batgrbproduct Analysis for Trigger=584697
Analysis Summary
Notes:
- 1) No attempt has been made to eliminate the non-significant decimal places.
- 2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
- 3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
- 4) This page will be updated for up to 10 downlinks after the trigger.
======================================================================
BAT GRB EVENT DATA PROCESSING REPORT
Process Script Ver: batgrbproduct v2.46
Process Start Time (local time): Fri Jan 24 00:55:21 EST 2014
Host Name: gcn5
Current Working Dir: /local/data/raid16/prebascript_archive/trigger584697/GCN5_download_cron
======================================================================
Trigger: 00584697 Segment: 000
BAT Trigger Time: 412160432 [s; MET]
Trigger Stop: 412162112 [s; MET]
UTC: 2014-01-23T09:00:20.446060 [includes UTCF correction]
Where From?: TDRSS position message
BAT
RA: 266.123018457217 Dec: -28.7343784011284 [deg; J2000]
Catalogged Source?: YES
Point Source?: YES
GRB Indicated?: NO [ by BAT flight software ]
Image S/N Ratio: 20.1
Image Trigger?: YES
Rate S/N Ratio: 0 [ if not an image trigger ]
Image S/N Ratio: 20.1
Flight Position: [ source = BAT ]
RA: 266.123018457217 Dec: -28.7343784011284 [deg; J2000]
Ground Position: [ source = BAT pre-slew burst ]
RA: 266.124657734867 Dec: -28.7420968596258 [deg; J2000]
{ 17h 44m 29.9s , -28d 44' 31.5" }
+/- 1.76009282852444 [arcmin] (estimated 90% radius based on SNR)
+/- 0.702339719441339 [arcmin] (formal 1-sigma fit error)
SNR: 13.5629223424865
Angular difference between Flight and Ground position is 0.471069 arcmin
Partial Coding Fraction: 0.921875 [ including projection effects ]
Duration
T90: 1680 +/-
Measured from: 0
to: 1680 [s; relative to TRIGTIME]
T50: 1680 +/-
Measured from: 0
to: 1680 [s; relative to TRIGTIME]
WARNING: battblocks failed. Used TDRSS fore/background intervals
Fluence
Peak Flux (peak 1680 second)
Measured from: 0
to: 1680 [s; relative to TRIGTIME]
Total Fluence
Measured from: 0
to: 1680 [s; relative to TRIGTIME]
Band 1 Band 2 Band 3 Band 4
15-25 25-50 50-100 100-350 keV
Total 5.023264 2.174256 0.404467 -0.016287
0.185075 0.156784 0.127716 0.107671 [error]
Peak 5.023264 2.174256 0.404467 -0.016287
0.185075 0.156784 0.127716 0.107671 [error]
[ fluence units of on-axis counts / fully illuminated detector ]
======================================================================
=== Fluence/Peak Flux Summary ===
Model Band1 Band2 Band3 Band4 Band5 Total
15-25 25-50 50-100 100-350 15-150 15-350 keV
Fluence Power-law 1.53e-06 9.15e-07 3.50e-07 1.79e-07 2.89e-06 2.97e-06 erg/cm2
Error 1.37e-07 8.79e-08 7.60e-08 6.98e-08 2.21e-07 2.43e-07 erg/cm2
Peak flux Power-law 8.83e-02 3.00e-02 5.73e-03 1.29e-03 1.25e-01 1.25e-01 ph/cm2/s
Error 8.13e-03 2.73e-03 1.20e-03 4.75e-04 9.18e-03 9.17e-03 ph/cm2/s
Fluence Cutoff-PL 1.51e-06 9.06e-07 7.46e-08 3.07e-10 2.49e-06 2.49e-06 erg/cm2
Error 1.46e-07 1.16e-07 9.59e-08 7.56e-09 2.37e-07 2.37e-07 erg/cm2
Peak flux Cutoff-PL 8.60e-02 3.07e-02 1.38e-03 3.06e-06 1.18e-01 1.18e-01 ph/cm2/s
Error 8.80e-03 3.43e-03 1.63e-03 6.96e-05 9.89e-03 9.89e-03 ph/cm2/s
Fluence Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 erg/cm2
Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 erg/cm2
Peak flux Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 ph/cm2/s
Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 ph/cm2/s
=== Time-averaged spectral analysis ===
Model Ph_index Ph_90err Epeak Epeak_90err Norm Nomr_90err chi2 dof
PL 3.386 0.204 - - 3.38e-04 5.47e-05 76.790 57
CPL 0.601 2.131 13.1 0.0 3.86e-02 0.00e+00 69.480 56
=== 1-s peak spectral analysis ===
Model Ph_index Ph_90err Epeak Epeak_90err Norm Nomr_90err chi2 dof
PL 3.386 0.204 - - 3.38e-04 5.47e-05 76.790 57
CPL 0.601 2.131 13.1 0.0 3.86e-02 0.00e+00 69.480 56
Model : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err : 90% error of the photon index
Epeak : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2 : Chi-Squared
dof : degree of freedom
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
T90 in the 50-300 keV band: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.
=== Table of the duration information ==
Value tstart tstop
T100 1680.000 0.000 1680.000
T90 1680.000 0.000 1680.000
T50 1680.000 0.000 1680.000
Peak 1680.000 0.000 1680.000
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
266.1247 -28.7421 0.0141 13.9 -73.5 7.8013 13.6 TRIG_00584697
------------------------------------------
Foreground time interval of the image:
360.000 363.070 (delta_t = 3.070 [sec])
376.000 697.020 (delta_t = 321.020 [sec])
698.000 704.860 (delta_t = 6.860 [sec])
706.000 709.180 (delta_t = 3.180 [sec])
710.000 817.600 (delta_t = 107.600 [sec])
819.000 820.980 (delta_t = 1.980 [sec])
822.000 876.450 (delta_t = 54.450 [sec])
879.000 933.370 (delta_t = 54.370 [sec])
934.000 934.700 (delta_t = 0.700 [sec])
936.000 963.063 (delta_t = 27.063 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
360.000000 363.070000
376.000000 697.019700
698.000000 704.860000
706.000000 709.180000
710.000000 817.600000
819.000000 820.980000
822.000000 876.450000
879.000000 933.370000
934.000000 934.700000
936.000000 963.063000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.38581 ( -0.198691 0.208515 )
Norm@50keV : 3.38276E-04 ( -5.33777e-05 5.612e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.79 using 59 PHA bins.
# Reduced chi-squared = 1.347 for 57 degrees of freedom
# Null hypothesis probability = 4.140604e-02
Photon flux (15-150 keV) in 580.3 sec: 0.124826 ( -0.00916761 0.00918471 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.88527e-06 ( -2.20226e-07 2.22703e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
360.000000 363.070000
376.000000 697.019700
698.000000 704.860000
706.000000 709.180000
710.000000 817.600000
819.000000 820.980000
822.000000 876.450000
879.000000 933.370000
934.000000 934.700000
936.000000 963.063000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.601263 ( -2.86607 1.39628 )
Epeak [keV] : 13.1143 ( )
Norm@50keV : 3.85534E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.48 using 59 PHA bins.
# Reduced chi-squared = 1.241 for 56 degrees of freedom
# Null hypothesis probability = 1.064725e-01
Photon flux (15-150 keV) in 580.3 sec: 0.118006 ( -0.009905 0.009874 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.49264e-06 ( -2.22017e-07 2.51873e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
360.000000 363.070000
376.000000 697.019700
698.000000 704.860000
706.000000 709.180000
710.000000 817.600000
819.000000 820.980000
822.000000 876.450000
879.000000 933.370000
934.000000 934.700000
936.000000 963.063000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.45665 ( -4.80953 -4.45665 )
beta : -4.19110 ( -0.646531 0.449767 )
Epeak [keV] : 19.2576 ( -1.35206 1.32379 )
Norm@50keV : 409.994 ( -28.9939 1923.84 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.48 using 59 PHA bins.
# Reduced chi-squared = 1.118 for 55 degrees of freedom
# Null hypothesis probability = 2.552929e-01
Photon flux (15-150 keV) in 580.3 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] : 4.75550 (-0.317605 0.346563)
R^2/D10^2 : 1.29391 (-0.398341 0.577282)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.52 using 59 PHA bins.
# Reduced chi-squared = 1.255 for 57 degrees of freedom
# Null hypothesis probability = 9.331333e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.488e-06 1.645e-07
25- 50 8.568e-07 1.004e-07
50-150 2.717e-08 1.135e-08
15-150 2.372e-06 2.504e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.2850 (-1.65747 2.09872)
Norm : 2.53174 (-0.499755 0.725402)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.08 using 59 PHA bins.
# Reduced chi-squared = 1.230 for 57 degrees of freedom
# Null hypothesis probability = 1.143501e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.523e-06 1.703e-07
25- 50 9.223e-07 1.024e-07
50-150 1.268e-07 4.169e-08
15-150 2.572e-06 2.342e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.46974 (-0.359759 0.366506)
R1^2/D10^2 : 1.71067 (-0.570448 1.08141)
kT2 [keV] : 27.5445 (-12.5032 40.8909)
R2^2/D10^2 : 2.54142E-04 (-0.000231592 0.00187338)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.01 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 55 degrees of freedom
# Null hypothesis probability = 4.001463e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.526e-06 2.173e-07
25- 50 8.486e-07 1.416e-07
50-150 6.207e-07 3.770e-07
15-150 2.996e-06 5.849e-07
Peak spectrum fit
Power-law model
Time interval is from 936.000 sec. to 963.063 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.38581 ( -0.198691 0.208515 )
Norm@50keV : 3.38276E-04 ( -5.33777e-05 5.612e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.79 using 59 PHA bins.
# Reduced chi-squared = 1.347 for 57 degrees of freedom
# Null hypothesis probability = 4.140604e-02
Photon flux (15-150 keV) in 580.3 sec: 0.124826 ( -0.00916761 0.00918471 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.88527e-06 ( -2.20226e-07 2.22703e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 936.000 sec. to 963.063 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.601263 ( -2.86607 1.39628 )
Epeak [keV] : 13.1143 ( )
Norm@50keV : 3.85534E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.48 using 59 PHA bins.
# Reduced chi-squared = 1.241 for 56 degrees of freedom
# Null hypothesis probability = 1.064725e-01
Photon flux (15-150 keV) in 580.3 sec: 0.118006 ( -0.009905 0.009874 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.49264e-06 ( -2.22017e-07 2.51873e-07 ) ergs/cm2
Band function
Time interval is from 936.000 sec. to 963.063 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.45665 ( -4.80953 -4.45665 )
beta : -4.19110 ( -0.646531 0.449767 )
Epeak [keV] : 19.2576 ( -1.35206 1.32379 )
Norm@50keV : 409.994 ( -28.9939 1923.84 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.48 using 59 PHA bins.
# Reduced chi-squared = 1.118 for 55 degrees of freedom
# Null hypothesis probability = 2.552929e-01
Photon flux (15-150 keV) in 580.3 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] : 4.75550 (-0.317605 0.346563)
R^2/D10^2 : 1.29391 (-0.398341 0.577282)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.52 using 59 PHA bins.
# Reduced chi-squared = 1.255 for 57 degrees of freedom
# Null hypothesis probability = 9.331333e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.488e-06 1.718e-07
25- 50 8.568e-07 1.103e-07
50-150 2.717e-08 1.173e-08
15-150 2.372e-06 2.196e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.2850 (-1.65747 2.09872)
Norm : 2.53174 (-0.499755 0.725402)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.08 using 59 PHA bins.
# Reduced chi-squared = 1.230 for 57 degrees of freedom
# Null hypothesis probability = 1.143501e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.523e-06 1.657e-07
25- 50 9.223e-07 9.691e-08
50-150 1.268e-07 4.042e-08
15-150 2.572e-06 2.504e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.46974 (-0.359759 0.366506)
R1^2/D10^2 : 1.71067 (-0.570448 1.08141)
kT2 [keV] : 27.5445 (-12.5032 40.8909)
R2^2/D10^2 : 2.54142E-04 (-0.000231592 0.00187338)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.01 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 55 degrees of freedom
# Null hypothesis probability = 4.001463e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.526e-06 2.098e-07
25- 50 8.486e-07 1.454e-07
50-150 6.207e-07 3.599e-07
15-150 2.996e-06 5.867e-07
Plot creation:
Fri Jan 24 01:05:55 EST 2014