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
133.8121 31.9677 0.0120 13.1836 19.0118 5.9715616 16.087 TRIG_01093860
Foreground time interval of the image:
25.404 366.604 (delta_t = 341.200 [sec])
Background time interval of the image:
-239.000 25.404 (delta_t = 264.404 [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 25.404 sec. to 366.604 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74904 ( -0.106138 0.10782 )
Norm@50keV : 1.32357E-03 ( -8.14243e-05 8.06801e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.27 using 59 bins.
Reduced chi-squared = 0.811754
# Null hypothesis probability of 8.44e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 341.2 sec: 0.178914 ( -0.010132 0.010151 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.16793e-06 ( -2.65823e-07 2.68454e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 25.404 sec. to 366.604 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59489 ( -0.425957 0.247881 )
Epeak [keV] : 123.127 ( -60.1284 -123.127 )
Norm@50keV : 1.59656E-03 ( -0.000345988 0.00105177 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.83 using 59 bins.
Reduced chi-squared = 0.818393
# Null hypothesis probability of 8.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 341.2 sec: 0.177292 ( -0.010929 0.010914 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.10269e-06 ( -3.12344e-07 3.10564e-07 ) ergs/cm2
Band function
Time interval is from 25.404 sec. to 366.604 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] : 12.5759 ( )
R^2/D10^2 : 3.49699E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 125.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.67e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.001e-07 4.180e-08
25- 50 1.329e-06 8.871e-08
50-150 1.302e-06 1.773e-07
15-150 3.031e-06 1.936e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 120.290 (-27.2947 38.1847)
Norm : 0.751168 (-0.0539498 0.0659272)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.15e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.675e-07 6.039e-08
25- 50 1.195e-06 9.451e-08
50-150 2.135e-06 6.703e-07
15-150 3.997e-06 6.655e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.56832 (-0.931984 1.08664)
R1^2/D10^2 : 0.474434 (-0.228848 0.512871)
kT2 [keV] : 21.0838 (-2.99647 4.43944)
R2^2/D10^2 : 4.28798E-03 (-0.00219779 0.00344829)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.96e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.169e-07 1.752e-07
25- 50 1.134e-06 1.989e-07
50-150 2.128e-06 4.540e-07
15-150 3.979e-06 6.039e-07
Peak spectrum fit
Power-law model
Time interval is from 183.240 sec. to 184.240 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66808 ( -0.411371 0.437334 )
Norm@50keV : 5.70302E-03 ( -0.00156235 0.0014979 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.11 using 59 bins.
Reduced chi-squared = 1.08965
# Null hypothesis probability of 2.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.749203 ( -0.171452 0.171453 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.29578e-08 ( -1.48442e-08 1.561e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 183.240 sec. to 184.240 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55562 ( -5.90668 1.00256 )
Epeak [keV] : 150.133 ( -211.447 -211.447 )
Norm@50keV : 6.66797E-03 ( -0.0062089 44.5662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.12 using 59 bins.
Reduced chi-squared = 1.10929
# Null hypothesis probability of 2.67e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.747865 ( -0.199512 0.172734 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.26393e-08 ( -2.45106e-08 1.57597e-08 ) ergs/cm2
Band function
Time interval is from 183.240 sec. to 184.240 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] : 9.75916 (-2.11112 3.06194)
R^2/D10^2 : 0.393249 (-0.252061 0.587063)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.561e-09 3.259e-09
25- 50 1.815e-08 7.400e-09
50-150 8.826e-09 5.576e-09
15-150 3.454e-08 1.648e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 126.728 (-77.3848 -124.962)
Norm : 3.16196 (-0.794792 1.32014)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.215e-09 4.719e-09
25- 50 1.483e-08 8.425e-09
50-150 2.718e-08 1.854e-08
15-150 5.023e-08 3.137e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.40669 (-1.89644 2.14502)
R1^2/D10^2 : 0.621871 (-0.372045 0.515144)
kT2 [keV] : 196.722 (-197.385 -197.385)
R2^2/D10^2 : 1.01583E-04 (-6.41226e-05 0.00731734)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.71e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.353e-09 4.913e-09
25- 50 1.675e-08 9.635e-09
50-150 3.126e-08 5.155e-09
15-150 5.636e-08 1.950e-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: 1.74904 ( -0.106138 0.10782 )
Norm@50keV : 1.32357E-03 ( -8.14243e-05 8.06801e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.44e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 341.2 sec: 0.178905 ( -0.0101306 0.01015 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.16731e-06 ( -2.65955e-07 2.68371e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59489 ( -0.425957 0.247881 )
Epeak [keV] : 123.127 ( -60.1284 -123.127 )
Norm@50keV : 1.59656E-03 ( -0.000345988 0.00105177 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 341.2 sec: 0.177260 ( -0.010925 0.010879 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.10399e-06 ( -3.12744e-07 3.10014e-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) = 1.15e-06
S(50-100 keV) = 1.37e-06
T90 vs. Hardness ratio plot
T90 = 270.840000033379 sec.
Hardness ratio (energy fluence ratio) = 1.1913
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.08527
Count Ratio (50-100 keV) / (15-25 keV) = 0.715928
Mask shadow pattern
IMX = 2.214689011210084E-01, IMY = -7.630873196229848E-02
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:
-239.000000 25.404000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6436 22.0083 0.9 36.6 -107.0 10.7128 13.5 0.7 Crab
91.6639 12.2427 3.3 31.8 -127.5 1.7310 3.5 ------ UNKNOWN
88.8389 7.7731 2.8 36.3 -132.6 2.2338 4.1 ------ UNKNOWN
121.8695 79.5268 2.3 56.9 -24.1 8.7095 5.1 ------ UNKNOWN
91.1068 71.1391 2.9 51.9 -36.5 6.0094 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
25.404000 366.604000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6541 21.9774 5.3 36.6 -107.1 1.8453 2.2 2.5 Crab
133.8121 31.9677 0.7 13.2 19.0 5.9715 16.1 ------ UNKNOWN
135.1752 65.0662 1.9 43.1 -16.5 3.8441 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
744.500610 963.102200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9660 -15.6305 1.0 32.8 75.4 6.7615 12.1 1.0 Sco X-1
254.3690 35.3152 8.1 52.6 150.7 2.1973 1.4 4.6 Her X-1
256.1161 -38.0301 0.0 32.8 29.3 -0.4451 -0.9 12.7 4U 1700-377
256.4683 -36.4962 14.2 31.5 31.0 0.3692 0.8 4.7 GX 349+2
263.0663 -24.8142 12.2 19.5 42.4 -0.3178 -0.9 5.2 GX 1+4
264.6543 -44.3601 4.0 34.5 13.3 1.2741 2.9 6.6 4U 1735-44
268.3724 -1.4441 179.1 14.6 131.1 -0.0211 -0.1 0.6 SW J1753.5-0127
270.2026 -24.9187 21.8 15.1 26.0 0.1532 0.5 10.6 GX 5-1
270.1313 -25.8721 10.2 16.0 24.3 0.3289 1.1 12.1 GRS 1758-258
273.8441 -14.1055 9.5 5.1 60.6 -0.3651 -1.2 10.3 GX 17+2
275.9219 -30.3705 16.2 18.5 2.9 0.2333 0.7 0.3 H1820-303
285.1916 -25.0265 12.6 14.5 -29.1 -0.2897 -0.9 10.6 HT1900.1-2455
288.7847 10.9437 21.6 25.1 -160.1 0.1712 0.5 0.8 GRS 1915+105
299.5992 35.1998 1.1 51.2 -162.2 7.9103 10.2 0.5 Cyg X-1
308.1447 40.9203 9.0 59.6 -158.7 -3.3608 -1.3 2.5 Cyg X-3
262.9629 -33.7687 4.8 26.0 26.3 0.8452 2.4 4.2 GX 354-0
299.0015 15.9368 2.9 34.5 -148.0 1.6307 3.9 ------ UNKNOWN
299.0269 38.2628 3.8 53.8 -164.5 2.7250 3.0 ------ UNKNOWN
322.2335 -32.3400 2.8 44.8 -60.2 5.9867 4.1 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:07:55 EDT 2022