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
261.5170 +22.2446 0.0159 28.6 25.9 0.3595 12.0 TRIG_01327910
------------------------------------------
Foreground time interval of the image:
-0.352 3.648 (delta_t = 4.000 [sec])
Background time interval of the image:
-239.352 -0.352 (delta_t = 239.000 [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 -0.352 sec. to 3.648 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00453 ( -0.222069 0.21327 )
Norm@50keV : 6.42778E-03 ( -0.000815065 0.000809663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.75 using 59 PHA bins.
# Reduced chi-squared = 0.8552 for 57 degrees of freedom
# Null hypothesis probability = 7.735750e-01
Photon flux (15-150 keV) in 4 sec: 0.740326 ( -0.0957092 0.0958897 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.77625e-07 ( -3.64774e-08 3.65838e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.352 sec. to 3.648 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.503974 ( -1.06491 0.633554 )
Epeak [keV] : 173.667 ( -173.665 -173.665 )
Norm@50keV : 1.06672E-02 ( -0.00485044 0.0188276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.83 using 59 PHA bins.
# Reduced chi-squared = 0.8541 for 56 degrees of freedom
# Null hypothesis probability = 7.732181e-01
Photon flux (15-150 keV) in 4 sec: 0.724995 ( -0.099535 0.099521 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.71622e-07 ( -3.90184e-08 3.85204e-08 ) ergs/cm2
Band function
Time interval is from -0.352 sec. to 3.648 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.500054 ( 0.479756 1.72223 )
beta : -1.44768 ( 1.48568 1.91025 )
Epeak [keV] : 170.065 ( -165.558 423.92 )
Norm@50keV : 1.07642E-02 ( -0.00348868 198023 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.76 using 59 PHA bins.
# Reduced chi-squared = 0.8683 for 55 degrees of freedom
# Null hypothesis probability = 7.450530e-01
Photon flux (15-150 keV) in 4 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] : 22.2242 (-3.3147 4.23387)
R^2/D10^2 : 2.58102E-02 (-0.0109434 0.0175982)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.93 using 59 PHA bins.
# Reduced chi-squared = 0.9636 for 57 degrees of freedom
# Null hypothesis probability = 5.532688e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.393e-09 2.402e-09
25- 50 4.997e-08 1.205e-08
50-150 1.844e-07 4.104e-08
15-150 2.438e-07 4.602e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-27.9798 -200)
Norm : 3.06876 (-0.397029 0.397029)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.057e-08 1.745e-08
25- 50 5.882e-08 3.246e-08
50-150 1.290e-07 7.148e-08
15-150 2.184e-07 1.226e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.71930 (-4.48449 8.35548)
R1^2/D10^2 : 0.228450 (-0.186546 2.36191)
kT2 [keV] : 31.9131 (-8.99642 -31.9131)
R2^2/D10^2 : 7.04196E-03 (-0.00664822 0.0172531)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.761e-08 1.043e-08
25- 50 5.416e-08 2.806e-08
50-150 2.005e-07 1.042e-07
15-150 2.722e-07 1.395e-07
Peak spectrum fit
Power-law model
Time interval is from 1.648 sec. to 2.648 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02607 ( -0.387396 0.363064 )
Norm@50keV : 7.03709E-03 ( -0.00162143 0.00160966 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.57 using 59 PHA bins.
# Reduced chi-squared = 0.9048 for 57 degrees of freedom
# Null hypothesis probability = 6.780504e-01
Photon flux (15-150 keV) in 1 sec: 0.811458 ( -0.189854 0.191333 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.53989e-08 ( -1.79198e-08 1.81118e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.648 sec. to 2.648 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.680390 ( -3.19433 1.81677 )
Epeak [keV] : 86.4144 ( -26.7007 -86.4144 )
Norm@50keV : 4.24681E-02 ( -0.0424681 1.01986 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.23 using 59 PHA bins.
# Reduced chi-squared = 0.8790 for 56 degrees of freedom
# Null hypothesis probability = 7.271317e-01
Photon flux (15-150 keV) in 1 sec: 0.762171 ( -0.197573 0.199722 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.86625e-08 ( -1.99725e-08 2.02488e-08 ) ergs/cm2
Band function
Time interval is from 1.648 sec. to 2.648 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -1.39866 ( -2.15752 0.526187 )
Epeak [keV] : 41.2316 ( -41.2308 20.4076 )
Norm@50keV : 30.4218 ( -6.67063 933.893 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.88 using 59 PHA bins.
# Reduced chi-squared = 0.8887 for 55 degrees of freedom
# Null hypothesis probability = 7.062960e-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] : 19.7419 (-4.32737 6.42845)
R^2/D10^2 : 4.26711E-02 (-0.0257678 0.0540448)
(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 3.222e-09 1.361e-09
25- 50 1.591e-08 7.582e-09
50-150 4.589e-08 2.056e-08
15-150 6.502e-08 2.595e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-67.9675 -200)
Norm : 3.36269 (-0.793325 0.793325)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.373e-09 5.145e-09
25- 50 1.611e-08 9.740e-09
50-150 3.533e-08 2.079e-08
15-150 5.980e-08 3.511e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 200.000 (-200 -200)
R1^2/D10^2 : 7.54125E-05 (-7.54379e-05 -7.54379e-05)
kT2 [keV] : 16.2930 (-4.10885 8.10488)
R2^2/D10^2 : 6.79209E-02 (-0.0467013 0.0378248)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.879e-09 2.729e-09
25- 50 1.660e-08 1.395e-08
50-150 5.021e-08 4.198e-08
15-150 7.069e-08 5.765e-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: 1.00453 ( -0.222069 0.21327 )
Norm@50keV : 6.42778E-03 ( -0.000815065 0.000809663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.75 using 59 PHA bins.
# Reduced chi-squared = 0.8552 for 57 degrees of freedom
# Null hypothesis probability = 7.735750e-01
Photon flux (15-150 keV) in 4 sec: 0.740326 ( -0.0957092 0.0958897 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.77625e-07 ( -3.64774e-08 3.65838e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.503974 ( -1.06491 0.633554 )
Epeak [keV] : 173.667 ( -173.665 -173.665 )
Norm@50keV : 1.06672E-02 ( -0.00485044 0.0188276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.83 using 59 PHA bins.
# Reduced chi-squared = 0.8541 for 56 degrees of freedom
# Null hypothesis probability = 7.732181e-01
Photon flux (15-150 keV) in 4 sec: 0.724995 ( -0.099535 0.099521 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.71622e-07 ( -3.90184e-08 3.85204e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.500054 ( 0.479756 1.72223 )
beta : -1.44768 ( 1.48568 1.91025 )
Epeak [keV] : 170.065 ( -165.558 423.92 )
Norm@50keV : 1.07642E-02 ( -0.00348868 198023 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.76 using 59 PHA bins.
# Reduced chi-squared = 0.8683 for 55 degrees of freedom
# Null hypothesis probability = 7.450530e-01
Photon flux (15-150 keV) in 4 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) = 5.15e-08
S(50-100 keV) = 1.03e-07
T90 vs. Hardness ratio plot
T90 = 4 sec.
Hardness ratio (energy fluence ratio) = 2
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.59471
Count Ratio (50-100 keV) / (15-25 keV) = 2.77493
Mask shadow pattern
IMX = 4.908272674567141E-01, IMY = -2.387296110807622E-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:
-239.352000 -0.352000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0051 -15.6518 1.2 35.9 107.5 7.9077 9.6 1.6 Sco X-1
254.6551 35.3635 5.4 27.2 -5.0 -0.8333 -2.1 9.7 Her X-1
268.2665 -1.5193 6.5 41.1 64.2 -2.7591 -1.8 7.3 SW J1753.5-0127
203.7652 -27.3747 2.2 52.4 161.5 6.6006 5.2 ------ UNKNOWN
280.0343 34.6993 2.5 46.3 8.7 2.6286 4.6 ------ UNKNOWN
273.7236 33.5933 3.0 41.0 8.9 2.0494 3.9 ------ UNKNOWN
211.8359 -4.3323 3.3 29.3 173.3 1.3604 3.5 ------ UNKNOWN
211.8836 1.5053 3.5 25.1 -177.8 1.1866 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.352000 3.648000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0149 -15.7248 4.2 36.0 107.5 -0.1543 -2.7 5.5 Sco X-1
254.4846 35.3721 3.5 27.1 -5.2 0.0856 3.3 2.2 Her X-1
268.4742 -1.3946 4.7 41.2 63.9 -0.2438 -2.5 7.3 SW J1753.5-0127
261.5170 22.2446 1.0 28.6 25.9 0.3596 12.0 ------ UNKNOWN
204.4022 -11.3209 2.3 39.4 174.7 0.1858 5.1 ------ UNKNOWN
279.0258 38.2172 2.1 46.2 3.7 0.2644 5.6 ------ UNKNOWN
226.9134 64.2792 2.1 46.7 -52.5 0.5596 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Fri Jun 27 16:41:09 EDT 2025