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
171.8514 -11.4292 0.0227 46.2422 -6.9428 0.5040978 8.462 TRIG_01177054
Foreground time interval of the image:
-0.504 4.808 (delta_t = 5.312 [sec])
Background time interval of the image:
-239.240 -0.504 (delta_t = 238.736 [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 2.048000
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 2.048000
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 2.048000
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 -0.504 sec. to 4.808 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44601 ( -0.298578 0.29592 )
Norm@50keV : 6.47195E-03 ( -0.00112655 0.00112635 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.88 using 59 bins.
Reduced chi-squared = 1.06807
# Null hypothesis probability of 3.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.312 sec: 0.796807 ( -0.148234 0.149496 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.29267e-07 ( -6.02014e-08 6.05026e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.504 sec. to 4.808 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.661499 ( -1.68171 1.00074 )
Epeak [keV] : 93.7694 ( -37.3984 -93.744 )
Norm@50keV : 1.49569E-02 ( -0.00932545 0.0659143 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.77 using 59 bins.
Reduced chi-squared = 1.06732
# Null hypothesis probability of 3.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.312 sec: 0.766862 ( -0.157489 0.157407 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.18228e-07 ( -6.354e-08 6.34513e-08 ) ergs/cm2
Band function
Time interval is from -0.504 sec. to 4.808 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] : 17.4608 (-3.1259 4.00438)
R^2/D10^2 : 5.53225E-02 (-0.0288264 0.0558617)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.54e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.811e-08 6.305e-09
25- 50 8.183e-08 2.659e-08
50-150 1.796e-07 6.088e-08
15-150 2.795e-07 7.524e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-84.8217 -199.363)
Norm : 3.33122 (-0.579324 0.579398)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.43e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.406e-08 2.561e-08
25- 50 8.476e-08 4.762e-08
50-150 1.859e-07 1.064e-07
15-150 3.147e-07 1.790e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.78471 (-4.4097 10.4621)
R1^2/D10^2 : 2.44101 (-2.31349 -2.38428)
kT2 [keV] : 20.6484 (-4.95194 -20.6801)
R2^2/D10^2 : 2.80304E-02 (-0.0274992 0.0368429)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.15e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.843e-08 2.134e-08
25- 50 7.685e-08 4.065e-08
50-150 1.954e-07 1.130e-07
15-150 3.107e-07 1.553e-07
Peak spectrum fit
Power-law model
Time interval is from 0.332 sec. to 1.332 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.987246 ( -0.584695 0.498225 )
Norm@50keV : 9.66727E-03 ( -0.00303335 0.00281126 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.73 using 59 bins.
Reduced chi-squared = 0.749649
# Null hypothesis probability of 9.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.11227 ( -0.338016 0.34935 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.05024e-07 ( -2.78324e-08 2.78745e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.332 sec. to 1.332 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.980778 ( -2.68747 -0.914471 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 9.72449E-03 ( -0.00304188 -0.00972494 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.73 using 59 bins.
Reduced chi-squared = 0.763036
# Null hypothesis probability of 9.04e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.11198 ( -0.3376 0.3494 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.05264e-07 ( -2.89911e-08 2.84694e-08 ) ergs/cm2
Band function
Time interval is from 0.332 sec. to 1.332 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] : 25.5402 (-7.6131 16.1753)
R^2/D10^2 : 2.45404E-02 (-0.0245223 0.0537569)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.749e-09 1.752e-09
25- 50 1.577e-08 9.605e-09
50-150 7.600e-08 4.551e-08
15-150 9.452e-08 5.547e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-79.8294 -200)
Norm : 4.98720 (-1.38009 1.38009)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.29e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.243e-08 7.405e-09
25- 50 2.391e-08 1.443e-08
50-150 5.245e-08 3.055e-08
15-150 8.880e-08 5.300e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.10913 (-4.10388 25.7957)
R1^2/D10^2 : 7.71172 (-7.7457 -7.7457)
kT2 [keV] : 29.6205 (-9.96618 -29.6196)
R2^2/D10^2 : 1.48349E-02 (-0.0148371 0.0412709)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.003e-08 6.085e-09
25- 50 1.570e-08 8.700e-09
50-150 7.847e-08 4.886e-08
15-150 1.042e-07 5.810e-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: 1.44601 ( -0.298578 0.29592 )
Norm@50keV : 6.47195E-03 ( -0.00112655 0.00112635 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.312 sec: 0.796789 ( -0.148229 0.149481 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.29226e-07 ( -6.01913e-08 6.05435e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.660792 ( -1.6816 0.928222 )
Epeak [keV] : 93.7448 ( -93.7433 -93.7433 )
Norm@50keV : 1.49669E-02 ( -0.00932538 0.0659197 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.312 sec: 0.766796 ( -0.157449 0.15736 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.18351e-07 ( -6.35618e-08 6.35453e-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) = 7.91e-08
S(50-100 keV) = 1.16e-07
T90 vs. Hardness ratio plot
T90 = 4.72000014781952 sec.
Hardness ratio (energy fluence ratio) = 1.4665
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.92701
Count Ratio (50-100 keV) / (15-25 keV) = 1.85599
Mask shadow pattern
IMX = 1.036670064867644E+00, IMY = 1.262367500860944E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.240000 -0.504000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5421 -40.5605 1.8 13.7 -77.5 2.7269 6.4 0.7 Vela X-1
170.1455 -60.7441 11.2 15.8 87.1 -0.4957 -1.0 8.8 Cen X-3
186.6551 -62.7805 0.7 23.9 87.5 9.4108 16.0 0.6 GX 301-2
202.0346 -57.2014 3.4 32.0 77.2 2.9582 3.5 ------ UNKNOWN
127.7390 -41.6860 3.4 16.0 -99.0 1.3881 3.4 ------ UNKNOWN
133.4035 -9.1287 2.8 44.4 -61.2 9.2974 4.2 ------ UNKNOWN
131.5088 -10.1431 4.6 43.8 -64.1 5.5151 2.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.504000 4.808000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3595 -40.5236 28.2 13.8 -77.9 -0.0124 -0.4 7.9 Vela X-1
170.4821 -60.8149 0.0 16.0 87.1 -0.0695 -2.0 12.5 Cen X-3
187.0234 -62.6577 0.0 24.0 87.2 0.0526 1.3 12.1 GX 301-2
171.8515 -11.4292 1.4 46.2 -6.9 0.5041 8.5 ------ UNKNOWN
72.7258 -48.6002 2.2 44.3 -159.7 0.2813 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
138.060600 151.460600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4956 -40.3477 0.0 53.9 -161.4 -0.4995 -3.3 12.5 Vela X-1
183.3917 -10.1798 2.1 14.5 122.1 0.2641 5.5 ------ UNKNOWN
148.7759 -26.2210 2.5 36.2 -157.2 0.3010 4.6 ------ UNKNOWN
127.5304 -18.1262 2.1 49.3 -132.2 1.1940 5.6 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:47:27 EDT 2023