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
122.3796 -37.0973 0.0232 21.3699 -3.0989 0.3581363 8.269 TRIG_01242223
Foreground time interval of the image:
-1.088 12.400 (delta_t = 13.488 [sec])
Background time interval of the image:
-239.624 -1.088 (delta_t = 238.536 [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 8.192000
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 8.192000
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 8.192000
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 -1.088 sec. to 12.400 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28988 ( -0.28219 0.278839 )
Norm@50keV : 1.97766E-03 ( -0.00032393 0.000323062 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.45 using 59 bins.
Reduced chi-squared = 0.902632
# Null hypothesis probability of 6.82e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.49 sec: 0.235509 ( -0.039312 0.039413 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.64322e-07 ( -4.77549e-08 4.8338e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.088 sec. to 12.400 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.697536 ( -1.34203 0.807222 )
Epeak [keV] : 118.266 ( -50.2251 -118.286 )
Norm@50keV : 3.77723E-03 ( -0.00205244 0.0110186 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.54 using 59 bins.
Reduced chi-squared = 0.9025
# Null hypothesis probability of 6.81e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.49 sec: 0.229636 ( -0.041074 0.04085 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.55565e-07 ( -5.02782e-08 5.0851e-08 ) ergs/cm2
Band function
Time interval is from -1.088 sec. to 12.400 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] : 18.6200 (-3.46059 4.44222)
R^2/D10^2 : 1.35807E-02 (-0.00694063 0.0135461)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.257e-08 4.322e-09
25- 50 5.962e-08 1.860e-08
50-150 1.513e-07 4.713e-08
15-150 2.235e-07 5.821e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-65.1529 -200)
Norm : 0.976241 (-0.160628 0.160628)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.13e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.280e-08 1.906e-08
25- 50 6.311e-08 3.644e-08
50-150 1.384e-07 7.851e-08
15-150 2.343e-07 1.317e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.13352 (-2.79106 5.18701)
R1^2/D10^2 : 0.542682 (-0.495258 2.87175)
kT2 [keV] : 23.2406 (-5.48978 12.4474)
R2^2/D10^2 : 5.86358E-03 (-0.00459784 0.00921619)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.91e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.746e-08 1.611e-08
25- 50 5.580e-08 2.774e-08
50-150 1.702e-07 9.497e-08
15-150 2.534e-07 1.350e-07
Peak spectrum fit
Power-law model
Time interval is from 1.240 sec. to 2.240 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31522 ( -0.490744 0.491387 )
Norm@50keV : 4.08154E-03 ( -0.00119553 0.00119343 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.06 using 59 bins.
Reduced chi-squared = 1.12386
# Null hypothesis probability of 2.43e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.488336 ( -0.145307 0.145971 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.01902e-08 ( -1.28054e-08 1.30562e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.240 sec. to 2.240 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -6.95244E-02 ( -3.67666 1.74954 )
Epeak [keV] : 82.0296 ( -57.9045 -82.0141 )
Norm@50keV : 1.78101E-02 ( -0.0178256 0.541714 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.91 using 59 bins.
Reduced chi-squared = 1.12339
# Null hypothesis probability of 2.45e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.462225 ( -0.154229 0.152935 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.79193e-08 ( -1.27952e-08 1.35632e-08 ) ergs/cm2
Band function
Time interval is from 1.240 sec. to 2.240 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] : 18.2027 (-4.90578 7.26246)
R^2/D10^2 : 3.15757E-02 (-0.0315757 0.0598102)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.60e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.087e-09 1.310e-09
25- 50 9.733e-09 5.975e-09
50-150 2.348e-08 1.524e-08
15-150 3.530e-08 2.110e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-112.895 -199.363)
Norm : 2.03251 (-0.595557 0.595549)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.34e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.061e-09 3.210e-09
25- 50 9.736e-09 6.165e-09
50-150 2.135e-08 1.285e-08
15-150 3.615e-08 2.245e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.23867 (-1.58095 5.00633)
R1^2/D10^2 : 2.14009E+04 (-20258.1 -20258.1)
kT2 [keV] : 19.1368 (-5.17388 8.01275)
R2^2/D10^2 : 2.60021E-02 (-0.0259559 0.0480156)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.67e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.364e-09 1.405e-09
25- 50 8.946e-09 5.240e-09
50-150 2.434e-08 1.566e-08
15-150 3.665e-08 2.168e-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: 1.28988 ( -0.28219 0.278839 )
Norm@50keV : 1.97766E-03 ( -0.00032393 0.000323062 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.82e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.49 sec: 0.235506 ( -0.0393109 0.0394117 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.64291e-07 ( -4.77448e-08 4.8367e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.697515 ( -1.34204 0.807212 )
Epeak [keV] : 118.259 ( -50.2256 -118.286 )
Norm@50keV : 3.77738E-03 ( -0.00205245 0.0110185 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.81e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.49 sec: 0.229620 ( -0.041062 0.040841 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.55677e-07 ( -5.02786e-08 5.09261e-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) = 5.85e-08
S(50-100 keV) = 9.56e-08
T90 vs. Hardness ratio plot
T90 = 12.7799999713898 sec.
Hardness ratio (energy fluence ratio) = 1.63419
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.68997
Count Ratio (50-100 keV) / (15-25 keV) = 1.63301
Mask shadow pattern
IMX = 3.907181005366667E-01, IMY = 2.115322218977296E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.624000 -1.088000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5732 -40.6120 2.9 32.0 2.1 1.6567 4.0 4.0 Vela X-1
76.3940 -59.5473 2.7 31.5 84.7 2.6055 4.2 ------ UNKNOWN
108.0142 -1.0897 2.4 31.8 -95.2 2.4393 4.8 ------ UNKNOWN
108.4480 8.5142 2.9 41.2 -98.9 5.6319 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.088000 12.400000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4747 -40.4256 4.1 31.9 1.7 0.1389 2.8 8.1 Vela X-1
166.0850 -51.1320 3.2 53.2 17.5 0.6964 3.6 ------ UNKNOWN
122.3796 -37.0973 1.4 21.4 -3.1 0.3581 8.3 ------ UNKNOWN
65.2175 2.1738 3.1 45.4 -164.0 0.2585 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
119.076600 962.475200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6246 -40.5388 2.2 10.9 34.0 4.8211 5.2 4.5 Vela X-1
170.3188 -60.6256 63.2 38.0 65.2 0.5293 0.2 0.2 Cen X-3
63.5016 -68.9900 2.6 44.7 127.3 25.7424 4.5 ------ UNKNOWN
144.3597 -50.3445 2.9 20.6 58.5 4.5779 4.0 ------ UNKNOWN
170.2531 -13.2173 2.9 48.8 -4.9 6.4089 4.0 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:23:47 EDT 2024