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
189.6895 76.6071 0.0127 26.9185 -142.9218 3.9692595 15.110 TRIG_00889748
Foreground time interval of the image:
-105.740 35.653 (delta_t = 141.393 [sec])
Background time interval of the image:
-239.448 -105.740 (delta_t = 133.708 [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 -105.740 sec. to 88.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.21422 ( -0.101869 0.104605 )
Norm@50keV : 2.07737E-03 ( -0.000131507 0.000129997 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.04 using 59 PHA bins.
# Reduced chi-squared = 0.8603 for 57 degrees of freedom
# Null hypothesis probability = 7.643119e-01
Photon flux (15-150 keV) in 194.2 sec: 0.346542 ( -0.017456 0.017498 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.80154e-06 ( -2.06042e-07 2.08041e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -105.740 sec. to 88.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.21264 ( -0.100277 0.106925 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 2.07761E-03 ( -0.000100578 0.000128894 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.06 using 59 PHA bins.
# Reduced chi-squared = 0.8760 for 56 degrees of freedom
# Null hypothesis probability = 7.329545e-01
Photon flux (15-150 keV) in 194.2 sec: 0.337678 ( -0.019312 0.019189 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.6384e-06 ( -2.5113e-07 2.5393e-07 ) ergs/cm2
Band function
Time interval is from -105.740 sec. to 88.496 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] : 9.39886 ( )
R^2/D10^2 : 0.187136 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 129.44 using 59 PHA bins.
# Reduced chi-squared = 2.2708 for 57 degrees of freedom
# Null hypothesis probability = 1.479126e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.382e-07 5.923e-08
25- 50 1.450e-06 8.467e-08
50-150 6.305e-07 8.720e-08
15-150 2.718e-06 1.447e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 50.7989 (-6.7682 8.69373)
Norm : 1.88842 (-0.16876 0.203732)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.12 using 59 PHA bins.
# Reduced chi-squared = 0.8617 for 57 degrees of freedom
# Null hypothesis probability = 7.617532e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.999e-07 5.913e-08
25- 50 1.300e-06 6.205e-08
50-150 1.281e-06 1.663e-07
15-150 3.480e-06 1.952e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.14226 (-0.765417 0.828888)
R1^2/D10^2 : 1.51914 (-0.668295 1.45231)
kT2 [keV] : 16.8460 (-2.43366 3.38631)
R2^2/D10^2 : 1.33972E-02 (-0.00718263 0.0128442)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.02 using 59 PHA bins.
# Reduced chi-squared = 0.8367 for 55 degrees of freedom
# Null hypothesis probability = 8.005619e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.524e-07 1.973e-07
25- 50 1.223e-06 2.068e-07
50-150 1.364e-06 3.455e-07
15-150 3.539e-06 6.816e-07
Peak spectrum fit
Power-law model
Time interval is from 65.524 sec. to 66.524 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.11879 ( -0.19907 0.212409 )
Norm@50keV : 1.11586E-02 ( -0.00166147 0.00162228 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.53 using 59 PHA bins.
# Reduced chi-squared = 1.062 for 57 degrees of freedom
# Null hypothesis probability = 3.497084e-01
Photon flux (15-150 keV) in 1 sec: 1.77215 ( -0.19172 0.19171 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03891e-07 ( -1.37069e-08 1.40025e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 65.524 sec. to 66.524 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64772 ( -1.16296 0.415662 )
Epeak [keV] : 28.6833 ( )
Norm@50keV : 2.17512E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.74 using 59 PHA bins.
# Reduced chi-squared = 1.067 for 56 degrees of freedom
# Null hypothesis probability = 3.414947e-01
Photon flux (15-150 keV) in 1 sec: 1.75036 ( -0.19661 0.19624 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 65.524 sec. to 66.524 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] : 8.44168 (-1.02844 1.17702)
R^2/D10^2 : 1.59611 (-0.64403 1.07784)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.43 using 59 PHA bins.
# Reduced chi-squared = 1.288 for 57 degrees of freedom
# Null hypothesis probability = 7.044517e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.134e-08 4.160e-09
25- 50 4.092e-08 6.075e-09
50-150 1.278e-08 4.359e-09
15-150 7.505e-08 1.204e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.0485 (-13.514 21.787)
Norm : 10.0028 (-1.76685 2.30538)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.94 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 57 degrees of freedom
# Null hypothesis probability = 3.694725e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.457e-08 3.295e-09
25- 50 3.555e-08 4.330e-09
50-150 3.519e-08 1.115e-08
15-150 9.532e-08 1.438e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.78484 (-2.4157 1.53915)
R1^2/D10^2 : 3.31607 (-1.64627 10.5958)
kT2 [keV] : 32.7902 (-21.1206 -33.8347)
R2^2/D10^2 : 5.26595E-03 (-0.00460685 0.222114)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.79 using 59 PHA bins.
# Reduced chi-squared = 1.069 for 55 degrees of freedom
# Null hypothesis probability = 3.385871e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.455e-08 6.660e-09
25- 50 3.589e-08 1.126e-08
50-150 4.353e-08 2.393e-08
15-150 1.040e-07 3.538e-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: 1.95906 ( -0.158138 0.164741 )
Norm@50keV : 1.50327E-03 ( -0.00015166 0.000148425 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.09 using 59 PHA bins.
# Reduced chi-squared = 0.8087 for 57 degrees of freedom
# Null hypothesis probability = 8.488510e-01
Photon flux (15-150 keV) in 141.4 sec: 0.221350 ( -0.0180661 0.0180866 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95672e-06 ( -1.87436e-07 1.90295e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87093 ( -0.609746 0.372216 )
Epeak [keV] : 65.5378 ( )
Norm@50keV : 1.68079E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.02 using 59 PHA bins.
# Reduced chi-squared = 0.8218 for 56 degrees of freedom
# Null hypothesis probability = 8.267945e-01
Photon flux (15-150 keV) in 141.4 sec: 0.220330 ( -0.019058 0.018431 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.94079e-06 ( -2.13231e-07 2.03206e-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) = 1.21e-06
S(50-100 keV) = 1.04e-06
T90 vs. Hardness ratio plot
T90 = 167.739999890327 sec.
Hardness ratio (energy fluence ratio) = 0.859504
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.931537
Count Ratio (50-100 keV) / (15-25 keV) = 0.401135
Mask shadow pattern
IMX = -4.050769346816848E-01, IMY = 3.061155258480396E-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:
-239.448000 -105.740000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-105.740000 35.652590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
189.6895 76.6071 0.8 26.9 -142.9 3.9688 15.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
89.652610 962.711300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4200 35.3473 5.0 49.9 -23.5 3.4155 2.3 1.9 Her X-1
227.4583 25.8679 2.6 53.9 8.0 8.4344 4.3 ------ UNKNOWN
272.6815 39.5012 3.1 50.2 -43.2 11.8160 3.8 ------ UNKNOWN
Plot creation:
Thu Mar 21 16:32:30 EDT 2019