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
29.8783 23.8396 0.0047 33.5753 -149.6076 2.7932499 41.286 TRIG_00882252
Foreground time interval of the image:
-0.124 11.885 (delta_t = 12.009 [sec])
Background time interval of the image:
-572.715 -554.030 (delta_t = 18.686 [sec])
-239.816 -0.124 (delta_t = 239.692 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -0.124 sec. to 96.616 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58844 ( -0.0516712 0.0517753 )
Norm@50keV : 6.47202E-03 ( -0.000173924 0.000173877 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.20 using 59 PHA bins.
# Reduced chi-squared = 0.7229 for 57 degrees of freedom
# Null hypothesis probability = 9.429108e-01
Photon flux (15-150 keV) in 96.74 sec: 0.828762 ( -0.024651 0.024735 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.86457e-06 ( -1.65606e-07 1.65966e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.124 sec. to 96.616 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36822 ( -0.210106 0.200549 )
Epeak [keV] : 154.628 ( -50.0653 738.298 )
Norm@50keV : 8.18970E-03 ( -0.00154095 0.00200013 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.68 using 59 PHA bins.
# Reduced chi-squared = 0.6728 for 56 degrees of freedom
# Null hypothesis probability = 9.714335e-01
Photon flux (15-150 keV) in 96.74 sec: 0.814324 ( -0.027627 0.027746 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.00365e-06 ( -2.40116e-07 2.08519e-07 ) ergs/cm2
Band function
Time interval is from -0.124 sec. to 96.616 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] : 15.8952 ( )
R^2/D10^2 : 7.17627E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 321.23 using 59 PHA bins.
# Reduced chi-squared = 5.6357 for 57 degrees of freedom
# Null hypothesis probability = 1.685011e-38
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.632e-07 1.944e-08
25- 50 1.520e-06 5.708e-08
50-150 2.677e-06 1.369e-07
15-150 4.560e-06 1.301e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-28.0712 -200)
Norm : 3.32453 (-0.0888785 0.0888785)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.50 using 59 PHA bins.
# Reduced chi-squared = 0.6755 for 57 degrees of freedom
# Null hypothesis probability = 9.714037e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.012e-07 2.399e-08
25- 50 1.541e-06 4.547e-08
50-150 3.378e-06 9.771e-08
15-150 5.720e-06 1.751e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.75736 (-0.714956 0.787472)
R1^2/D10^2 : 0.955867 (-0.306586 0.497602)
kT2 [keV] : 25.2621 (-2.11978 2.71608)
R2^2/D10^2 : 1.13913E-02 (-0.00358001 0.00445603)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.46 using 59 PHA bins.
# Reduced chi-squared = 0.7901 for 55 degrees of freedom
# Null hypothesis probability = 8.695029e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.745e-07 8.455e-08
25- 50 1.527e-06 8.755e-08
50-150 3.395e-06 2.380e-07
15-150 5.697e-06 3.483e-07
Peak spectrum fit
Power-law model
Time interval is from 75.276 sec. to 76.276 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60516 ( -0.0812595 0.0820543 )
Norm@50keV : 3.79181E-02 ( -0.00191809 0.00191124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.56 using 59 PHA bins.
# Reduced chi-squared = 1.273 for 57 degrees of freedom
# Null hypothesis probability = 8.025763e-02
Photon flux (15-150 keV) in 1 sec: 4.88064 ( -0.24029 0.24046 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.54446e-07 ( -1.91642e-08 1.92513e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 75.276 sec. to 76.276 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.892926 ( -0.389094 0.35556 )
Epeak [keV] : 74.7712 ( -11.8985 28.2012 )
Norm@50keV : 8.92257E-02 ( -0.0304938 0.0523995 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.88 using 59 PHA bins.
# Reduced chi-squared = 1.069 for 56 degrees of freedom
# Null hypothesis probability = 3.369476e-01
Photon flux (15-150 keV) in 1 sec: 4.74436 ( -0.24939 0.24935 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.35885e-07 ( -2.13782e-08 2.14043e-08 ) ergs/cm2
Band function
Time interval is from 75.276 sec. to 76.276 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] : 13.4071 ( )
R^2/D10^2 : 0.821321 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 124.79 using 59 PHA bins.
# Reduced chi-squared = 2.1893 for 57 degrees of freedom
# Null hypothesis probability = 5.670674e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.128e-08 2.575e-09
25- 50 1.113e-07 5.750e-09
50-150 1.288e-07 1.220e-08
15-150 2.714e-07 1.580e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 161.683 (-33.3307 -161.695)
Norm : 20.1903 (-1.09054 1.17)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.73 using 59 PHA bins.
# Reduced chi-squared = 1.100 for 57 degrees of freedom
# Null hypothesis probability = 2.804552e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.150e-08 3.705e-09
25- 50 9.648e-08 1.014e-08
50-150 1.963e-07 6.267e-08
15-150 3.442e-07 7.095e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.56957 (-1.42074 1.35746)
R1^2/D10^2 : 2.81230 (-0.9584 1.89447)
kT2 [keV] : 28.3580 (-6.36089 12.7457)
R2^2/D10^2 : 3.64541E-02 (-0.0263269 0.0356712)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.98 using 59 PHA bins.
# Reduced chi-squared = 1.054 for 55 degrees of freedom
# Null hypothesis probability = 3.659068e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.386e-08 6.225e-09
25- 50 1.055e-07 1.552e-08
50-150 1.908e-07 7.813e-08
15-150 3.401e-07 8.735e-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: 1.36898 ( -0.0722635 0.0721771 )
Norm@50keV : 1.56359E-02 ( -0.000611321 0.000611317 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.34 using 59 PHA bins.
# Reduced chi-squared = 0.5499 for 57 degrees of freedom
# Null hypothesis probability = 9.977353e-01
Photon flux (15-150 keV) in 12.01 sec: 1.89119 ( -0.0791204 0.0793887 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.82641e-06 ( -7.70697e-08 7.73545e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23766 ( -0.286252 0.165595 )
Epeak [keV] : 322.638 ( -322.527 -322.527 )
Norm@50keV : 1.79573E-02 ( -0.00278935 0.0061068 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 30.67 using 59 PHA bins.
# Reduced chi-squared = 0.5476 for 56 degrees of freedom
# Null hypothesis probability = 9.976756e-01
Photon flux (15-150 keV) in 12.01 sec: 1.87593 ( -0.08458 0.07867 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81351e-06 ( -8.26408e-08 4.15066e-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) = 1.51e-06
S(50-100 keV) = 2.01e-06
T90 vs. Hardness ratio plot
T90 = 78.095999956131 sec.
Hardness ratio (energy fluence ratio) = 1.33113
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.2789
Count Ratio (50-100 keV) / (15-25 keV) = 0.945637
Mask shadow pattern
IMX = -5.725623150005047E-01, IMY = 3.358176116065797E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-572.715410 -554.029900
-239.816000 -0.124000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6476 22.0126 0.7 33.2 111.9 9.3900 15.6 0.8 Crab
40.8992 61.4309 0.6 16.3 -53.9 5.8787 19.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.124000 11.884600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5102 21.9351 7.4 33.2 112.1 -0.1738 -1.6 8.3 Crab
90.6392 18.2681 3.1 39.8 105.8 0.7299 3.7 ------ UNKNOWN
29.8783 23.8396 0.3 33.6 -149.6 2.7932 41.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
70.484590 901.984600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
72.2663 44.2358 4.1 40.0 65.5 6.5769 2.8 ------ UNKNOWN
40.9248 61.4357 0.7 38.3 25.2 17.4535 16.2 ------ UNKNOWN
16.4508 59.1153 3.1 36.5 5.2 3.1101 3.7 ------ UNKNOWN
16.4341 19.9694 2.2 13.1 -88.0 3.3134 5.2 ------ UNKNOWN
2.6690 27.6441 2.8 24.7 -58.7 2.9084 4.0 ------ UNKNOWN
8.1009 -22.5756 3.4 51.0 -137.1 12.8108 3.4 ------ UNKNOWN
Plot creation:
Thu Mar 21 14:33:48 EDT 2019