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
357.3805 +9.0007 0.0459 53.2 -166.3 0.1311 4.2 TRIG_01439093
------------------------------------------
Foreground time interval of the image:
0.000 1.024 (delta_t = 1.024 [sec])
Background time interval of the image:
-60.584 -3.584 (delta_t = 57.000 [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: 3.70875 ( -0.892731 1.21208 )
Norm@50keV : 3.16750E-03 ( -0.00317026 0.00363124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.88 using 59 PHA bins.
# Reduced chi-squared = 0.9979 for 57 degrees of freedom
# Null hypothesis probability = 4.794675e-01
Photon flux (15-150 keV) in 1.024 sec: 1.52208 ( -0.508969 0.512729 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83327e-08 ( -2.22913e-08 2.56702e-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: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.11497E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.48 using 59 PHA bins.
# Reduced chi-squared = 1.259 for 56 degrees of freedom
# Null hypothesis probability = 9.226363e-02
Photon flux (15-150 keV) in 1.024 sec: 1.60734 1.60828 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.70201e-15 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38550 ( 1.58134 1.58134 )
beta : -8.80399 ( 6.52911 15.3054 )
Epeak [keV] : 16.9839 ( -3.39441 4.27781 )
Norm@50keV : 1.32594E+04 ( -13221.5 225730 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.55 using 59 PHA bins.
# Reduced chi-squared = 0.9555 for 55 degrees of freedom
# Null hypothesis probability = 5.687445e-01
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] : 3.79267 (-0.838909 1.0949)
R^2/D10^2 : 56.1988 (-56.163 172.438)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.69 using 59 PHA bins.
# Reduced chi-squared = 0.9420 for 57 degrees of freedom
# Null hypothesis probability = 5.998775e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.020e-08 2.446e-08
25- 50 1.244e-08 7.869e-09
50-150 1.086e-10 1.104e-10
15-150 5.275e-08 3.190e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.26449 (-3.58371 7.95852)
Norm : 62.7317 (-62.6817 142.892)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.757e-08 2.248e-08
25- 50 1.455e-08 1.035e-08
50-150 8.055e-10 8.637e-10
15-150 5.293e-08 3.243e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.79118 (-0.866919 1.047)
R1^2/D10^2 : 56.0934 (-41.3374 158.513)
kT2 [keV] : 199.363 (-199.363 -199.363)
R2^2/D10^2 : 3.86579E-05 (-3.8711e-05 0.00279047)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.006e-08 2.385e-08
25- 50 1.260e-08 8.397e-09
50-150 5.037e-09 1.405e-10
15-150 5.770e-08 3.215e-08
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: 3.70875 ( -0.892731 1.21208 )
Norm@50keV : 3.16750E-03 ( -0.00317026 0.00363124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.88 using 59 PHA bins.
# Reduced chi-squared = 0.9979 for 57 degrees of freedom
# Null hypothesis probability = 4.794675e-01
Photon flux (15-150 keV) in 1.024 sec: 1.52208 ( -0.508969 0.512729 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83327e-08 ( -2.22913e-08 2.56702e-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: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.11497E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.48 using 59 PHA bins.
# Reduced chi-squared = 1.259 for 56 degrees of freedom
# Null hypothesis probability = 9.226363e-02
Photon flux (15-150 keV) in 1.024 sec: 1.60734 1.60828 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.70201e-15 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38550 ( 1.58134 1.58134 )
beta : -8.80399 ( 6.52911 15.3054 )
Epeak [keV] : 16.9839 ( -3.39441 4.27781 )
Norm@50keV : 1.32594E+04 ( -13221.5 225730 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.55 using 59 PHA bins.
# Reduced chi-squared = 0.9555 for 55 degrees of freedom
# Null hypothesis probability = 5.687445e-01
Photon flux (15-150 keV) in 1.024 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] : 3.79267 (-0.838909 1.0949)
R^2/D10^2 : 56.1988 (-56.163 172.438)
(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 4.020e-08 2.407e-08
25- 50 1.244e-08 8.049e-09
50-150 1.086e-10 1.175e-10
15-150 5.275e-08 3.211e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.26449 (-3.58371 7.95852)
Norm : 62.7317 (-62.6817 142.892)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.757e-08 2.187e-08
25- 50 1.455e-08 9.708e-09
50-150 8.055e-10 8.428e-10
15-150 5.293e-08 3.242e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.79118 (-0.866919 1.047)
R1^2/D10^2 : 56.0934 (-41.3374 158.531)
kT2 [keV] : 199.363 (-199.363 -199.363)
R2^2/D10^2 : 3.86579E-05 (-3.8711e-05 0.00303669)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.006e-08 2.359e-08
25- 50 1.260e-08 8.499e-09
50-150 5.037e-09 1.424e-10
15-150 5.770e-08 3.076e-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: 3.70875 ( -0.892731 1.21208 )
Norm@50keV : 3.16750E-03 ( -0.00317026 0.00363124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.88 using 59 PHA bins.
# Reduced chi-squared = 0.9979 for 57 degrees of freedom
# Null hypothesis probability = 4.794675e-01
Photon flux (15-150 keV) in 1.024 sec: 1.52208 ( -0.508969 0.512729 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83327e-08 ( -2.22913e-08 2.56702e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.11497E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.48 using 59 PHA bins.
# Reduced chi-squared = 1.259 for 56 degrees of freedom
# Null hypothesis probability = 9.226363e-02
Photon flux (15-150 keV) in 1.024 sec: 1.60734 1.60828 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.70201e-15 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38550 ( 1.58134 1.58134 )
beta : -8.80399 ( 6.52911 15.3054 )
Epeak [keV] : 16.9839 ( -3.39441 4.27781 )
Norm@50keV : 1.32594E+04 ( -13221.5 225730 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.55 using 59 PHA bins.
# Reduced chi-squared = 0.9555 for 55 degrees of freedom
# Null hypothesis probability = 5.687445e-01
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) = 1.73e-08
S(50-100 keV) = 5.28e-09
T90 vs. Hardness ratio plot
T90 = 1.02400004863739 sec.
Hardness ratio (energy fluence ratio) = 0.305202
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.10208
Count Ratio (50-100 keV) / (15-25 keV) = 0.120085
Mask shadow pattern
IMX = -1.298080530371251E+00, IMY = 3.158210712614559E-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:
-60.584000 -3.584000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4658 35.2239 9.7 42.9 -0.5 -0.2120 -1.2 7.1 Her X-1
288.9017 11.0281 19.7 35.8 -64.0 0.1191 0.6 7.8 GRS 1915+105
299.5966 35.1932 1.0 10.3 -47.6 1.2252 11.5 0.6 Cyg X-1
308.1181 40.9663 5.3 1.5 -48.2 0.2320 2.2 0.9 Cyg X-3
326.0602 38.5121 0.0 12.9 179.2 -0.0281 -0.2 12.6 Cyg X-2
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] [']
254.3476 35.2443 4.7 43.0 -0.4 -0.0473 -2.5 8.0 Her X-1
288.6704 10.9167 4.7 36.0 -63.7 0.0513 2.5 7.7 GRS 1915+105
299.6337 35.0494 109.8 10.4 -48.3 -0.0012 -0.1 9.4 Cyg X-1
308.1103 40.9525 14.0 1.5 -48.5 -0.0087 -0.8 0.0 Cyg X-3
326.4174 38.4035 0.0 13.2 179.2 -0.0092 -0.8 12.6 Cyg X-2
264.7256 7.2369 2.2 52.6 -38.6 0.3017 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
119.116600 242.506000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1761 41.0422 5.7 53.8 -17.3 -1.0533 -2.0 6.1 Cyg X-3
326.2635 38.4175 8.2 40.5 -10.8 0.3697 1.4 7.2 Cyg X-2
12.4927 -36.8208 2.6 48.0 -168.6 1.6322 4.5 ------ UNKNOWN
8.4626 -47.0178 2.4 56.9 -161.3 4.2951 4.8 ------ UNKNOWN
310.7194 27.5157 2.3 47.6 -33.1 2.1077 5.1 ------ UNKNOWN
Plot creation:
Wed Jan 14 09:56:20 EST 2026