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
212.9611 35.9953 0.0134 32.4196 -22.1333 1.6556148 14.286 TRIG_01044236
Foreground time interval of the image:
11.960 72.501 (delta_t = 60.541 [sec])
Background time interval of the image:
-203.899 11.960 (delta_t = 215.859 [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 11.960 sec. to 88.780 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42570 ( -0.245422 0.272017 )
Norm@50keV : 1.03667E-03 ( -0.000200566 0.000197202 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.59 using 59 bins.
Reduced chi-squared = 0.992807
# Null hypothesis probability of 4.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 76.82 sec: 0.194760 ( -0.022761 0.022761 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.81674e-07 ( -1.13877e-07 1.17956e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 11.960 sec. to 88.780 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61098 ( -1.41116 0.398179 )
Epeak [keV] : 17.5623 ( -15.0695 14.6765 )
Norm@50keV : 3.33265E-03 ( -0.00180141 0.0228322 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.04 using 59 bins.
Reduced chi-squared = 0.982857
# Null hypothesis probability of 5.11e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 76.82 sec: 0.189889 ( -0.023447 0.023577 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.2416e-07 ( -1.18743e-07 1.32097e-07 ) ergs/cm2
Band function
Time interval is from 11.960 sec. to 88.780 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] : 7.81820 (-1.01424 1.1334)
R^2/D10^2 : 0.230840 (-0.0975114 0.176286)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.10e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.926e-07 3.995e-08
25- 50 3.238e-07 5.800e-08
50-150 7.877e-08 3.148e-08
15-150 5.951e-07 1.022e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 35.4177 (-9.06121 13.3951)
Norm : 1.36668 (-0.298376 0.409385)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.43e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.305e-07 3.576e-08
25- 50 2.869e-07 4.828e-08
50-150 1.932e-07 7.924e-08
15-150 7.106e-07 1.197e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.86937 (-1.47386 2.53194)
R1^2/D10^2 : 11.4031 (-10.6298 2771.41)
kT2 [keV] : 10.1353 (-2.02046 5.16702)
R2^2/D10^2 : 6.75236E-02 (-0.0589194 0.113959)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.325e-07 1.172e-07
25- 50 2.916e-07 1.498e-07
50-150 1.499e-07 8.767e-08
15-150 6.740e-07 3.110e-07
Peak spectrum fit
Power-law model
Time interval is from 47.972 sec. to 48.972 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87677 ( -0.436885 0.483855 )
Norm@50keV : 5.77815E-03 ( -0.00170785 0.0015984 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.21 using 59 bins.
Reduced chi-squared = 1.33702
# Null hypothesis probability of 4.55e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.821217 ( -0.192549 0.192673 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.31276e-08 ( -1.48134e-08 1.52935e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 47.972 sec. to 48.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.26113 ( -0.598576 0.483741 )
Epeak [keV] : 100.789 ( -9999.32 -9999.33 )
Norm@50keV : 3.56048E-03 ( -0.00167181 0.026067 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.78 using 59 bins.
Reduced chi-squared = 1.35321
# Null hypothesis probability of 4.03e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.665916 ( -0.29162 0.475754 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.8463e-08 ( -2.09435e-08 1.51169e-08 ) ergs/cm2
Band function
Time interval is from 47.972 sec. to 48.972 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] : 9.43100 (-2.31052 3.53196)
R^2/D10^2 : 0.472079 (-0.333738 0.932089)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.56e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.359e-09 4.655e-09
25- 50 1.908e-08 9.547e-09
50-150 8.386e-09 5.407e-09
15-150 3.583e-08 1.539e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 88.8909 (-50.5508 -88.9222)
Norm : 3.70835 (-1.12124 1.91164)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.91e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.672e-09 3.652e-09
25- 50 1.631e-08 7.868e-09
50-150 2.465e-08 2.005e-08
15-150 5.064e-08 2.997e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21983 (-3.30409 2.95954)
R1^2/D10^2 : 1.12611 (-0.721079 6.96155)
kT2 [keV] : 47.4475 (-43.5779 -60.2922)
R2^2/D10^2 : 1.21276E-03 (-0.000698043 0.0397513)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.26e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.004e-08 6.005e-09
25- 50 1.635e-08 9.700e-09
50-150 2.830e-08 1.683e-08
15-150 5.469e-08 2.809e-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: 2.38037 ( -0.242345 0.268027 )
Norm@50keV : 1.19275E-03 ( -0.000226253 0.000221901 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 60.54 sec: 0.218179 ( -0.0256846 0.0256846 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.01301e-07 ( -1.02579e-07 1.06234e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56310 ( -1.4165 0.437489 )
Epeak [keV] : 19.9628 ( -19.5754 13.9865 )
Norm@50keV : 3.81127E-03 ( -0.00214237 0.0262655 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 60.54 sec: 0.212674 ( -0.026435 0.026568 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.50206e-07 ( -1.08248e-07 1.22696e-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) = 2.57e-07
S(50-100 keV) = 1.91e-07
T90 vs. Hardness ratio plot
T90 = 54.4919998645782 sec.
Hardness ratio (energy fluence ratio) = 0.743191
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.98469
Count Ratio (50-100 keV) / (15-25 keV) = 0.263172
Mask shadow pattern
IMX = 5.882977985748454E-01, IMY = 2.392812365451210E-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:
-203.899390 11.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
161.3357 23.4290 3.0 32.3 -116.0 1.4078 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
11.960000 72.500590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
183.3775 -12.3301 2.9 23.7 146.6 0.4245 4.0 ------ UNKNOWN
217.9949 35.5287 2.6 35.0 -16.3 0.5639 4.4 ------ UNKNOWN
212.9611 35.9954 0.8 32.4 -22.1 1.6548 14.3 ------ UNKNOWN
228.8389 41.2229 2.4 45.2 -15.3 0.8059 4.8 ------ UNKNOWN
154.2576 18.6884 1.7 37.6 -126.8 1.1509 6.6 ------ UNKNOWN
149.1931 26.6425 2.2 43.8 -116.2 2.1575 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
136.100600 408.100600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5446 35.4389 73.8 33.5 -18.0 0.0500 0.2 7.2 Her X-1
209.3279 14.7456 2.5 21.5 93.3 1.4814 4.6 ------ UNKNOWN
213.1117 39.3191 2.7 3.3 -94.4 0.9888 4.3 ------ UNKNOWN
275.1574 23.9230 2.3 54.3 -11.8 3.8642 5.1 ------ UNKNOWN
141.2798 48.3952 3.7 52.5 -148.9 2.5935 3.1 ------ UNKNOWN
270.0378 63.6232 2.8 43.8 -63.7 4.6163 4.1 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:05:25 EDT 2022