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
60.4932 -15.1200 0.0099 35.1842 -38.5996 2.5939648 19.410 TRIG_00748947
Foreground time interval of the image:
0.276 56.909 (delta_t = 56.633 [sec])
Background time interval of the image:
-239.992 0.276 (delta_t = 240.268 [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 0.276 sec. to 87.228 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37166 ( -0.130805 0.130307 )
Norm@50keV : 2.28536E-03 ( -0.000174851 0.000174705 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.33 using 59 PHA bins.
# Reduced chi-squared = 0.9882 for 57 degrees of freedom
# Null hypothesis probability = 5.001910e-01
Photon flux (15-150 keV) in 86.95 sec: 0.276581 ( -0.021701 0.021739 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.93179e-06 ( -1.62045e-07 1.63242e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.276 sec. to 87.228 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.706223 ( -0.637726 0.552629 )
Epeak [keV] : 99.3333 ( -26.4529 205.875 )
Norm@50keV : 4.87690E-03 ( -0.0022378 0.00500094 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.01 using 59 PHA bins.
# Reduced chi-squared = 0.9288 for 56 degrees of freedom
# Null hypothesis probability = 6.264913e-01
Photon flux (15-150 keV) in 86.95 sec: 0.268384 ( -0.022855 0.022802 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.83886e-06 ( -1.80957e-07 1.81316e-07 ) ergs/cm2
Band function
Time interval is from 0.276 sec. to 87.228 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] : 16.2044 (-1.44604 1.63379)
R^2/D10^2 : 2.48974E-02 (-0.00709123 0.00960463)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.31 using 59 PHA bins.
# Reduced chi-squared = 1.304 for 57 degrees of freedom
# Null hypothesis probability = 6.151389e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.172e-07 1.687e-08
25- 50 4.985e-07 5.230e-08
50-150 9.193e-07 1.266e-07
15-150 1.535e-06 1.552e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-29.156 -200)
Norm : 1.14901 (-0.0875761 0.0875761)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.64 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 57 degrees of freedom
# Null hypothesis probability = 4.152339e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.488e-07 2.304e-08
25- 50 4.785e-07 6.295e-08
50-150 1.049e-06 3.873e-07
15-150 1.777e-06 4.191e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.27112 (-3.08501 3.72207)
R1^2/D10^2 : 0.137213 (-0.0836287 0.445891)
kT2 [keV] : 26.3094 (-6.81885 34.1563)
R2^2/D10^2 : 3.57462E-03 (-0.00331359 0.00445953)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.90 using 59 PHA bins.
# Reduced chi-squared = 0.9618 for 55 degrees of freedom
# Null hypothesis probability = 5.552492e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.875e-07 8.602e-08
25- 50 4.915e-07 1.664e-07
50-150 1.158e-06 5.435e-07
15-150 1.837e-06 7.614e-07
Peak spectrum fit
Power-law model
Time interval is from 1.984 sec. to 2.984 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.808829 ( -0.181911 0.173414 )
Norm@50keV : 2.04680E-02 ( -0.00214991 0.0021139 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.50 using 59 PHA bins.
# Reduced chi-squared = 1.132 for 57 degrees of freedom
# Null hypothesis probability = 2.310546e-01
Photon flux (15-150 keV) in 1 sec: 2.35171 ( -0.23927 0.24036 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38325e-07 ( -2.39718e-08 2.40183e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.984 sec. to 2.984 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.800945 ( -0.572752 0.175457 )
Epeak [keV] : 9997.64 ( -9998.23 -9998.23 )
Norm@50keV : 2.05945E-02 ( -0.00201415 0.0143313 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.51 using 59 PHA bins.
# Reduced chi-squared = 1.152 for 56 degrees of freedom
# Null hypothesis probability = 2.035585e-01
Photon flux (15-150 keV) in 1 sec: 2.35490 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.3877e-07 ( -2.82953e-08 2.46144e-08 ) ergs/cm2
Band function
Time interval is from 1.984 sec. to 2.984 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] : 26.5767 (-3.77774 4.87957)
R^2/D10^2 : 4.92198E-02 (-0.0192455 0.0291553)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.81 using 59 PHA bins.
# Reduced chi-squared = 1.488 for 57 degrees of freedom
# Null hypothesis probability = 9.854073e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.841e-09 1.140e-09
25- 50 3.415e-08 5.465e-09
50-150 1.769e-07 2.675e-08
15-150 2.169e-07 3.035e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 ( )
Norm : 9.51578 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 115.14 using 59 PHA bins.
# Reduced chi-squared = 2.0201 for 57 degrees of freedom
# Null hypothesis probability = 8.209186e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.370e-08 1.301e-08
25- 50 4.558e-08 1.919e-08
50-150 9.997e-08 5.505e-08
15-150 1.692e-07 9.290e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 13.7900 (-3.22174 3.81233)
R1^2/D10^2 : 0.258584 (-0.145455 0.217744)
kT2 [keV] : 199.621 (-153.789 -199.621)
R2^2/D10^2 : 4.93615E-04 (-0.000124576 0.00822667)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.85 using 59 PHA bins.
#Fit statistic : Chi-Squared = 61.77 using 59 PHA bins.
# Reduced chi-squared = 1.124 for 55 degrees of freedom
# Reduced chi-squared = 1.123 for 55 degrees of freedom
# Null hypothesis probability = 2.449575e-01
# Null hypothesis probability = 2.469490e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.138e-08 5.762e-09
25- 50 4.318e-08 2.075e-08
50-150 1.821e-07 1.595e-07
15-150 2.367e-07 1.659e-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: 1.32720 ( -0.123425 0.122528 )
Norm@50keV : 2.99471E-03 ( -0.000220341 0.000220284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.24 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 57 degrees of freedom
# Null hypothesis probability = 2.379847e-01
Photon flux (15-150 keV) in 56.63 sec: 0.359129 ( -0.0273014 0.0273522 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66502e-06 ( -1.33529e-07 1.34231e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.362673 ( -0.670157 0.575135 )
Epeak [keV] : 87.0147 ( -17.2343 53.123 )
Norm@50keV : 8.93154E-03 ( -0.00420546 0.00974183 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.31 using 59 PHA bins.
# Reduced chi-squared = 0.9878 for 56 degrees of freedom
# Null hypothesis probability = 5.007759e-01
Photon flux (15-150 keV) in 56.63 sec: 0.344625 ( -0.028765 0.028689 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5557e-06 ( -1.49968e-07 1.50409e-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) = 4.47e-07
S(50-100 keV) = 6.91e-07
T90 vs. Hardness ratio plot
T90 = 65.8559999465942 sec.
Hardness ratio (energy fluence ratio) = 1.54586
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.59182
Count Ratio (50-100 keV) / (15-25 keV) = 1.38149
Mask shadow pattern
IMX = 5.509820165708345E-01, IMY = 4.398373453890435E-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:
-239.992000 0.276000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
316.2088 -53.5929 3.0 52.5 161.8 3.4821 3.8 ------ UNKNOWN
89.9250 -12.8635 2.8 51.4 -3.4 1.7095 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.276000 56.908590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
333.3822 -74.2691 2.7 39.6 137.2 0.8500 4.3 ------ UNKNOWN
89.4393 -21.0057 1.9 44.9 3.2 0.9032 6.0 ------ UNKNOWN
60.4932 -15.1200 0.6 35.2 -38.6 2.5934 19.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
202.508600 302.138000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6028 21.9275 9.8 29.6 -107.0 1.7651 1.2 5.5 Crab
172.2524 43.5636 2.2 46.5 47.9 18.0227 5.3 ------ UNKNOWN
127.4978 39.4218 3.5 13.6 34.4 2.9610 3.3 ------ UNKNOWN
116.2877 0.2826 2.9 29.8 169.5 4.1625 3.9 ------ UNKNOWN
104.9274 -10.0883 4.0 41.4 -173.0 4.2258 2.9 ------ UNKNOWN
86.0805 -16.8578 3.3 54.8 -153.7 15.9539 3.5 ------ UNKNOWN
75.0917 24.9717 3.6 36.0 -96.8 6.7542 3.2 ------ UNKNOWN
75.5424 0.5438 2.7 48.0 -129.1 18.1140 4.3 ------ UNKNOWN
Plot creation:
Wed May 3 17:58:46 EDT 2017