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
20.6248 4.6468 0.0383 28.6928 -80.7352 0.8242906 5.018 TRIG_01069551
Foreground time interval of the image:
0.760 64.613 (delta_t = 63.853 [sec])
Background time interval of the image:
-239.288 0.760 (delta_t = 240.048 [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 16.384000
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 16.384000
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 16.384000
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 0.760 sec. to 160.204 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.09686 ( -0.211691 0.227318 )
Norm@50keV : 8.53766E-04 ( -0.000141413 0.000139686 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.83 using 59 bins.
Reduced chi-squared = 0.874211
# Null hypothesis probability of 7.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 159.4 sec: 0.134122 ( -0.015879 0.015886 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26412e-06 ( -1.87212e-07 1.9405e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.760 sec. to 160.204 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.720458 ( -1.77316 1.3724 )
Epeak [keV] : 35.8048 ( -4.54293 5.05782 )
Norm@50keV : 4.59707E-02 ( -0.0477179 0.55274 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.44 using 59 bins.
Reduced chi-squared = 0.615
# Null hypothesis probability of 9.90e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 159.4 sec: 0.125754 ( -0.015555 0.015685 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03803e-06 ( -1.4848e-07 1.68393e-07 ) ergs/cm2
Band function
Time interval is from 0.760 sec. to 160.204 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] : 9.19789 (-0.971048 1.08183)
R^2/D10^2 : 9.17545E-02 (-0.0323021 0.0495075)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.90e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.435e-07 4.535e-08
25- 50 5.353e-07 7.611e-08
50-150 2.182e-07 7.227e-08
15-150 9.971e-07 1.392e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 49.5454 (-12.6531 20.1555)
Norm : 0.778778 (-0.134483 0.172153)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.43e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.029e-07 4.224e-08
25- 50 4.336e-07 6.759e-08
50-150 4.174e-07 1.724e-07
15-150 1.154e-06 2.047e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.571032 (-1.35748 10.9353)
R1^2/D10^2 : 8.22877E+08 (-9.14436e+08 7.72489e+14)
kT2 [keV] : 9.41079 (-1.01169 1.65024)
R2^2/D10^2 : 8.27133E-02 (-0.030256 0.0331431)
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.506e-07 5.760e-08
25- 50 5.233e-07 1.050e-07
50-150 2.385e-07 7.967e-08
15-150 1.012e-06 1.898e-07
Peak spectrum fit
Power-law model
Time interval is from 10.916 sec. to 11.916 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.19324 ( -0.700131 0.990184 )
Norm@50keV : 5.03925E-03 ( -0.00282273 0.0023934 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.14 using 59 bins.
Reduced chi-squared = 1.24807
# Null hypothesis probability of 9.86e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.831338 ( -0.242276 0.242092 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.73086e-08 ( -1.95748e-08 2.12197e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 10.916 sec. to 11.916 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.11012 ( -0.872007 0.722953 )
Epeak [keV] : 47.0245 ( )
Norm@50keV : 4.48488E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.87 using 59 bins.
Reduced chi-squared = 1.26554
# Null hypothesis probability of 8.71e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.739584 ( -0.560162 0.052621 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.49101e-08 ( -9.86535e-09 2.59915e-08 ) ergs/cm2
Band function
Time interval is from 10.916 sec. to 11.916 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] : 6.96193 (-4.10889 5.27774)
R^2/D10^2 : 1.43831 (-1.38826 91.791)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.06e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.114e-08 6.895e-09
25- 50 1.509e-08 9.620e-09
50-150 2.452e-09 2.211e-09
15-150 2.868e-08 1.727e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 57.4844 (-42.4299 -58.0826)
Norm : 4.30913 (-1.87711 7.84473)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.11e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.075e-08 5.829e-09
25- 50 1.615e-08 9.578e-09
50-150 1.772e-08 1.395e-08
15-150 4.462e-08 2.846e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.30833 (-1.70928 3.46809)
R1^2/D10^2 : 39.2157 (-37.1736 5262.57)
kT2 [keV] : 34.7263 (-24.6977 -35.0121)
R2^2/D10^2 : 4.28838E-03 (-0.00398751 0.224839)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.52e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.387e-08 8.210e-09
25- 50 7.460e-09 4.125e-09
50-150 3.807e-08 2.305e-08
15-150 5.940e-08 3.150e-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: 2.18015 ( -0.399703 0.471861 )
Norm@50keV : 8.51162E-04 ( -0.000276326 0.000268042 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.41e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 63.85 sec: 0.139458 ( -0.0295743 0.0295997 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.09586e-07 ( -1.37686e-07 1.47836e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.380514 ( -3.17341 1.90203 )
Epeak [keV] : 33.4682 ( -30.2584 -33.5443 )
Norm@50keV : 1.09696E-02 ( -0.0114753 1.12333 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.75e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 63.85 sec: 0.133337 ( -0.029234 0.029776 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.3943e-07 ( -1.14956e-07 1.56889e-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) = 3.91e-07
S(50-100 keV) = 3.65e-07
T90 vs. Hardness ratio plot
T90 = 151.740000009537 sec.
Hardness ratio (energy fluence ratio) = 0.933504
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29231
Count Ratio (50-100 keV) / (15-25 keV) = 0.289044
Mask shadow pattern
IMX = 8.811704475905083E-02, IMY = 5.401816746833300E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000
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:
-239.288000 0.760000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0353 38.3040 13.4 48.0 175.7 0.6751 0.9 6.5 Cyg X-2
30.0871 -34.1680 2.8 46.7 -19.2 2.1233 4.2 ------ UNKNOWN
7.2471 36.6296 3.0 41.6 -138.4 2.0655 3.9 ------ UNKNOWN
33.5500 -18.4036 2.7 42.8 -41.4 2.2187 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.760000 64.612600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0616 38.2695 6.7 47.9 175.7 -0.4779 -1.7 6.1 Cyg X-2
330.2114 35.6836 2.3 43.9 177.3 1.0221 5.0 ------ UNKNOWN
20.6241 4.6451 2.3 28.7 -80.7 0.8336 5.1 ------ UNKNOWN
21.6564 33.8732 2.0 45.6 -121.8 2.6920 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
114.412620 662.878000
720.712000 723.464900
725.712000 733.205700
735.712000 743.530000
745.712000 753.463100
754.712000 763.632000
764.712000 786.372000
787.712000 796.032600
797.712000 816.882000
818.712000 962.752000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
0.7903 8.3271 3.3 20.0 121.0 2.6306 3.6 501.9 UNKNOWN
32.2002 14.1510 2.8 14.9 -111.4 2.5176 4.1 ------ UNKNOWN
55.0617 37.2172 2.7 45.3 -121.4 12.4474 4.3 ------ UNKNOWN
59.4050 21.7621 3.9 41.3 -98.9 10.9023 2.9 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:22:42 EDT 2022