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
2.7783 -33.0024 0.0077 20.1553 -113.4665 5.4642150 24.944 TRIG_01040345
Foreground time interval of the image:
-41.512 137.180 (delta_t = 178.692 [sec])
Background time interval of the image:
-239.736 -41.512 (delta_t = 198.224 [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 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)
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 -41.512 sec. to 137.180 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.13894 ( -0.0954955 0.0979627 )
Norm@50keV : 1.80855E-03 ( -0.000109565 0.000108536 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.24 using 59 bins.
Reduced chi-squared = 1.30246
# Null hypothesis probability of 6.21e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 178.7 sec: 0.290152 ( -0.014311 0.014336 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.01567e-06 ( -1.62849e-07 1.64458e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -41.512 sec. to 137.180 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.964136 ( -0.547066 0.486828 )
Epeak [keV] : 36.9070 ( -5.62927 4.35887 )
Norm@50keV : 8.30175E-03 ( -0.00385535 0.00860376 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.47 using 59 bins.
Reduced chi-squared = 0.972679
# Null hypothesis probability of 5.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 178.7 sec: 0.271190 ( -0.015865 0.015938 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.69565e-06 ( -1.85591e-07 1.94324e-07 ) ergs/cm2
Band function
Time interval is from -41.512 sec. to 137.180 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] : 9.96694 (-0.5185 0.546634)
R^2/D10^2 : 0.130360 (-0.024857 0.0307391)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 94.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.24e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.708e-07 4.092e-08
25- 50 1.165e-06 5.611e-08
50-150 6.022e-07 7.925e-08
15-150 2.238e-06 1.305e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 54.2665 (-6.9296 8.70951)
Norm : 1.55248 (-0.123866 0.150414)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.16e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.902e-07 3.565e-08
25- 50 1.020e-06 9.864e-08
50-150 1.067e-06 2.646e-07
15-150 2.777e-06 3.931e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.49130 (-1.2691 1.68976)
R1^2/D10^2 : 1.55417 (-1.05251 5.59501)
kT2 [keV] : 13.0502 (-1.59746 2.96271)
R2^2/D10^2 : 3.66696E-02 (-0.0232305 0.0306145)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.33e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.676e-07 2.595e-07
25- 50 1.032e-06 2.095e-07
50-150 8.883e-07 1.997e-07
15-150 2.588e-06 5.453e-07
Peak spectrum fit
Power-law model
Time interval is from 0.368 sec. to 1.368 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69418 ( -0.256013 0.271593 )
Norm@50keV : 7.91094E-03 ( -0.00139898 0.00136814 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.53 using 59 bins.
Reduced chi-squared = 0.851404
# Null hypothesis probability of 7.80e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.04858 ( -0.163681 0.16371 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.32909e-08 ( -1.34029e-08 1.36852e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.368 sec. to 1.368 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.384593 ( -1.83573 1.24868 )
Epeak [keV] : 56.0632 ( -13.1877 152.948 )
Norm@50keV : 4.07524E-02 ( -0.0407595 0.357404 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.31 using 59 bins.
Reduced chi-squared = 0.809107
# Null hypothesis probability of 8.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.00665 ( -0.170954 0.16977 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.65426e-08 ( -1.38924e-08 1.50799e-08 ) ergs/cm2
Band function
Time interval is from 0.368 sec. to 1.368 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] : 12.5378 (-1.88396 2.27632)
R^2/D10^2 : 0.230606 (-0.105421 0.18458)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.95e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.686e-09 2.173e-09
25- 50 2.544e-08 5.770e-09
50-150 2.473e-08 8.075e-09
15-150 5.786e-08 1.326e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 125.327 (-54.0648 -121.647)
Norm : 4.44515 (-0.748757 1.04109)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.156e-08 4.990e-09
25- 50 2.083e-08 9.770e-09
50-150 3.796e-08 2.424e-08
15-150 7.034e-08 3.918e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.09154 (-1.70051 8.656)
R1^2/D10^2 : 21.8767 (-21.4798 207.791)
kT2 [keV] : 14.1967 (-2.55391 -14.1963)
R2^2/D10^2 : 0.135903 (-0.135562 0.0627889)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.57e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.070e-08 4.739e-09
25- 50 2.258e-08 9.700e-09
50-150 2.912e-08 1.497e-08
15-150 6.240e-08 2.684e-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: 2.13894 ( -0.0954955 0.0979627 )
Norm@50keV : 1.80855E-03 ( -0.000109565 0.000108536 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.21e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 178.7 sec: 0.290125 ( -0.014308 0.0143344 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.0151e-06 ( -1.62936e-07 1.64435e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.964137 ( -0.547066 0.486828 )
Epeak [keV] : 36.9070 ( -5.62927 4.35887 )
Norm@50keV : 8.30174E-03 ( -0.00385535 0.00860376 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 178.7 sec: 0.271135 ( -0.015856 0.015928 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.69621e-06 ( -1.85526e-07 1.9439e-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) = 9.42e-07
S(50-100 keV) = 8.56e-07
T90 vs. Hardness ratio plot
T90 = 167.659999966621 sec.
Hardness ratio (energy fluence ratio) = 0.908705
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.11145
Count Ratio (50-100 keV) / (15-25 keV) = 0.424751
Mask shadow pattern
IMX = -1.461605609976621E-01, IMY = 3.366851304624006E-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:
-239.736000 -41.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
94.3481 -61.4081 3.1 43.0 45.0 1.9623 3.8 ------ UNKNOWN
26.8542 -69.4599 2.2 18.8 72.6 1.1696 5.1 ------ UNKNOWN
69.5482 -55.9502 2.5 33.1 29.1 1.2864 4.6 ------ UNKNOWN
33.9071 -58.6690 2.7 14.1 35.7 0.8063 4.3 ------ UNKNOWN
83.9040 -28.7338 3.0 57.0 4.7 4.3488 3.8 ------ UNKNOWN
70.0206 -18.3488 3.1 56.2 -14.9 2.8399 3.7 ------ UNKNOWN
315.4872 -12.7469 2.8 59.6 -161.2 7.5057 4.2 ------ UNKNOWN
319.0764 -10.4510 2.9 59.4 -156.4 5.7685 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-41.512000 137.180000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
48.1719 -71.3138 2.0 25.1 62.4 1.4940 5.8 ------ UNKNOWN
2.7782 -33.0024 0.5 20.2 -113.5 5.4644 24.9 ------ UNKNOWN
14.9765 -16.5643 2.5 35.6 -85.8 2.1129 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
877.464610 944.440700
945.264000 962.364000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6262 22.0020 2.4 56.4 -4.0 2.4380 4.8 0.8 Crab
Plot creation:
Sat Jul 30 07:07:40 EDT 2022