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
150.6470 52.3411 0.0176 5.2311 -58.3355 0.5131218 10.945 TRIG_00727167
Foreground time interval of the image:
32.872 48.748 (delta_t = 15.876 [sec])
Background time interval of the image:
-337.799 -310.156 (delta_t = 27.643 [sec])
-239.000 32.872 (delta_t = 271.872 [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 32.872 sec. to 48.748 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.60255 ( -0.303881 0.348751 )
Norm@50keV : 1.20796E-03 ( -0.000315673 0.000319805 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.63 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 57 degrees of freedom
# Null hypothesis probability = 3.463845e-01
Photon flux (15-150 keV) in 15.88 sec: 0.253067 ( -0.035461 0.035498 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.97657e-07 ( -3.58224e-08 3.79299e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 32.872 sec. to 48.748 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25161 ( -2.08377 1.05805 )
Epeak [keV] : 18.2668 ( -16.7256 10.4402 )
Norm@50keV : 9.49867E-03 ( -0.00949383 0.253715 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.20 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 56 degrees of freedom
# Null hypothesis probability = 3.942713e-01
Photon flux (15-150 keV) in 15.88 sec: 0.246701 ( -0.035077 0.035471 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76946e-07 ( -3.27643e-08 4.03393e-08 ) ergs/cm2
Band function
Time interval is from 32.872 sec. to 48.748 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] : 6.65054 (-0.993543 1.1415)
R^2/D10^2 : 0.597753 (-0.288724 0.58595)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.84 using 59 PHA bins.
# Reduced chi-squared = 1.102 for 57 degrees of freedom
# Null hypothesis probability = 2.771552e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.376e-08 1.492e-08
25- 50 7.890e-08 1.879e-08
50-150 1.082e-08 5.587e-09
15-150 1.535e-07 3.404e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 27.3453 (-7.65856 11.4997)
Norm : 2.22185 (-0.59602 0.904137)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.22 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 57 degrees of freedom
# Null hypothesis probability = 4.303013e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.827e-08 1.249e-08
25- 50 7.397e-08 1.727e-08
50-150 3.575e-08 1.851e-08
15-150 1.780e-07 3.832e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.28800 (-4.31539 2.11422)
R1^2/D10^2 : 2.48220 (-1.82344 -2.42491)
kT2 [keV] : 10.7986 (-10.8767 14.5056)
R2^2/D10^2 : 4.80339E-02 (-0.0457972 0.578959)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.24 using 59 PHA bins.
# Reduced chi-squared = 1.059 for 55 degrees of freedom
# Null hypothesis probability = 3.568954e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.822e-08 3.676e-08
25- 50 7.290e-08 3.652e-08
50-150 3.358e-08 2.045e-08
15-150 1.747e-07 8.591e-08
Peak spectrum fit
Power-law model
Time interval is from 42.644 sec. to 43.644 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.61465 ( -0.60386 0.821776 )
Norm@50keV : 2.04484E-03 ( -0.00114677 0.00124542 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.87 using 59 PHA bins.
# Reduced chi-squared = 1.208 for 57 degrees of freedom
# Null hypothesis probability = 1.347618e-01
Photon flux (15-150 keV) in 1 sec: 0.431724 ( -0.132322 0.133388 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.115e-08 ( -8.35854e-09 9.68543e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 42.644 sec. to 43.644 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.963694 ( )
Epeak [keV] : 18.1091 ( )
Norm@50keV : 3.11054E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.23 using 59 PHA bins.
# Reduced chi-squared = 1.218 for 56 degrees of freedom
# Null hypothesis probability = 1.265387e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 42.644 sec. to 43.644 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] : 5.73343 (-1.68325 2.33703)
R^2/D10^2 : 1.97958 (-1.97899 7.15514)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.83 using 59 PHA bins.
# Reduced chi-squared = 1.208 for 57 degrees of freedom
# Null hypothesis probability = 1.354148e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.076e-09 4.782e-09
25- 50 7.283e-09 4.724e-09
50-150 5.515e-10 5.250e-10
15-150 1.591e-08 9.655e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 23.9328 (-12.0831 29.934)
Norm : 4.35618 (-2.13329 5.31217)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.25 using 59 PHA bins.
# Reduced chi-squared = 1.197 for 57 degrees of freedom
# Null hypothesis probability = 1.461273e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.749e-09 3.886e-09
25- 50 7.719e-09 4.721e-09
50-150 3.076e-09 2.921e-09
15-150 1.855e-08 1.113e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.47134 (-4.53295 3.00936)
R1^2/D10^2 : 4.52517 (-4.34556 -4.34556)
kT2 [keV] : 12.0715 (-12.5334 -12.5334)
R2^2/D10^2 : 3.94424E-02 (-0.0330629 6.59985)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.87 using 59 PHA bins.
# Reduced chi-squared = 1.234 for 55 degrees of freedom
# Null hypothesis probability = 1.140380e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.101e-09 5.140e-09
25- 50 7.232e-09 4.393e-09
50-150 3.468e-09 2.325e-09
15-150 1.880e-08 1.121e-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: 2.60255 ( -0.303881 0.348751 )
Norm@50keV : 1.20796E-03 ( -0.000315673 0.000319805 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.63 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 57 degrees of freedom
# Null hypothesis probability = 3.463845e-01
Photon flux (15-150 keV) in 15.88 sec: 0.253028 ( -0.0354579 0.0354939 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.97604e-07 ( -3.58175e-08 3.79516e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25175 ( -2.08384 0.742875 )
Epeak [keV] : 18.2653 ( -17.0004 10.4397 )
Norm@50keV : 9.49669E-03 ( -0.00949356 0.253722 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.20 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 56 degrees of freedom
# Null hypothesis probability = 3.942713e-01
Photon flux (15-150 keV) in 15.88 sec: 0.246621 ( -0.03506 0.035451 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.7696e-07 ( -3.27514e-08 4.06893e-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) = 6.61e-08
S(50-100 keV) = 4.35e-08
T90 vs. Hardness ratio plot
T90 = 12.0359999537468 sec.
Hardness ratio (energy fluence ratio) = 0.658094
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.824041
Count Ratio (50-100 keV) / (15-25 keV) = 0.212473
Mask shadow pattern
IMX = 4.806145865922342E-02, IMY = 7.792598460053093E-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:
-337.799400 -310.156200
-239.000000 32.872000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
145.0533 8.3375 2.7 45.2 18.1 2.1667 4.3 ------ UNKNOWN
190.8309 19.0228 5.1 50.7 -44.4 3.3269 2.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
32.872000 48.748000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
96.3441 72.6348 2.5 27.0 174.0 0.2347 4.6 ------ UNKNOWN
150.6470 52.3411 1.1 5.2 -58.3 0.5131 10.9 ------ UNKNOWN
171.0804 3.5523 2.7 55.3 -13.8 0.6445 4.3 ------ UNKNOWN
190.5354 73.1688 2.6 27.9 -130.3 0.2367 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
143.500600 963.057200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
137.4926 31.7778 2.1 22.7 34.3 2.7777 5.4 ------ UNKNOWN
228.0095 76.2493 2.9 36.8 -152.9 3.0294 4.0 ------ UNKNOWN
183.6172 51.0590 3.7 20.3 -95.2 1.7358 3.1 ------ UNKNOWN
187.0670 11.1130 3.3 50.6 -44.6 11.4465 3.5 ------ UNKNOWN
Plot creation:
Thu Jan 5 10:40:15 EST 2017