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
149.6010 -24.3607 0.0204 33.0060 8.9684 0.3040143 9.391 TRIG_01088376
Foreground time interval of the image:
-1.304 2.972 (delta_t = 4.276 [sec])
Background time interval of the image:
-239.992 -1.304 (delta_t = 238.688 [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 -1.304 sec. to 2.972 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71518 ( -0.294775 0.314738 )
Norm@50keV : 4.67777E-03 ( -0.000881097 0.000850935 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.35 using 59 bins.
Reduced chi-squared = 1.18158
# Null hypothesis probability of 1.64e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 4.276 sec: 0.624618 ( -0.102047 0.10212 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.85011e-07 ( -3.57598e-08 3.65318e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.304 sec. to 2.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69842 ( -1.25961 1.9755 )
Epeak [keV] : 840.849 ( -826.61 -826.62 )
Norm@50keV : 4.77525E-03 ( -0.000981027 0.0172159 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.35 using 59 bins.
Reduced chi-squared = 1.20268
# Null hypothesis probability of 1.42e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 4.276 sec: 0.624207 ( -0.10421 0.102063 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84756e-07 ( -3.91234e-08 3.6125e-08 ) ergs/cm2
Band function
Time interval is from -1.304 sec. to 2.972 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] : 12.4252 (-2.44777 3.17721)
R^2/D10^2 : 0.132378 (-0.0740683 0.160487)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.25e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.852e-08 6.023e-09
25- 50 6.068e-08 1.688e-08
50-150 5.762e-08 2.172e-08
15-150 1.368e-07 3.575e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 139.664 (-69.9913 -137.256)
Norm : 2.57639 (-0.464635 0.67658)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.845e-08 1.558e-08
25- 50 5.218e-08 2.910e-08
50-150 9.992e-08 6.245e-08
15-150 1.805e-07 1.050e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.04930 (-1.79541 6.64225)
R1^2/D10^2 : 23.7796 (-20.5727 132.263)
kT2 [keV] : 16.5732 (-4.5146 73.517)
R2^2/D10^2 : 4.20282E-02 (-0.0313078 0.0941176)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.84e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.114e-08 1.660e-08
25- 50 4.711e-08 2.325e-08
50-150 8.531e-08 4.202e-08
15-150 1.636e-07 7.242e-08
Peak spectrum fit
Power-law model
Time interval is from -0.152 sec. to 0.848 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56004 ( -0.373015 0.39674 )
Norm@50keV : 7.33184E-03 ( -0.00179196 0.00175792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.04 using 59 bins.
Reduced chi-squared = 1.1586
# Null hypothesis probability of 1.93e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.930918 ( -0.213908 0.214232 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.89334e-08 ( -1.78688e-08 1.83316e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.152 sec. to 0.848 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.23266E-02 ( -3.13305 1.82364 )
Epeak [keV] : 62.8684 ( -14.6765 -62.7733 )
Norm@50keV : 4.62132E-02 ( -0.0469938 1.61633 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.92 using 59 bins.
Reduced chi-squared = 1.14143
# Null hypothesis probability of 2.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.878142 ( -0.226049 0.224458 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.27581e-08 ( -1.80115e-08 1.96595e-08 ) ergs/cm2
Band function
Time interval is from -0.152 sec. to 0.848 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] : 14.3980 (-3.04015 3.97905)
R^2/D10^2 : 0.128786 (-0.0750525 0.166464)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.26e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.622e-09 2.643e-09
25- 50 2.149e-08 8.146e-09
50-150 2.975e-08 1.535e-08
15-150 5.687e-08 2.303e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 184.449 (-108.628 -178.969)
Norm : 3.83526 (-0.884979 1.14088)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.13e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.644e-09 5.595e-09
25- 50 1.838e-08 1.067e-08
50-150 3.925e-08 2.278e-08
15-150 6.728e-08 3.841e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.51724 (-2.48728 14.0669)
R1^2/D10^2 : 62.8329 (-65.1706 -65.1706)
kT2 [keV] : 15.5945 (-3.56291 -15.5846)
R2^2/D10^2 : 9.26266E-02 (-0.0928046 0.116521)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.16e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.305e-09 3.718e-09
25- 50 1.954e-08 1.094e-08
50-150 3.243e-08 2.057e-08
15-150 6.028e-08 3.510e-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: 1.71518 ( -0.294775 0.314738 )
Norm@50keV : 4.67777E-03 ( -0.000881097 0.000850935 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.64e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 4.276 sec: 0.624591 ( -0.102041 0.102113 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84984e-07 ( -3.57518e-08 3.65494e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69781 ( -1.2595 1.97561 )
Epeak [keV] : 826.917 ( -826.12 -826.131 )
Norm@50keV : 4.77887E-03 ( -0.000981037 0.0172159 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.42e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 4.276 sec: 0.624212 ( -0.105294 0.102 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84884e-07 ( -3.92686e-08 3.65679e-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) = 5.05e-08
S(50-100 keV) = 6.16e-08
T90 vs. Hardness ratio plot
T90 = 3.7279999256134 sec.
Hardness ratio (energy fluence ratio) = 1.2198
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.41961
Count Ratio (50-100 keV) / (15-25 keV) = 0.754325
Mask shadow pattern
IMX = 6.416148507647752E-01, IMY = -1.012591665025407E-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:
-239.992000 -1.304000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4300 -40.4738 6.1 52.9 12.3 1.6362 1.9 6.6 Vela X-1
189.8198 -2.8156 2.4 28.1 -86.6 1.8037 4.8 ------ UNKNOWN
188.3276 -19.9533 3.2 35.8 -57.2 1.5307 3.6 ------ UNKNOWN
213.4814 36.4109 3.8 55.1 -144.9 5.0286 3.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.304000 2.972000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5550 -40.6035 20.9 52.9 12.1 0.0464 0.6 3.2 Vela X-1
133.4481 2.0971 2.3 29.8 69.9 0.2034 5.0 ------ UNKNOWN
149.6010 -24.3607 1.2 33.0 9.0 0.3040 9.4 ------ UNKNOWN
182.0644 29.1655 2.2 29.4 -158.6 0.1426 5.3 ------ UNKNOWN
205.4777 53.4457 2.6 58.6 -166.0 0.5559 4.5 ------ UNKNOWN
196.9903 -25.0231 2.1 45.2 -59.4 0.5052 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.708610 962.039800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5058 -40.5751 1.0 20.1 6.1 8.1694 11.7 1.6 Vela X-1
170.4575 -60.4927 5.9 38.9 -42.8 2.5294 1.9 8.9 Cen X-3
186.5932 -62.6475 9.1 45.5 -49.4 3.0272 1.3 7.6 GX 301-2
92.5683 -33.0337 4.2 50.2 39.7 12.3287 2.7 ------ UNKNOWN
156.5385 28.8356 3.4 53.6 160.9 10.2342 3.4 ------ UNKNOWN
164.6153 26.2338 4.1 52.6 170.3 6.4796 2.9 ------ UNKNOWN
145.9252 -6.8460 3.8 17.9 141.3 2.1546 3.0 ------ UNKNOWN
187.8417 -3.8507 2.3 42.1 -139.7 6.5832 5.0 ------ UNKNOWN
193.6214 14.6383 3.0 58.0 -154.2 16.1165 3.8 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:14:17 EDT 2022