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
206.4278 -44.0390 0.0070 23.6957 -0.6225 1.5616886 27.351 TRIG_01121751
Foreground time interval of the image:
-0.200 10.213 (delta_t = 10.413 [sec])
Background time interval of the image:
-239.488 -0.200 (delta_t = 239.288 [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 0.512000
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 0.512000
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 0.512000
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 -0.200 sec. to 13.008 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43909 ( -0.0968579 0.0971864 )
Norm@50keV : 9.17556E-03 ( -0.000488026 0.000486297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.95 using 59 bins.
Reduced chi-squared = 1.05175
# Null hypothesis probability of 3.69e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 13.21 sec: 1.12776 ( -0.06046 0.06058 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16239e-06 ( -6.8782e-08 6.92444e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.200 sec. to 13.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30578 ( -0.394728 0.183188 )
Epeak [keV] : 265.724 ( -265.975 -265.975 )
Norm@50keV : 1.06780E-02 ( -0.00192314 0.00586828 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.58 using 59 bins.
Reduced chi-squared = 1.06393
# Null hypothesis probability of 3.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 13.21 sec: 1.11906 ( -0.06501 0.06481 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14898e-06 ( -7.84408e-08 7.69412e-08 ) ergs/cm2
Band function
Time interval is from -0.200 sec. to 13.008 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] : 15.6012 ( )
R^2/D10^2 : 0.110017 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 137.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.34e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.353e-08 7.979e-09
25- 50 3.027e-07 2.054e-08
50-150 5.099e-07 5.522e-08
15-150 8.861e-07 6.044e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-22.0414 -200)
Norm : 4.62565 (-0.241094 0.241094)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.41e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.522e-07 8.388e-09
25- 50 2.927e-07 1.658e-08
50-150 6.420e-07 1.347e-07
15-150 1.087e-06 1.475e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.58239 (-1.5569 1.64601)
R1^2/D10^2 : 0.844790 (-0.379633 0.961746)
kT2 [keV] : 28.9100 (-5.65807 10.7655)
R2^2/D10^2 : 1.06215E-02 (-0.00681668 0.0125771)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.299e-07 2.764e-08
25- 50 2.908e-07 5.033e-08
50-150 7.208e-07 2.062e-07
15-150 1.142e-06 3.275e-07
Peak spectrum fit
Power-law model
Time interval is from 6.580 sec. to 7.580 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10452 ( -0.153743 0.151309 )
Norm@50keV : 2.25137E-02 ( -0.00194657 0.00194628 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.37 using 59 bins.
Reduced chi-squared = 1.09421
# Null hypothesis probability of 2.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.61259 ( -0.23022 0.23046 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35072e-07 ( -2.286e-08 2.30589e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.580 sec. to 7.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.859342 ( -0.674033 0.320213 )
Epeak [keV] : 250.851 ( -250.868 -250.868 )
Norm@50keV : 2.94452E-02 ( -0.00855239 0.0307103 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.89 using 59 bins.
Reduced chi-squared = 1.10518
# Null hypothesis probability of 2.74e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.58626 ( -0.23977 0.23895 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.31143e-07 ( -2.52934e-08 2.47097e-08 ) ergs/cm2
Band function
Time interval is from 6.580 sec. to 7.580 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] : 19.0873 (-2.12499 2.54422)
R^2/D10^2 : 0.142527 (-0.0475519 0.0673328)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.42e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.019e-08 1.806e-09
25- 50 4.917e-08 7.015e-09
50-150 1.318e-07 2.220e-08
15-150 1.911e-07 2.240e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-18.8915 -200)
Norm : 10.6056 (-0.946073 0.946073)
------------------------------------------------------------
#Fit statistic : Chi-Squared 84.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.04e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.640e-08 7.145e-09
25- 50 5.079e-08 1.532e-08
50-150 1.114e-07 5.871e-08
15-150 1.886e-07 1.016e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.8578 (-4.43536 3.70693)
R1^2/D10^2 : 0.576381 (-0.310541 1.78434)
kT2 [keV] : 45.9755 (-20.7889 -46.4595)
R2^2/D10^2 : 7.12078E-03 (-0.00670557 0.0407519)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.14e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.591e-08 6.221e-09
25- 50 5.178e-08 2.224e-08
50-150 1.652e-07 8.391e-08
15-150 2.329e-07 1.111e-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: 1.42422 ( -0.100488 0.100816 )
Norm@50keV : 1.00308E-02 ( -0.000554228 0.000552288 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.41 sec: 1.22845 ( -0.0684066 0.0685397 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00412e-06 ( -6.19298e-08 6.23341e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30095 ( -0.403106 0.211728 )
Epeak [keV] : 291.013 ( -291.013 -291.013 )
Norm@50keV : 1.15348E-02 ( -0.00199145 0.00646889 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.41 sec: 1.21970 ( -0.0732 0.07301 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.9415e-07 ( -7.0078e-08 6.87945e-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) = 2.79e-07
S(50-100 keV) = 4.11e-07
T90 vs. Hardness ratio plot
T90 = 11.1399999856949 sec.
Hardness ratio (energy fluence ratio) = 1.47312
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.4094
Count Ratio (50-100 keV) / (15-25 keV) = 1.09228
Mask shadow pattern
IMX = 4.388532200155590E-01, IMY = 4.767913310125819E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.488000 -0.200000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5209 -40.5818 3.4 33.3 -128.2 2.1161 3.4 1.7 Vela X-1
170.4556 -60.4223 0.0 4.2 -137.9 0.0233 0.1 12.7 Cen X-3
186.6194 -62.5880 9.1 3.9 56.1 0.5900 1.3 11.0 GX 301-2
21.8140 -70.7269 3.5 47.0 133.6 7.9432 3.3 ------ UNKNOWN
305.0102 -81.0425 2.5 34.7 110.7 4.7993 4.6 ------ UNKNOWN
329.7758 -81.9303 3.1 35.9 116.8 4.5408 3.7 ------ UNKNOWN
228.0397 -31.5563 2.2 43.4 13.3 3.8768 5.2 ------ UNKNOWN
227.6188 -15.7041 2.2 57.2 3.0 8.4008 5.2 ------ UNKNOWN
217.8959 -18.8621 2.7 50.5 -5.9 3.3671 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.200000 10.212600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3596 -40.6710 175.5 33.3 -128.5 -0.0051 -0.1 10.4 Vela X-1
169.9089 -60.5536 0.0 4.4 -140.5 -0.0727 -1.4 12.7 Cen X-3
186.1959 -62.7523 0.0 3.7 59.4 -0.0156 -0.3 12.7 GX 301-2
206.4278 -44.0390 0.4 23.7 -0.6 1.5617 27.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
69.412600 873.112600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4457 -40.5591 6.2 51.0 -148.1 6.9572 1.9 3.8 Vela X-1
170.3479 -60.4672 112.3 27.0 -176.0 -0.1564 -0.1 9.4 Cen X-3
187.1092 -62.7877 0.0 21.8 168.3 -0.9530 -0.7 12.5 GX 301-2
245.0052 -15.6413 1.2 43.2 25.5 24.1148 9.9 1.5 Sco X-1
255.9758 -37.8377 824.8 37.4 62.3 0.0579 0.0 0.6 4U 1700-377
256.5352 -36.3501 3.8 38.4 60.4 13.3408 3.0 6.5 GX 349+2
228.5568 -51.9521 2.3 16.7 90.3 7.6471 4.9 ------ UNKNOWN
119.4297 -49.8030 2.7 56.3 -164.9 21.6836 4.4 ------ UNKNOWN
147.6734 -29.7177 2.7 48.1 -129.1 26.2417 4.2 ------ UNKNOWN
Plot creation:
Wed Jun 14 14:01:36 EDT 2023