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
89.0187 6.9049 0.0150 23.5826 149.2167 0.2066859 12.798 TRIG_00995004
Foreground time interval of the image:
-0.640 0.284 (delta_t = 0.924 [sec])
Background time interval of the image:
-239.768 -0.640 (delta_t = 239.128 [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 0.256000
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 0.256000
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 0.256000
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 -0.640 sec. to 0.284 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.679718 ( -0.263759 0.244503 )
Norm@50keV : 1.38031E-02 ( -0.00199794 0.001923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.31 using 59 bins.
Reduced chi-squared = 0.707193
# Null hypothesis probability of 9.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.924 sec: 1.59818 ( -0.21042 0.21135 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57142e-07 ( -2.05415e-08 2.05722e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.640 sec. to 0.284 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.680110 ( -0.274924 0.238497 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.39431E-02 ( -0.00185433 0.00736631 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.35 using 59 bins.
Reduced chi-squared = 0.720536
# Null hypothesis probability of 9.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.924 sec: 1.59768 ( -0.21049 0.21121 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57066e-07 ( 0 0 ) ergs/cm2
Band function
Time interval is from -0.640 sec. to 0.284 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] : 33.1291 (-6.52571 9.80307)
R^2/D10^2 : 1.83569E-02 (-0.00904533 0.0156132)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.17e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.734e-09 7.734e-10
25- 50 1.753e-08 4.366e-09
50-150 1.299e-07 3.038e-08
15-150 1.501e-07 3.799e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-23.7992 -200)
Norm : 6.36239 (-0.875719 0.875719)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.35e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.463e-08 8.395e-09
25- 50 2.815e-08 1.580e-08
50-150 6.173e-08 3.450e-08
15-150 1.045e-07 5.844e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.95984 (-2.9875 5.13494)
R1^2/D10^2 : 1.12503 (-0.943715 9.23637)
kT2 [keV] : 48.7135 (-14.782 91.4861)
R2^2/D10^2 : 6.25338E-03 (-0.00535116 0.0100051)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.48e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.568e-09 5.555e-09
25- 50 2.186e-08 1.087e-08
50-150 1.324e-07 7.074e-08
15-150 1.639e-07 7.836e-08
Peak spectrum fit
Power-law model
Time interval is from -0.676 sec. to 0.324 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.636501 ( -0.263498 0.243258 )
Norm@50keV : 1.29407E-02 ( -0.0019213 0.00184716 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.97 using 59 bins.
Reduced chi-squared = 0.771404
# Null hypothesis probability of 8.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.50460 ( -0.19948 0.2006 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6266e-07 ( -2.11165e-08 2.11546e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.676 sec. to 0.324 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.627300 ( -0.66186 0.333849 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 1.30420E-02 ( -0.00177689 0.00958245 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.99 using 59 bins.
Reduced chi-squared = 0.785536
# Null hypothesis probability of 8.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.51491 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62619e-07 ( -2.11146e-08 2.11575e-08 ) ergs/cm2
Band function
Time interval is from -0.676 sec. to 0.324 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] : 33.4580 (-6.42223 9.59914)
R^2/D10^2 : 1.70937E-02 (-0.00826421 0.0139609)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.88e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.793e-09 8.410e-10
25- 50 1.797e-08 4.670e-09
50-150 1.351e-07 2.918e-08
15-150 1.558e-07 3.495e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-22.8378 -200)
Norm : 5.96926 (-0.835302 0.835302)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.18e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.487e-08 8.420e-09
25- 50 2.860e-08 1.601e-08
50-150 6.272e-08 3.476e-08
15-150 1.062e-07 5.925e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.93013 (-3.12336 5.99702)
R1^2/D10^2 : 0.957319 (-0.838719 9.42294)
kT2 [keV] : 45.8954 (-12.9379 71.5354)
R2^2/D10^2 : 6.97030E-03 (-0.00543743 0.0100375)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.77e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.020e-09 5.047e-09
25- 50 2.194e-08 1.099e-08
50-150 1.373e-07 7.202e-08
15-150 1.682e-07 7.591e-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: 0.679718 ( -0.263759 0.244503 )
Norm@50keV : 1.38031E-02 ( -0.00199794 0.001923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.924 sec: 1.59821 ( -0.210428 0.211346 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5712e-07 ( -2.04981e-08 2.05953e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.668849 ( -0.264363 0.249469 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.38480E-02 ( -0.00181598 0.00741227 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.924 sec: 1.60332 ( -0.21661 0.20608 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57147e-07 ( -2.02541e-08 2.01164e-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) = 2.32e-08
S(50-100 keV) = 5.79e-08
T90 vs. Hardness ratio plot
T90 = 0.832000017166138 sec.
Hardness ratio (energy fluence ratio) = 2.49569
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.44227
Count Ratio (50-100 keV) / (15-25 keV) = 2.03961
Mask shadow pattern
IMX = -3.750242461204163E-01, IMY = -2.234109063977873E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.768000 -0.640000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6246 22.0214 0.5 38.1 162.5 10.0430 22.6 0.6 Crab
135.5163 -40.5616 0.9 40.9 -14.9 5.1852 13.1 0.7 Vela X-1
133.7143 -31.6969 3.3 34.0 -24.5 1.1604 3.5 ------ UNKNOWN
135.1554 -1.6035 3.0 29.0 -83.4 1.6617 3.8 ------ UNKNOWN
145.1719 -25.0569 2.4 40.0 -42.0 2.1697 4.9 ------ UNKNOWN
150.4771 -33.9376 2.4 47.4 -32.2 2.7769 4.7 ------ UNKNOWN
141.4932 -12.4832 3.0 34.2 -61.5 1.6880 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.640000 0.284000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4922 22.0262 6.3 38.2 162.3 0.0395 1.8 7.9 Crab
135.4960 -40.6077 5.4 40.9 -14.8 0.0427 2.2 3.5 Vela X-1
89.0187 6.9049 0.9 23.6 149.2 0.2067 12.8 ------ UNKNOWN
122.4411 -58.5859 1.9 51.4 8.6 0.2353 6.1 ------ UNKNOWN
88.3929 46.2912 2.4 57.3 -176.3 0.3889 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.732600 837.132600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6281 22.0187 0.3 16.0 166.0 30.8433 44.0 0.4 Crab
Plot creation:
Thu Oct 20 00:50:43 EDT 2022