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
358.1895 -39.1041 0.0174 17.6795 59.1062 0.3035949 10.940 TRIG_01048783
Foreground time interval of the image:
-0.168 3.128 (delta_t = 3.296 [sec])
Background time interval of the image:
-239.608 -0.168 (delta_t = 239.440 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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 0.512000
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 0.512000
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 -0.168 sec. to 3.128 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85241 ( -0.246014 0.260135 )
Norm@50keV : 4.98189E-03 ( -0.000872253 0.000851568 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.73 using 59 bins.
Reduced chi-squared = 1.18825
# Null hypothesis probability of 1.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 3.296 sec: 0.700981 ( -0.101592 0.101609 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.51004e-07 ( -2.59842e-08 2.66431e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.168 sec. to 3.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.979100 ( -1.40894 0.976657 )
Epeak [keV] : 48.3822 ( -16.4716 -48.3825 )
Norm@50keV : 1.61425E-02 ( -0.016142 0.098804 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.50 using 59 bins.
Reduced chi-squared = 1.16964
# Null hypothesis probability of 1.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 3.296 sec: 0.684401 ( -0.102988 0.10317 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38385e-07 ( -2.80613e-08 2.99787e-08 ) ergs/cm2
Band function
Time interval is from -0.168 sec. to 3.128 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] : 10.0707 (-1.55124 1.91192)
R^2/D10^2 : 0.331191 (-0.160952 0.294388)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.45e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.260e-08 5.392e-09
25- 50 5.675e-08 1.172e-08
50-150 3.023e-08 1.129e-08
15-150 1.096e-07 2.332e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 81.4003 (-30.1176 67.5394)
Norm : 3.31426 (-0.644722 0.83241)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.838e-08 5.127e-09
25- 50 4.691e-08 8.734e-09
50-150 6.698e-08 3.732e-08
15-150 1.423e-07 4.403e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.07062 (-2.13151 2.17893)
R1^2/D10^2 : 0.939022 (-0.559522 2.0902)
kT2 [keV] : 24.0049 (-17.2791 33.4605)
R2^2/D10^2 : 7.71556E-03 (-0.00744118 0.0588926)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.771e-08 1.569e-08
25- 50 4.951e-08 2.607e-08
50-150 6.802e-08 3.813e-08
15-150 1.452e-07 7.571e-08
Peak spectrum fit
Power-law model
Time interval is from -0.180 sec. to 0.820 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77938 ( -0.218147 0.229124 )
Norm@50keV : 1.07693E-02 ( -0.0017041 0.00167544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.47 using 59 bins.
Reduced chi-squared = 1.20123
# Null hypothesis probability of 1.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.47237 ( -0.20413 0.20417 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.92385e-08 ( -1.58761e-08 1.61573e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.180 sec. to 0.820 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.650391 ( -1.98061 1.43356 )
Epeak [keV] : 46.2521 ( -6.3817 11.1353 )
Norm@50keV : 0.256358 ( -0.270148 3.16881 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.24 using 59 bins.
Reduced chi-squared = 1.04
# Null hypothesis probability of 3.93e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.39211 ( -0.2078 0.2086 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.4598e-08 ( -1.43183e-08 1.63319e-08 ) ergs/cm2
Band function
Time interval is from -0.180 sec. to 0.820 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] : 11.5414 (-1.3713 1.56943)
R^2/D10^2 : 0.452652 (-0.173791 0.271496)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.270e-08 2.966e-09
25- 50 3.814e-08 6.855e-09
50-150 2.974e-08 9.515e-09
15-150 8.058e-08 1.411e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 91.4229 (-31.2107 66.7425)
Norm : 6.81922 (-1.18149 1.43094)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.47e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.780e-08 3.360e-09
25- 50 3.021e-08 5.080e-09
50-150 4.645e-08 2.495e-08
15-150 9.446e-08 2.828e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.21497 (-2.21602 84.3998)
R1^2/D10^2 : 3.08068E+04 (-33127.9 -33127.9)
kT2 [keV] : 11.8377 (-1.46946 2.65046)
R2^2/D10^2 : 0.404741 (-0.405214 0.220815)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.89e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.409e-08 4.267e-09
25- 50 3.654e-08 1.133e-08
50-150 3.162e-08 1.223e-08
15-150 8.226e-08 2.006e-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: 1.85241 ( -0.246014 0.260135 )
Norm@50keV : 4.98189E-03 ( -0.000872253 0.000851568 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 3.296 sec: 0.700941 ( -0.101586 0.101602 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50976e-07 ( -2.59632e-08 2.66625e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.979118 ( -1.40894 0.976655 )
Epeak [keV] : 48.3825 ( -16.4717 -48.3825 )
Norm@50keV : 1.61421E-02 ( -0.016142 0.0988039 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 3.296 sec: 0.684285 ( -0.10296 0.101605 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38421e-07 ( -2.80707e-08 3.0013e-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) = 4.32e-08
S(50-100 keV) = 4.81e-08
T90 vs. Hardness ratio plot
T90 = 3.05600011348724 sec.
Hardness ratio (energy fluence ratio) = 1.11343
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.04756
Count Ratio (50-100 keV) / (15-25 keV) = 0.541184
Mask shadow pattern
IMX = 1.636593379262233E-01, IMY = -2.735224024754572E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.608000 -0.168000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
42.3231 -65.0125 3.5 50.1 26.4 3.5501 3.3 ------ UNKNOWN
318.6359 -4.6968 2.8 46.2 152.1 2.7202 4.1 ------ UNKNOWN
28.3906 -6.4829 2.7 29.0 -71.4 1.5877 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.168000 3.128000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
358.1895 -39.1041 1.0 17.7 59.1 0.3036 10.9 ------ UNKNOWN
341.9549 31.7016 2.2 57.2 -154.4 0.5603 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
50.892590 962.452000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
322.8268 6.9284 2.7 56.5 173.6 15.7234 4.3 ------ UNKNOWN
80.2454 -47.0264 3.1 57.7 -15.8 11.7771 3.7 ------ UNKNOWN
341.8970 15.9558 3.0 57.1 -161.5 13.1687 3.9 ------ UNKNOWN
359.0919 11.1470 3.7 50.3 -141.7 7.2871 3.1 ------ UNKNOWN
10.6898 6.1884 3.1 46.7 -125.6 11.2863 3.7 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:00:33 EDT 2022