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
170.3186 39.1343 0.0163 41.9099 -162.4949 0.2943256 11.784 TRIG_01080859
Foreground time interval of the image:
-0.012 1.452 (delta_t = 1.464 [sec])
Background time interval of the image:
-239.096 -0.012 (delta_t = 239.084 [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 -0.012 sec. to 1.452 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99344 ( -0.244405 0.262283 )
Norm@50keV : 1.24896E-02 ( -0.00213603 0.00206606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.55 using 59 bins.
Reduced chi-squared = 0.869298
# Null hypothesis probability of 7.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.464 sec: 1.86795 ( -0.26064 0.26077 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68594e-07 ( -2.69395e-08 2.73267e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.012 sec. to 1.452 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98198 ( -1.10201 0.254876 )
Epeak [keV] : 64.1709 ( -52.3872 -53.6476 )
Norm@50keV : 1.26867E-02 ( -0.00801636 0.043286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.55 using 59 bins.
Reduced chi-squared = 0.884821
# Null hypothesis probability of 7.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.464 sec: 1.86662 ( -0.26364 0.26318 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68164e-07 ( -3.0414e-08 2.75679e-08 ) ergs/cm2
Band function
Time interval is from -0.012 sec. to 1.452 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] : 8.94055 (-1.42452 1.77712)
R^2/D10^2 : 1.33557 (-0.676118 1.30111)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.91e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.032e-08 8.960e-09
25- 50 6.379e-08 1.333e-08
50-150 2.384e-08 8.889e-09
15-150 1.180e-07 2.588e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.2258 (-24.494 48.5203)
Norm : 9.22943 (-1.94491 2.51262)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.462e-08 6.339e-09
25- 50 5.492e-08 9.575e-09
50-150 6.996e-08 3.257e-08
15-150 1.595e-07 3.323e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.98540 (-1.36667 1.52963)
R1^2/D10^2 : 3.03646 (-1.60108 3.60456)
kT2 [keV] : 37.9870 (-17.0209 -37.987)
R2^2/D10^2 : 4.34582E-03 (-0.00392126 0.0279522)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.14e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.600e-08 1.577e-08
25- 50 5.568e-08 2.368e-08
50-150 8.169e-08 4.463e-08
15-150 1.734e-07 6.882e-08
Peak spectrum fit
Power-law model
Time interval is from 0.244 sec. to 1.244 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.95060 ( -0.241214 0.257596 )
Norm@50keV : 1.51730E-02 ( -0.00256514 0.00249103 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.61 using 59 bins.
Reduced chi-squared = 0.922982
# Null hypothesis probability of 6.40e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.22593 ( -0.31657 0.31677 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.39659e-07 ( -2.25015e-08 2.27986e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.244 sec. to 1.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66722 ( -1.26168 0.511996 )
Epeak [keV] : 50.9341 ( -50.8416 -50.9108 )
Norm@50keV : 2.20452E-02 ( -0.0120185 0.0995767 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.36 using 59 bins.
Reduced chi-squared = 0.935
# Null hypothesis probability of 6.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.21203 ( -0.32063 0.32031 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36518e-07 ( -2.56235e-08 2.47432e-08 ) ergs/cm2
Band function
Time interval is from 0.244 sec. to 1.244 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] : 9.54573 (-1.50735 1.82155)
R^2/D10^2 : 1.26344 (-0.619251 1.18428)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.94e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.304e-08 5.770e-09
25- 50 5.355e-08 1.118e-08
50-150 2.439e-08 1.014e-08
15-150 1.010e-07 2.046e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 73.8508 (-26.087 52.6581)
Norm : 10.8044 (-2.22297 2.80483)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.41e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.786e-08 5.730e-09
25- 50 4.496e-08 7.330e-09
50-150 6.005e-08 2.960e-08
15-150 1.329e-07 2.896e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.48740 (-1.52826 1.68959)
R1^2/D10^2 : 2.77971 (-1.46481 3.51998)
kT2 [keV] : 39.5397 (-19.107 -39.5397)
R2^2/D10^2 : 4.42680E-03 (-0.00421169 0.0377364)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.761e-08 1.036e-08
25- 50 4.765e-08 1.927e-08
50-150 6.640e-08 3.500e-08
15-150 1.417e-07 5.598e-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: 1.99344 ( -0.244405 0.262283 )
Norm@50keV : 1.24896E-02 ( -0.00213603 0.00206606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.464 sec: 1.86781 ( -0.260617 0.260748 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68563e-07 ( -2.69336e-08 2.73332e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96312 ( -1.09149 0.222033 )
Epeak [keV] : 52.5981 ( -46.6644 -52.6888 )
Norm@50keV : 1.30021E-02 ( -0.00802299 0.0432757 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.464 sec: 1.86560 ( -0.26302 0.26214 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.67493e-07 ( -2.97658e-08 2.83782e-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) = 5.07e-08
S(50-100 keV) = 5.09e-08
T90 vs. Hardness ratio plot
T90 = 1.29999995231628 sec.
Hardness ratio (energy fluence ratio) = 1.00394
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.27362
Count Ratio (50-100 keV) / (15-25 keV) = 0.599605
Mask shadow pattern
IMX = -8.559957113769353E-01, IMY = 2.699789472553979E-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:
-239.096000 -0.012000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5544 -40.5738 2.9 44.3 7.6 1.8169 3.9 1.6 Vela X-1
119.2150 -7.8218 2.7 31.5 64.4 1.5986 4.3 ------ UNKNOWN
161.2801 -33.6724 3.2 37.4 -23.9 1.2850 3.6 ------ UNKNOWN
159.7279 -53.6995 2.8 56.3 -14.7 3.4506 4.1 ------ UNKNOWN
180.2194 17.2289 2.6 34.1 -125.9 1.7838 4.5 ------ UNKNOWN
185.1550 -26.6019 2.3 44.9 -55.3 4.6842 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.012000 1.452000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5350 -40.5241 7.1 44.2 7.7 0.0461 1.6 1.9 Vela X-1
170.3188 39.1344 1.0 41.9 -162.5 0.2942 11.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
79.004600 962.967500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
138.7786 -0.7184 3.5 49.2 -2.8 4.3016 3.3 ------ UNKNOWN
197.9379 25.2200 2.9 27.1 -113.8 3.7735 4.0 ------ UNKNOWN
200.7377 19.7643 3.3 32.6 -108.8 4.4654 3.5 ------ UNKNOWN
202.1651 9.2723 3.6 41.3 -98.7 12.6428 3.2 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:17:35 EDT 2022