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
336.6046 -41.1846 0.0218 10.1330 25.6601 0.5484048 8.823 TRIG_00915091
Foreground time interval of the image:
0.568 17.669 (delta_t = 17.101 [sec])
Background time interval of the image:
-58.331 0.568 (delta_t = 58.899 [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 0.512000
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 0.512000
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 0.512000
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 0.568 sec. to 720.568 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50000 ( -1.5 -1.5 )
Norm@50keV : 0.0 ( 0 4.25539e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.39 using 59 PHA bins.
# Reduced chi-squared = 1.235 for 57 degrees of freedom
# Null hypothesis probability = 1.095918e-01
Photon flux (15-150 keV) in 720 sec: 4.29911E-12 ( -4.29911e-12 0.00363074 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.20828e-28 ( 720 -6.62195e-31 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.568 sec. to 720.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.94279 ( )
Epeak [keV] : 44.5214 ( )
Norm@50keV : 43.4657 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.50 using 59 PHA bins.
# Reduced chi-squared = 1.223 for 56 degrees of freedom
# Null hypothesis probability = 1.219986e-01
Photon flux (15-150 keV) in 720 sec: 3.05994E-03 ( -0.00305994 0.00465684 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.43963e-07 ( 720 2.073e-07 ) ergs/cm2
Band function
Time interval is from 0.568 sec. to 720.568 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] : 5.00000 (-5 -5)
R^2/D10^2 : 0.0 (0 0)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.39 using 59 PHA bins.
# Reduced chi-squared = 1.235 for 57 degrees of freedom
# Null hypothesis probability = 1.095918e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.00000 (-7 -7)
Norm : 0.0 (0 0)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.39 using 59 PHA bins.
# Reduced chi-squared = 1.235 for 57 degrees of freedom
# Null hypothesis probability = 1.095918e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.63509E-02 (-0.0863509 -0.0863509)
R1^2/D10^2 : 1.16411E-05 (-1.15918e-05 -1.15918e-05)
kT2 [keV] : 11.6504 (-11.4614 -11.4614)
R2^2/D10^2 : 8.91501E-04 (-0.000946209 -0.000946209)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.62 using 59 PHA bins.
# Reduced chi-squared = 1.266 for 55 degrees of freedom
# Null hypothesis probability = 8.869117e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Peak spectrum fit
Power-law model
Time interval is from 8.068 sec. to 9.068 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.349481 ( -0.349445 1.30807 )
Norm@50keV : 1.92630E-03 ( -0.00192626 0.00145322 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.99 using 59 PHA bins.
# Reduced chi-squared = 1.017 for 57 degrees of freedom
# Null hypothesis probability = 4.387097e-01
Photon flux (15-150 keV) in 1 sec: 0.234900 ( -0.2349 0.152951 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.80175e-08 ( -1.53928e-08 1.53845e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.068 sec. to 9.068 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.324650 ( )
Epeak [keV] : 9971.57 ( )
Norm@50keV : 1.93272E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.99 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 56 degrees of freedom
# Null hypothesis probability = 4.019434e-01
Photon flux (15-150 keV) in 1 sec: 0.226563 ( -0.226563 0.155392 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.50738e-08 ( -1.30926e-08 1.7271e-08 ) ergs/cm2
Band function
Time interval is from 8.068 sec. to 9.068 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] : 43.8500 (-44.0874 -44.0874)
R^2/D10^2 : 1.47365E-03 (-0.00146129 0.00939976)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.82 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.447871e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.878e-09 2.091e-09
25- 50 1.838e-09 1.579e-09
50-150 7.152e-11 1.185e-10
15-150 4.788e-09 3.927e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 0.990819 (-0.636257 0.636257)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.68 using 59 PHA bins.
# Reduced chi-squared = 1.065 for 57 degrees of freedom
# Null hypothesis probability = 3.446811e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.467e-09 1.922e-09
25- 50 4.746e-09 3.389e-09
50-150 1.041e-08 7.410e-09
15-150 1.762e-08 1.251e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.96125 (-3.93333 137.662)
R1^2/D10^2 : 2.68088 (-2.72135 3.12579e+06)
kT2 [keV] : 51.1199 (-28.3195 -51.0847)
R2^2/D10^2 : 9.86377E-04 (-0.000941198 0.00389341)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.29 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 55 degrees of freedom
# Null hypothesis probability = 4.264301e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.602e-09 1.668e-09
25- 50 2.825e-09 1.368e-09
50-150 2.509e-08 1.499e-08
15-150 3.052e-08 1.696e-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: 1.51020 ( -0.309037 0.318251 )
Norm@50keV : 1.72292E-03 ( -0.000336905 0.000330455 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.08 using 59 PHA bins.
# Reduced chi-squared = 0.8259 for 57 degrees of freedom
# Null hypothesis probability = 8.228293e-01
Photon flux (15-150 keV) in 17.1 sec: 0.215683 ( -0.0390171 0.0390306 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.79031e-07 ( -5.9272e-08 6.09381e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.928057 ( -1.62016 1.27969 )
Epeak [keV] : 85.0646 ( )
Norm@50keV : 3.55984E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.45 using 59 PHA bins.
# Reduced chi-squared = 0.8295 for 56 degrees of freedom
# Null hypothesis probability = 8.146783e-01
Photon flux (15-150 keV) in 17.1 sec: 0.211138 ( -0.040352 0.040226 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.63605e-07 ( -6.60539e-08 6.89609e-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) = 7.20e-28
S(50-100 keV) = 7.20e-28
T90 vs. Hardness ratio plot
T90 = 704 sec.
Hardness ratio (energy fluence ratio) = 1
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = -2.97829
Count Ratio (50-100 keV) / (15-25 keV) = 1.1714
Mask shadow pattern
IMX = 1.610953789587414E-01, IMY = -7.739188991114443E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-58.331410 0.568000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
265.8008 -81.3761 2.4 55.8 2.9 2.8084 4.9 ------ UNKNOWN
352.5788 -38.2587 2.5 8.9 -57.5 0.6270 4.6 ------ UNKNOWN
354.0227 -1.1510 2.9 33.1 -168.6 0.6939 4.1 365.2 UNKNOWN
7.9273 20.5100 2.4 58.1 -160.6 4.1824 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.568000 17.668600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
310.2743 -7.4639 2.0 40.2 114.4 1.5260 5.8 ------ UNKNOWN
312.8573 -12.4551 1.9 35.0 111.1 0.9284 5.9 ------ UNKNOWN
314.3789 -65.8334 1.8 37.4 12.1 0.6154 6.5 ------ UNKNOWN
336.6042 -41.1847 1.3 10.1 25.7 0.5497 8.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
50.268600 962.687700
1244.568000 1385.944700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
347.5151 14.1702 2.7 56.3 173.8 55.4093 4.2 ------ UNKNOWN
348.6581 10.7127 2.6 53.1 175.9 46.1055 4.5 ------ UNKNOWN
Plot creation:
Thu Aug 15 14:50:01 EDT 2019