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
340.0347 -17.3400 0.0033 44.4987 -170.5020 18.9034484 57.701 TRIG_00930285
Foreground time interval of the image:
-0.828 84.320 (delta_t = 85.148 [sec])
Background time interval of the image:
-239.408 -0.828 (delta_t = 238.580 [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 0.256000
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 0.256000
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 0.256000
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 -0.828 sec. to 84.320 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.25484 ( -0.0525186 0.0529935 )
Norm@50keV : 1.29244E-02 ( -0.000350335 0.000349037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.03 using 59 PHA bins.
# Reduced chi-squared = 1.018 for 57 degrees of freedom
# Null hypothesis probability = 4.370189e-01
Photon flux (15-150 keV) in 85.15 sec: 2.20354 ( -0.06683 0.06733 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04362e-05 ( -2.59359e-07 2.59594e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.828 sec. to 84.320 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99360 ( -0.194221 -1.9936 )
Epeak [keV] : 1.18857 ( -0.210851 0.311669 )
Norm@50keV : 1.74665E-02 ( -0.000827872 0.0010213 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.51 using 59 PHA bins.
# Reduced chi-squared = 0.9735 for 56 degrees of freedom
# Null hypothesis probability = 5.312836e-01
Photon flux (15-150 keV) in 85.15 sec: 2.14664 ( -0.0559 0.056 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -0.828 sec. to 84.320 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] : 10.8739 ( )
R^2/D10^2 : 0.629287 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 404.75 using 59 PHA bins.
# Reduced chi-squared = 7.1009 for 57 degrees of freedom
# Null hypothesis probability = 6.803651e-54
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.321e-06 6.259e-08
25- 50 3.679e-06 1.013e-07
50-150 2.435e-06 1.371e-07
15-150 7.435e-06 1.937e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 56.3167 (-3.90664 4.3025)
Norm : 11.0386 (-0.587825 0.499999)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.05 using 59 PHA bins.
# Reduced chi-squared = 1.369 for 57 degrees of freedom
# Null hypothesis probability = 3.352537e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.336e-06 1.069e-07
25- 50 3.486e-06 1.022e-07
50-150 3.758e-06 1.771e-07
15-150 9.580e-06 2.384e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.35837 (-0.496208 0.507692)
R1^2/D10^2 : 4.22246 (-1.08179 1.61686)
kT2 [keV] : 21.2134 (-2.03387 2.54505)
R2^2/D10^2 : 2.99323E-02 (-0.0111273 0.0159907)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.00 using 59 PHA bins.
# Reduced chi-squared = 1.200 for 55 degrees of freedom
# Null hypothesis probability = 1.471438e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.305e-06 1.873e-07
25- 50 3.474e-06 1.950e-07
50-150 4.018e-06 3.564e-07
15-150 9.797e-06 5.364e-07
Peak spectrum fit
Power-law model
Time interval is from -0.136 sec. to 0.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87572 ( -0.123328 0.127486 )
Norm@50keV : 4.01073E-02 ( -0.00326792 0.00323552 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.57 using 59 PHA bins.
# Reduced chi-squared = 0.8522 for 57 degrees of freedom
# Null hypothesis probability = 7.789149e-01
Photon flux (15-150 keV) in 1 sec: 5.69774 ( -0.42911 0.42973 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.68765e-07 ( -2.9796e-08 3.00027e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.136 sec. to 0.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.804774 ( -0.636655 0.559719 )
Epeak [keV] : 53.5219 ( -7.37517 11.8432 )
Norm@50keV : 0.145358 ( -0.070172 0.165065 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.80 using 59 PHA bins.
# Reduced chi-squared = 0.6571 for 56 degrees of freedom
# Null hypothesis probability = 9.778870e-01
Photon flux (15-150 keV) in 1 sec: 5.46529 ( -0.44355 0.44479 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.48739e-07 ( -3.13148e-08 3.17131e-08 ) ergs/cm2
Band function
Time interval is from -0.136 sec. to 0.864 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] : 12.3557 (-0.996753 1.07857)
R^2/D10^2 : 1.25216 (-0.338548 0.462802)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.76 using 59 PHA bins.
# Reduced chi-squared = 1.101 for 57 degrees of freedom
# Null hypothesis probability = 2.795245e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.051e-08 5.010e-09
25- 50 1.319e-07 1.200e-08
50-150 1.234e-07 1.972e-08
15-150 2.958e-07 2.695e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.3676 (-18.2189 26.2805)
Norm : 26.0806 (-2.54681 3.01333)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.96 using 59 PHA bins.
# Reduced chi-squared = 0.6835 for 57 degrees of freedom
# Null hypothesis probability = 9.675705e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.804e-08 7.720e-09
25- 50 1.149e-07 9.100e-09
50-150 1.742e-07 5.815e-08
15-150 3.571e-07 6.020e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.07093 (-1.93647 2.00396)
R1^2/D10^2 : 9.33539 (-5.57687 31.1235)
kT2 [keV] : 17.8636 (-2.99031 4.9161)
R2^2/D10^2 : 0.237298 (-0.159226 0.301431)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.73 using 59 PHA bins.
# Reduced chi-squared = 0.6678 for 55 degrees of freedom
# Null hypothesis probability = 9.724542e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.168e-08 2.714e-08
25- 50 1.174e-07 4.484e-08
50-150 1.661e-07 6.883e-08
15-150 3.452e-07 1.185e-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: 2.25484 ( -0.0525186 0.0529935 )
Norm@50keV : 1.29244E-02 ( -0.000350335 0.000349037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.03 using 59 PHA bins.
# Reduced chi-squared = 1.018 for 57 degrees of freedom
# Null hypothesis probability = 4.370189e-01
Photon flux (15-150 keV) in 85.15 sec: 2.20330 ( -0.0668105 0.0673188 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04342e-05 ( -2.59333e-07 2.59386e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99422 ( -0.20782 -1.99422 )
Epeak [keV] : 1.07549 ( -0.191201 0.282893 )
Norm@50keV : 1.74546E-02 ( -0.000826669 0.00103106 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.51 using 59 PHA bins.
# Reduced chi-squared = 0.9734 for 56 degrees of freedom
# Null hypothesis probability = 5.313643e-01
Photon flux (15-150 keV) in 85.15 sec: 2.15238 ( -0.07939 0.08014 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02154e-05 ( -3.25358e-07 3.24507e-07 ) 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) = 3.34e-06
S(50-100 keV) = 2.80e-06
T90 vs. Hardness ratio plot
T90 = 64.3479999303818 sec.
Hardness ratio (energy fluence ratio) = 0.838323
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.02106
Count Ratio (50-100 keV) / (15-25 keV) = 0.478598
Mask shadow pattern
IMX = -9.691802042739096E-01, IMY = 1.621506513189872E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.408000 -0.828000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1419 38.2096 5.2 35.7 -75.5 1.2400 2.2 6.9 Cyg X-2
50.9229 51.5467 3.3 48.0 16.5 1.8967 3.5 ------ UNKNOWN
318.5164 -13.1252 3.0 55.3 -146.5 5.2279 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.828000 84.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1662 38.4455 24.2 35.7 -75.1 -0.2439 -0.5 7.4 Cyg X-2
47.4717 38.4081 2.4 42.0 33.4 1.7784 4.8 ------ UNKNOWN
62.0873 56.5575 3.3 55.7 12.9 3.2077 3.5 ------ UNKNOWN
340.0347 -17.3400 0.2 44.5 -170.5 18.9020 57.7 ------ UNKNOWN
11.5020 63.7623 2.4 43.0 -16.5 1.4363 4.8 ------ UNKNOWN
339.0416 29.0276 2.4 22.8 -87.3 1.2534 4.8 ------ UNKNOWN
351.8325 76.5406 3.4 55.6 -25.2 2.3383 3.4 ------ UNKNOWN
318.4745 12.7231 3.4 43.0 -116.2 2.7329 3.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
537.092590 962.646400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
108.7823 50.0293 3.5 40.8 98.0 4.7513 3.3 ------ UNKNOWN
123.1532 59.7090 3.5 35.9 116.9 2.6872 3.4 ------ UNKNOWN
147.0895 61.2472 2.4 29.4 135.3 2.7342 4.8 ------ UNKNOWN
157.2680 38.2457 2.4 5.6 126.9 1.8750 4.8 ------ UNKNOWN
Plot creation:
Wed Nov 27 16:25:28 EST 2019