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
38.5388 -38.0817 0.0118 37.6 14.7 1.8044 16.3 TRIG_01328546
------------------------------------------
Foreground time interval of the image:
-9.424 27.425 (delta_t = 36.849 [sec])
Background time interval of the image:
-239.576 -9.424 (delta_t = 230.152 [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 2.048000
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 2.048000
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 2.048000
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 -9.424 sec. to 68.560 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99308 ( -0.121805 0.125571 )
Norm@50keV : 2.59074E-03 ( -0.000207703 0.000205008 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.97 using 59 PHA bins.
# Reduced chi-squared = 1.122 for 57 degrees of freedom
# Null hypothesis probability = 2.451242e-01
Photon flux (15-150 keV) in 77.98 sec: 0.387381 ( -0.0266215 0.0266486 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8624e-06 ( -1.41887e-07 1.431e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -9.424 sec. to 68.560 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36328 ( -0.587792 0.510702 )
Epeak [keV] : 43.8948 ( -13.5253 17.2423 )
Norm@50keV : 5.84589E-03 ( -0.00277835 0.00664928 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.41 using 59 PHA bins.
# Reduced chi-squared = 1.061 for 56 degrees of freedom
# Null hypothesis probability = 3.524359e-01
Photon flux (15-150 keV) in 77.98 sec: 0.377536 ( -0.027723 0.027735 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76346e-06 ( -1.60592e-07 1.62986e-07 ) ergs/cm2
Band function
Time interval is from -9.424 sec. to 68.560 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.96942 ( -5.49916 -4.04279 )
beta : -2.21405 ( -0.21808 0.185941 )
Epeak [keV] : 27.7355 ( -3.79787 3.07411 )
Norm@50keV : 1.63437 ( -1.63281 129.004 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.25 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 55 degrees of freedom
# Null hypothesis probability = 4.280000e-01
Photon flux (15-150 keV) in 77.98 sec: 0.374327 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79151e-06 ( -1.79097e-06 -1.47827e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.2525 (-0.80918 0.883769)
R^2/D10^2 : 0.162826 (-0.0447065 0.061271)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 98.80 using 59 PHA bins.
# Reduced chi-squared = 1.733 for 57 degrees of freedom
# Null hypothesis probability = 4.976180e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.740e-07 3.197e-08
25- 50 7.054e-07 5.544e-08
50-150 3.956e-07 6.897e-08
15-150 1.375e-06 1.127e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.1822 (-12.8857 17.7605)
Norm : 1.90923 (-0.207368 0.237127)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.815e-07 3.412e-08
25- 50 6.050e-07 4.340e-08
50-150 7.703e-07 1.235e-07
15-150 1.757e-06 1.622e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.58449 (-1.19743 1.23296)
R1^2/D10^2 : 0.653655 (-0.285816 0.64646)
kT2 [keV] : 21.6447 (-5.06526 9.6028)
R2^2/D10^2 : 5.90450E-03 (-0.00444096 0.00745502)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.719e-07 9.143e-08
25- 50 6.128e-07 1.201e-07
50-150 7.899e-07 3.858e-07
15-150 1.775e-06 5.413e-07
Peak spectrum fit
Power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85427 ( -0.311855 0.346687 )
Norm@50keV : 8.58743E-03 ( -0.00196149 0.00190554 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.34 using 59 PHA bins.
# Reduced chi-squared = 1.006 for 57 degrees of freedom
# Null hypothesis probability = 4.623932e-01
Photon flux (15-150 keV) in 1 sec: 1.20915 ( -0.247653 0.247992 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.8956e-08 ( -1.77196e-08 1.79239e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.786581 ( -1.77195 1.27326 )
Epeak [keV] : 56.8938 ( -50.3911 -56.901 )
Norm@50keV : 3.04118E-02 ( -0.030408 0.213233 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.36 using 59 PHA bins.
# Reduced chi-squared = 0.9885 for 56 degrees of freedom
# Null hypothesis probability = 4.991510e-01
Photon flux (15-150 keV) in 1 sec: 1.18218 ( -0.252238 0.25105 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.72462e-08 ( -1.81025e-08 1.83959e-08 ) ergs/cm2
Band function
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.791712 ( -1.19567 1.68347 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 56.9856 ( -18.515 -56.9856 )
Norm@50keV : 3.01995E-02 ( -0.0301996 0.213313 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.36 using 59 PHA bins.
# Reduced chi-squared = 1.006 for 55 degrees of freedom
# Null hypothesis probability = 4.611347e-01
Photon flux (15-150 keV) in 1 sec: 1.19695 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.73353e-08 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.1734 (-2.8105 3.39459)
R^2/D10^2 : 0.218409 (-0.125331 0.303474)
(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 8.037e-09 3.219e-09
25- 50 2.808e-08 1.015e-08
50-150 3.104e-08 1.353e-08
15-150 6.715e-08 2.325e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 95.9453 (-42.3653 -95.9425)
Norm : 5.50113 (-1.33972 1.77054)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.437e-08 3.838e-09
25- 50 2.464e-08 7.380e-09
50-150 3.900e-08 2.635e-08
15-150 7.802e-08 3.144e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.21593 (-3.34397 5.82729)
R1^2/D10^2 : 8.09323 (-7.72803 3.67767)
kT2 [keV] : 16.6452 (-4.55124 11.2782)
R2^2/D10^2 : 7.98943E-02 (-0.0731132 0.205833)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.397e-08 7.915e-09
25- 50 2.367e-08 1.235e-08
50-150 3.880e-08 2.391e-08
15-150 7.645e-08 4.095e-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: 2.05786 ( -0.155723 0.163122 )
Norm@50keV : 2.97274E-03 ( -0.000324557 0.000318787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.54 using 59 PHA bins.
# Reduced chi-squared = 1.027 for 57 degrees of freedom
# Null hypothesis probability = 4.188241e-01
Photon flux (15-150 keV) in 36.85 sec: 0.458196 ( -0.039983 0.0400018 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01405e-06 ( -1.01893e-07 1.03258e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30110 ( -0.849307 0.682564 )
Epeak [keV] : 37.8887 ( )
Norm@50keV : 8.23388E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.89 using 59 PHA bins.
# Reduced chi-squared = 0.9801 for 56 degrees of freedom
# Null hypothesis probability = 5.169895e-01
Photon flux (15-150 keV) in 36.85 sec: 0.446905 ( -0.041213 0.041215 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.45634e-07 ( -1.15624e-07 1.19409e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.30215 ( -0.380956 0.993095 )
beta : -10.00000 ( 10 1.67098e-10 )
Epeak [keV] : 37.8898 ( -8.25152 14.1959 )
Norm@50keV : 8.21951E-03 ( -0.00487233 0.000707834 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.89 using 59 PHA bins.
# Reduced chi-squared = 0.9980 for 55 degrees of freedom
# Null hypothesis probability = 4.788948e-01
Photon flux (15-150 keV) in 36.85 sec: 0.446332 ( 6.55367 -0.043017 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.69781e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.60e-07
S(50-100 keV) = 5.62e-07
T90 vs. Hardness ratio plot
T90 = 64.0119999647141 sec.
Hardness ratio (energy fluence ratio) = 1.00357
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17147
Count Ratio (50-100 keV) / (15-25 keV) = 0.597357
Mask shadow pattern
IMX = 7.439711368087202E-01, IMY = -1.950075841462621E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.576000 -9.424000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
64.1985 33.5378 2.8 44.7 -122.1 5.5008 4.1 ------ UNKNOWN
63.0619 38.0263 3.3 47.3 -127.3 6.1463 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-9.424000 27.424590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
38.5388 -38.0817 0.7 37.6 14.7 1.8045 16.3 ------ UNKNOWN
15.6482 50.3244 3.3 53.4 -173.3 0.6891 3.5 ------ UNKNOWN
39.7239 56.4956 2.2 57.5 -155.1 1.7753 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
108.724590 786.224580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
359.5747 -4.0793 2.3 49.1 161.8 12.3096 5.0 246.1 UNKNOWN
125.1351 -57.6979 2.2 56.9 -1.7 12.2363 5.2 ------ UNKNOWN
71.4093 -18.8341 2.2 34.4 -76.9 7.6081 5.2 ------ UNKNOWN
Plot creation:
Sat Jun 28 23:48:22 EDT 2025