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
207.7497 31.1946 0.0158 43.5663 1.0423 2.8278250 12.119 TRIG_01183217
Foreground time interval of the image:
-17.656 75.253 (delta_t = 92.909 [sec])
Background time interval of the image:
-145.347 -17.656 (delta_t = 127.691 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -17.656 sec. to 109.308 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40922 ( -0.19711 0.195135 )
Norm@50keV : 1.54992E-03 ( -0.000174666 0.000174445 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.78 using 59 bins.
Reduced chi-squared = 0.943509
# Null hypothesis probability of 5.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 127 sec: 0.189153 ( -0.022342 0.022433 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.89869e-06 ( -2.30389e-07 2.31577e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -17.656 sec. to 109.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40627 ( -0.698002 0.363678 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.55546E-03 ( -0.000175307 0.000174552 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.78 using 59 bins.
Reduced chi-squared = 0.960357
# Null hypothesis probability of 5.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 127 sec: 0.189223 ( -0.022641 0.022278 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90039e-06 ( -2.4811e-07 2.07674e-07 ) ergs/cm2
Band function
Time interval is from -17.656 sec. to 109.308 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] : 16.7454 (-2.60851 3.21951)
R^2/D10^2 : 1.46361E-02 (-0.00660362 0.0117881)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.48e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.066e-07 2.437e-08
25- 50 4.659e-07 7.004e-08
50-150 9.281e-07 1.948e-07
15-150 1.501e-06 2.499e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-51.0421 -200)
Norm : 0.786511 (-0.0887919 0.0887919)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.16e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.488e-07 1.396e-07
25- 50 4.785e-07 2.348e-07
50-150 1.049e-06 5.733e-07
15-150 1.777e-06 9.823e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.24087 (-1.62937 2.2178)
R1^2/D10^2 : 0.195397 (-0.11742 0.2985)
kT2 [keV] : 34.5230 (-9.91626 29.6992)
R2^2/D10^2 : 1.06332E-03 (-0.000864224 0.00153447)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.63e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.392e-07 1.123e-07
25- 50 4.655e-07 1.946e-07
50-150 1.236e-06 6.529e-07
15-150 1.941e-06 8.033e-07
Peak spectrum fit
Power-law model
Time interval is from -17.664 sec. to -16.664 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.761752 ( -0.379351 0.337054 )
Norm@50keV : 1.03131E-02 ( -0.00249088 0.0024009 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.72 using 59 bins.
Reduced chi-squared = 0.924912
# Null hypothesis probability of 6.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.18727 ( -0.267346 0.27213 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22512e-07 ( -2.52216e-08 2.52218e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -17.664 sec. to -16.664 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.472855 ( -2.43314 1.36682 )
Epeak [keV] : 129.388 ( -46.8302 -129.507 )
Norm@50keV : 3.11895E-02 ( -0.0311285 0.184972 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.95 using 59 bins.
Reduced chi-squared = 0.909821
# Null hypothesis probability of 6.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.14629 ( -0.266159 0.27484 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20687e-07 ( -2.65522e-08 2.59691e-08 ) ergs/cm2
Band function
Time interval is from -17.664 sec. to -16.664 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] : 26.7338 (-5.86402 9.3116)
R^2/D10^2 : 2.60762E-02 (-0.0155102 0.0307144)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.121e-09 1.492e-09
25- 50 1.830e-08 7.264e-09
50-150 9.576e-08 3.903e-08
15-150 1.172e-07 4.885e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-45.879 -200)
Norm : 4.99439 (-1.15325 1.15325)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.68e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.245e-08 7.365e-09
25- 50 2.395e-08 1.372e-08
50-150 5.253e-08 3.148e-08
15-150 8.893e-08 5.235e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 200.000 (-200 -200)
R1^2/D10^2 : 1.31907E-04 (-0.000131949 -0.000131949)
kT2 [keV] : 20.4062 (-5.73313 13.5257)
R2^2/D10^2 : 4.69861E-02 (-0.0343799 0.0309169)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.42e-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: 1.30065 ( -0.208338 0.203446 )
Norm@50keV : 1.78481E-03 ( -0.00021037 0.000210154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 92.91 sec: 0.212958 ( -0.0267177 0.0268624 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6384e-06 ( -2.04652e-07 2.05786e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29684 ( -0.712429 0.385174 )
Epeak [keV] : 9998.87 ( -9998.93 -9998.93 )
Norm@50keV : 1.79240E-03 ( -0.000705808 0.0014073 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.29e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 92.91 sec: 0.213007 ( -0.027128 0.026708 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.63812e-06 ( -2.10255e-07 2.0534e-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) = 4.48e-07
S(50-100 keV) = 6.76e-07
T90 vs. Hardness ratio plot
T90 = 114.519999980927 sec.
Hardness ratio (energy fluence ratio) = 1.50893
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.44599
Count Ratio (50-100 keV) / (15-25 keV) = 1.20734
Mask shadow pattern
IMX = 9.510104169653882E-01, IMY = -1.730260021096620E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-145.347410 -17.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5288 -40.5544 109.5 54.6 -172.8 0.0664 0.1 0.0 Vela X-1
220.9644 2.8747 2.5 41.2 47.6 2.0408 4.6 ------ UNKNOWN
171.5085 -37.1512 3.2 34.5 158.6 1.1379 3.6 ------ UNKNOWN
212.5488 26.0468 3.4 43.1 10.7 1.2356 3.4 ------ UNKNOWN
132.0558 -6.4493 2.8 48.1 -129.2 4.1065 4.2 ------ UNKNOWN
158.7964 37.4014 2.7 45.7 -57.9 3.9425 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-17.656000 75.252590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5210 -40.5696 7.4 54.6 -172.8 0.6397 1.6 1.0 Vela X-1
207.7497 31.1946 0.9 43.6 1.0 2.8275 12.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
174.652590 962.212000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3517 35.4243 10.9 38.8 64.8 3.0874 1.1 7.1 Her X-1
248.5952 14.7159 2.6 40.8 98.2 11.4091 4.4 ------ UNKNOWN
180.9168 39.8177 2.7 23.3 -67.1 4.6095 4.2 ------ UNKNOWN
169.1478 -0.0927 2.6 48.1 -129.2 19.6213 4.4 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:44:49 EDT 2023