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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
330.1941 -52.2166 0.0476 17.4 164.3 0.0815 4.0 TRIG_00416140
------------------------------------------
Foreground time interval of the image:
0.000 1.024 (delta_t = 1.024 [sec])
Background time interval of the image:
-60.072 -11.072 (delta_t = 49.000 [sec])
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 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 1.024000
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 1.024000
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 1.024000
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 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.35319 ( -0.588377 0.894032 )
Norm@50keV : 1.21564E-03 ( -0.00119307 0.00142842 )
------------------------------------------------------------
# Chi-Squared = 58.96 using 59 PHA bins.
# Reduced chi-squared = 1.034 for 57 degrees of freedom
# Null hypothesis probability = 4.037881e-01
Photon flux (15-150 keV) in 1.024 sec: 0.332473 ( -0.173655 0.167643 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.80343e-08 ( -5.80344e-08 2.65184e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.71185 ( 2.71186 1.71202 )
Epeak [keV] : 999.850 ( -999.896 -999.896 )
Norm@50keV : 7.02161E-04 ( -0.000701922 0.00510469 )
------------------------------------------------------------
# Chi-Squared = 57.62 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 56 degrees of freedom
# Null hypothesis probability = 4.150799e-01
Photon flux (15-150 keV) in 1.024 sec: 0.302566 ( -0.118699 0.173723 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.84263e-08 ( -5.84263e-08 2.66159e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.109107 ( 0.0304935 0.0304935 )
beta : 1.38665 ( -0.932231 0.545639 )
Epeak [keV] : 25.8831 ( -25.125 -25.125 )
Norm@50keV : 1.70087E-03 ( 105.28 -0.00166352 )
------------------------------------------------------------
# Chi-Squared = 58.95 using 59 PHA bins.
# Reduced chi-squared = 1.072 for 55 degrees of freedom
# Null hypothesis probability = 3.332612e-01
Photon flux (15-150 keV) in 1.024 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.35054 ( -0.589718 0.89085 )
Norm@50keV : 1.22474E-03 ( -0.00120154 0.00143045 )
------------------------------------------------------------
# Chi-Squared = 59.43 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 57 degrees of freedom
# Null hypothesis probability = 3.870541e-01
Photon flux (15-150 keV) in 1.024 sec: 0.334135 ( -0.173911 0.167676 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83236e-08 ( -5.83236e-08 2.6498e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -3.07754 ( )
Epeak [keV] : 3011.87 ( -807.065 -1000.36 )
Norm@50keV : 3.03515E-04 ( -0.000305824 0.00369993 )
------------------------------------------------------------
# Chi-Squared = 57.96 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 56 degrees of freedom
# Null hypothesis probability = 4.027527e-01
Photon flux (15-150 keV) in 1.024 sec: 0.330853 ( -0.171398 0.171172 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.87056e-08 ( -5.87056e-08 2.66109e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.991278 ( 0.994936 0.994936 )
beta : 1.41505 ( -0.93911 0.535417 )
Epeak [keV] : 10.2723 ( -10.2934 -10.2934 )
Norm@50keV : 1.84378E-03 ( 0.822497 -0.001848 )
------------------------------------------------------------
# Chi-Squared = 59.42 using 59 PHA bins.
# Reduced chi-squared = 1.080 for 55 degrees of freedom
# Null hypothesis probability = 3.179612e-01
Photon flux (15-150 keV) in 1.024 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
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: -1.35319 ( -0.588377 0.894032 )
Norm@50keV : 1.21564E-03 ( -0.00119307 0.00142842 )
------------------------------------------------------------
# Chi-Squared = 58.96 using 59 PHA bins.
# Reduced chi-squared = 1.034 for 57 degrees of freedom
# Null hypothesis probability = 4.037881e-01
Photon flux (15-150 keV) in 1.024 sec: 0.332473 ( -0.173655 0.167643 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.80343e-08 ( -5.80344e-08 2.65184e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.71185 ( 2.71186 1.71126 )
Epeak [keV] : 999.850 ( -999.896 -999.896 )
Norm@50keV : 7.02161E-04 ( -0.000701922 0.00510469 )
------------------------------------------------------------
# Chi-Squared = 57.62 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 56 degrees of freedom
# Null hypothesis probability = 4.150799e-01
Photon flux (15-150 keV) in 1.024 sec: 0.302566 ( -0.118699 0.173723 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.84263e-08 ( -5.84263e-08 2.66159e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.109107 ( 0.0304935 0.0304935 )
beta : 1.38665 ( -0.932231 0.545639 )
Epeak [keV] : 25.8831 ( -25.125 -25.125 )
Norm@50keV : 1.70087E-03 ( 105.28 -0.00166352 )
------------------------------------------------------------
# Chi-Squared = 58.95 using 59 PHA bins.
# Reduced chi-squared = 1.072 for 55 degrees of freedom
# Null hypothesis probability = 3.332612e-01
Photon flux (15-150 keV) in 1.024 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) = 1.23825e-09
S(50-100 keV) = 1.31868e-08
T90 vs. Hardness ratio plot
T90 = 1.02399998903275 sec.
Hardness ratio (energy fluence ratio) = 10.6495
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = -2.73053
Count Ratio (50-100 keV) / (15-25 keV) = 12.7496
Mask shadow pattern
IMX = -3.019345215000961E-01, IMY = -8.508680189354928E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-60.072000 -11.072000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
343.8737 -71.3888 2.5 22.4 104.1 1.3136 4.6 ------ UNKNOWN
48.7260 -14.6266 3.7 54.1 -19.8 2.6213 3.1 ------ UNKNOWN
39.7356 -10.9567 2.8 52.0 -31.4 3.4970 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 1.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
79.0707 -86.7794 3.2 39.7 87.4 0.2928 3.6 ------ UNKNOWN
270.7913 -62.5919 2.3 46.0 132.1 0.4492 5.1 ------ UNKNOWN
42.2434 -7.6061 2.2 56.1 -31.1 0.6378 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Tue Mar 16 19:28:01 EDT 2010