2.6 Cyg X-3
326.2373 38.5126 6.4 21.5 116.6 -2.3649 -1.8 11.9 Cyg X-2
281.6154 65.3414 2.2 32.1 29.5 8.0618 5.3 ------ UNKNOWN
265.5371 35.5340 2.4 27.7 -35.5 6.0265 4.8 ------ UNKNOWN
252.2366 18.7501 2.2 44.8 -55.1 17.6576 5.2 ------ UNKNOWN
Plot creation:
Mon Dec 5 16:01:02 EST 2022