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
291.3824 +11.1167 0.0104 43.8 -11.7 0.2940 18.5 TRIG_01350381
------------------------------------------
Foreground time interval of the image:
0.000 0.372 (delta_t = 0.372 [sec])
Background time interval of the image:
-239.664 -21.404 (delta_t = 218.260 [sec])
-14.664 0.000 (delta_t = 14.664 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
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 0.372 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65581 ( -0.165893 0.170393 )
Norm@50keV : 4.82246E-02 ( -0.00496699 0.00492491 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.26 using 59 PHA bins.
# Reduced chi-squared = 0.9695 for 57 degrees of freedom
# Null hypothesis probability = 5.405225e-01
Photon flux (15-150 keV) in 0.372 sec: 6.30906 ( -0.639866 0.641136 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66748e-07 ( -1.80243e-08 1.81309e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.372 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45949 ( -0.724147 0.357229 )
Epeak [keV] : 142.590 ( -142.583 -142.583 )
Norm@50keV : 6.04723E-02 ( -0.0144703 0.0759291 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.00 using 59 PHA bins.
# Reduced chi-squared = 0.9822 for 56 degrees of freedom
# Null hypothesis probability = 5.126218e-01
Photon flux (15-150 keV) in 0.372 sec: 6.26808 ( -0.65411 0.65316 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.65563e-07 ( -1.86569e-08 1.85959e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.372 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51576 ( 1.51574 0.541607 )
beta : -2.77322 ( 9.09657 19.0966 )
Epeak [keV] : 181.552 ( -104.05 -181.459 )
Norm@50keV : 5.65780E-02 ( -0.00554971 0.034509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.02 using 59 PHA bins.
# Reduced chi-squared = 1.000 for 55 degrees of freedom
# Null hypothesis probability = 4.736899e-01
Photon flux (15-150 keV) in 0.372 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] : 14.6378 (-1.67913 1.90162)
R^2/D10^2 : 0.773313 (-0.277944 0.426354)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.74 using 59 PHA bins.
# Reduced chi-squared = 1.452 for 57 degrees of freedom
# Null hypothesis probability = 1.457153e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.295e-08 2.703e-09
25- 50 5.031e-08 6.715e-09
50-150 7.254e-08 1.375e-08
15-150 1.358e-07 1.815e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 160.054 (-56.0919 -161.744)
Norm : 25.8514 (-2.84751 3.30338)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.455e-08 5.813e-09
25- 50 4.593e-08 1.626e-08
50-150 9.307e-08 4.916e-08
15-150 1.636e-07 7.593e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.54396 (-1.5798 2.71339)
R1^2/D10^2 : 34.5318 (-28.7798 256.607)
kT2 [keV] : 20.1855 (-3.5094 6.76201)
R2^2/D10^2 : 0.207232 (-0.14129 0.208251)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.700e-08 1.293e-08
25- 50 4.097e-08 1.296e-08
50-150 9.171e-08 2.701e-08
15-150 1.597e-07 4.678e-08
Peak spectrum fit
Power-law model
Time interval is from -0.312 sec. to 0.688 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51909 ( -0.204241 0.208398 )
Norm@50keV : 1.92837E-02 ( -0.00238699 0.00237671 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.06 using 59 PHA bins.
# Reduced chi-squared = 0.9308 for 57 degrees of freedom
# Null hypothesis probability = 6.237134e-01
Photon flux (15-150 keV) in 1 sec: 2.41994 ( -0.304659 0.305348 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.82378e-07 ( -2.41891e-08 2.43151e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.312 sec. to 0.688 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16359 ( -0.954561 0.530632 )
Epeak [keV] : 125.953 ( -125.95 -125.95 )
Norm@50keV : 2.86467E-02 ( -0.0114382 0.0519845 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.51 using 59 PHA bins.
# Reduced chi-squared = 0.9376 for 56 degrees of freedom
# Null hypothesis probability = 6.078956e-01
Photon flux (15-150 keV) in 1 sec: 2.38866 ( -0.31382 0.31316 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.80043e-07 ( -2.5228e-08 2.5061e-08 ) ergs/cm2
Band function
Time interval is from -0.312 sec. to 0.688 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.16444 ( 1.24728 0.818539 )
beta : -10.00000 ( 10 20 )
Epeak [keV] : 126.076 ( -50.5152 -126.076 )
Norm@50keV : 2.86193E-02 ( -0.0114149 0.00846644 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.51 using 59 PHA bins.
# Reduced chi-squared = 0.9547 for 55 degrees of freedom
# Null hypothesis probability = 5.704665e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.82554e-07 ( -1.82547e-07 -1.82554e-07 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.8405 (-2.15081 2.58588)
R^2/D10^2 : 0.232153 (-0.0967531 0.156851)
(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 1.207e-08 2.553e-09
25- 50 5.036e-08 1.010e-08
50-150 8.798e-08 2.049e-08
15-150 1.504e-07 2.365e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.349 (-72.5857 -199.357)
Norm : 9.95402 (-1.20645 1.20843)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.479e-08 7.805e-09
25- 50 4.768e-08 2.636e-08
50-150 1.046e-07 5.747e-08
15-150 1.770e-07 9.755e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.57676 (-1.69128 7.03126)
R1^2/D10^2 : 34.5179 (-33.9676 2043.23)
kT2 [keV] : 19.3969 (-3.53336 19.7933)
R2^2/D10^2 : 0.103805 (-0.0971889 0.114027)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.540e-08 1.212e-08
25- 50 4.178e-08 1.250e-08
50-150 1.032e-07 3.421e-08
15-150 1.704e-07 4.463e-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: 1.65581 ( -0.165893 0.170393 )
Norm@50keV : 4.82246E-02 ( -0.00496699 0.00492491 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.26 using 59 PHA bins.
# Reduced chi-squared = 0.9695 for 57 degrees of freedom
# Null hypothesis probability = 5.405225e-01
Photon flux (15-150 keV) in 0.372 sec: 6.30906 ( -0.639866 0.641136 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66748e-07 ( -1.80243e-08 1.81309e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45949 ( -0.724147 0.357229 )
Epeak [keV] : 142.590 ( -142.583 -142.583 )
Norm@50keV : 6.04723E-02 ( -0.0144703 0.0759291 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.00 using 59 PHA bins.
# Reduced chi-squared = 0.9822 for 56 degrees of freedom
# Null hypothesis probability = 5.126218e-01
Photon flux (15-150 keV) in 0.372 sec: 6.26808 ( -0.65411 0.65316 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.65563e-07 ( -1.86569e-08 1.85959e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51576 ( 1.51574 0.541604 )
beta : -2.77322 ( 9.09657 19.0966 )
Epeak [keV] : 181.552 ( -104.05 -181.459 )
Norm@50keV : 5.65780E-02 ( -0.00554971 0.034509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.02 using 59 PHA bins.
# Reduced chi-squared = 1.000 for 55 degrees of freedom
# Null hypothesis probability = 4.736899e-01
Photon flux (15-150 keV) in 0.372 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) = 4.43e-08
S(50-100 keV) = 5.62e-08
T90 vs. Hardness ratio plot
T90 = 0.287999987602234 sec.
Hardness ratio (energy fluence ratio) = 1.26862
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29821
Count Ratio (50-100 keV) / (15-25 keV) = 1.08364
Mask shadow pattern
IMX = 9.397117595923099E-01, IMY = 1.944700519328101E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000
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:
-239.664000 -21.404000
-14.664000 0.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.1407 -24.9230 4.7 37.0 -68.7 -1.6229 -2.4 5.7 HT1900.1-2455
288.7993 10.9458 30.4 45.6 -14.2 0.1964 0.4 0.1 GRS 1915+105
333.1827 -34.9125 2.4 18.5 -164.3 1.3290 4.7 ------ UNKNOWN
275.6144 16.7847 2.6 59.4 -17.9 5.8487 4.5 ------ UNKNOWN
327.1661 -71.2842 2.4 53.1 -142.2 7.7317 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.372000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
284.8920 -24.9899 6.7 37.2 -68.8 0.0328 1.7 8.9 HT1900.1-2455
288.7957 11.1049 7.5 45.7 -14.0 -0.0272 -1.5 9.6 GRS 1915+105
2.1744 -17.1226 2.7 35.9 133.2 0.0699 4.2 ------ UNKNOWN
308.3984 29.6345 2.1 50.2 20.7 0.2010 5.4 ------ UNKNOWN
291.3824 11.1167 0.6 43.8 -11.7 0.2941 18.5 ------ UNKNOWN
304.9458 -59.6520 2.0 43.8 -127.0 0.1585 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
116.236590 185.516000
186.336000 192.536000
193.336000 193.516000
194.336000 306.386000
307.336000 650.146000
651.336000 652.162900
653.336000 665.946000
668.336000 764.216000
765.336000 768.506000
769.336000 775.636000
776.336000 962.447200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2858 35.4335 0.0 41.4 -55.5 2.8731 0.9 10.0 Her X-1
256.4384 -36.4077 59.6 57.8 -154.6 -1.3939 -0.2 0.9 GX 349+2
263.0085 -24.7453 12.3 45.3 -150.2 2.3263 0.9 0.0 GX 1+4
268.3678 -1.4520 37.4 26.1 -125.0 -0.4606 -0.3 0.0 SW J1753.5-0127
270.1541 -25.0715 11.3 41.7 -158.0 2.0985 1.0 7.1 GX 5-1
270.2050 -25.8696 8.9 42.4 -158.7 2.7697 1.3 9.2 GRS 1758-258
273.8810 -13.8633 0.0 30.4 -152.4 4.6956 3.0 12.7 GX 17+2
275.9442 -30.4210 5.6 44.1 -168.3 4.0343 2.0 3.4 H1820-303
284.9050 -24.8999 6.1 36.6 -177.7 3.0684 1.9 7.2 HT1900.1-2455
288.6902 11.1097 31.3 2.6 -97.8 0.4125 0.4 11.7 GRS 1915+105
299.6055 35.1997 0.4 25.2 8.4 32.3374 26.7 0.8 Cyg X-1
307.9293 40.9239 5.7 33.2 15.6 3.4539 2.0 8.4 Cyg X-3
326.1650 38.2809 5.2 41.2 35.3 5.7143 2.2 2.5 Cyg X-2
262.9823 -33.7409 10.0 52.4 -157.6 -3.8354 -1.2 5.6 GX 354-0
324.0814 12.0622 3.2 32.0 77.4 8.7267 3.6 ------ UNKNOWN
311.3780 19.1573 2.8 20.9 57.4 5.7929 4.2 ------ UNKNOWN
286.1487 10.7148 2.3 5.2 -101.7 5.2731 5.1 ------ UNKNOWN
252.1366 -25.8199 2.7 53.1 -142.2 26.9861 4.3 ------ UNKNOWN
Plot creation:
Thu Sep 18 13:22:52 EDT 2025