Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
350.8588 -47.4828 0.0161 3.3436 -179.8910 0.3680266 11.800 TRIG_00727610
Foreground time interval of the image:
-3.428 4.464 (delta_t = 7.892 [sec])
Background time interval of the image:
-576.183 -559.744 (delta_t = 16.439 [sec])
-239.584 -3.428 (delta_t = 236.156 [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 2.048000
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 2.048000
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 2.048000
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 -3.428 sec. to 4.464 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.01424 ( -0.241764 0.261935 )
Norm@50keV : 2.52918E-03 ( -0.000457764 0.000445284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.99 using 59 PHA bins.
# Reduced chi-squared = 1.386 for 57 degrees of freedom
# Null hypothesis probability = 2.856032e-02
Photon flux (15-150 keV) in 7.892 sec: 0.381912 ( -0.05057 0.050572 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8425e-07 ( -3.05735e-08 3.15928e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.428 sec. to 4.464 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38797 ( -1.09426 0.754358 )
Epeak [keV] : 39.5104 ( )
Norm@50keV : 5.95041E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.58 using 59 PHA bins.
# Reduced chi-squared = 1.385 for 56 degrees of freedom
# Null hypothesis probability = 2.972149e-02
Photon flux (15-150 keV) in 7.892 sec: 0.374994 ( -0.051105 0.051316 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72821e-07 ( -3.22144e-08 3.50129e-08 ) ergs/cm2
Band function
Time interval is from -3.428 sec. to 4.464 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] : 9.25675 (-1.56961 1.91855)
R^2/D10^2 : 0.238079 (-0.237368 0.247612)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 90.79 using 59 PHA bins.
# Reduced chi-squared = 1.593 for 57 degrees of freedom
# Null hypothesis probability = 2.948871e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.178e-08 7.198e-09
25- 50 7.055e-08 1.357e-08
50-150 2.931e-08 1.156e-08
15-150 1.316e-07 2.600e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 62.5316 (-20.6951 38.3687)
Norm : 1.97728 (-0.389085 0.491202)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.60 using 59 PHA bins.
# Reduced chi-squared = 1.361 for 57 degrees of freedom
# Null hypothesis probability = 3.615184e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.947e-08 7.245e-09
25- 50 6.082e-08 9.991e-09
50-150 7.159e-08 2.863e-08
15-150 1.719e-07 3.776e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.16596 (-1.43206 1.6374)
R1^2/D10^2 : 1.56484 (-0.99908 4.10094)
kT2 [keV] : 17.6369 (-4.69371 8.35473)
R2^2/D10^2 : 1.46809E-02 (-0.0113268 0.0232885)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.46 using 59 PHA bins.
# Reduced chi-squared = 1.372 for 55 degrees of freedom
# Null hypothesis probability = 3.494570e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.143e-08 2.271e-08
25- 50 5.723e-08 2.854e-08
50-150 7.541e-08 4.522e-08
15-150 1.741e-07 9.076e-08
Peak spectrum fit
Power-law model
Time interval is from 2.420 sec. to 3.420 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.17406 ( -0.488602 0.595524 )
Norm@50keV : 3.47182E-03 ( -0.00138059 0.00130721 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.72 using 59 PHA bins.
# Reduced chi-squared = 1.293 for 57 degrees of freedom
# Null hypothesis probability = 6.739804e-02
Photon flux (15-150 keV) in 1 sec: 0.567101 ( -0.140719 0.14086 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.25349e-08 ( -1.05649e-08 1.14071e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.420 sec. to 3.420 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.18098 ( -1.58849 1.00007 )
Epeak [keV] : 273.931 ( )
Norm@50keV : 3.39289E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.70 using 59 PHA bins.
# Reduced chi-squared = 1.316 for 56 degrees of freedom
# Null hypothesis probability = 5.653754e-02
Photon flux (15-150 keV) in 1 sec: 0.560628 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 2.420 sec. to 3.420 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] : 6.22105 (-1.7128 2.90007)
R^2/D10^2 : 1.64724 (-1.6404 4.90481)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.35 using 59 PHA bins.
# Reduced chi-squared = 1.392 for 57 degrees of freedom
# Null hypothesis probability = 2.681260e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.906e-09 5.410e-09
25- 50 9.600e-09 5.786e-09
50-150 1.017e-09 8.985e-10
15-150 1.952e-08 1.216e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 48.5729 (-27.539 98.6681)
Norm : 3.25045 (-1.2255 2.83274)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.90 using 59 PHA bins.
# Reduced chi-squared = 1.314 for 57 degrees of freedom
# Null hypothesis probability = 5.605488e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.894e-09 2.739e-09
25- 50 1.122e-08 5.459e-09
50-150 1.060e-08 7.468e-09
15-150 2.971e-08 1.462e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.66341 (-1.4802 1.95166)
R1^2/D10^2 : 4.67159 (-3.60069 22.5109)
kT2 [keV] : 23.3562 (-10.6126 55.9149)
R2^2/D10^2 : 7.62829E-03 (-0.00739804 0.0432295)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.78 using 59 PHA bins.
# Reduced chi-squared = 1.305 for 55 degrees of freedom
# Null hypothesis probability = 6.387274e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.273e-09 5.180e-09
25- 50 8.765e-09 4.921e-09
50-150 1.681e-08 1.102e-08
15-150 3.485e-08 2.042e-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: 2.01424 ( -0.241764 0.261935 )
Norm@50keV : 2.52918E-03 ( -0.000457764 0.000445284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.99 using 59 PHA bins.
# Reduced chi-squared = 1.386 for 57 degrees of freedom
# Null hypothesis probability = 2.856032e-02
Photon flux (15-150 keV) in 7.892 sec: 0.381883 ( -0.0505664 0.0505682 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84217e-07 ( -3.0547e-08 3.16049e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38798 ( -1.09426 0.754599 )
Epeak [keV] : 39.5104 ( )
Norm@50keV : 5.95038E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.58 using 59 PHA bins.
# Reduced chi-squared = 1.385 for 56 degrees of freedom
# Null hypothesis probability = 2.972149e-02
Photon flux (15-150 keV) in 7.892 sec: 0.374916 ( -0.051095 0.051296 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72858e-07 ( -3.2223e-08 3.50578e-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) = 5.57e-08
S(50-100 keV) = 5.52e-08
T90 vs. Hardness ratio plot
T90 = 7.21999996900558 sec.
Hardness ratio (energy fluence ratio) = 0.991023
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.950745
Count Ratio (50-100 keV) / (15-25 keV) = 0.548227
Mask shadow pattern
IMX = -5.842229921328191E-02, IMY = 1.111033683784135E-04
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-576.183400 -559.744000
-239.584000 -3.428000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
359.3279 7.1626 2.7 52.2 29.5 5.4665 4.3 431.6 UNKNOWN
77.1081 -60.3212 2.6 51.6 157.9 4.2755 4.4 ------ UNKNOWN
18.1142 -38.5543 2.7 22.1 102.1 1.1505 4.2 ------ UNKNOWN
343.3834 5.2701 2.6 49.9 9.2 2.4794 4.4 ------ UNKNOWN
313.0101 3.8337 2.4 58.1 -27.2 7.4635 4.8 ------ UNKNOWN
305.6220 -10.3598 4.0 50.7 -44.6 3.5451 2.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.428000 4.464000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
1.2577 -34.0501 2.2 13.7 62.8 0.1704 5.3 ------ UNKNOWN
350.8588 -47.4829 1.0 3.3 -179.9 0.3681 11.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
56.716590 97.366000
98.416000 962.483600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
22.0403 -23.0114 3.7 34.9 67.6 4.2215 3.1 ------ UNKNOWN
352.8748 -7.6631 3.1 39.9 14.3 2.8734 3.7 ------ UNKNOWN
357.7353 -29.8542 2.7 18.4 30.4 2.1623 4.2 ------ UNKNOWN
341.4895 7.2342 2.9 55.3 -0.2 8.0950 3.9 ------ UNKNOWN
324.0279 -9.2389 2.5 44.5 -28.4 4.6382 4.7 ------ UNKNOWN
213.5274 -71.4788 4.0 57.2 -154.1 12.5427 2.9 ------ UNKNOWN
310.4142 -9.9585 4.8 50.6 -44.6 8.1130 2.4 ------ UNKNOWN
Plot creation:
Thu Jan 5 10:34:57 EST 2017