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
78.8906 0.9128 0.0153 7.1543 72.9221 2.8357197 12.547 TRIG_01090472
Foreground time interval of the image:
-129.340 15.181 (delta_t = 144.521 [sec])
Background time interval of the image:
-239.120 -129.340 (delta_t = 109.780 [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 -129.340 sec. to 26.356 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27647 ( -0.156383 0.155253 )
Norm@50keV : 1.11758E-03 ( -0.000102293 0.000102133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.38 using 59 bins.
Reduced chi-squared = 0.901404
# Null hypothesis probability of 6.85e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 155.7 sec: 0.132771 ( -0.012168 0.012179 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72981e-06 ( -1.7918e-07 1.81532e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -129.340 sec. to 26.356 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.438363 ( -0.845839 0.697526 )
Epeak [keV] : 91.1456 ( -24.4686 185.423 )
Norm@50keV : 2.99960E-03 ( -0.00165692 0.00496774 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.06 using 59 bins.
Reduced chi-squared = 0.840357
# Null hypothesis probability of 7.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 155.7 sec: 0.127684 ( -0.012992 0.012923 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.59312e-06 ( -1.90281e-07 2.13838e-07 ) ergs/cm2
Band function
Time interval is from -129.340 sec. to 26.356 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] : 15.8212 (-1.66889 1.94656)
R^2/D10^2 : 1.31794E-02 (-0.00431261 0.00613836)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.065e-07 1.982e-08
25- 50 4.437e-07 5.418e-08
50-150 7.729e-07 1.415e-07
15-150 1.323e-06 1.789e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-31.3711 -200)
Norm : 0.545172 (-0.0497675 0.0497675)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.94e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.113e-07 2.756e-08
25- 50 4.065e-07 1.622e-07
50-150 8.916e-07 4.518e-07
15-150 1.510e-06 6.954e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.3628 (-3.82369 2.97261)
R1^2/D10^2 : 3.10162E-02 (-0.0159564 0.0543318)
kT2 [keV] : 51.1152 (-25.4346 -47.0013)
R2^2/D10^2 : 1.96399E-04 (-0.000173156 0.0034468)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.21e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.412e-07 5.601e-08
25- 50 4.465e-07 1.738e-07
50-150 1.064e-06 5.350e-07
15-150 1.652e-06 7.012e-07
Peak spectrum fit
Power-law model
Time interval is from 0.236 sec. to 1.236 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14920 ( -0.294944 0.286969 )
Norm@50keV : 7.77692E-03 ( -0.00137978 0.00137884 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.81 using 59 bins.
Reduced chi-squared = 1.0493
# Null hypothesis probability of 3.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.906869 ( -0.161894 0.162081 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.00848e-08 ( -1.59786e-08 1.62826e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.236 sec. to 1.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.188996 ( -1.60467 1.0746 )
Epeak [keV] : 92.9824 ( -34.3026 -92.9952 )
Norm@50keV : 2.41538E-02 ( -0.0241453 0.136535 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.80 using 59 bins.
Reduced chi-squared = 1.03214
# Null hypothesis probability of 4.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.876004 ( -0.166702 0.166596 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.33398e-08 ( -1.81537e-08 1.8392e-08 ) ergs/cm2
Band function
Time interval is from 0.236 sec. to 1.236 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] : 16.6974 (-3.41292 4.75995)
R^2/D10^2 : 7.75591E-02 (-0.0437222 0.0896057)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.425e-09 1.644e-09
25- 50 1.930e-08 6.012e-09
50-150 3.819e-08 1.434e-08
15-150 6.191e-08 1.635e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-62.2402 -200)
Norm : 3.66784 (-0.664019 0.664019)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.58e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.133e-09 5.290e-09
25- 50 1.757e-08 1.016e-08
50-150 3.853e-08 2.168e-08
15-150 6.523e-08 3.775e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.0039 (-4.71922 6.12114)
R1^2/D10^2 : 0.267194 (-0.182929 1.07017)
kT2 [keV] : 34.1424 (-23.3657 -35.2126)
R2^2/D10^2 : 5.21807E-03 (-0.00436578 0.0505272)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.20e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.323e-09 3.720e-09
25- 50 1.923e-08 1.155e-08
50-150 5.102e-08 2.693e-08
15-150 7.657e-08 3.900e-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: 1.25314 ( -0.163869 0.162251 )
Norm@50keV : 1.10348E-03 ( -0.000105872 0.000105745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 144.5 sec: 0.130579 ( -0.0125827 0.012595 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.59449e-06 ( -1.73302e-07 1.75449e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.358682 ( -0.915014 0.744179 )
Epeak [keV] : 89.7154 ( -24.0132 180.529 )
Norm@50keV : 3.16583E-03 ( -0.00182409 0.00595395 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 144.5 sec: 0.125294 ( -0.013448 0.013375 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4603e-06 ( -2.04414e-07 2.08326e-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) = 3.80e-07
S(50-100 keV) = 6.27e-07
T90 vs. Hardness ratio plot
T90 = 136.527999997139 sec.
Hardness ratio (energy fluence ratio) = 1.65
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.85937
Count Ratio (50-100 keV) / (15-25 keV) = 1.37176
Mask shadow pattern
IMX = 3.686134579391920E-02, IMY = -1.199847013855260E-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:
-239.120000 -129.340000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6329 22.0285 0.8 28.8 72.0 3.7422 14.9 0.8 Crab
63.7565 -40.4099 3.8 36.4 -103.0 1.1936 3.0 ------ UNKNOWN
20.0287 -2.9450 2.0 57.1 -30.0 5.4847 5.7 ------ UNKNOWN
88.8603 -53.2947 2.4 48.2 -129.7 4.1727 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-129.340000 15.180590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7327 21.9465 5.0 28.7 72.2 0.9021 2.3 6.9 Crab
78.8906 0.9128 0.9 7.2 72.9 2.8357 12.6 ------ UNKNOWN
133.5027 -31.2078 2.3 58.2 -177.2 8.0872 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
42.980590 963.023700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6339 22.0224 0.3 21.6 77.0 39.7659 33.7 0.5 Crab
114.0495 0.5421 2.6 35.1 155.4 6.4208 4.5 ------ UNKNOWN
61.7803 0.6624 6.3 17.1 -25.7 1.5964 1.8 ------ UNKNOWN
126.7128 -34.7100 3.2 57.1 -161.4 14.7239 3.6 ------ UNKNOWN
123.7202 -40.4233 3.6 58.0 -154.2 16.7233 3.2 ------ UNKNOWN
114.3121 -44.5330 5.7 55.3 -145.1 13.0549 2.0 ------ UNKNOWN
94.4920 -45.2549 3.1 48.2 -129.6 17.4754 3.7 ------ UNKNOWN
98.6984 -45.6740 3.2 49.8 -133.0 17.4026 3.6 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:12:59 EDT 2022