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
155.3654 6.3493 0.0183 33.3040 2.2313 0.0858576 10.509 TRIG_01273071
Foreground time interval of the image:
-0.072 0.184 (delta_t = 0.256 [sec])
Background time interval of the image:
-51.051 -0.072 (delta_t = 50.979 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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 0.256000
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 0.256000
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 -0.072 sec. to 0.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04966 ( -0.289438 0.278251 )
Norm@50keV : 2.00266E-02 ( -0.00369314 0.00365912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.58 using 59 bins.
Reduced chi-squared = 0.887368
# Null hypothesis probability of 7.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.256 sec: 2.31294 ( -0.43666 0.43841 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.45004e-08 ( -1.01098e-08 1.01142e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.072 sec. to 0.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.357039 ( -1.52659 0.878831 )
Epeak [keV] : 146.921 ( -63.1751 -146.92 )
Norm@50keV : 3.92575E-02 ( -0.0219367 0.113816 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.56 using 59 bins.
Reduced chi-squared = 0.885
# Null hypothesis probability of 7.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.256 sec: 2.28396 ( -0.44 0.44188 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.46675e-08 ( -1.03424e-08 1.02826e-08 ) ergs/cm2
Band function
Time interval is from -0.072 sec. to 0.184 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] : 23.1282 (-4.53707 6.00318)
R^2/D10^2 : 7.42661E-02 (-0.0390346 0.0753084)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.27e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.838e-09 6.973e-10
25- 50 1.000e-08 3.045e-09
50-150 3.996e-08 1.242e-08
15-150 5.180e-08 1.443e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-45.7302 -200)
Norm : 9.62162 (-1.8118 1.8118)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.133e-09 3.575e-09
25- 50 1.180e-08 6.834e-09
50-150 2.587e-08 1.512e-08
15-150 4.381e-08 2.509e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.0417 (-10.3102 85.9838)
R1^2/D10^2 : 0.365460 (-0.338241 0.80407)
kT2 [keV] : 34.6728 (-34.6888 -34.689)
R2^2/D10^2 : 1.57735E-02 (-0.00787268 0.0744239)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.70e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.077e-09 1.870e-09
25- 50 1.128e-08 6.884e-09
50-150 4.035e-08 2.088e-08
15-150 5.471e-08 2.720e-08
Peak spectrum fit
Power-law model
Time interval is from -0.412 sec. to 0.588 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.842147 ( -0.439454 0.383891 )
Norm@50keV : 6.43494E-03 ( -0.00172921 0.00165948 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.51 using 59 bins.
Reduced chi-squared = 0.851053
# Null hypothesis probability of 7.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.738763 ( -0.18918 0.192275 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.39061e-08 ( -1.75034e-08 1.75073e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.412 sec. to 0.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.168230 ( -2.72819 1.30795 )
Epeak [keV] : 132.255 ( -57.1582 -132.257 )
Norm@50keV : 1.68449E-02 ( -0.0168444 0.164646 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.62 using 59 bins.
Reduced chi-squared = 0.850357
# Null hypothesis probability of 7.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.718602 ( -0.189519 0.195136 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24086e-08 ( -1.86559e-08 1.80917e-08 ) ergs/cm2
Band function
Time interval is from -0.412 sec. to 0.588 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] : 24.6594 (-6.07675 10.2939)
R^2/D10^2 : 2.01299E-02 (-0.0133096 0.0298756)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.82e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.142e-09 1.182e-09
25- 50 1.207e-08 6.162e-09
50-150 5.451e-08 2.571e-08
15-150 6.871e-08 2.665e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-58.6938 -200)
Norm : 3.12343 (-0.805023 0.805023)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.777e-09 4.775e-09
25- 50 1.496e-08 8.815e-09
50-150 3.281e-08 2.004e-08
15-150 5.555e-08 3.406e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.287441 (-0.361061 199.639)
R1^2/D10^2 : 2.15347E+18 (-2.22936e+18 4.99999e+23)
kT2 [keV] : 24.9758 (-6.17977 10.5993)
R2^2/D10^2 : 1.92492E-02 (-0.0127926 0.0249025)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.45e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.151e-09 1.159e-09
25- 50 1.210e-08 5.944e-09
50-150 5.440e-08 2.416e-08
15-150 6.865e-08 2.939e-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: 1.04966 ( -0.289438 0.278251 )
Norm@50keV : 2.00266E-02 ( -0.00369314 0.00365912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.256 sec: 2.31298 ( -0.436674 0.438345 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.44934e-08 ( -1.01074e-08 1.01233e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.357046 ( -1.52659 0.878819 )
Epeak [keV] : 146.921 ( -63.1751 -146.92 )
Norm@50keV : 3.92573E-02 ( -0.0219367 0.113816 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.256 sec: 2.28390 ( -0.43945 0.44196 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.46941e-08 ( -1.03473e-08 1.02956e-08 ) 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) = 1.04e-08
S(50-100 keV) = 2.01e-08
T90 vs. Hardness ratio plot
T90 = 0.25599992275238 sec.
Hardness ratio (energy fluence ratio) = 1.93269
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.85333
Count Ratio (50-100 keV) / (15-25 keV) = 2.34966
Mask shadow pattern
IMX = 6.564799123820915E-01, IMY = -2.557807202558693E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-51.051400 -0.072000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
93.4828 69.7761 2.3 48.6 136.4 2.4014 5.1 ------ UNKNOWN
137.6329 46.3023 2.3 22.4 102.8 0.6419 5.1 ------ UNKNOWN
138.2111 36.4430 2.6 22.2 76.7 0.5478 4.5 ------ UNKNOWN
160.5510 -16.9668 3.9 55.4 -11.0 0.9466 3.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.072000 0.184000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
110.3697 81.4289 2.7 47.4 152.9 0.0799 4.3 ------ UNKNOWN
155.3655 6.3493 1.1 33.3 2.2 0.0858 10.5 ------ UNKNOWN
214.1874 26.4534 2.3 41.8 -105.8 0.1515 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
89.748600 962.307800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5290 -40.5481 1.3 50.3 -2.3 14.8192 8.8 0.4 Vela X-1
143.3480 -46.7349 2.4 54.1 -11.7 11.0675 4.7 ------ UNKNOWN
177.3465 -8.1024 2.7 26.2 -78.9 5.5209 4.3 ------ UNKNOWN
Plot creation:
Fri Jun 20 02:02:43 EDT 2025