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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
59.3779 -44.3666 0.1294 22.9 -35.7 0.3361 1.5 TRIG_00594286
------------------------------------------
Foreground time interval of the image:
0.000 320.000 (delta_t = 320.000 [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
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.78286 ( -0.841941 1.27321 )
Norm@50keV : 4.75080E-05 ( -4.74512e-05 4.86005e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.59 using 59 PHA bins.
# Reduced chi-squared = 1.537 for 57 degrees of freedom
# Null hypothesis probability = 5.701028e-03
Photon flux (15-150 keV) in 320 sec: 1.12143E-02 ( -0.00650702 0.00651294 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66604e-07 ( -1.04608e-07 1.26434e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -8.72402 ( )
Epeak [keV] : 27.9605 ( -3.22385 6.45447 )
Norm@50keV : 4478.14 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.89 using 59 PHA bins.
# Reduced chi-squared = 1.427 for 56 degrees of freedom
# Null hypothesis probability = 1.972616e-02
Photon flux (15-150 keV) in 320 sec: 1.34450E-02 ( -0.00560795 0.0060474 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81561e-07 ( -7.6001e-08 8.71798e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -4.83585 -5 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 27.5151 ( -5.84618 7.412 )
Norm@50keV : 12.2573 ( -5.61737 49.4164 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.40 using 59 PHA bins.
# Reduced chi-squared = 1.462 for 55 degrees of freedom
# Null hypothesis probability = 1.436557e-02
Photon flux (15-150 keV) in 320 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] : 6.67842 (-1.98682 2.43522)
R^2/D10^2 : 3.57594E-02 (-0.0353216 0.10221)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.83 using 59 PHA bins.
# Reduced chi-squared = 1.436 for 57 degrees of freedom
# Null hypothesis probability = 1.722470e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.788e-08 4.760e-08
25- 50 9.719e-08 6.923e-08
50-150 1.354e-08 1.475e-08
15-150 1.886e-07 1.213e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 22.2641 (-11.6454 29.4308)
Norm : 0.139506 (-0.0869663 0.203437)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.98 using 59 PHA bins.
# Reduced chi-squared = 1.491 for 57 degrees of freedom
# Null hypothesis probability = 9.532287e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.541e-08 5.042e-08
25- 50 7.149e-08 5.072e-08
50-150 2.549e-08 2.680e-08
15-150 1.724e-07 1.225e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.75526 (-6.75199 -6.75199)
R1^2/D10^2 : 1.97097E-02 (-0.0197364 -0.0197364)
kT2 [keV] : 6.75222 (-6.7512 -6.7512)
R2^2/D10^2 : 1.46650E-02 (-0.0146961 -0.0146961)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.83 using 59 PHA bins.
# Reduced chi-squared = 1.488 for 55 degrees of freedom
# Null hypothesis probability = 1.094080e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.755e-08 6.659e+01
25- 50 9.899e-08 5.074e+02
50-150 1.439e-08 1.356e+04
15-150 1.909e-07 1.397e+04
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.78286 ( -0.841941 1.27321 )
Norm@50keV : 4.75080E-05 ( -4.74512e-05 4.86005e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.59 using 59 PHA bins.
# Reduced chi-squared = 1.537 for 57 degrees of freedom
# Null hypothesis probability = 5.701028e-03
Photon flux (15-150 keV) in 320 sec: 1.12143E-02 ( -0.00650702 0.00651294 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66604e-07 ( -1.04608e-07 1.26434e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -8.72402 ( )
Epeak [keV] : 27.9605 ( -3.22385 6.45447 )
Norm@50keV : 4478.14 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.89 using 59 PHA bins.
# Reduced chi-squared = 1.427 for 56 degrees of freedom
# Null hypothesis probability = 1.972616e-02
Photon flux (15-150 keV) in 320 sec: 1.34450E-02 ( -0.00560795 0.0060474 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81561e-07 ( -7.6001e-08 8.71798e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -4.83585 -5 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 27.5151 ( -5.84618 7.412 )
Norm@50keV : 12.2573 ( -5.61737 49.4164 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.40 using 59 PHA bins.
# Reduced chi-squared = 1.462 for 55 degrees of freedom
# Null hypothesis probability = 1.436557e-02
Photon flux (15-150 keV) in 320 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] : 6.67842 (-1.98682 2.43522)
R^2/D10^2 : 3.57594E-02 (-0.0353216 0.10221)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.83 using 59 PHA bins.
# Reduced chi-squared = 1.436 for 57 degrees of freedom
# Null hypothesis probability = 1.722470e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.788e-08 4.627e-08
25- 50 9.719e-08 6.621e-08
50-150 1.354e-08 1.456e-08
15-150 1.886e-07 1.350e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 22.2641 (-11.6454 29.4308)
Norm : 0.139506 (-0.0869663 0.203437)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.98 using 59 PHA bins.
# Reduced chi-squared = 1.491 for 57 degrees of freedom
# Null hypothesis probability = 9.532287e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.541e-08 4.922e-08
25- 50 7.149e-08 5.506e-08
50-150 2.549e-08 2.843e-08
15-150 1.724e-07 1.231e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.75526 (-6.75199 -6.75199)
R1^2/D10^2 : 1.97097E-02 (-0.0197364 -0.0197364)
kT2 [keV] : 6.75222 (-6.7512 -6.7512)
R2^2/D10^2 : 1.46650E-02 (-0.0146961 -0.0146961)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.83 using 59 PHA bins.
# Reduced chi-squared = 1.488 for 55 degrees of freedom
# Null hypothesis probability = 1.094080e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.755e-08 6.555e+01
25- 50 9.899e-08 5.360e+02
50-150 1.439e-08 1.320e+04
15-150 1.909e-07 1.347e+04
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: 2.78286 ( -0.841941 1.27321 )
Norm@50keV : 4.75080E-05 ( -4.74512e-05 4.86005e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.59 using 59 PHA bins.
# Reduced chi-squared = 1.537 for 57 degrees of freedom
# Null hypothesis probability = 5.701028e-03
Photon flux (15-150 keV) in 320 sec: 1.12143E-02 ( -0.00650702 0.00651294 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66604e-07 ( -1.04608e-07 1.26434e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -8.72402 ( )
Epeak [keV] : 27.9605 ( -3.22385 6.45447 )
Norm@50keV : 4478.14 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.89 using 59 PHA bins.
# Reduced chi-squared = 1.427 for 56 degrees of freedom
# Null hypothesis probability = 1.972616e-02
Photon flux (15-150 keV) in 320 sec: 1.34450E-02 ( -0.00560795 0.0060474 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81561e-07 ( -7.6001e-08 8.71798e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -4.83585 -5 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 27.5151 ( -5.84618 7.412 )
Norm@50keV : 12.2573 ( -5.61737 49.4164 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.40 using 59 PHA bins.
# Reduced chi-squared = 1.462 for 55 degrees of freedom
# Null hypothesis probability = 1.436557e-02
Photon flux (15-150 keV) in 320 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) = 5.59981e-08
S(50-100 keV) = 3.24816e-08
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 0.580048
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.862313
Count Ratio (50-100 keV) / (15-25 keV) = -0.371273
Mask shadow pattern
IMX = 3.423724659749711E-01, IMY = 2.460899734836091E-01
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 320.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
117.9722 -40.4370 2.4 45.1 36.0 2.8259 4.8 ------ UNKNOWN
281.8816 -66.9302 3.0 41.5 153.9 1.7512 3.8 ------ UNKNOWN
321.8603 -55.7307 2.0 39.9 -172.7 1.7422 5.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
382.500630 963.080300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
105.5751 -24.9090 3.9 41.8 43.2 2.4537 3.0 ------ UNKNOWN
97.8774 -14.3748 3.0 44.2 24.7 2.6042 3.8 ------ UNKNOWN
96.7930 -23.2325 2.5 36.9 32.8 2.3567 4.6 ------ UNKNOWN
89.5618 -20.0155 2.3 34.8 20.6 2.0701 4.9 ------ UNKNOWN
334.7121 -43.9375 3.7 57.9 -156.8 7.8767 3.1 ------ UNKNOWN
51.2601 5.2279 2.5 50.2 -45.5 8.0604 4.7 ------ UNKNOWN
Plot creation:
Wed May 7 21:27:07 EDT 2014