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
104.8832 4.9286 0.0077 34.1798 24.9301 3.7244045 25.102 TRIG_01044426
Foreground time interval of the image:
-21.744 23.517 (delta_t = 45.261 [sec])
Background time interval of the image:
-239.184 -21.744 (delta_t = 217.440 [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 -21.744 sec. to 73.216 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.14293 ( -0.128413 0.133211 )
Norm@50keV : 2.43501E-03 ( -0.000212842 0.000209833 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.71 using 59 bins.
Reduced chi-squared = 1.11772
# Null hypothesis probability of 2.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 94.96 sec: 0.391447 ( -0.026619 0.026638 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.15859e-06 ( -1.6732e-07 1.69503e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -21.744 sec. to 73.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.13245 ( -0.119649 0.144751 )
Epeak [keV] : 9999.36 ( )
Norm@50keV : 2.45667E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.74 using 59 bins.
Reduced chi-squared = 1.13821
# Null hypothesis probability of 2.23e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 94.96 sec: 0.378954 ( -0.02844 0.028413 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -21.744 sec. to 73.216 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] : 9.06148 (-0.662826 0.716016)
R^2/D10^2 : 0.260538 (-0.0683496 0.0925492)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.13e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.969e-07 4.563e-08
25- 50 8.526e-07 6.619e-08
50-150 3.321e-07 6.609e-08
15-150 1.582e-06 1.277e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.6579 (-8.92083 12.1334)
Norm : 2.16957 (-0.247576 0.303383)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.074e-07 4.914e-08
25- 50 7.372e-07 5.232e-08
50-150 7.378e-07 1.291e-07
15-150 1.982e-06 1.714e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.18879 (-1.47307 1.12519)
R1^2/D10^2 : 0.554772 (-0.215332 0.585627)
kT2 [keV] : 28.4962 (-12.7597 69.3359)
R2^2/D10^2 : 1.63988E-03 (-0.00149246 0.0151134)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.02e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.696e-07 7.915e-08
25- 50 7.706e-07 1.405e-07
50-150 8.376e-07 3.981e-07
15-150 2.078e-06 5.228e-07
Peak spectrum fit
Power-law model
Time interval is from 2.468 sec. to 3.468 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90520 ( -0.216109 0.231347 )
Norm@50keV : 1.40632E-02 ( -0.00232672 0.00228206 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.77 using 59 bins.
Reduced chi-squared = 0.995965
# Null hypothesis probability of 4.84e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.02282 ( -0.29281 0.29293 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.29318e-07 ( -2.08829e-08 2.10966e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.468 sec. to 3.468 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.108457 ( -1.65311 1.16323 )
Epeak [keV] : 46.6161 ( -8.16965 13.6602 )
Norm@50keV : 0.142076 ( -0.142979 1.11356 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.77 using 59 bins.
Reduced chi-squared = 0.870893
# Null hypothesis probability of 7.42e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.98206 ( -0.29618 0.29574 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20224e-07 ( -2.09741e-08 2.1963e-08 ) ergs/cm2
Band function
Time interval is from 2.468 sec. to 3.468 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] : 11.2341 (-1.47617 1.70513)
R^2/D10^2 : 0.682969 (-0.285906 0.474233)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.78e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.808e-08 4.590e-09
25- 50 5.251e-08 1.107e-08
50-150 3.804e-08 1.202e-08
15-150 1.086e-07 2.009e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 78.1597 (-24.8312 44.9592)
Norm : 9.90871 (-1.84674 2.23877)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.567e-08 4.875e-09
25- 50 4.202e-08 6.430e-09
50-150 5.839e-08 3.013e-08
15-150 1.261e-07 2.821e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.27079 (-8.32002 4.85724)
R1^2/D10^2 : 1.39957 (-1.32351 -1.33911)
kT2 [keV] : 18.6692 (-19.6026 -19.6028)
R2^2/D10^2 : 4.96464E-02 (-0.0382914 0.654349)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.11e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.115e-08 1.254e-08
25- 50 4.910e-08 3.137e-08
50-150 5.110e-08 2.994e-08
15-150 1.214e-07 7.140e-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: 2.06282 ( -0.112746 0.116002 )
Norm@50keV : 4.78722E-03 ( -0.000350901 0.000346517 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.07e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 45.26 sec: 0.739626 ( -0.0453984 0.0454543 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.00647e-06 ( -1.35886e-07 1.3704e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49626 ( -0.559345 0.48539 )
Epeak [keV] : 37.6917 ( -30.7994 11.2019 )
Norm@50keV : 1.00438E-02 ( -0.00464601 0.0108298 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 45.26 sec: 0.720517 ( -0.048113 0.048116 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.89974e-06 ( -1.60578e-07 1.63248e-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) = 6.75e-07
S(50-100 keV) = 6.12e-07
T90 vs. Hardness ratio plot
T90 = 79.1999999284744 sec.
Hardness ratio (energy fluence ratio) = 0.906667
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.06086
Count Ratio (50-100 keV) / (15-25 keV) = 0.4567
Mask shadow pattern
IMX = 6.158086990259720E-01, IMY = -2.862423554189181E-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:
-239.184000 -21.744000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6337 22.0220 0.6 44.0 -15.4 8.8795 20.7 0.5 Crab
87.2798 19.2404 2.7 41.4 -10.1 1.5981 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-21.744000 23.516590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5217 22.0562 27.7 44.0 -15.5 -0.0666 -0.4 6.7 Crab
104.8832 4.9286 0.5 34.2 24.9 3.7252 25.1 ------ UNKNOWN
32.0933 -55.5871 2.2 50.5 -161.0 1.0231 5.2 ------ UNKNOWN
24.8496 -39.2538 2.3 52.2 -139.2 2.2571 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.116590 483.616600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6311 22.0145 0.4 26.7 -59.1 16.6718 28.2 0.1 Crab
143.6054 -8.3299 3.7 40.8 98.0 4.9131 3.1 ------ UNKNOWN
145.2109 9.1288 6.7 40.2 70.9 3.1567 1.7 ------ UNKNOWN
122.1410 -41.3478 2.9 48.9 152.0 5.5198 4.0 ------ UNKNOWN
110.4368 -45.7212 3.3 50.9 164.2 5.2659 3.5 ------ UNKNOWN
81.0799 -40.1381 4.0 50.1 -167.1 3.1660 2.9 ------ UNKNOWN
84.4844 22.9084 2.8 26.7 -56.5 2.2305 4.1 ------ UNKNOWN
66.1696 -40.3651 3.0 57.6 -156.4 8.7421 3.8 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:04:20 EDT 2022