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
145.4681 75.8231 0.0050 11.9844 41.0101 5.5486797 38.738 TRIG_01111672
Foreground time interval of the image:
-3.844 73.792 (delta_t = 77.636 [sec])
Background time interval of the image:
-293.776 -3.844 (delta_t = 289.932 [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 -3.844 sec. to 73.792 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34235 ( -0.0682466 0.0681622 )
Norm@50keV : 4.61898E-03 ( -0.000160989 0.000160979 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.78 using 59 bins.
Reduced chi-squared = 0.961053
# Null hypothesis probability of 5.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 77.64 sec: 0.555593 ( -0.020577 0.020645 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.50902e-06 ( -1.3517e-07 1.3563e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.844 sec. to 73.792 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34232 ( -0.0713049 0.0663264 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 4.62836E-03 ( -0.000161484 0.000876617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.83 using 59 bins.
Reduced chi-squared = 0.979107
# Null hypothesis probability of 5.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 77.64 sec: 0.559488 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.5309e-06 ( 0 0 ) ergs/cm2
Band function
Time interval is from -3.844 sec. to 73.792 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] : 18.0201 ( )
R^2/D10^2 : 3.34026E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 250.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.31e-26 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.685e-07 1.242e-08
25- 50 7.801e-07 4.045e-08
50-150 1.839e-06 1.297e-07
15-150 2.788e-06 1.234e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-6.95355 -200)
Norm : 2.30967 (-0.0811327 0.0811327)
------------------------------------------------------------
#Fit statistic : Chi-Squared 91.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.73e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.466e-07 1.716e-08
25- 50 8.592e-07 3.455e-08
50-150 1.884e-06 7.337e-08
15-150 3.190e-06 1.211e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.20646 (-0.911274 1.01538)
R1^2/D10^2 : 0.489765 (-0.176691 0.306135)
kT2 [keV] : 31.4870 (-3.79281 5.44074)
R2^2/D10^2 : 4.49063E-03 (-0.00178661 0.00239632)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.67e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.791e-07 4.953e-08
25- 50 8.029e-07 5.819e-08
50-150 2.351e-06 2.450e-07
15-150 3.533e-06 3.416e-07
Peak spectrum fit
Power-law model
Time interval is from -0.148 sec. to 0.852 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04678 ( -0.104253 0.103454 )
Norm@50keV : 3.89449E-02 ( -0.00211571 0.00211571 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 90.08 using 59 bins.
Reduced chi-squared = 1.58035
# Null hypothesis probability of 3.42e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.49692 ( -0.24657 0.24672 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.1441e-07 ( -2.66973e-08 2.6886e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.148 sec. to 0.852 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04257 ( -0.105644 0.103477 )
Epeak [keV] : 9999.01 ( -9999.09 -9999.09 )
Norm@50keV : 3.91646E-02 ( -0.00212788 0.00738342 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 90.19 using 59 bins.
Reduced chi-squared = 1.61054
# Null hypothesis probability of 2.56e-03 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.49570 ( -0.24479 0.24663 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.14171e-07 ( -2.67082e-08 2.68812e-08 ) ergs/cm2
Band function
Time interval is from -0.148 sec. to 0.852 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] : 20.6341 ( )
R^2/D10^2 : 0.187188 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 192.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.16e-16 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.517e-08 1.725e-09
25- 50 7.711e-08 6.615e-09
50-150 2.443e-07 2.465e-08
15-150 3.366e-07 2.640e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 17.8300 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 155.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.10e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.440e-08 2.760e-09
25- 50 8.541e-08 7.090e-09
50-150 1.873e-07 4.560e-08
15-150 3.171e-07 4.190e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.15729 (-1.2754 1.48477)
R1^2/D10^2 : 2.46967 (-1.0076 1.86229)
kT2 [keV] : 48.8810 (-11.0477 24.0089)
R2^2/D10^2 : 1.35145E-02 (-0.00812731 0.0131895)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.62e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.372e-08 6.895e-09
25- 50 8.034e-08 1.291e-08
50-150 3.235e-07 8.590e-08
15-150 4.376e-07 1.074e-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: 1.34235 ( -0.0682466 0.0681622 )
Norm@50keV : 4.61898E-03 ( -0.000160989 0.000160979 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 77.64 sec: 0.555586 ( -0.0205758 0.0206433 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.50859e-06 ( -1.35148e-07 1.35821e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34173 ( -0.160388 0.0666083 )
Epeak [keV] : 9999.34 ( -9999.36 -9999.36 )
Norm@50keV : 4.62918E-03 ( -0.000161487 0.000876467 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 77.64 sec: 0.555750 ( -0.010798 0.020236 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.5075e-06 ( -1.33968e-07 1.34278e-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) = 8.00e-07
S(50-100 keV) = 1.26e-06
T90 vs. Hardness ratio plot
T90 = 56.7959998846054 sec.
Hardness ratio (energy fluence ratio) = 1.575
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.33005
Count Ratio (50-100 keV) / (15-25 keV) = 1.12255
Mask shadow pattern
IMX = 1.601788840656498E-01, IMY = -1.392908094200087E-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:
-293.776000 -3.844000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
154.5756 79.3917 3.6 16.0 40.9 1.2796 3.2 ------ UNKNOWN
122.1411 22.9811 3.6 42.2 -136.8 2.1218 3.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.844000 73.792000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
145.4681 75.8232 0.3 12.0 41.0 5.5487 38.7 ------ UNKNOWN
54.6769 59.6121 2.3 35.0 -32.9 0.8401 5.0 ------ UNKNOWN
37.1205 43.0816 2.7 54.6 -35.7 3.1410 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
260.924600 618.124680
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5777 -40.5553 2.6 48.7 166.2 7.5090 4.5 2.2 Vela X-1
120.7138 -14.3022 2.1 35.3 -154.0 3.2866 5.5 ------ UNKNOWN
119.8316 43.9287 2.3 45.6 -57.8 10.9346 5.0 ------ UNKNOWN
Plot creation:
Mon Oct 24 12:43:50 EDT 2022