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
263.1146 +54.0629 0.0455 6.2 35.4 0.0980 4.2 TRIG_01045571
------------------------------------------
Foreground time interval of the image:
0.000 1.024 (delta_t = 1.024 [sec])
Background time interval of the image:
-60.624 -10.624 (delta_t = 50.000 [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
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.07802 ( -1.38034 1.55997 )
Norm@50keV : 1.36725E-03 ( -0.00136725 0.00253814 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.024 sec: 0.319884 ( -0.319884 0.218638 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.35432e-08 ( -5.35431e-08 2.98168e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.10407 ( 1.32756 1.80426 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.41078E-03 ( -0.0014108 -0.0014108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.67e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.024 sec: 0.329149 ( -0.329149 0.209178 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43927e-08 ( -5.43927e-08 3.15853e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.501525 ( -0.50546 -0.50546 )
beta : 1.07808 ( -1.07804 1.37986 )
Epeak [keV] : 19.1825 ( -19.1961 -19.1961 )
Norm@50keV : 2.59427E-03 ( -0.0025958 510.446 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1.024 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] : 199.363 (-199.363 -199.363)
R^2/D10^2 : 1.93791E-04 (-0.000104782 0.00462782)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.540e-10 1.119e-10
25- 50 2.158e-09 7.880e-10
50-150 5.254e-08 2.175e-08
15-150 5.495e-08 2.714e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.00000 (-7 -7)
Norm : 0.0 (0 0)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.09e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.79677 (-2.39338 -2.39338)
R1^2/D10^2 : 7.91082E-06 (-1.52385e-09 -1.52385e-09)
kT2 [keV] : 199.333 (-199.344 -199.344)
R2^2/D10^2 : 1.94978E-04 (-0.000104781 0.00463182)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.57e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.556e-10 3.324e-09
25- 50 2.171e-09 3.979e-08
50-150 5.285e-08 1.179e-06
15-150 5.528e-08 8.494e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.07802 ( -1.38034 1.55997 )
Norm@50keV : 1.36725E-03 ( -0.00136725 0.00253814 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.024 sec: 0.319884 ( -0.319884 0.218638 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.35432e-08 ( -5.35431e-08 2.98168e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.10407 ( 1.32756 1.80426 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.41078E-03 ( -0.0014108 -0.0014108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.67e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.024 sec: 0.329149 ( -0.329149 0.209178 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43927e-08 ( -5.43927e-08 3.15853e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.501525 ( -0.50546 -0.50546 )
beta : 1.07808 ( -1.07804 1.37986 )
Epeak [keV] : 19.1825 ( -19.1961 -19.1961 )
Norm@50keV : 2.59427E-03 ( -0.0025958 510.446 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1.024 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] : 199.363 (-199.363 -199.363)
R^2/D10^2 : 1.93791E-04 (-0.000104782 0.00462782)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.540e-10 8.617e-11
25- 50 2.158e-09 9.334e-10
50-150 5.254e-08 2.093e-08
15-150 5.495e-08 2.685e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.00000 (-7 -7)
Norm : 0.0 (0 0)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.09e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.79677 (-2.39338 -2.39338)
R1^2/D10^2 : 7.91082E-06 (-1.52385e-09 -1.52385e-09)
kT2 [keV] : 199.333 (-199.344 -199.344)
R2^2/D10^2 : 1.94978E-04 (-0.000104781 0.00463182)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.57e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.556e-10 3.838e-09
25- 50 2.171e-09 3.501e-08
50-150 5.285e-08 7.803e-07
15-150 5.528e-08 1.422e-06
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: -1.07802 ( -1.38034 1.55997 )
Norm@50keV : 1.36725E-03 ( -0.00136725 0.00253814 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.024 sec: 0.319884 ( -0.319884 0.218638 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.35432e-08 ( -5.35431e-08 2.98168e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.10407 ( 1.32756 1.80342 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.41078E-03 ( -0.0014108 -0.0014108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.67e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.024 sec: 0.329149 ( -0.329149 0.209178 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43927e-08 ( -5.43927e-08 3.15853e-08 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.501525 ( -0.50546 -0.50546 )
beta : 1.07808 ( -1.07804 1.37986 )
Epeak [keV] : 19.1825 ( -19.1961 -19.1961 )
Norm@50keV : 2.59427E-03 ( -0.0025958 510.446 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1.024 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) = 1.61e-09
S(50-100 keV) = 1.36e-08
T90 vs. Hardness ratio plot
T90 = 1.02400004863739 sec.
Hardness ratio (energy fluence ratio) = 8.4472
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = -4.03433
Count Ratio (50-100 keV) / (15-25 keV) = -115.974
Mask shadow pattern
IMX = 8.793429077259836E-02, IMY = -6.250148028793873E-02
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:
-60.624000 -10.624000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3989 35.5142 22.8 24.7 63.9 -0.1717 -0.5 10.7 Her X-1
288.7191 10.8879 12.3 53.5 17.1 1.0748 0.9 5.8 GRS 1915+105
299.5151 35.1337 5.3 35.5 -10.6 0.7841 2.2 5.5 Cyg X-1
308.1830 40.9749 6.8 35.0 -26.1 0.6087 1.7 3.6 Cyg X-3
326.1971 38.3911 33.4 45.9 -39.9 -0.2456 -0.3 4.3 Cyg X-2
263.7606 13.4985 2.7 46.6 48.0 4.2784 4.2 ------ UNKNOWN
201.4324 36.0922 2.6 43.8 137.2 3.9967 4.4 ------ UNKNOWN
293.8929 10.2792 3.1 55.7 11.4 4.9513 3.7 ------ UNKNOWN
174.7489 54.6241 2.9 43.1 175.5 1.7402 4.0 ------ UNKNOWN
232.5211 71.0284 2.9 15.6 -160.7 1.0721 4.0 ------ UNKNOWN
152.7570 52.7648 3.2 53.1 -173.2 2.4444 3.7 ------ UNKNOWN
128.4000 56.0282 2.7 57.8 -156.5 5.5709 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 1.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5783 35.4554 5.9 24.8 63.5 0.0576 2.0 9.0 Her X-1
288.9973 10.8835 0.0 53.6 16.8 0.1029 1.1 12.3 GRS 1915+105
299.5698 35.3579 7.2 35.4 -10.9 0.0477 1.6 9.4 Cyg X-1
308.2750 40.8416 12.2 35.1 -26.1 -0.0296 -0.9 10.0 Cyg X-3
326.3562 38.4128 3.5 46.0 -40.1 0.2083 3.3 10.3 Cyg X-2
231.2054 30.6875 2.0 35.0 99.2 0.2755 5.9 ------ UNKNOWN
297.0331 27.1760 2.3 41.4 -1.2 0.1912 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Wed Apr 28 16:52:12 EDT 2021