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
191.9894 -28.7620 0.0254 12.5029 30.9171 0.5312100 7.538 TRIG_01093611
Foreground time interval of the image:
-2.728 23.288 (delta_t = 26.016 [sec])
Background time interval of the image:
-239.608 -2.728 (delta_t = 236.880 [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 4.096000
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 4.096000
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 4.096000
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 -2.728 sec. to 23.288 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.94384 ( -0.309294 0.336631 )
Norm@50keV : 1.21028E-03 ( -0.000280404 0.000272533 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.54 using 59 bins.
Reduced chi-squared = 1.41298
# Null hypothesis probability of 2.18e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.02 sec: 0.177023 ( -0.030979 0.030984 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.89806e-07 ( -6.29354e-08 6.58891e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.728 sec. to 23.288 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.637247 ( -2.97674 1.58898 )
Epeak [keV] : 38.2440 ( -37.9963 80.5102 )
Norm@50keV : 7.96806E-03 ( -0.00847553 0.791566 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.74 using 59 bins.
Reduced chi-squared = 1.40607
# Null hypothesis probability of 2.42e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.02 sec: 0.169720 ( -0.031603 0.032198 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44145e-07 ( -6.46311e-08 8.5873e-08 ) ergs/cm2
Band function
Time interval is from -2.728 sec. to 23.288 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] : 8.83745 (-1.51671 1.90971)
R^2/D10^2 : 0.137191 (-0.0730127 0.146918)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.14e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.375e-08 1.821e-08
25- 50 1.110e-07 2.956e-08
50-150 4.004e-08 1.944e-08
15-150 2.048e-07 5.839e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.0149 (-25.7269 63.6817)
Norm : 0.916769 (-0.22918 0.315783)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.80e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.040e-08 1.475e-08
25- 50 9.330e-08 2.520e-08
50-150 1.105e-07 6.378e-08
15-150 2.642e-07 7.966e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.20028 (-3.01498 1.92274)
R1^2/D10^2 : 0.254117 (-0.140628 0.668116)
kT2 [keV] : 27.7392 (-16.3878 -35.1578)
R2^2/D10^2 : 8.50300E-04 (-0.000424469 0.0568233)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.73e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.945e-08 3.519e-08
25- 50 9.854e-08 5.581e-08
50-150 1.079e-07 7.920e-08
15-150 2.659e-07 1.388e-07
Peak spectrum fit
Power-law model
Time interval is from -0.132 sec. to 0.868 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41181 ( -0.60216 0.584754 )
Norm@50keV : 4.25328E-03 ( -0.00135168 0.00131658 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.66 using 59 bins.
Reduced chi-squared = 1.22211
# Null hypothesis probability of 1.21e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.519384 ( -0.15975 0.160246 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.10053e-08 ( -1.42044e-08 1.48044e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.132 sec. to 0.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42320 ( -1.0543 0.577941 )
Epeak [keV] : 9999.30 ( -9999.36 -9999.36 )
Norm@50keV : 4.23822E-03 ( -0.00135583 0.0471917 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.66 using 59 bins.
Reduced chi-squared = 1.24393
# Null hypothesis probability of 1.04e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.520802 ( -0.161533 0.159299 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19411e-08 ( -1.62342e-08 1.35994e-08 ) ergs/cm2
Band function
Time interval is from -0.132 sec. to 0.868 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] : 11.4715 (-3.72739 10.9384)
R^2/D10^2 : 0.146077 (-0.145202 0.476295)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.83e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.045e-09 2.558e-09
25- 50 1.206e-08 7.465e-09
50-150 9.248e-09 6.575e-09
15-150 2.535e-08 1.613e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-199.363 -199.363)
Norm : 2.12354 (-0.647277 0.647275)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.15e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.288e-09 3.308e-09
25- 50 1.017e-08 6.270e-09
50-150 2.231e-08 1.341e-08
15-150 3.777e-08 2.338e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.28546 (-3.01315 4.54823)
R1^2/D10^2 : 0.407125 (-0.3262 1.68578)
kT2 [keV] : 144.622 (-121.826 -144.064)
R2^2/D10^2 : 1.51699E-04 (-0.000114577 0.0108313)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.18e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.277e-09 3.274e-09
25- 50 1.076e-08 6.410e-09
50-150 2.883e-08 1.628e-08
15-150 4.486e-08 2.101e-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: 1.94384 ( -0.309294 0.336631 )
Norm@50keV : 1.21028E-03 ( -0.000280404 0.000272533 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.18e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.02 sec: 0.177011 ( -0.0309778 0.0309815 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.89759e-07 ( -6.28219e-08 6.59573e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.593792 ( -2.94853 1.5826 )
Epeak [keV] : 38.0513 ( -37.8861 76.9056 )
Norm@50keV : 8.52789E-03 ( -0.00857491 0.786243 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.42e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.02 sec: 0.169685 ( -0.031588 0.032186 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44174e-07 ( -6.45569e-08 8.60611e-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) = 8.59e-08
S(50-100 keV) = 8.92e-08
T90 vs. Hardness ratio plot
T90 = 24.3680000305176 sec.
Hardness ratio (energy fluence ratio) = 1.03842
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.56695
Count Ratio (50-100 keV) / (15-25 keV) = 0.611302
Mask shadow pattern
IMX = 1.902394694622780E-01, IMY = -1.139329220769786E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.608000 -2.728000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2684 -60.6251 4.0 45.0 -2.2 1.4277 2.9 1.4 Cen X-3
186.6297 -62.7046 17.8 42.2 -13.1 0.2920 0.6 4.0 GX 301-2
244.9459 -15.6451 1.1 39.4 -116.9 6.3811 10.4 2.0 Sco X-1
163.0911 -13.4384 3.0 39.6 70.9 3.9015 3.8 ------ UNKNOWN
192.5181 -30.0471 2.6 12.8 24.8 1.1671 4.5 ------ UNKNOWN
189.3391 -44.7288 2.5 25.5 -0.5 1.2987 4.6 ------ UNKNOWN
213.6585 -18.9264 3.2 9.8 -132.1 0.8618 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.728000 23.288000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4796 -60.5203 4.7 44.8 -2.2 0.2838 2.4 7.8 Cen X-3
186.4822 -62.6895 21.2 42.2 -13.0 0.0580 0.5 6.8 GX 301-2
245.1265 -15.6702 8.1 39.6 -116.7 0.2358 1.4 8.7 Sco X-1
191.9891 -28.7619 1.5 12.5 30.9 0.5315 7.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.692590 306.292620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5998 -40.3534 23.0 47.0 33.7 -0.3465 -0.5 12.5 Vela X-1
170.0640 -60.5731 4.7 35.0 -7.8 0.8095 2.5 8.0 Cen X-3
186.6076 -62.6669 8.2 34.1 -22.1 0.4500 1.4 6.3 GX 301-2
207.3323 -86.5141 1.8 57.9 -27.5 9.0730 6.3 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:09:06 EDT 2022