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
102.4727 -6.5374 0.0140 30.9319 -63.0790 0.7003248 13.735 TRIG_01238732
Foreground time interval of the image:
-0.064 7.040 (delta_t = 7.104 [sec])
Background time interval of the image:
-229.579 -0.064 (delta_t = 229.515 [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 0.512000
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 0.512000
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 0.512000
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 -0.064 sec. to 7.040 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33057 ( -0.17253 0.171124 )
Norm@50keV : 7.12057E-03 ( -0.00075713 0.000756761 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.72 using 59 bins.
Reduced chi-squared = 1.13544
# Null hypothesis probability of 2.25e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 7.104 sec: 0.854485 ( -0.093148 0.093337 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.96298e-07 ( -5.74211e-08 5.78207e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.064 sec. to 7.040 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.166332 ( -0.983366 0.803203 )
Epeak [keV] : 80.5018 ( -17.0815 65.1399 )
Norm@50keV : 2.68299E-02 ( -0.0158552 0.052418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.17 using 59 bins.
Reduced chi-squared = 1.03875
# Null hypothesis probability of 3.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 7.104 sec: 0.819737 ( -0.096784 0.096713 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.61066e-07 ( -6.22587e-08 6.3105e-08 ) ergs/cm2
Band function
Time interval is from -0.064 sec. to 7.040 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] : 16.4405 (-1.86771 2.1771)
R^2/D10^2 : 7.64018E-02 (-0.0269055 0.0398481)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.014e-08 5.577e-09
25- 50 1.298e-07 2.113e-08
50-150 2.476e-07 5.275e-08
15-150 4.075e-07 5.811e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-40.4669 -200)
Norm : 3.56976 (-0.379691 0.379691)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.88e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.316e-08 3.512e-08
25- 50 1.215e-07 6.664e-08
50-150 2.665e-07 1.470e-07
15-150 4.511e-07 2.430e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.43703 (-5.20784 -9.43866)
R1^2/D10^2 : 0.261866 (-0.166251 2.42972)
kT2 [keV] : 25.2828 (-21.0636 -25.2901)
R2^2/D10^2 : 1.22087E-02 (-0.0118996 0.047564)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.257e-08 2.334e-08
25- 50 1.300e-07 6.884e-08
50-150 2.917e-07 1.600e-07
15-150 4.642e-07 2.372e-07
Peak spectrum fit
Power-law model
Time interval is from 0.876 sec. to 1.876 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26682 ( -0.176403 0.174403 )
Norm@50keV : 1.93570E-02 ( -0.00229704 0.00229703 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.68 using 59 bins.
Reduced chi-squared = 1.38035
# Null hypothesis probability of 3.01e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.29579 ( -0.28095 0.2816 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.92903e-07 ( -2.4337e-08 2.44472e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.876 sec. to 1.876 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.06942 ( -1.33757 1.04564 )
Epeak [keV] : 69.8632 ( -9.14842 16.2378 )
Norm@50keV : 0.250647 ( -0.250647 0.749871 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.40 using 59 bins.
Reduced chi-squared = 1.07857
# Null hypothesis probability of 3.20e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.18104 ( -0.28536 0.2873 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.78066e-07 ( -2.45301e-08 2.51837e-08 ) ergs/cm2
Band function
Time interval is from 0.876 sec. to 1.876 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] : 17.3731 (-1.8091 2.09589)
R^2/D10^2 : 0.186560 (-0.0620155 0.087387)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.44e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.140e-08 2.686e-09
25- 50 5.130e-08 8.625e-09
50-150 1.113e-07 1.956e-08
15-150 1.740e-07 2.635e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-36.2928 -200)
Norm : 9.68822 (-1.15805 1.15805)
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.87e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.412e-08 1.352e-08
25- 50 4.640e-08 2.559e-08
50-150 1.018e-07 5.565e-08
15-150 1.723e-07 8.790e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.86965E-02 (0.822496 -0.0186965)
R1^2/D10^2 : 9.90608E+23 (-9.90608e+23 -9.90608e+23)
kT2 [keV] : 17.3733 (-1.80953 2.09545)
R2^2/D10^2 : 0.186550 (-0.0619997 0.0874028)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.33057 ( -0.17253 0.171124 )
Norm@50keV : 7.12057E-03 ( -0.00075713 0.000756761 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.25e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 7.104 sec: 0.854473 ( -0.0931428 0.0933328 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.96241e-07 ( -5.74091e-08 5.78213e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.166333 ( -0.983367 0.803203 )
Epeak [keV] : 80.5018 ( -17.0815 65.1399 )
Norm@50keV : 2.68298E-02 ( -0.0158552 0.052418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 7.104 sec: 0.819685 ( -0.096709 0.096698 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.61251e-07 ( -6.22701e-08 6.31496e-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) = 1.12e-07
S(50-100 keV) = 1.79e-07
T90 vs. Hardness ratio plot
T90 = 5.8879998922348 sec.
Hardness ratio (energy fluence ratio) = 1.59821
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.27759
Count Ratio (50-100 keV) / (15-25 keV) = 1.62553
Mask shadow pattern
IMX = 2.713152141104851E-01, IMY = 5.343054176126579E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-229.579410 -0.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4893 -40.5403 3.0 51.8 1.0 3.2828 3.8 2.0 Vela X-1
86.4460 -38.9737 2.7 17.2 29.0 1.5304 4.3 ------ UNKNOWN
48.2442 -1.2821 2.8 35.3 -176.2 2.0015 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.064000 7.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4403 -40.4646 6.8 51.7 0.9 -0.1829 -1.7 6.7 Vela X-1
69.8805 -47.1662 1.8 23.4 68.0 0.2681 6.5 ------ UNKNOWN
34.6312 3.4427 2.5 48.8 176.2 0.3453 4.6 ------ UNKNOWN
102.4727 -6.5375 0.8 30.9 -63.1 0.7003 13.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
619.720630 962.364300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5222 -40.5521 2.8 30.9 116.5 3.5308 4.1 0.3 Vela X-1
158.9973 -40.6114 2.0 40.5 90.6 9.6886 5.7 ------ UNKNOWN
153.0894 -32.3218 2.4 31.6 84.8 4.8996 4.8 ------ UNKNOWN
128.3845 -39.6630 2.4 29.4 127.1 3.8153 4.8 ------ UNKNOWN
169.3730 34.4470 3.6 59.2 -14.1 5.8074 3.3 ------ UNKNOWN
69.8306 -19.8482 2.4 57.2 -160.1 9.9552 4.8 ------ UNKNOWN
80.3593 -10.5701 2.5 47.3 -148.0 4.8089 4.6 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:24:27 EDT 2024