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
352.8818 -2.9961 0.0184 47.4 -149.3 6.5791 10.3 TRIG_01500287
------------------------------------------
Foreground time interval of the image:
4.092 54.890 (delta_t = 50.798 [sec])
56.000 155.801 (delta_t = 99.801 [sec])
Background time interval of the image:
-67.499 -55.880 (delta_t = 11.619 [sec])
-55.000 4.092 (delta_t = 59.092 [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
4.092200 54.890000
56.000000 180.168200
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.63942 ( )
Norm@50keV : 1.66221E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 168.48 using 59 PHA bins.
# Reduced chi-squared = 2.9559 for 57 degrees of freedom
# Null hypothesis probability = 5.965604e-13
Photon flux (15-150 keV) in 175 sec: 0.356541 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.03152e-06 ( 0 0 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
4.092200 54.890000
56.000000 180.168200
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85017 ( )
Epeak [keV] : 12.3746 ( )
Norm@50keV : 3.58830E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 175.96 using 59 PHA bins.
# Reduced chi-squared = 3.1421 for 56 degrees of freedom
# Null hypothesis probability = 2.561485e-14
Photon flux (15-150 keV) in 175 sec: 0.356296 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.00984e-06 ( 0 0 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
4.092200 54.890000
56.000000 180.168200
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.98037 ( )
beta : -9.37167 ( )
Epeak [keV] : 2.06060 ( )
Norm@50keV : 3.09779E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 174.48 using 59 PHA bins.
# Reduced chi-squared = 3.1724 for 55 degrees of freedom
# Null hypothesis probability = 2.375168e-14
Photon flux (15-150 keV) in 175 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] : 11.1492 ( )
R^2/D10^2 : 8.73901E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 220.25 using 59 PHA bins.
# Reduced chi-squared = 3.8640 for 57 degrees of freedom
# Null hypothesis probability = 4.892593e-21
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.982e-07 7.753e-08
25- 50 1.146e-06 1.491e-07
50-150 8.127e-07 2.003e-07
15-150 2.357e-06 3.098e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 45.8853 ( )
Norm : 1.88155 ( )
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.881e-07 1.072e-07
25- 50 1.096e-06 1.331e-07
50-150 9.794e-07 2.466e-07
15-150 2.864e-06 3.500e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.71551 (-0.20193 0.238645)
R1^2/D10^2 : 5840.60 (-4250.48 16561.4)
kT2 [keV] : 14.3720 (-1.62345 1.86203)
R2^2/D10^2 : 2.87364E-02 (-0.0109004 0.0168914)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.438e-06 1.210e-06
25- 50 8.616e-07 1.756e-07
50-150 1.151e-06 2.742e-07
15-150 4.451e-06 1.264e-06
Peak spectrum fit
Power-law model
Time interval is from 41.252 sec. to 42.252 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.68707 ( -2.22887 2.29274 )
Norm@50keV : 1.94640E-04 ( -0.000193665 0.00160077 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.49 using 59 PHA bins.
# Reduced chi-squared = 1.061 for 57 degrees of freedom
# Null hypothesis probability = 3.508580e-01
Photon flux (15-150 keV) in 1 sec: 1.61027 ( -0.42081 0.413795 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.69418e-08 ( -1.36267e-08 1.48015e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 41.252 sec. to 42.252 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.78334 ( )
Epeak [keV] : 6.05575 ( )
Norm@50keV : 3.22640E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.32 using 59 PHA bins.
# Reduced chi-squared = 1.274 for 56 degrees of freedom
# Null hypothesis probability = 8.148453e-02
Photon flux (15-150 keV) in 1 sec: 1.58918 ( -0.39914 0.42609 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.67768e-08 ( 0 0 ) ergs/cm2
Band function
Time interval is from 41.252 sec. to 42.252 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.72251 ( -3.72303 -3.72303 )
beta : -6.75148 ( -2.26336 2.28278 )
Epeak [keV] : 2.23638 ( 6.57997 -2.23638 )
Norm@50keV : 8.30223E+07 ( -8.21904e+07 2.246e+08 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.50 using 59 PHA bins.
# Reduced chi-squared = 1.100 for 55 degrees of freedom
# Null hypothesis probability = 2.841065e-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] : 1.86682 (-0.455698 0.716312)
R^2/D10^2 : 8628.14 (-8533.31 127398)
(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 3.807e-08 2.432e-08
25- 50 1.611e-09 1.481e-09
50-150 1.316e-13 3.995e-13
15-150 3.968e-08 2.548e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 3.11341 (-1.0374 2.16842)
Norm : 3017.47 (-3088.92 35572.1)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.260e-08 2.460e-08
25- 50 1.465e-09 9.440e-10
50-150 3.622e-13 4.988e-13
15-150 4.407e-08 2.449e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.58162 (-0.411495 0.53842)
R1^2/D10^2 : 3.69393E+04 (-36569 1.08452e+06)
kT2 [keV] : 13.0594 (-3.96979 4.32387)
R2^2/D10^2 : 0.145495 (-0.106986 0.421206)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.972e-08 2.135e-08
25- 50 1.847e-08 1.185e-08
50-150 1.969e-08 1.555e-08
15-150 7.788e-08 4.128e-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: 2.65415 ( )
Norm@50keV : 1.51853E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 161.23 using 59 PHA bins.
# Reduced chi-squared = 2.8286 for 57 degrees of freedom
# Null hypothesis probability = 6.833512e-12
Photon flux (15-150 keV) in 150.6 sec: 0.328904 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.3944e-06 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69663 ( )
Epeak [keV] : 33.3172 ( )
Norm@50keV : 3.10720E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 171.81 using 59 PHA bins.
# Reduced chi-squared = 3.0680 for 56 degrees of freedom
# Null hypothesis probability = 1.082855e-13
Photon flux (15-150 keV) in 150.6 sec: 0.329759 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.3624e-06 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.67251 ( )
beta : -9.20884 ( )
Epeak [keV] : 22.6903 ( )
Norm@50keV : 3.87070E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 169.75 using 59 PHA bins.
# Reduced chi-squared = 3.0863 for 55 degrees of freedom
# Null hypothesis probability = 1.236341e-13
Photon flux (15-150 keV) in 150.6 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) = 1.02e-06
S(50-100 keV) = 6.52e-07
T90 vs. Hardness ratio plot
T90 = 162.212000012398 sec.
Hardness ratio (energy fluence ratio) = 0.639216
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.291278
Count Ratio (50-100 keV) / (15-25 keV) = 0.202064
Mask shadow pattern
IMX = -9.340864148309894E-01, IMY = 5.546808034903962E-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:
-67.499380 -55.880000
-55.000000 4.092200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4711 35.4512 9.6 53.3 10.6 0.6239 1.2 6.6 Her X-1
288.6401 11.0967 0.0 36.0 -41.5 -0.1124 -0.5 13.0 GRS 1915+105
299.5943 35.2178 0.7 17.1 2.3 2.1229 16.1 1.0 Cyg X-1
308.2943 40.8408 4.8 12.4 32.6 -0.3085 -2.4 10.7 Cyg X-3
326.2751 38.3419 7.2 7.6 118.7 0.2132 1.6 5.0 Cyg X-2
347.6818 40.3143 2.3 23.4 141.3 0.7525 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
4.092200 54.890000
56.000000 155.800600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4492 35.4497 17.4 53.3 10.6 -0.7981 -0.7 6.4 Her X-1
288.6435 11.0662 12.1 36.0 -41.5 0.3744 1.0 11.6 GRS 1915+105
299.4058 35.0588 0.0 17.2 1.7 0.6270 2.7 12.5 Cyg X-1
308.0314 40.8322 5.3 12.5 32.0 0.5228 2.2 8.1 Cyg X-3
326.0387 38.4826 7.8 7.6 116.9 0.3434 1.5 11.5 Cyg X-2
313.3798 66.5329 2.3 34.0 73.5 2.4564 5.0 ------ UNKNOWN
356.1746 55.4440 2.0 33.9 115.1 2.5253 5.7 ------ UNKNOWN
354.5745 38.7651 2.4 28.5 146.1 1.4613 4.7 ------ UNKNOWN
352.8818 -2.9962 1.1 47.4 -149.3 6.5801 10.4 463.2 UNKNOWN
303.7360 1.3200 2.3 34.9 -72.5 2.6395 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
176.300600 395.600600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7378 10.9064 5.1 38.0 -39.9 1.4232 2.3 4.3 GRS 1915+105
299.5853 35.2134 0.7 18.5 -0.1 6.4490 17.2 0.8 Cyg X-1
308.3137 41.0947 4.6 13.1 27.1 0.9459 2.5 12.6 Cyg X-3
326.2253 38.2465 9.1 5.6 115.6 0.4707 1.3 5.2 Cyg X-2
20.4742 22.2173 2.2 52.2 165.9 6.1795 5.2 ------ UNKNOWN
263.1744 21.6015 2.8 52.8 -8.1 3.7822 4.1 ------ UNKNOWN
352.8928 -3.0319 1.9 47.0 -145.4 5.6462 6.2 463.4 UNKNOWN
Plot creation:
Sat Mar 14 09:15:10 EDT 2026