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
133.7536 +12.0408 0.0051 40.2 -38.5 5.6199 37.4 TRIG_01513082
------------------------------------------
Foreground time interval of the image:
-5.960 16.717 (delta_t = 22.677 [sec])
Background time interval of the image:
-179.784 -5.960 (delta_t = 173.824 [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 1.024000
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 1.024000
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 1.024000
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 -5.960 sec. to 455.684 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24498 ( -0.0225932 0.0224977 )
Norm@50keV : 1.22358E-02 ( -0.000165702 0.000165091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 23.05 using 59 PHA bins.
# Reduced chi-squared = 0.4044 for 57 degrees of freedom
# Null hypothesis probability = 9.999823e-01
Photon flux (15-150 keV) in 461.6 sec: 1.44598 ( -0.0225003 0.0225846 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.66005e-05 ( -6.68812e-07 6.68808e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.960 sec. to 455.684 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15904 ( -0.0940573 0.0468749 )
Epeak [keV] : 663.549 ( -307.226 -663.549 )
Norm@50keV : 1.31593E-02 ( -0.000756603 0.00106807 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 20.56 using 59 PHA bins.
# Reduced chi-squared = 0.3672 for 56 degrees of freedom
# Null hypothesis probability = 9.999963e-01
Photon flux (15-150 keV) in 461.6 sec: 1.43439 ( -0.0253 0.02437 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.65252e-05 ( -6.7809e-07 6.7809e-07 ) ergs/cm2
Band function
Time interval is from -5.960 sec. to 455.684 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.15905 ( 1.03726 1.18613 )
beta : -10.00000 ( 10 2.31191e-09 )
Epeak [keV] : 663.520 ( -187.919 -663.52 )
Norm@50keV : 1.31577E-02 ( -0.000155275 0.00106771 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 20.56 using 59 PHA bins.
# Reduced chi-squared = 0.3738 for 55 degrees of freedom
# Null hypothesis probability = 9.999937e-01
Photon flux (15-150 keV) in 461.6 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] : 24.1448 ( )
R^2/D10^2 : 3.45918E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1270.44 using 59 PHA bins.
# Reduced chi-squared = 22.2884 for 57 degrees of freedom
# Null hypothesis probability = 2.941404e-228
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.647e-06 4.501e-08
25- 50 9.174e-06 2.008e-07
50-150 3.982e-05 5.724e-07
15-150 5.065e-05 6.693e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 6.60594 ( )
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.593e-06 1.085e-07
25- 50 1.461e-05 2.193e-07
50-150 3.203e-05 4.754e-07
15-150 5.423e-05 7.616e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.86558 (-0.468543 0.489547)
R1^2/D10^2 : 0.560238 (-0.0924406 0.115227)
kT2 [keV] : 35.9012 (-1.48171 1.69962)
R2^2/D10^2 : 8.01133E-03 (-0.0011557 0.0012428)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.589e-06 2.645e-07
25- 50 1.252e-05 3.000e-07
50-150 3.930e-05 6.878e-07
15-150 5.642e-05 8.540e-07
Peak spectrum fit
Power-law model
Time interval is from 338.784 sec. to 339.784 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14380 ( -0.0600891 0.0599289 )
Norm@50keV : 9.03364E-02 ( -0.00303874 0.00303723 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.48 using 59 PHA bins.
# Reduced chi-squared = 1.079 for 57 degrees of freedom
# Null hypothesis probability = 3.188278e-01
Photon flux (15-150 keV) in 1 sec: 10.5274 ( -0.367825 0.36826 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.31702e-07 ( -3.41787e-08 3.42426e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 338.784 sec. to 339.784 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.972759 ( -0.24164 0.194249 )
Epeak [keV] : 347.220 ( -347.22 -347.22 )
Norm@50keV : 0.107602 ( -0.0191492 0.0291748 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.88 using 59 PHA bins.
# Reduced chi-squared = 1.069 for 56 degrees of freedom
# Null hypothesis probability = 3.367795e-01
Photon flux (15-150 keV) in 1 sec: 10.4435 ( -0.3832 0.3837 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.25466e-07 ( -3.5714e-08 3.5566e-08 ) ergs/cm2
Band function
Time interval is from 338.784 sec. to 339.784 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.689933 ( 0.690376 0.690376 )
beta : -1.20723 ( 1.20651 0.101517 )
Epeak [keV] : 119.146 ( -119.011 661.973 )
Norm@50keV : 0.160861 ( -0.0723204 2634.46 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.73 using 59 PHA bins.
# Reduced chi-squared = 1.086 for 55 degrees of freedom
# Null hypothesis probability = 3.079360e-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] : 20.5761 ( )
R^2/D10^2 : 0.448897 ( )
(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 3.622e-08 2.360e-09
25- 50 1.838e-07 9.100e-09
50-150 5.788e-07 3.260e-08
15-150 7.988e-07 3.290e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 43.7521 ( )
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.090e-07 3.650e-09
25- 50 2.096e-07 7.450e-09
50-150 4.596e-07 1.635e-08
15-150 7.782e-07 2.740e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.30962 (-1.17473 1.32025)
R1^2/D10^2 : 4.73824 (-1.68195 2.97276)
kT2 [keV] : 33.8449 (-4.00418 6.02233)
R2^2/D10^2 : 7.66690E-02 (-0.0313087 0.0401155)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.349e-08 9.350e-09
25- 50 1.957e-07 1.725e-08
50-150 6.619e-07 6.855e-08
15-150 9.310e-07 7.990e-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: 0.947883 ( -0.0629105 0.0620838 )
Norm@50keV : 1.67623E-02 ( -0.000614792 0.000611958 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.53 using 59 PHA bins.
# Reduced chi-squared = 0.7285 for 57 degrees of freedom
# Null hypothesis probability = 9.384625e-01
Photon flux (15-150 keV) in 22.68 sec: 1.92570 ( -0.0717634 0.0718948 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.18961e-06 ( -1.48626e-07 1.48596e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.788908 ( -0.251157 0.182039 )
Epeak [keV] : 478.495 ( -478.495 -478.495 )
Norm@50keV : 1.94483E-02 ( -0.00302438 0.00495414 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.24 using 59 PHA bins.
# Reduced chi-squared = 0.7186 for 56 degrees of freedom
# Null hypothesis probability = 9.443974e-01
Photon flux (15-150 keV) in 22.68 sec: 1.91174 ( -0.07444 0.07462 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17698e-06 ( -1.51434e-07 1.50935e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.777070 ( 0.777807 0.777807 )
beta : -3.80865 ( -0.0620798 0.062916 )
Epeak [keV] : 455.869 ( -144.838 -455.869 )
Norm@50keV : 1.96095E-02 ( -0.000667838 0.00276952 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.25 using 59 PHA bins.
# Reduced chi-squared = 0.7318 for 55 degrees of freedom
# Null hypothesis probability = 9.320670e-01
Photon flux (15-150 keV) in 22.68 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) = 1.22e-05
S(50-100 keV) = 2.06e-05
T90 vs. Hardness ratio plot
T90 = 344.824000000954 sec.
Hardness ratio (energy fluence ratio) = 1.68852
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.59241
Count Ratio (50-100 keV) / (15-25 keV) = 1.6058
Mask shadow pattern
IMX = 6.612046647019300E-01, IMY = 5.260602157087735E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-179.784000 -5.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6103 22.0350 1.2 39.2 42.0 6.1190 9.9 1.8 Crab
23.9813 75.5957 3.3 42.9 143.8 2.8565 3.5 ------ UNKNOWN
112.2919 24.9517 2.5 25.7 -2.0 1.3600 4.6 ------ UNKNOWN
242.7486 70.3708 2.8 52.9 -174.6 3.3097 4.1 ------ UNKNOWN
129.9711 5.7411 2.2 45.5 -31.1 2.9268 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.960000 16.716590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5291 21.8793 7.6 39.3 42.0 -0.2546 -1.5 10.0 Crab
53.9912 54.0303 2.6 38.4 106.5 0.9221 4.4 ------ UNKNOWN
96.9538 15.4125 2.2 38.9 19.3 0.6136 5.2 ------ UNKNOWN
274.5736 72.1350 3.3 56.5 173.7 1.5029 3.5 ------ UNKNOWN
108.3674 -0.1521 2.1 51.1 -1.9 1.1248 5.4 ------ UNKNOWN
133.7536 12.0408 0.3 40.2 -38.5 5.6191 37.4 ------ UNKNOWN
131.3664 -1.2169 3.1 52.6 -31.3 1.3214 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
98.716620 372.716610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4973 -40.5693 2.4 52.6 -12.9 8.2418 4.8 1.7 Vela X-1
133.7566 12.0434 0.2 0.0 -137.6 42.1242 66.5 ------ UNKNOWN
183.8371 47.0664 2.9 54.6 -151.3 8.7944 4.1 ------ UNKNOWN
Plot creation:
Thu Sep 24 09:11:40 EDT 2026