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
165.4075 56.4790 0.0023 8.8308 79.2831 14.2750048 83.082 TRIG_00758766
Foreground time interval of the image:
-21.344 15.701 (delta_t = 37.045 [sec])
Background time interval of the image:
-240.099 -21.344 (delta_t = 218.755 [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 -21.344 sec. to 17.924 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60178 ( -0.0331262 0.0331147 )
Norm@50keV : 2.28323E-02 ( -0.00038966 0.000389639 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.82 using 59 PHA bins.
# Reduced chi-squared = 1.225 for 57 degrees of freedom
# Null hypothesis probability = 1.184757e-01
Photon flux (15-150 keV) in 39.27 sec: 2.93577 ( -0.05974 0.05998 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.38477e-06 ( -1.45273e-07 1.45067e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -21.344 sec. to 17.924 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25611 ( -0.143289 0.138998 )
Epeak [keV] : 120.873 ( -19.6144 42.5142 )
Norm@50keV : 3.24975E-02 ( -0.00420155 0.00498245 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.11 using 59 PHA bins.
# Reduced chi-squared = 0.9127 for 56 degrees of freedom
# Null hypothesis probability = 6.599583e-01
Photon flux (15-150 keV) in 39.27 sec: 2.84426 ( -0.06837 0.06882 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.18882e-06 ( -1.64447e-07 1.64154e-07 ) ergs/cm2
Band function
Time interval is from -21.344 sec. to 17.924 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] : 16.5866 ( )
R^2/D10^2 : 0.216786 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 643.73 using 59 PHA bins.
# Reduced chi-squared = 11.294 for 57 degrees of freedom
# Null hypothesis probability = 2.861246e-100
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.801e-07 1.669e-08
25- 50 2.082e-06 4.968e-08
50-150 4.057e-06 1.194e-07
15-150 6.619e-06 1.296e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.527 (-18.5904 -198.534)
Norm : 11.7341 (-0.204589 0.242482)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.72 using 59 PHA bins.
# Reduced chi-squared = 0.8898 for 57 degrees of freedom
# Null hypothesis probability = 7.081782e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.148e-06 2.297e-08
25- 50 2.207e-06 4.673e-08
50-150 4.835e-06 9.228e-08
15-150 8.190e-06 1.689e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.97525 (-0.552788 0.57819)
R1^2/D10^2 : 1.87753 (-0.385953 0.520271)
kT2 [keV] : 27.6554 (-1.87382 2.30689)
R2^2/D10^2 : 2.72438E-02 (-0.00704604 0.00837826)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.34 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 55 degrees of freedom
# Null hypothesis probability = 3.885146e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.805e-07 6.597e-08
25- 50 2.273e-06 7.383e-08
50-150 4.827e-06 1.944e-07
15-150 8.080e-06 2.847e-07
Peak spectrum fit
Power-law model
Time interval is from -0.064 sec. to 0.936 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28424 ( -0.0376994 0.0376683 )
Norm@50keV : 0.198390 ( -0.00435274 0.00435231 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 101.13 using 59 PHA bins.
# Reduced chi-squared = 1.7742 for 57 degrees of freedom
# Null hypothesis probability = 2.877827e-04
Photon flux (15-150 keV) in 1 sec: 0.638909 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.96834e-06 ( -4.57353e-08 4.58016e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.064 sec. to 0.936 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.574078 ( -0.17846 0.171915 )
Epeak [keV] : 113.944 ( -12.1454 18.603 )
Norm@50keV : 0.412998 ( -0.0655989 0.0811096 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.93 using 59 PHA bins.
# Reduced chi-squared = 0.8201 for 56 degrees of freedom
# Null hypothesis probability = 8.293732e-01
Photon flux (15-150 keV) in 1 sec: 22.7767 ( -0.577 0.5783 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90818e-06 ( -4.89205e-08 4.88163e-08 ) ergs/cm2
Band function
Time interval is from -0.064 sec. to 0.936 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] : 18.6297 ( )
R^2/D10^2 : 1.37222 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 285.92 using 59 PHA bins.
# Reduced chi-squared = 5.0161 for 57 degrees of freedom
# Null hypothesis probability = 3.278501e-32
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.427e-08 4.040e-09
25- 50 4.471e-07 1.315e-08
50-150 1.136e-06 3.750e-08
15-150 1.677e-06 4.100e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 99.8220 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 226.60 using 59 PHA bins.
# Reduced chi-squared = 3.9754 for 57 degrees of freedom
# Null hypothesis probability = 4.430286e-22
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.486e-07 5.750e-09
25- 50 4.782e-07 1.085e-08
50-150 1.049e-06 2.250e-08
15-150 1.775e-06 4.100e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.2002 (-1.11413 1.15446)
R1^2/D10^2 : 5.92688 (-1.36412 2.04498)
kT2 [keV] : 32.5428 (-3.88439 6.04626)
R2^2/D10^2 : 0.152469 (-0.0689748 0.0934832)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.06 using 59 PHA bins.
# Reduced chi-squared = 0.8011 for 55 degrees of freedom
# Null hypothesis probability = 8.547604e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.504e-07 1.210e-08
25- 50 4.759e-07 2.720e-08
50-150 1.281e-06 1.577e-07
15-150 1.907e-06 1.455e-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: 1.59686 ( -0.0327946 0.0327803 )
Norm@50keV : 2.41256E-02 ( -0.000408653 0.000408626 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.50 using 59 PHA bins.
# Reduced chi-squared = 1.149 for 57 degrees of freedom
# Null hypothesis probability = 2.057152e-01
Photon flux (15-150 keV) in 37.04 sec: 3.09723 ( -0.062636 0.0628799 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.36037e-06 ( -1.43474e-07 1.43518e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25618 ( -0.141571 0.137383 )
Epeak [keV] : 123.049 ( -20.2047 43.9684 )
Norm@50keV : 3.41308E-02 ( -0.00435364 0.00514973 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.91 using 59 PHA bins.
# Reduced chi-squared = 0.8377 for 56 degrees of freedom
# Null hypothesis probability = 8.013330e-01
Photon flux (15-150 keV) in 37.04 sec: 3.00188 ( -0.07153 0.07202 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.17506e-06 ( -1.62235e-07 1.61717e-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) = 2.18e-06
S(50-100 keV) = 2.87e-06
T90 vs. Hardness ratio plot
T90 = 12.9479999542236 sec.
Hardness ratio (energy fluence ratio) = 1.31651
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39759
Count Ratio (50-100 keV) / (15-25 keV) = 0.971907
Mask shadow pattern
IMX = 2.889018277273836E-02, IMY = -1.526496343074728E-01
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:
-240.099410 -21.344000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
265.2522 71.2651 2.3 46.1 31.4 2.8585 5.1 ------ UNKNOWN
125.3249 28.3420 3.1 31.8 -127.9 1.2219 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-21.344000 15.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
165.0868 13.6807 2.1 42.6 165.9 1.7382 5.5 ------ UNKNOWN
165.4075 56.4790 0.1 8.8 79.3 14.2749 83.1 ------ UNKNOWN
87.8512 46.1226 2.7 39.2 -68.2 2.1054 4.3 ------ UNKNOWN
117.0800 19.1761 2.7 43.4 -123.9 2.2811 4.2 ------ UNKNOWN
85.2929 43.3271 2.4 42.4 -69.9 3.8926 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
47.500600 962.696700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
217.2132 34.8456 3.0 40.9 102.5 10.0515 3.8 ------ UNKNOWN
231.4073 48.5532 3.1 39.3 75.6 9.7066 3.7 ------ UNKNOWN
196.9263 17.0984 2.6 46.0 139.0 11.7826 4.4 ------ UNKNOWN
146.6283 77.1041 3.5 21.7 -8.1 2.2116 3.3 ------ UNKNOWN
134.2814 71.1746 2.9 19.7 -26.6 2.5391 4.0 ------ UNKNOWN
Plot creation:
Mon Jul 10 16:31:16 EDT 2017