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
12.5027 -55.8622 0.0095 29.1128 12.9936 1.8343177 20.117 TRIG_01001130
Foreground time interval of the image:
-4.188 27.952 (delta_t = 32.140 [sec])
Background time interval of the image:
-239.512 -4.188 (delta_t = 235.324 [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 4.096000
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 4.096000
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 4.096000
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 -4.188 sec. to 27.952 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62583 ( -0.147874 0.150283 )
Norm@50keV : 3.41855E-03 ( -0.000298831 0.000295852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.15 using 59 bins.
Reduced chi-squared = 0.809649
# Null hypothesis probability of 8.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 32.14 sec: 0.442903 ( -0.03676 0.036812 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0246e-06 ( -9.56891e-08 9.67067e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.188 sec. to 27.952 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55024 ( -0.542977 0.629536 )
Epeak [keV] : 261.139 ( -390.827 -390.827 )
Norm@50keV : 3.73832E-03 ( -0.00198731 0.00324655 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.19 using 59 bins.
Reduced chi-squared = 0.824821
# Null hypothesis probability of 8.22e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 32.14 sec: 0.442135 ( -0.038142 0.037418 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02133e-06 ( -1.05539e-07 9.89751e-08 ) ergs/cm2
Band function
Time interval is from -4.188 sec. to 27.952 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] : 13.6804 (-1.54295 1.76339)
R^2/D10^2 : 6.61749E-02 (-0.0232381 0.0356243)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 92.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.24e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.424e-08 1.287e-08
25- 50 3.061e-07 3.161e-08
50-150 3.727e-07 6.639e-08
15-150 7.630e-07 8.469e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.887 (-56.912 -168.751)
Norm : 1.80497 (-0.160971 0.185586)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.473e-07 2.938e-08
25- 50 2.776e-07 1.028e-07
50-150 5.742e-07 2.892e-07
15-150 9.992e-07 4.197e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.05515 (-1.28683 1.55151)
R1^2/D10^2 : 0.862141 (-0.479587 1.30703)
kT2 [keV] : 25.1374 (-5.06287 8.92189)
R2^2/D10^2 : 6.20702E-03 (-0.00400918 0.00787514)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.17e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.586e-07 5.419e-08
25- 50 2.633e-07 8.588e-08
50-150 5.948e-07 2.285e-07
15-150 1.017e-06 3.212e-07
Peak spectrum fit
Power-law model
Time interval is from -3.624 sec. to -2.624 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98377 ( -0.346917 0.38614 )
Norm@50keV : 6.57166E-03 ( -0.0017547 0.00169303 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.22 using 59 bins.
Reduced chi-squared = 0.968772
# Null hypothesis probability of 5.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.978536 ( -0.201858 0.201854 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.05662e-08 ( -1.49468e-08 1.5505e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.624 sec. to -2.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07451 ( -1.71231 1.05153 )
Epeak [keV] : 41.9411 ( -40.497 -41.9421 )
Norm@50keV : 2.25474E-02 ( -0.0225433 0.224852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.78 using 59 bins.
Reduced chi-squared = 0.960357
# Null hypothesis probability of 5.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.962681 ( -0.201233 0.202179 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.63417e-08 ( -1.48224e-08 1.63475e-08 ) ergs/cm2
Band function
Time interval is from -3.624 sec. to -2.624 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] : 9.76572 (-2.54207 3.39706)
R^2/D10^2 : 0.511306 (-0.3446 1.11179)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.94e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.847e-09 4.398e-09
25- 50 2.367e-08 8.250e-09
50-150 1.153e-08 6.691e-09
15-150 4.504e-08 1.723e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 65.4534 (-28.5162 74.0808)
Norm : 5.02872 (-1.40008 1.97402)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.94e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.280e-08 4.091e-09
25- 50 1.999e-08 6.830e-09
50-150 2.440e-08 1.627e-08
15-150 5.718e-08 2.119e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.17903 (-1.79821 2.48593)
R1^2/D10^2 : 3.90321 (-3.00514 7.53533)
kT2 [keV] : 17.3406 (-5.68508 12.1576)
R2^2/D10^2 : 4.19294E-02 (-0.0338409 0.169994)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.88e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.346e-08 8.005e-09
25- 50 1.924e-08 1.014e-08
50-150 2.516e-08 1.559e-08
15-150 5.786e-08 2.950e-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: 1.62583 ( -0.147874 0.150283 )
Norm@50keV : 3.41855E-03 ( -0.000298831 0.000295852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 32.14 sec: 0.442887 ( -0.0367571 0.0368099 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02446e-06 ( -9.58174e-08 9.67228e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58754 ( -0.557464 0.600147 )
Epeak [keV] : 523.558 ( -523.558 -523.558 )
Norm@50keV : 3.57931E-03 ( -0.00168071 0.00326533 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 32.14 sec: 0.441929 ( -0.038007 0.037477 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01865e-06 ( -1.0271e-07 1.02051e-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) = 2.69e-07
S(50-100 keV) = 3.47e-07
T90 vs. Hardness ratio plot
T90 = 24.3839999437332 sec.
Hardness ratio (energy fluence ratio) = 1.28996
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.20774
Count Ratio (50-100 keV) / (15-25 keV) = 0.893784
Mask shadow pattern
IMX = 5.426257485623531E-01, IMY = -1.252113140484960E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.512000 -4.188000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6163 -40.4993 6.3 47.4 -130.1 2.0289 1.8 5.2 Vela X-1
0.0334 -52.3766 2.6 37.2 13.0 1.7400 4.5 ------ UNKNOWN
275.8011 -70.5796 3.9 52.6 -40.8 4.1478 2.9 ------ UNKNOWN
148.2935 -61.7937 3.7 41.2 -98.7 3.4608 3.2 ------ UNKNOWN
135.9069 -37.2959 2.8 49.8 -133.0 5.2639 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.188000 27.952000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5457 -40.5341 9.5 47.4 -130.1 -0.4008 -1.2 1.5 Vela X-1
28.8062 -24.4720 2.0 40.4 70.8 1.7599 5.6 ------ UNKNOWN
47.6077 -28.9056 2.7 28.8 94.0 0.5343 4.3 ------ UNKNOWN
58.0369 -47.4452 2.2 8.6 93.7 0.4164 5.1 ------ UNKNOWN
12.5027 -55.8622 0.6 29.1 13.0 1.8344 20.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
85.988620 916.788600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
41.1089 -37.9249 2.8 26.2 133.8 3.9295 4.1 ------ UNKNOWN
25.1144 -47.8780 2.5 11.1 124.3 3.1642 4.6 ------ UNKNOWN
291.1834 -38.6342 3.0 54.4 -33.2 16.0317 3.9 ------ UNKNOWN
289.9973 -44.8292 2.8 50.6 -39.5 9.5226 4.1 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:29:20 EDT 2022