Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
284.7005 61.9041 0.0169 55.7959 -177.9100 1.5690446 11.405 TRIG_01442454
Foreground time interval of the image:
-0.352 4.656 (delta_t = 5.008 [sec])
Background time interval of the image:
-239.232 -0.352 (delta_t = 238.880 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) 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.
- 4) 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.
- 5) 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)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -0.352 sec. to 4.656 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.961923 ( -0.212188 0.200204 )
Norm@50keV : 2.19009E-02 ( -0.00308999 0.00303231 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.98 using 59 bins.
Reduced chi-squared = 1.01719
# Null hypothesis probability of 4.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.008 sec: 2.51713 ( -0.35727 0.36437 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20255e-06 ( -1.45017e-07 1.45028e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.352 sec. to 4.656 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.981287 ( -1.58065 1.18292 )
Epeak [keV] : 102.128 ( -18.1695 54.3616 )
Norm@50keV : 0.114518 ( -0.0711622 0.272205 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.89 using 59 bins.
Reduced chi-squared = 0.873036
# Null hypothesis probability of 7.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.008 sec: 2.30885 ( -0.35025 0.36829 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.1768e-06 ( -1.51402e-07 1.49839e-07 ) ergs/cm2
Band function
Time interval is from -0.352 sec. to 4.656 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 24.6154 (-2.97929 3.7313)
R^2/D10^2 : 6.83659E-02 (-0.0255198 0.0369197)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.58e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.633e-08 9.523e-09
25- 50 2.045e-07 4.294e-08
50-150 9.207e-07 1.650e-07
15-150 1.161e-06 1.810e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-20.7851 -200)
Norm : 11.5425 (-1.49436 1.49436)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.49e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.440e-07 8.128e-08
25- 50 2.771e-07 1.523e-07
50-150 6.077e-07 3.340e-07
15-150 1.029e-06 5.709e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.52619E-02 (0.822496 -0.0752619)
R1^2/D10^2 : 9.08017E+12 (-9.08017e+12 -9.08017e+12)
kT2 [keV] : 24.6150 (-2.97892 3.73166)
R2^2/D10^2 : 6.83691E-02 (-0.0255231 0.0369164)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Peak spectrum fit
Power-law model
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20353 ( -0.295158 0.281373 )
Norm@50keV : 2.74116E-02 ( -0.00671304 0.00663545 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.70 using 59 bins.
Reduced chi-squared = 1.3807
# Null hypothesis probability of 3.00e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.21552 ( -0.82598 0.85194 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.77818e-07 ( -6.24407e-08 6.24021e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.79557 ( -3.92018 2.31373 )
Epeak [keV] : 84.0149 ( -9.42104 11.7771 )
Norm@50keV : 1.34383 ( -1.34383 12.3934 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.31 using 59 bins.
Reduced chi-squared = 1.02339
# Null hypothesis probability of 4.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.06316 ( -0.67666 0.73043 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.33181e-07 ( -6.56525e-08 6.55225e-08 ) ergs/cm2
Band function
Time interval is from 0.516 sec. to 1.516 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 22.8204 (-3.10285 3.67089)
R^2/D10^2 : 0.129130 (-0.0553787 0.0860164)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.69e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.223e-08 4.111e-09
25- 50 6.608e-08 2.263e-08
50-150 2.571e-07 6.750e-08
15-150 3.354e-07 9.160e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-52.257 -200)
Norm : 14.9987 (-3.45396 3.45396)
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.90e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.739e-08 2.248e-08
25- 50 7.193e-08 4.178e-08
50-150 1.577e-07 9.180e-08
15-150 2.671e-07 1.550e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.108473 (3.28998 -0.108473)
R1^2/D10^2 : 7.37972E+09 (-7.37972e+09 -7.37972e+09)
kT2 [keV] : 22.8221 (-3.10194 3.67165)
R2^2/D10^2 : 0.129098 (-0.0553837 0.0860118)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.00e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 0.961923 ( -0.212188 0.200204 )
Norm@50keV : 2.19009E-02 ( -0.00308999 0.00303231 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.008 sec: 2.51705 ( -0.357157 0.364439 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20244e-06 ( -1.45005e-07 1.45013e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.981295 ( -1.58065 1.18292 )
Epeak [keV] : 102.128 ( -18.1694 54.3616 )
Norm@50keV : 0.114519 ( -0.0711622 0.272205 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.008 sec: 2.30889 ( -0.35024 0.36824 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17741e-06 ( -1.51497e-07 1.4996e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 2.17e-07
S(50-100 keV) = 4.46e-07
T90 vs. Hardness ratio plot
T90 = 4.46399998664856 sec.
Hardness ratio (energy fluence ratio) = 2.0553
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 4.32544
Count Ratio (50-100 keV) / (15-25 keV) = 6.79371
Mask shadow pattern
IMX = -1.470250168903059E+00, IMY = 5.365393966006989E-02
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:
-239.232000 -0.352000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9726 -15.6293 0.3 32.5 -33.2 18.3508 37.5 0.8 Sco X-1
254.2248 35.2790 0.0 23.5 -169.0 -0.7900 -1.8 12.0 Her X-1
268.3149 -1.5051 5.6 34.2 -83.4 1.6177 2.1 4.5 SW J1753.5-0127
202.4599 38.1393 2.3 38.6 109.6 5.9599 5.0 ------ UNKNOWN
203.8802 18.5972 2.7 33.3 77.2 3.3532 4.2 ------ UNKNOWN
217.9841 -24.8539 2.0 45.9 4.6 3.5007 5.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.352000 4.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1589 -15.5452 11.1 32.5 -33.5 0.0389 1.0 11.8 Sco X-1
254.3972 35.5434 0.0 23.7 -169.1 0.0380 1.2 12.4 Her X-1
268.2358 -1.5054 4.4 34.1 -83.3 -0.1513 -2.6 8.5 SW J1753.5-0127
243.6556 51.8729 2.9 35.8 163.1 0.1609 4.0 ------ UNKNOWN
284.7005 61.9041 1.0 55.8 -177.9 1.5691 11.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
128.668590 649.662400
660.768000 714.111100
720.768000 776.568610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2300 35.3226 6.2 32.7 -22.7 1.9599 1.9 11.2 Her X-1
299.5846 35.2117 0.8 28.3 -98.9 18.9587 13.6 0.7 Cyg X-1
308.1164 40.9553 1017.2 25.3 -117.4 0.0116 0.0 0.3 Cyg X-3
325.9415 38.2158 7.6 34.5 -138.7 1.9627 1.5 12.6 Cyg X-2
356.5795 28.2412 2.5 56.9 -161.3 20.3713 4.7 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:06:42 EST 2026