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
291.0341 80.0123 0.0049 37.3609 -147.3329 6.8326550 39.734 TRIG_01162001
Foreground time interval of the image:
-7.376 16.149 (delta_t = 23.525 [sec])
Background time interval of the image:
-239.552 -7.376 (delta_t = 232.176 [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 -7.376 sec. to 31.760 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63337 ( -0.0700832 0.0703932 )
Norm@50keV : 1.25712E-02 ( -0.000490979 0.00049044 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.16 using 59 bins.
Reduced chi-squared = 0.65193
# Null hypothesis probability of 9.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 39.14 sec: 1.63266 ( -0.06768 0.06786 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.5847e-06 ( -1.87861e-07 1.884e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -7.376 sec. to 31.760 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25771 ( -0.304497 0.284774 )
Epeak [keV] : 102.879 ( -24.7679 144.102 )
Norm@50keV : 1.91007E-02 ( -0.00508048 0.00750722 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.00 using 59 bins.
Reduced chi-squared = 0.571429
# Null hypothesis probability of 9.96e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 39.14 sec: 1.59419 ( -0.07303 0.07343 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.46901e-06 ( -2.08503e-07 2.07817e-07 ) ergs/cm2
Band function
Time interval is from -7.376 sec. to 31.760 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] : 14.8245 ( )
R^2/D10^2 : 0.183574 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 161.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.78e-12 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.312e-07 2.679e-08
25- 50 1.302e-06 6.576e-08
50-150 1.937e-06 1.485e-07
15-150 3.570e-06 1.624e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.798 (-29.8321 -168.437)
Norm : 6.62667 (-0.301363 0.325921)
------------------------------------------------------------
#Fit statistic : Chi-Squared 31.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.97e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.587e-07 4.168e-08
25- 50 1.241e-06 1.029e-07
50-150 2.567e-06 7.259e-07
15-150 4.467e-06 8.090e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.26995 (-1.23831 1.30824)
R1^2/D10^2 : 1.46574 (-0.595729 1.31703)
kT2 [keV] : 24.8846 (-3.48806 5.43939)
R2^2/D10^2 : 2.18876E-02 (-0.011537 0.0180017)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.36e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.981e-07 8.161e-08
25- 50 1.267e-06 1.327e-07
50-150 2.544e-06 3.826e-07
15-150 4.409e-06 4.873e-07
Peak spectrum fit
Power-law model
Time interval is from 0.260 sec. to 1.260 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25132 ( -0.105286 0.104965 )
Norm@50keV : 7.09162E-02 ( -0.00439566 0.00439563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.87 using 59 bins.
Reduced chi-squared = 1.08544
# Null hypothesis probability of 3.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 8.38933 ( -0.54009 0.54079 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.09561e-07 ( -4.78932e-08 4.80565e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.260 sec. to 1.260 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.912834 ( -0.457495 0.379689 )
Epeak [keV] : 178.684 ( -72.4941 -178.684 )
Norm@50keV : 0.101884 ( -0.033 0.0618033 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.97 using 59 bins.
Reduced chi-squared = 1.07089
# Null hypothesis probability of 3.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 8.28825 ( -0.55414 0.55472 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.78867e-07 ( -4.77769e-08 5.45487e-08 ) ergs/cm2
Band function
Time interval is from 0.260 sec. to 1.260 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] : 18.6649 (-1.45754 1.61239)
R^2/D10^2 : 0.487448 (-0.118277 0.152967)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 106.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.41e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.359e-08 3.810e-09
25- 50 1.595e-07 1.440e-08
50-150 4.069e-07 4.425e-08
15-150 6.001e-07 4.530e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-12.5875 -200)
Norm : 34.9723 (-2.20314 2.20314)
------------------------------------------------------------
#Fit statistic : Chi-Squared 84.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.13e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.710e-08 5.815e-09
25- 50 1.676e-07 1.310e-08
50-150 3.675e-07 8.090e-08
15-150 6.222e-07 9.650e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.36058 (-2.79522 2.77126)
R1^2/D10^2 : 2.85180 (-1.39305 5.71428)
kT2 [keV] : 34.0700 (-8.76975 26.3439)
R2^2/D10^2 : 5.11285E-02 (-0.041141 0.0972869)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.11e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.814e-08 1.433e-08
25- 50 1.674e-07 4.552e-08
50-150 4.758e-07 2.071e-07
15-150 7.013e-07 2.292e-07
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: 1.61465 ( -0.0640213 0.0642865 )
Norm@50keV : 1.94191E-02 ( -0.000691643 0.00069108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 23.52 sec: 2.50689 ( -0.0955193 0.0957799 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.26403e-06 ( -1.59555e-07 1.59863e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22706 ( -0.278016 0.261797 )
Epeak [keV] : 104.826 ( -23.5766 101.753 )
Norm@50keV : 2.97905E-02 ( -0.00730903 0.0104127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 28.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 23.52 sec: 2.44527 ( -0.10314 0.10361 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.15859e-06 ( -1.76706e-07 1.75765e-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) = 1.21e-06
S(50-100 keV) = 1.55e-06
T90 vs. Hardness ratio plot
T90 = 22.336000084877 sec.
Hardness ratio (energy fluence ratio) = 1.28099
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.34375
Count Ratio (50-100 keV) / (15-25 keV) = 1.02144
Mask shadow pattern
IMX = -6.427102760570491E-01, IMY = 4.120911943418059E-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:
-239.552000 -7.376000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5901 35.2298 6.5 9.8 44.6 0.5653 1.8 9.4 Her X-1
268.2034 -1.3470 0.0 46.6 10.9 -0.6351 -1.2 11.7 SW J1753.5-0127
288.8775 10.8997 6.3 42.4 -23.0 0.9967 1.8 5.4 GRS 1915+105
299.5859 35.1910 0.8 32.3 -63.7 7.9539 14.8 0.7 Cyg X-1
308.1640 41.0248 3.5 35.8 -78.3 2.2572 3.3 5.0 Cyg X-3
261.8048 -10.9570 2.7 55.5 20.4 6.7834 4.3 ------ UNKNOWN
161.1663 83.7326 2.8 46.7 -164.7 3.0319 4.1 ------ UNKNOWN
286.4519 14.7063 3.0 37.9 -23.0 1.7781 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-7.376000 16.148600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5510 35.3835 3.4 9.7 45.1 -0.3439 -3.4 5.2 Her X-1
268.3109 -1.5285 7.8 46.8 10.8 -0.2949 -1.5 5.7 SW J1753.5-0127
288.6815 10.8699 5.8 42.3 -22.7 0.3796 2.0 8.2 GRS 1915+105
299.5900 35.2014 15.0 32.3 -63.7 -0.1523 -0.8 0.0 Cyg X-1
308.1891 40.9408 18.7 35.9 -78.2 -0.1790 -0.6 3.6 Cyg X-3
213.5794 26.1148 3.1 40.6 102.5 1.2724 3.7 ------ UNKNOWN
252.7378 -6.0404 2.4 50.8 31.7 1.7459 4.9 ------ UNKNOWN
291.0341 80.0123 0.3 37.4 -147.3 6.8323 39.8 ------ UNKNOWN
58.0738 79.1616 2.3 55.7 -151.5 2.5677 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
93.148590 719.636300
720.448000 871.748600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4050 35.3875 4.4 46.8 28.7 3.9284 2.6 3.7 Her X-1
299.5860 35.2180 0.7 44.9 -23.0 24.8150 15.7 1.0 Cyg X-1
308.1542 40.9328 3.1 39.6 -33.5 5.0430 3.7 2.3 Cyg X-3
326.2084 38.2453 6.8 43.9 -53.8 5.1135 1.7 4.9 Cyg X-2
248.0804 35.4345 3.0 47.6 35.7 7.8135 3.8 ------ UNKNOWN
274.5848 25.2223 2.8 55.2 5.1 10.1764 4.2 ------ UNKNOWN
274.3015 31.4931 2.7 49.0 5.9 5.7363 4.3 ------ UNKNOWN
92.8796 55.0995 2.6 44.5 -178.3 8.1283 4.4 ------ UNKNOWN
76.9432 51.9051 3.0 46.7 -164.6 7.5308 3.8 ------ UNKNOWN
49.0029 55.1864 2.5 40.4 -141.9 8.0099 4.6 ------ UNKNOWN
8.9589 50.5768 3.5 38.4 -103.3 9.9111 3.3 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:11:13 EDT 2023