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
347.7070 4.8739 0.0150 5.1529 -177.8834 0.6553221 12.852 TRIG_00849018
Foreground time interval of the image:
-0.392 19.605 (delta_t = 19.997 [sec])
Background time interval of the image:
-239.696 -0.392 (delta_t = 239.304 [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 1.024000
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 1.024000
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 1.024000
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 -0.392 sec. to 48.916 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25642 ( -0.224546 0.221323 )
Norm@50keV : 1.20549E-03 ( -0.000156342 0.00015608 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.53 using 59 PHA bins.
# Reduced chi-squared = 0.9217 for 57 degrees of freedom
# Null hypothesis probability = 6.430922e-01
Photon flux (15-150 keV) in 49.31 sec: 0.142728 ( -0.018802 0.018835 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.93969e-07 ( -8.59902e-08 8.69966e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.392 sec. to 48.916 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.756874 ( -1.09284 0.670011 )
Epeak [keV] : 127.875 ( -57.2748 -127.874 )
Norm@50keV : 2.12987E-03 ( -0.00104658 0.00502338 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.61 using 59 PHA bins.
# Reduced chi-squared = 0.9217 for 56 degrees of freedom
# Null hypothesis probability = 6.414416e-01
Photon flux (15-150 keV) in 49.31 sec: 0.139783 ( -0.019659 0.01956 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71365e-07 ( -9.66915e-08 9.57723e-08 ) ergs/cm2
Band function
Time interval is from -0.392 sec. to 48.916 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] : 16.8848 (-2.58101 3.27357)
R^2/D10^2 : 1.13853E-02 (-0.00512558 0.00865235)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.07 using 59 PHA bins.
# Reduced chi-squared = 1.054 for 57 degrees of freedom
# Null hypothesis probability = 3.650655e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.266e-08 8.343e-09
25- 50 1.437e-07 2.796e-08
50-150 2.919e-07 7.811e-08
15-150 4.683e-07 8.516e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-47.3433 -200)
Norm : 0.588814 (-0.0769889 0.0769889)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.43 using 59 PHA bins.
# Reduced chi-squared = 0.9900 for 57 degrees of freedom
# Null hypothesis probability = 4.965011e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.230e-08 4.048e-08
25- 50 1.391e-07 7.823e-08
50-150 3.050e-07 1.681e-07
15-150 5.164e-07 2.830e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.4894 (-6.17588 4.29381)
R1^2/D10^2 : 3.84104E-02 (-0.0225195 0.432214)
kT2 [keV] : 40.2650 (-23.184 -42.662)
R2^2/D10^2 : 4.67280E-04 (-0.000370896 0.00603322)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.64 using 59 PHA bins.
# Reduced chi-squared = 0.9390 for 55 degrees of freedom
# Null hypothesis probability = 6.037055e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.786e-08 2.751e-08
25- 50 1.472e-07 8.336e-08
50-150 3.844e-07 2.041e-07
15-150 5.794e-07 2.882e-07
Peak spectrum fit
Power-law model
Time interval is from 1.816 sec. to 2.816 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20735 ( -0.268923 0.26328 )
Norm@50keV : 7.49900E-03 ( -0.00118294 0.0011808 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.15 using 59 PHA bins.
# Reduced chi-squared = 1.020 for 57 degrees of freedom
# Null hypothesis probability = 4.328866e-01
Photon flux (15-150 keV) in 1 sec: 0.881153 ( -0.140406 0.140597 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.59329e-08 ( -1.34228e-08 1.36139e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.816 sec. to 2.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.636364 ( -1.46262 0.911124 )
Epeak [keV] : 120.411 ( -56.6719 -120.427 )
Norm@50keV : 1.45716E-02 ( -0.00802312 0.0650766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.33 using 59 PHA bins.
# Reduced chi-squared = 1.024 for 56 degrees of freedom
# Null hypothesis probability = 4.254969e-01
Photon flux (15-150 keV) in 1 sec: 0.863229 ( -0.146032 0.144891 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24303e-08 ( -1.56523e-08 1.51467e-08 ) ergs/cm2
Band function
Time interval is from 1.816 sec. to 2.816 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] : 16.2160 (-2.8721 3.95319)
R^2/D10^2 : 8.18963E-02 (-0.0427025 0.0771314)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.18 using 59 PHA bins.
# Reduced chi-squared = 1.091 for 57 degrees of freedom
# Null hypothesis probability = 2.970374e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.439e-09 1.494e-09
25- 50 1.889e-08 4.835e-09
50-150 3.490e-08 1.158e-08
15-150 5.823e-08 1.557e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-56.7546 -200)
Norm : 3.60630 (-0.576594 0.576594)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.81 using 59 PHA bins.
# Reduced chi-squared = 1.084 for 57 degrees of freedom
# Null hypothesis probability = 3.082543e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.980e-09 5.140e-09
25- 50 1.727e-08 9.800e-09
50-150 3.788e-08 2.144e-08
15-150 6.414e-08 3.591e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.5792 (-3.59991 4.0753)
R1^2/D10^2 : 0.197089 (-0.112512 0.204329)
kT2 [keV] : 65.9151 (-44.9051 -68.9007)
R2^2/D10^2 : 8.08142E-04 (-0.000677583 0.0156935)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.30 using 59 PHA bins.
#Fit statistic : Chi-Squared = 55.22 using 59 PHA bins.
# Reduced chi-squared = 1.005 for 55 degrees of freedom
# Reduced chi-squared = 1.004 for 55 degrees of freedom
# Null hypothesis probability = 4.634694e-01
# Null hypothesis probability = 4.664731e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.956e-09 3.411e-09
25- 50 1.901e-08 1.074e-08
50-150 4.949e-08 2.644e-08
15-150 7.445e-08 3.693e-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: 1.26637 ( -0.207871 0.206028 )
Norm@50keV : 2.12065E-03 ( -0.000250774 0.000250261 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.32 using 59 PHA bins.
# Reduced chi-squared = 1.199 for 57 degrees of freedom
# Null hypothesis probability = 1.448695e-01
Photon flux (15-150 keV) in 20 sec: 0.251498 ( -0.0301837 0.0302325 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.22666e-07 ( -5.60824e-08 5.67098e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.914680 ( -0.963261 0.457145 )
Epeak [keV] : 161.046 ( -161.046 -161.046 )
Norm@50keV : 3.14924E-03 ( -0.00258991 0.00589466 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.77 using 59 PHA bins.
# Reduced chi-squared = 1.210 for 56 degrees of freedom
# Null hypothesis probability = 1.346351e-01
Photon flux (15-150 keV) in 20 sec: 0.247617 ( -0.031632 0.03147 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.12046e-07 ( -6.2566e-08 6.1772e-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) = 1.29e-07
S(50-100 keV) = 2.16e-07
T90 vs. Hardness ratio plot
T90 = 47.6000000238419 sec.
Hardness ratio (energy fluence ratio) = 1.67442
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.85998
Count Ratio (50-100 keV) / (15-25 keV) = 1.47902
Mask shadow pattern
IMX = -9.011741394393637E-02, IMY = 3.330606477325693E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.696000 -0.392000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0482 40.9491 8.5 55.6 168.8 -1.6915 -1.4 2.8 Cyg X-3
326.0775 38.4459 3.4 44.0 179.4 -1.4493 -3.4 8.7 Cyg X-2
3.2584 -42.9055 2.5 44.7 12.4 1.8085 4.7 ------ UNKNOWN
359.2477 -9.5791 2.5 13.5 -17.2 0.9766 4.7 576.5 UNKNOWN
20.4249 -38.0211 2.5 47.5 -6.6 1.7428 4.5 ------ UNKNOWN
32.2938 -42.9078 3.3 57.4 -9.5 3.7520 3.5 ------ UNKNOWN
12.2930 11.9418 3.1 25.2 -92.3 1.0664 3.7 ------ UNKNOWN
27.3883 -20.3829 3.0 42.1 -32.1 1.2855 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.392000 19.604590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1681 41.0447 73.3 55.6 168.9 -0.0497 -0.2 6.1 Cyg X-3
326.0227 38.3941 7.1 44.0 179.3 0.1601 1.6 8.2 Cyg X-2
347.7071 4.8739 0.9 5.2 -177.9 0.6552 12.8 ------ UNKNOWN
12.6728 45.5359 3.1 49.6 -132.7 1.0039 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
43.204590 96.044000
97.304000 962.452000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7034 35.0803 13.4 53.5 161.5 3.0618 0.9 9.2 Cyg X-1
308.0451 40.8810 5.7 50.5 171.9 4.4478 2.0 5.2 Cyg X-3
326.2305 38.3436 6.3 38.7 -176.7 1.6941 1.8 3.1 Cyg X-2
342.0786 -39.6582 3.5 44.8 36.8 5.8670 3.3 ------ UNKNOWN
343.3238 -11.2713 2.4 16.7 45.7 3.1225 4.9 ------ UNKNOWN
316.2732 40.0811 2.6 45.2 176.4 6.1715 4.4 ------ UNKNOWN
309.4217 45.4984 3.0 52.5 177.4 8.9307 3.9 ------ UNKNOWN
314.8907 44.4172 2.8 48.9 179.7 6.4585 4.1 ------ UNKNOWN
26.9699 -31.3103 3.9 52.1 -12.7 4.6390 3.0 ------ UNKNOWN
23.4218 28.2403 5.4 41.2 -98.0 7.3919 2.2 ------ UNKNOWN
Plot creation:
Mon Aug 6 22:26:16 EDT 2018