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
174.8679 18.8815 0.0207 35.8443 2.3629 0.9408097 9.299 TRIG_00883818
Foreground time interval of the image:
-1.164 27.900 (delta_t = 29.064 [sec])
Background time interval of the image:
-239.336 -1.164 (delta_t = 238.172 [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 -1.164 sec. to 27.900 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97693 ( -0.272865 0.293731 )
Norm@50keV : 1.91405E-03 ( -0.00037894 0.000367713 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.72 using 59 PHA bins.
# Reduced chi-squared = 0.9599 for 57 degrees of freedom
# Null hypothesis probability = 5.612851e-01
Photon flux (15-150 keV) in 29.06 sec: 0.284124 ( -0.042406 0.042407 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12467e-07 ( -9.42178e-08 9.76393e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.164 sec. to 27.900 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32448 ( -2.69269 0.818616 )
Epeak [keV] : 39.2310 ( -36.1731 -39.1694 )
Norm@50keV : 4.83357E-03 ( -0.00491556 0.263807 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.12 using 59 PHA bins.
# Reduced chi-squared = 0.9664 for 56 degrees of freedom
# Null hypothesis probability = 5.464953e-01
Photon flux (15-150 keV) in 29.06 sec: 0.277288 ( -0.046203 0.045038 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.67041e-07 ( -1.24781e-07 1.26644e-07 ) ergs/cm2
Band function
Time interval is from -1.164 sec. to 27.900 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] : 8.83387 (-1.28067 1.54299)
R^2/D10^2 : 0.216824 (-0.101554 0.183079)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.24 using 59 PHA bins.
# Reduced chi-squared = 1.004 for 57 degrees of freedom
# Null hypothesis probability = 4.660455e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.479e-08 2.381e-08
25- 50 1.956e-07 4.738e-08
50-150 7.047e-08 3.044e-08
15-150 3.609e-07 8.023e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 61.7582 (-22.9818 49.8641)
Norm : 1.47487 (-0.335659 0.449011)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.06 using 59 PHA bins.
# Reduced chi-squared = 0.9485 for 57 degrees of freedom
# Null hypothesis probability = 5.859981e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.082e-07 2.100e-08
25- 50 1.661e-07 3.271e-08
50-150 1.936e-07 8.377e-08
15-150 4.679e-07 1.096e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.66453 (-1.38522 1.68159)
R1^2/D10^2 : 0.340959 (-0.161694 0.387606)
kT2 [keV] : 55.7694 (-51.7863 -72.5108)
R2^2/D10^2 : 2.27081E-04 (-0.000121771 0.00396684)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.80 using 59 PHA bins.
# Reduced chi-squared = 0.9055 for 55 degrees of freedom
# Null hypothesis probability = 6.729472e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.038e-07 3.861e-08
25- 50 1.803e-07 6.985e-08
50-150 2.431e-07 1.381e-07
15-150 5.272e-07 1.864e-07
Peak spectrum fit
Power-law model
Time interval is from 3.624 sec. to 4.624 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.00433 ( -1.03696 1.3614 )
Norm@50keV : 3.55813E-03 ( -0.00355692 0.00208544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.73 using 59 PHA bins.
# Reduced chi-squared = 1.065 for 57 degrees of freedom
# Null hypothesis probability = 3.431013e-01
Photon flux (15-150 keV) in 1 sec: 0.534821 ( -0.231008 0.23098 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.28148e-08 ( -1.82095e-08 2.05457e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.624 sec. to 4.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.10573 ( -2.10575 0.900979 )
Epeak [keV] : 44.4878 ( )
Norm@50keV : 2.75659E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.46 using 59 PHA bins.
# Reduced chi-squared = 1.080 for 56 degrees of freedom
# Null hypothesis probability = 3.178922e-01
Photon flux (15-150 keV) in 1 sec: 0.475655 ( -0.475655 0.28638 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 3.624 sec. to 4.624 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] : 5.93491 (-2.24917 4.25007)
R^2/D10^2 : 1.88348 (-1.88348 13.9162)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.44 using 59 PHA bins.
# Reduced chi-squared = 1.095 for 57 degrees of freedom
# Null hypothesis probability = 2.891786e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.676e-09 5.495e-09
25- 50 8.448e-09 5.705e-09
50-150 7.397e-10 7.190e-10
15-150 1.787e-08 1.184e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 72.7090 (-75.8231 -75.8231)
Norm : 2.50652 (-1.29552 11.4664)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.76 using 59 PHA bins.
# Reduced chi-squared = 1.084 for 57 degrees of freedom
# Null hypothesis probability = 3.099257e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.455e-09 4.471e-09
25- 50 1.037e-08 6.770e-09
50-150 1.370e-08 1.310e-08
15-150 3.053e-08 2.244e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.35665 (-2.18124 1.96621)
R1^2/D10^2 : 2.68260 (-2.27494 25.6449)
kT2 [keV] : 84.8824 (-161.042 -183.027)
R2^2/D10^2 : 3.67566E-04 (-8.38342e-05 0.0102177)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.48 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 55 degrees of freedom
# Null hypothesis probability = 3.834173e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.714e-09 5.515e-09
25- 50 8.051e-09 5.085e-09
50-150 2.704e-08 1.540e-08
15-150 4.380e-08 2.382e-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: 1.97693 ( -0.272865 0.293731 )
Norm@50keV : 1.91405E-03 ( -0.00037894 0.000367713 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.72 using 59 PHA bins.
# Reduced chi-squared = 0.9599 for 57 degrees of freedom
# Null hypothesis probability = 5.612851e-01
Photon flux (15-150 keV) in 29.06 sec: 0.284104 ( -0.0424034 0.0424035 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12377e-07 ( -9.41285e-08 9.76788e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32666 ( -2.69413 0.817242 )
Epeak [keV] : 39.2459 ( )
Norm@50keV : 4.81791E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.12 using 59 PHA bins.
# Reduced chi-squared = 0.9664 for 56 degrees of freedom
# Null hypothesis probability = 5.464997e-01
Photon flux (15-150 keV) in 29.06 sec: 0.277153 ( -0.046133 0.045091 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.67049e-07 ( -1.24897e-07 1.31188e-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) = 1.53e-07
S(50-100 keV) = 1.56e-07
T90 vs. Hardness ratio plot
T90 = 26.4919999837875 sec.
Hardness ratio (energy fluence ratio) = 1.01961
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.3651
Count Ratio (50-100 keV) / (15-25 keV) = 0.46196
Mask shadow pattern
IMX = 7.217858374019105E-01, IMY = -2.978403258128292E-02
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:
-239.336000 -1.164000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
41.0282 61.3932 2.5 55.9 -178.3 5.1531 4.5 ------ UNKNOWN
174.0115 32.8705 2.9 22.7 -8.0 0.9473 4.0 ------ UNKNOWN
180.6633 32.6107 2.4 26.0 -19.1 1.2548 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.164000 27.900000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
174.8681 18.8814 1.2 35.8 2.4 0.9520 9.4 ------ UNKNOWN
131.3818 68.8508 2.2 20.9 -172.0 0.3915 5.3 ------ UNKNOWN
181.6292 14.3285 2.1 42.5 -4.6 0.6392 5.4 ------ UNKNOWN
148.7744 69.5958 2.3 18.3 -155.2 0.3558 5.0 ------ UNKNOWN
187.6714 11.7017 1.9 47.3 -10.6 0.7837 6.1 ------ UNKNOWN
181.3797 51.6652 2.4 15.5 -66.8 0.3612 4.8 ------ UNKNOWN
27.3035 64.0473 2.3 57.7 -170.5 2.0904 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
141.164620 962.714000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
144.1040 -3.4900 3.1 37.7 43.7 4.4730 3.7 ------ UNKNOWN
235.2149 52.5725 3.9 57.2 -154.1 14.8196 3.0 ------ UNKNOWN
Plot creation:
Thu Mar 21 14:26:18 EDT 2019