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
328.4532 37.8578 0.0083 12.6449 142.6552 1.3068170 23.269 TRIG_01185673
Foreground time interval of the image:
-5.564 16.484 (delta_t = 22.048 [sec])
Background time interval of the image:
-239.128 -5.564 (delta_t = 233.564 [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 -5.564 sec. to 16.484 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42592 ( -0.131524 0.131674 )
Norm@50keV : 3.50490E-03 ( -0.000255731 0.000254788 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.40 using 59 bins.
Reduced chi-squared = 1.18246
# Null hypothesis probability of 1.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 22.05 sec: 0.429419 ( -0.031206 0.031252 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.42999e-07 ( -6.07096e-08 6.13204e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.564 sec. to 16.484 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42313 ( -0.368952 0.159294 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 3.51679E-03 ( -0.000257269 0.000249923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.41 using 59 bins.
Reduced chi-squared = 1.20375
# Null hypothesis probability of 1.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 22.05 sec: 0.431268 ( -0.041085 0.03719 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.49252e-07 ( -7.30003e-08 5.82032e-08 ) ergs/cm2
Band function
Time interval is from -5.564 sec. to 16.484 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] : 15.0821 ( )
R^2/D10^2 : 4.69571E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 121.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.49e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.927e-08 6.847e-09
25- 50 1.967e-07 2.045e-08
50-150 3.053e-07 4.333e-08
15-150 5.513e-07 5.479e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-33.2159 -200)
Norm : 1.76038 (-0.125577 0.125577)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.40e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.667e-08 7.927e-09
25- 50 1.860e-07 3.423e-08
50-150 4.078e-07 1.212e-07
15-150 6.905e-07 1.643e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.13536 (-1.85495 2.06742)
R1^2/D10^2 : 0.290586 (-0.143777 0.38172)
kT2 [keV] : 38.6038 (-12.7622 58.0304)
R2^2/D10^2 : 1.66710E-03 (-0.00139165 0.00284099)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.64e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.487e-08 2.027e-08
25- 50 1.888e-07 4.219e-08
50-150 4.861e-07 2.284e-07
15-150 7.597e-07 2.534e-07
Peak spectrum fit
Power-law model
Time interval is from 0.596 sec. to 1.596 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46257 ( -0.26299 0.268483 )
Norm@50keV : 8.04819E-03 ( -0.00123911 0.00122079 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.95 using 59 bins.
Reduced chi-squared = 0.771053
# Null hypothesis probability of 8.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.994980 ( -0.146071 0.14619 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.68493e-08 ( -1.31433e-08 1.33618e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.596 sec. to 1.596 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45565 ( -0.317304 0.271495 )
Epeak [keV] : 9999.32 ( -9999.36 -9999.36 )
Norm@50keV : 8.07697E-03 ( -0.0012493 0.0127897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.96 using 59 bins.
Reduced chi-squared = 0.785
# Null hypothesis probability of 8.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.997995 ( -0.157694 0.150125 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.77141e-08 ( -1.43767e-08 1.23559e-08 ) ergs/cm2
Band function
Time interval is from 0.596 sec. to 1.596 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] : 15.1644 (-3.02027 3.85052)
R^2/D10^2 : 0.107382 (-0.0577517 0.123726)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.160e-09 1.583e-09
25- 50 2.071e-08 5.385e-09
50-150 3.257e-08 1.058e-08
15-150 5.844e-08 1.379e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-83.0722 -199.363)
Norm : 4.06440 (-0.593263 0.593259)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.78e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.012e-08 5.840e-09
25- 50 1.947e-08 1.099e-08
50-150 4.270e-08 2.421e-08
15-150 7.229e-08 4.046e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.02432 (-2.19448 3.32703)
R1^2/D10^2 : 1.85929 (-1.40811 5.17369)
kT2 [keV] : 27.9130 (-9.04199 37.27)
R2^2/D10^2 : 1.12678E-02 (-0.0102324 0.0325021)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.045e-08 5.951e-09
25- 50 1.765e-08 9.300e-09
50-150 4.923e-08 2.812e-08
15-150 7.733e-08 4.017e-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: 1.42592 ( -0.131524 0.131674 )
Norm@50keV : 3.50490E-03 ( -0.000255731 0.000254788 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 22.05 sec: 0.429411 ( -0.0312041 0.0312503 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.42917e-07 ( -6.07868e-08 6.13155e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43027 ( -0.390083 0.12833 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.50363E-03 ( -0.000925503 0.00192072 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 22.05 sec: 0.429526 ( -0.031458 0.030947 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.42465e-07 ( -6.19958e-08 6.08382e-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) = 1.77e-07
S(50-100 keV) = 2.65e-07
T90 vs. Hardness ratio plot
T90 = 19.4479999542236 sec.
Hardness ratio (energy fluence ratio) = 1.49718
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.20663
Count Ratio (50-100 keV) / (15-25 keV) = 0.965585
Mask shadow pattern
IMX = -1.783571186160879E-01, IMY = -1.360920252802561E-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:
-239.128000 -5.564000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5865 35.1904 0.6 35.4 155.7 10.9299 18.1 0.7 Cyg X-1
308.1893 41.0349 4.3 27.3 162.7 1.1804 2.7 6.1 Cyg X-3
326.1432 38.1874 9.4 14.3 146.2 0.4250 1.2 8.2 Cyg X-2
354.0541 -5.4229 2.4 46.8 46.4 4.8529 4.9 482.5 UNKNOWN
269.5498 83.3047 3.3 48.1 -129.1 5.6146 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.564000 16.484000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7642 35.3106 6.0 35.2 155.8 -0.1664 -1.9 10.7 Cyg X-1
308.0499 40.8845 7.9 27.4 162.4 0.0982 1.4 4.9 Cyg X-3
326.1548 38.4822 8.2 14.2 147.3 0.0847 1.4 9.7 Cyg X-2
340.4687 16.6829 2.1 24.1 68.9 0.4173 5.5 ------ UNKNOWN
328.4532 37.8578 0.5 12.6 142.7 1.3069 23.2 ------ UNKNOWN
283.8020 46.7014 2.0 43.2 178.8 0.5568 5.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
71.972600 962.961900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4360 35.4145 4.6 57.8 -160.7 -14.0469 -2.5 4.4 Her X-1
288.6996 10.8177 66.3 44.6 150.4 -0.6476 -0.2 9.6 GRS 1915+105
299.5919 35.1894 0.4 23.2 179.4 37.3832 27.6 0.7 Cyg X-1
308.1528 40.9858 3.9 15.9 -165.2 3.8512 3.0 2.8 Cyg X-3
326.1581 38.1720 7.5 1.8 -171.5 1.8080 1.5 9.0 Cyg X-2
7.8716 4.8086 1.8 48.8 29.7 16.4865 6.5 553.0 UNKNOWN
258.3148 62.1128 3.3 48.1 -129.2 19.3366 3.5 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:43:22 EDT 2023