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
343.5141 28.1695 0.0093 25.5432 80.6202 1.9449755 20.889 TRIG_01181187
Foreground time interval of the image:
-5.620 10.740 (delta_t = 16.360 [sec])
Background time interval of the image:
-188.043 -5.620 (delta_t = 182.423 [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 -5.620 sec. to 10.740 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57958 ( -0.13113 0.132749 )
Norm@50keV : 7.33479E-03 ( -0.000584226 0.000580296 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.73 using 59 bins.
Reduced chi-squared = 0.925088
# Null hypothesis probability of 6.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 16.36 sec: 0.936721 ( -0.071591 0.071649 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12526e-06 ( -9.66207e-08 9.7618e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.620 sec. to 10.740 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08841 ( -0.570281 0.502612 )
Epeak [keV] : 89.3253 ( -25.9643 3148.92 )
Norm@50keV : 1.32320E-02 ( -0.0058565 0.0126059 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.94 using 59 bins.
Reduced chi-squared = 0.891786
# Null hypothesis probability of 7.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 16.36 sec: 0.916938 ( -0.07448 0.074421 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.07995e-06 ( -1.06926e-07 1.07823e-07 ) ergs/cm2
Band function
Time interval is from -5.620 sec. to 10.740 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] : 13.9127 (-1.30604 1.46291)
R^2/D10^2 : 0.136273 (-0.0408619 0.0576618)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.10e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.121e-08 1.342e-08
25- 50 3.371e-07 3.460e-08
50-150 4.283e-07 6.920e-08
15-150 8.566e-07 7.894e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 179.288 (-57.135 -178.255)
Norm : 3.83223 (-0.304755 0.341596)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.25e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.582e-07 3.284e-08
25- 50 3.004e-07 9.027e-08
50-150 6.351e-07 3.401e-07
15-150 1.094e-06 4.263e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.60180 (-1.55988 1.82055)
R1^2/D10^2 : 1.18000 (-0.642331 1.87024)
kT2 [keV] : 23.2608 (-4.53167 8.19171)
R2^2/D10^2 : 1.70581E-02 (-0.011445 0.0224078)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.05e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.539e-07 5.606e-08
25- 50 3.030e-07 9.095e-08
50-150 6.208e-07 2.894e-07
15-150 1.078e-06 3.469e-07
Peak spectrum fit
Power-law model
Time interval is from 0.408 sec. to 1.408 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58072 ( -0.20035 0.207181 )
Norm@50keV : 1.91516E-02 ( -0.00261887 0.00258964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.06 using 59 bins.
Reduced chi-squared = 0.983509
# Null hypothesis probability of 5.11e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.44667 ( -0.3134 0.31354 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79568e-07 ( -2.62193e-08 2.65424e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.408 sec. to 1.408 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.295425 ( -1.12332 0.90232 )
Epeak [keV] : 64.3755 ( -12.8133 40.6796 )
Norm@50keV : 8.94205E-02 ( -0.0894194 0.244121 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.73 using 59 bins.
Reduced chi-squared = 0.888036
# Null hypothesis probability of 7.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.93944 ( -0.44304 0.34006 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.67888e-07 ( -2.6605e-08 2.75549e-08 ) ergs/cm2
Band function
Time interval is from 0.408 sec. to 1.408 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] : 14.1555 (-1.85085 2.15141)
R^2/D10^2 : 0.360509 (-0.143669 0.232131)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.26e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.524e-08 3.831e-09
25- 50 5.731e-08 9.915e-09
50-150 7.604e-08 1.936e-08
15-150 1.486e-07 2.480e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 166.663 (-69.8251 -165.912)
Norm : 10.2810 (-1.34387 1.50778)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.27e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.615e-08 1.457e-08
25- 50 4.918e-08 2.622e-08
50-150 1.012e-07 5.780e-08
15-150 1.765e-07 9.810e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.08908 (-3.30674 5.41264)
R1^2/D10^2 : 5.34167 (-4.76223 26.0636)
kT2 [keV] : 17.5151 (-3.62305 9.45646)
R2^2/D10^2 : 0.146574 (-0.126882 0.221068)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.96e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.301e-08 1.198e-08
25- 50 5.063e-08 2.593e-08
50-150 9.133e-08 5.058e-08
15-150 1.650e-07 8.825e-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: 1.57958 ( -0.13113 0.132749 )
Norm@50keV : 7.33479E-03 ( -0.000584226 0.000580296 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 16.36 sec: 0.936691 ( -0.0715862 0.0716488 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12512e-06 ( -9.67439e-08 9.7624e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08841 ( -0.570281 0.502612 )
Epeak [keV] : 89.3259 ( -25.9643 2539.46 )
Norm@50keV : 1.32319E-02 ( -0.00585871 0.0126059 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 16.36 sec: 0.916822 ( -0.07446 0.074398 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08033e-06 ( -1.07102e-07 1.07901e-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) = 2.90e-07
S(50-100 keV) = 3.86e-07
T90 vs. Hardness ratio plot
T90 = 14.7599999904633 sec.
Hardness ratio (energy fluence ratio) = 1.33103
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29759
Count Ratio (50-100 keV) / (15-25 keV) = 0.928082
Mask shadow pattern
IMX = 7.788767482658679E-02, IMY = -4.715112162178338E-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:
-188.043400 -5.620000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4827 35.1254 4.7 43.5 143.4 3.0471 2.4 7.0 Cyg X-1
308.0455 41.0063 5.7 34.6 144.2 1.3191 2.0 4.4 Cyg X-3
326.1724 38.3222 49.8 25.2 122.6 0.1132 0.2 0.0 Cyg X-2
342.8763 21.3983 3.0 32.2 77.5 2.9241 3.9 ------ UNKNOWN
354.4359 31.2312 2.4 20.5 58.4 2.1276 4.8 ------ UNKNOWN
40.9047 61.4449 1.0 25.6 -77.0 5.4107 11.2 ------ UNKNOWN
195.2330 78.5237 2.2 49.3 -132.2 9.0921 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.620000 10.740000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6457 35.0720 7.3 43.5 143.2 -0.2894 -1.6 8.2 Cyg X-1
308.0534 41.0914 12.2 34.5 144.3 -0.1000 -0.9 8.7 Cyg X-3
326.3243 38.2171 8.6 25.2 122.2 0.1096 1.3 9.5 Cyg X-2
343.5141 28.1695 0.6 25.5 80.6 1.9449 20.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.956600 962.188000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6126 35.1581 1.9 37.7 161.3 16.6854 6.0 2.8 Cyg X-1
308.0570 41.0208 5.2 31.6 172.7 4.5546 2.2 4.8 Cyg X-3
326.1753 38.2703 5.3 17.7 178.7 -3.1168 -2.2 3.1 Cyg X-2
344.6609 -9.0428 3.5 37.2 47.4 10.1150 3.3 ------ UNKNOWN
349.9288 66.8751 2.3 38.9 -126.7 14.4238 4.9 ------ UNKNOWN
36.8614 27.4639 2.4 46.8 -53.2 32.5689 4.7 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:46:15 EDT 2023