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
23.8233 83.7942 0.0024 20.1363 -43.3119 13.8237120 79.025 TRIG_01194500
Foreground time interval of the image:
-13.392 14.077 (delta_t = 27.469 [sec])
Background time interval of the image:
-168.923 -13.392 (delta_t = 155.531 [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 -13.392 sec. to 55.832 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23926 ( -0.0308713 0.030772 )
Norm@50keV : 1.87600E-02 ( -0.000308644 0.000307866 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.26 using 59 bins.
Reduced chi-squared = 0.829123
# Null hypothesis probability of 8.18e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 69.22 sec: 2.21500 ( -0.04101 0.04122 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30344e-05 ( -2.0662e-07 2.07232e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -13.392 sec. to 55.832 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23491 ( -0.0315365 0.0306619 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.88293E-02 ( -0.000293811 0.00172402 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.32 using 59 bins.
Reduced chi-squared = 0.845
# Null hypothesis probability of 7.89e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 69.22 sec: 2.21917 ( -0.04606 0.03611 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.18444e-06 ( -2.32201e-07 8.83642e-08 ) ergs/cm2
Band function
Time interval is from -13.392 sec. to 55.832 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] : 21.8412 ( )
R^2/D10^2 : 7.29578E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 824.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.27e-136 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.473e-07 1.516e-08
25- 50 2.355e-06 6.368e-08
50-150 8.392e-06 1.904e-07
15-150 1.119e-05 1.869e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 9.70562 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 452.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.29e-63 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.673e-06 3.253e-08
25- 50 3.218e-06 5.711e-08
50-150 7.058e-06 1.281e-07
15-150 1.195e-05 2.180e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.67091 (-0.572352 0.602722)
R1^2/D10^2 : 0.954731 (-0.187892 0.246976)
kT2 [keV] : 36.2831 (-2.31093 2.82442)
R2^2/D10^2 : 1.19456E-02 (-0.00253839 0.00287194)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.098e-06 7.026e-08
25- 50 2.894e-06 9.137e-08
50-150 9.033e-06 2.665e-07
15-150 1.302e-05 3.669e-07
Peak spectrum fit
Power-law model
Time interval is from 0.240 sec. to 1.240 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.824163 ( -0.0429028 0.0426581 )
Norm@50keV : 0.217964 ( -0.00519388 0.00517721 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.03 using 59 bins.
Reduced chi-squared = 0.912807
# Null hypothesis probability of 6.62e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 25.0326 ( -0.5879 0.5882 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.52185e-06 ( -6.34644e-08 6.35039e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.240 sec. to 1.240 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.747172 ( -0.166692 0.0913525 )
Epeak [keV] : 999.584 ( -999.962 -999.962 )
Norm@50keV : 0.234600 ( -0.00533861 0.0391374 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.42 using 59 bins.
Reduced chi-squared = 0.918214
# Null hypothesis probability of 6.49e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 24.9502 ( -0.61 0.5848 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.51495e-06 ( -6.521e-08 5.98885e-08 ) ergs/cm2
Band function
Time interval is from 0.240 sec. to 1.240 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] : 25.6560 ( )
R^2/D10^2 : 0.583399 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 322.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.81e-39 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.579e-08 3.195e-09
25- 50 3.781e-07 1.310e-08
50-150 1.838e-06 6.250e-08
15-150 2.282e-06 6.400e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 98.8888 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 816.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.64e-135 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.462e-07 6.150e-09
25- 50 4.737e-07 1.165e-08
50-150 1.039e-06 2.500e-08
15-150 1.759e-06 4.150e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.89435 (-1.10583 1.20859)
R1^2/D10^2 : 5.35562 (-1.42559 2.1484)
kT2 [keV] : 44.6090 (-4.96323 7.2986)
R2^2/D10^2 : 0.102173 (-0.0347182 0.0414994)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.10e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.306e-07 1.395e-08
25- 50 4.308e-07 2.865e-08
50-150 1.980e-06 1.605e-07
15-150 2.541e-06 1.680e-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: 1.07237 ( -0.0310315 0.0309073 )
Norm@50keV : 3.32608E-02 ( -0.000568187 0.000566388 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 27.47 sec: 3.84838 ( -0.0697438 0.0698862 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.63862e-06 ( -1.5848e-07 1.58546e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06714 ( -0.122594 0.0309734 )
Epeak [keV] : 9997.10 ( -9993.32 -9993.32 )
Norm@50keV : 3.34599E-02 ( -0.00054299 0.00559098 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.06e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 27.47 sec: 3.83353 ( -0.07532 0.07956 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.6226e-06 ( -1.59244e-07 1.53283e-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) = 2.80e-06
S(50-100 keV) = 4.75e-06
T90 vs. Hardness ratio plot
T90 = 46.7119998931885 sec.
Hardness ratio (energy fluence ratio) = 1.69643
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.52003
Count Ratio (50-100 keV) / (15-25 keV) = 1.34559
Mask shadow pattern
IMX = 2.667976350640010E-01, IMY = 2.515223821690920E-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:
-168.923400 -13.392000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5879 35.1903 1.2 48.8 -141.5 6.2656 9.7 0.7 Cyg X-1
308.1383 40.9963 2.9 40.2 -144.8 1.6622 4.0 2.9 Cyg X-3
326.1313 38.2766 8.0 35.0 -166.4 0.4537 1.4 3.3 Cyg X-2
75.4520 53.6428 3.1 35.2 25.0 1.5623 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.392000 14.076590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6329 35.1725 12.0 48.8 -141.5 0.4695 1.0 2.7 Cyg X-1
308.1459 41.0018 6.0 40.2 -144.8 0.4986 1.9 3.4 Cyg X-3
326.3257 38.2912 7.8 34.9 -166.6 0.3010 1.5 7.5 Cyg X-2
23.7510 30.4309 3.0 35.3 105.0 1.5301 3.9 ------ UNKNOWN
332.8280 22.7971 2.3 46.8 175.7 1.7818 5.1 ------ UNKNOWN
23.8231 83.7941 0.1 20.1 -43.3 13.8197 79.0 ------ UNKNOWN
308.8190 20.7062 2.2 57.5 -159.2 4.0826 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
70.676590 719.756000
720.776000 962.889800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5916 35.1806 2.3 54.4 -165.5 18.2610 5.1 1.3 Cyg X-1
308.2232 40.9708 3.7 47.8 -173.1 8.3396 3.1 5.2 Cyg X-3
325.9646 38.2115 0.0 48.7 168.2 -5.5969 -1.5 11.8 Cyg X-2
349.0709 45.5702 3.0 39.4 144.8 12.0508 3.9 ------ UNKNOWN
154.4647 61.2929 2.4 33.1 -32.2 7.0391 4.7 ------ UNKNOWN
263.7796 45.3222 2.8 48.0 -129.1 21.3483 4.1 ------ UNKNOWN
Plot creation:
Tue Dec 26 17:03:00 EST 2023