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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
162.4807 -10.4613 0.0558 43.0 -155.8 0.4636 3.4 TRIG_00317393
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
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 64.000000
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 64.000000
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 64.000000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Flight mask-tagged light curves
Caution: Mask-weight map is always using the same on-axis map
Quad-rate summed light curves (from T0-300 to T0+1000)
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 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.58677 ( -0.548835 0.71847 )
Norm@50keV : 4.17195E-04 ( -0.000414814 0.000223238 )
------------------------------------------------------------
# Chi-Squared = 50.10 using 59 PHA bins.
# Reduced chi-squared = 0.8790 for 57 degrees of freedom
# Null hypothesis probability = 7.293619e-01
Photon flux (15-150 keV) in 64 sec: 8.64009E-02 ( -0.027807 0.0280516 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7179e-07 ( -1.02424e-07 1.15044e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.25202 ( )
Epeak [keV] : 27.3675 ( -4.89471 5.7319 )
Norm@50keV : 22.6672 ( )
------------------------------------------------------------
# Chi-Squared = 42.61 using 59 PHA bins.
# Reduced chi-squared = 0.7608 for 56 degrees of freedom
# Null hypothesis probability = 9.064221e-01
Photon flux (15-150 keV) in 64 sec: 8.87979E-02 ( -0.0252902 0.0252811 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.41478e-07 ( -7.23014e-08 7.5751e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.53876 ( -6.50224 -6.05989 )
beta : -9.37167 ( 10 19.9939 )
Epeak [keV] : 27.5363 ( -5.12292 5.63534 )
Norm@50keV : 34.8338 ( -34.8731 16.7718 )
------------------------------------------------------------
# Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7750 for 55 degrees of freedom
# Null hypothesis probability = 8.882729e-01
Photon flux (15-150 keV) in 64 sec: 8.901737E-02 ( -0.0254795 0.0253836 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38764e-07 ( -6.80653e-08 6.78355e-08 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.58276 ( -0.54316 0.713431 )
Norm@50keV : 4.19544E-04 ( -0.000417059 0.000222604 )
------------------------------------------------------------
# Chi-Squared = 50.40 using 59 PHA bins.
# Reduced chi-squared = 0.8841 for 57 degrees of freedom
# Null hypothesis probability = 7.193937e-01
Photon flux (15-150 keV) in 64 sec: 8.66577E-02 ( -0.0275757 0.0278371 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.72884e-07 ( -1.02113e-07 1.14767e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.25613 ( )
Epeak [keV] : 27.3737 ( -4.85329 5.66122 )
Norm@50keV : 22.8622 ( )
------------------------------------------------------------
# Chi-Squared = 42.79 using 59 PHA bins.
# Reduced chi-squared = 0.7641 for 56 degrees of freedom
# Null hypothesis probability = 9.028504e-01
Photon flux (15-150 keV) in 64 sec: 8.90414E-02 ( -0.0250904 0.0251036 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.42458e-07 ( -7.21434e-08 4.1433e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.53274 ( -6.41541 -6.00549 )
beta : -9.36425 ( 9.98654 19.98 )
Epeak [keV] : 27.2641 ( -4.84518 5.80241 )
Norm@50keV : 36.9730 ( -36.5503 14.59 )
------------------------------------------------------------
# Chi-Squared = 42.81 using 59 PHA bins.
# Reduced chi-squared = 0.7783 for 55 degrees of freedom
# Null hypothesis probability = 8.842670e-01
Photon flux (15-150 keV) in 64 sec: 8.901737E-02 ( -0.0254795 0.0253836 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38764e-07 ( -6.80653e-08 6.78355e-08 ) 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: 2.58677 ( -0.548835 0.71847 )
Norm@50keV : 4.17195E-04 ( -0.000414814 0.000223238 )
------------------------------------------------------------
# Chi-Squared = 50.10 using 59 PHA bins.
# Reduced chi-squared = 0.8790 for 57 degrees of freedom
# Null hypothesis probability = 7.293619e-01
Photon flux (15-150 keV) in 64 sec: 8.64009E-02 ( -0.027807 0.0280516 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7179e-07 ( -1.02424e-07 1.15044e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.25202 ( )
Epeak [keV] : 27.3675 ( -4.89471 5.7319 )
Norm@50keV : 22.6672 ( )
------------------------------------------------------------
# Chi-Squared = 42.61 using 59 PHA bins.
# Reduced chi-squared = 0.7608 for 56 degrees of freedom
# Null hypothesis probability = 9.064221e-01
Photon flux (15-150 keV) in 64 sec: 8.87979E-02 ( -0.0252902 0.0252811 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.41478e-07 ( -7.23014e-08 7.5751e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.53876 ( -15.9143 -6.05989 )
beta : -9.37167 ( 10 19.9939 )
Epeak [keV] : 27.5363 ( -5.12292 5.63534 )
Norm@50keV : 34.8338 ( -34.8731 16.7718 )
------------------------------------------------------------
# Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7750 for 55 degrees of freedom
# Null hypothesis probability = 8.882729e-01
Photon flux (15-150 keV) in 64 sec: 8.901737E-02 ( -0.0254795 0.0253836 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.38764e-07 ( -6.80653e-08 6.78355e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 9.09619e-08
S(50-100 keV) = 5.97948e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.657361
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.894054
Count Ratio (50-100 keV) / (15-25 keV) = -0.194837
Mask shadow pattern
IMX = 0, IMY = 0
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Post-slew image of 15-350 keV band
Time interval of the image:
135.500590 415.390000
416.000000 869.450000
871.000000 963.007100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5043 -40.5540 0.6 38.4 177.4 12.5746 18.6 1.1 Vela X-1
171.8285 -28.5563 2.8 20.1 119.2 2.0351 4.1 ------ UNKNOWN
194.1717 24.7705 3.7 46.8 4.4 3.0887 3.1 ------ UNKNOWN
122.2418 -46.5141 3.5 49.6 179.4 3.9002 3.3 ------ UNKNOWN
177.8622 21.5971 2.8 35.4 -11.3 2.4676 4.2 ------ UNKNOWN
122.3393 -28.1736 2.9 41.6 -157.4 3.2079 4.0 ------ UNKNOWN
154.3650 39.6617 3.6 50.7 -44.5 9.7988 3.2 ------ UNKNOWN
Plot creation:
Wed Feb 17 13:57:49 EST 2010