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
166.9627 -19.7862 0.0077 33.0 49.1 10.5884 24.9 TRIG_01321323
------------------------------------------
Foreground time interval of the image:
-94.707 13.193 (delta_t = 107.900 [sec])
Background time interval of the image:
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 -100.300 sec. to 126.692 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83474 ( -0.0501769 0.0503758 )
Norm@50keV : 5.68032E-03 ( -0.000150945 0.000150795 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.05 using 59 PHA bins.
# Reduced chi-squared = 1.387 for 57 degrees of freedom
# Null hypothesis probability = 2.824070e-02
Photon flux (15-150 keV) in 227 sec: 0.793527 ( -0.0237805 0.0238864 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.18591e-05 ( -3.17394e-07 3.17666e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -100.300 sec. to 126.692 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50022 ( -0.221298 0.210612 )
Epeak [keV] : 76.6508 ( -12.5072 42.6432 )
Norm@50keV : 8.24646E-03 ( -0.00168783 0.00225579 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.54 using 59 PHA bins.
# Reduced chi-squared = 1.278 for 56 degrees of freedom
# Null hypothesis probability = 7.882783e-02
Photon flux (15-150 keV) in 227 sec: 0.771925 ( -0.026909 0.027062 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.1556e-05 ( -3.71644e-07 3.70078e-07 ) ergs/cm2
Band function
Time interval is from -100.300 sec. to 126.692 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.22142 ( -0.347632 0.761363 )
beta : -2.03787 ( -0.254285 0.138328 )
Epeak [keV] : 57.4188 ( -18.7504 23.3189 )
Norm@50keV : 1.18807E-02 ( -0.00419854 0.0269093 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.90 using 59 PHA bins.
# Reduced chi-squared = 1.235 for 55 degrees of freedom
# Null hypothesis probability = 1.136190e-01
Photon flux (15-150 keV) in 227 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.1505e-05 ( -1.15035e-05 -3.60113e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.5598 ( )
R^2/D10^2 : 0.113756 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 351.74 using 59 PHA bins.
# Reduced chi-squared = 6.1709 for 57 degrees of freedom
# Null hypothesis probability = 4.761628e-44
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.005e-06 5.459e-08
25- 50 3.620e-06 1.158e-07
50-150 4.310e-06 2.066e-07
15-150 8.936e-06 2.588e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 105.422 (-9.28667 14.1809)
Norm : 3.38874 (-0.155842 0.135791)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.042e-06 1.326e-07
25- 50 3.530e-06 1.396e-07
50-150 5.718e-06 1.284e-06
15-150 1.129e-05 1.350e-06
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.44007 (-0.829149 0.862658)
R1^2/D10^2 : 0.732711 (-0.219935 0.365952)
kT2 [keV] : 24.8895 (-3.02994 4.41206)
R2^2/D10^2 : 8.50857E-03 (-0.00395986 0.00588014)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.777e-06 1.590e-07
25- 50 3.590e-06 2.134e-07
50-150 5.916e-06 5.380e-07
15-150 1.128e-05 7.378e-07
Peak spectrum fit
Power-law model
Time interval is from -0.004 sec. to 0.996 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25329 ( -0.122865 0.122448 )
Norm@50keV : 5.12062E-02 ( -0.00354781 0.00354729 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.73 using 59 PHA bins.
# Reduced chi-squared = 0.9777 for 57 degrees of freedom
# Null hypothesis probability = 5.229193e-01
Photon flux (15-150 keV) in 1 sec: 6.05956 ( -0.432873 0.433757 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12026e-07 ( -3.94704e-08 3.96152e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.004 sec. to 0.996 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24922 ( -0.318982 0.165668 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 5.14370E-02 ( -0.00356327 0.00356178 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.74 using 59 PHA bins.
# Reduced chi-squared = 0.9954 for 56 degrees of freedom
# Null hypothesis probability = 4.845492e-01
Photon flux (15-150 keV) in 1 sec: 6.06206 ( -0.43723 0.42948 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.1161e-07 ( -3.8975e-08 3.9753e-08 ) ergs/cm2
Band function
Time interval is from -0.004 sec. to 0.996 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97395 ( -4.97395 -4.97395 )
beta : -1.26720 ( -0.128566 0.126221 )
Epeak [keV] : 20.6637 ( -20.6637 5.54075 )
Norm@50keV : 1.31039E+04 ( -907.12 1.49579e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.44 using 59 PHA bins.
# Reduced chi-squared = 1.008 for 55 degrees of freedom
# Null hypothesis probability = 4.581804e-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] : 19.3642 ( )
R^2/D10^2 : 0.303259 ( )
(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 2.220e-08 3.195e-09
25- 50 1.082e-07 1.176e-08
50-150 2.992e-07 3.580e-08
15-150 4.295e-07 3.810e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-15.9346 -200)
Norm : 25.0648 (-1.7661 1.7661)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.243e-08 5.220e-09
25- 50 1.201e-07 1.150e-08
50-150 2.634e-07 6.635e-08
15-150 4.459e-07 1.148e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.52823 (-1.41534 1.7991)
R1^2/D10^2 : 7.20538 (-4.06225 10.8204)
kT2 [keV] : 31.0477 (-5.31233 9.28927)
R2^2/D10^2 : 5.66351E-02 (-0.0317301 0.0490289)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.398e-08 1.637e-08
25- 50 1.067e-07 2.386e-08
50-150 3.580e-07 8.820e-08
15-150 5.186e-07 1.105e-07
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: 1.66229 ( -0.0684694 0.0686559 )
Norm@50keV : 6.28676E-03 ( -0.000235138 0.000234703 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.45 using 59 PHA bins.
# Reduced chi-squared = 1.096 for 57 degrees of freedom
# Null hypothesis probability = 2.886893e-01
Photon flux (15-150 keV) in 107.9 sec: 0.824252 ( -0.0331581 0.033261 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.30126e-06 ( -2.45579e-07 2.46074e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51982 ( -0.281216 0.196172 )
Epeak [keV] : 173.017 ( )
Norm@50keV : 7.38412E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.63 using 59 PHA bins.
# Reduced chi-squared = 1.101 for 56 degrees of freedom
# Null hypothesis probability = 2.817067e-01
Photon flux (15-150 keV) in 107.9 sec: 0.816568 ( -0.035904 0.035949 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.23754e-06 ( -2.76375e-07 2.68272e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.169819 ( 0.166502 0.166502 )
beta : -1.71454 ( 1.71456 0.0893837 )
Epeak [keV] : 35.2372 ( -35.161 142.017 )
Norm@50keV : 6.65892E-02 ( -0.0680341 415.99 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.90 using 59 PHA bins.
# Reduced chi-squared = 1.089 for 55 degrees of freedom
# Null hypothesis probability = 3.024744e-01
Photon flux (15-150 keV) in 107.9 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.20303e-06 ( -6.20228e-06 -2.68876e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.38e-06
S(50-100 keV) = 3.79e-06
T90 vs. Hardness ratio plot
T90 = 176.051999926567 sec.
Hardness ratio (energy fluence ratio) = 1.1213
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.23307
Count Ratio (50-100 keV) / (15-25 keV) = 0.773066
Mask shadow pattern
IMX = 4.256397910221273E-01, IMY = -4.917990820038269E-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:
-94.707400 -38.484000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5472 -40.5619 0.8 9.2 137.3 0.7804 14.5 1.0 Vela X-1
170.1070 -60.7642 6.5 38.1 122.8 0.3053 1.8 10.5 Cen X-3
181.3492 -55.5955 3.1 41.4 111.8 1.0458 3.7 ------ UNKNOWN
154.7032 11.8598 2.7 48.4 1.3 0.5391 4.3 ------ UNKNOWN
153.9946 17.2672 2.0 53.1 -2.3 1.0006 5.8 ------ UNKNOWN
93.8429 -50.8940 2.4 34.3 -163.8 0.3204 4.8 ------ UNKNOWN
118.5343 -6.2135 2.5 28.6 -58.4 0.3420 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-94.707400 13.192620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5417 -40.5636 0.8 9.2 137.3 3.0154 14.0 0.8 Vela X-1
170.3541 -60.4917 12.7 38.0 122.4 0.6006 0.9 8.0 Cen X-3
166.9627 -19.7863 0.5 33.0 49.1 10.5895 24.9 ------ UNKNOWN
128.6729 -19.4142 2.2 12.7 -45.0 1.1239 5.3 ------ UNKNOWN
130.4133 1.3370 2.3 33.0 -32.1 1.3289 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
85.592610 155.442000
156.992000 157.652000
158.992000 162.012000
162.992000 168.032000
168.992000 206.992000
208.992000 218.852000
220.992000 249.592600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5435 -40.5631 1.2 33.9 -155.1 2.9956 9.4 0.8 Vela X-1
170.3695 -60.5847 2.7 40.9 157.1 2.1460 4.4 2.8 Cen X-3
186.7608 -62.7068 3.1 45.0 146.9 3.2662 3.7 4.8 GX 301-2
166.9289 -19.7788 1.5 0.1 -97.9 1.8799 7.7 ------ UNKNOWN
115.7776 -25.4583 4.2 47.3 -127.2 3.4453 2.8 ------ UNKNOWN
Plot creation:
Fri Jun 6 20:45:45 EDT 2025