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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
82.9784 +20.6243 0.0072 21.0 117.5 2.6913 26.9 TRIG_00373684
------------------------------------------
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: 2.04734 ( -0.12365 0.127225 )
Norm@50keV : 2.31263E-03 ( -0.000173804 0.000170923 )
------------------------------------------------------------
# Chi-Squared = 57.88 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 57 degrees of freedom
# Null hypothesis probability = 4.425262e-01
Photon flux (15-150 keV) in 64 sec: 0.354665 ( -0.0212138 0.0212608 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.369e-06 ( -9.40269e-08 9.52896e-08 ) 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: 1.99842 ( )
Epeak [keV] : 2.26361 ( )
Norm@50keV : 2.42037E-03 ( )
------------------------------------------------------------
# Chi-Squared = 58.13 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 56 degrees of freedom
# Null hypothesis probability = 3.968744e-01
Photon flux (15-150 keV) in 64 sec: 0.352875 ( -0.021291 0.021339 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36655e-06 ( -9.4784e-08 9.60704e-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 : -1.52188 ( 1.52102 1.52102 )
beta : -2.05079 ( 2.05229 0.128064 )
Epeak [keV] : 17.0924 ( -17.8875 82.6889 )
Norm@50keV : 6.55580E-03 ( -0.00648055 8.82611 )
------------------------------------------------------------
# Chi-Squared = 57.86 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 55 degrees of freedom
# Null hypothesis probability = 3.700963e-01
Photon flux (15-150 keV) in 64 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 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03583 ( -0.09904 0.10254 )
Norm@50keV : 2.32033E-03 ( -0.00016977 0.000167445 )
------------------------------------------------------------
# Chi-Squared = 59.24 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 57 degrees of freedom
# Null hypothesis probability = 3.936862e-01
Photon flux (15-150 keV) in 64 sec: 0.353910 ( -0.0176244 0.0176285 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.37244e-06 ( -9.23034e-08 9.36909e-08 ) 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: 2.09867 ( -0.322906 0.0989541 )
Epeak [keV] : 60.4284 ( )
Norm@50keV : 2.11781E-03 ( )
------------------------------------------------------------
# Chi-Squared = 59.01 using 59 PHA bins.
# Reduced chi-squared = 1.054 for 56 degrees of freedom
# Null hypothesis probability = 3.660632e-01
Photon flux (15-150 keV) in 64 sec: 0.353795 ( -0.017619 0.017623 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.37225e-06 ( -9.23008e-08 9.36832e-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 : -1.40001 ( 1.40001 1.40001 )
beta : -2.05212 ( -0.182043 0.112742 )
Epeak [keV] : 19.7159 ( -19.7159 -19.7159 )
Norm@50keV : 7.72015E-03 ( -0.00772015 152.961 )
------------------------------------------------------------
# Chi-Squared = 59.12 using 59 PHA bins.
# Reduced chi-squared = 1.075 for 55 degrees of freedom
# Null hypothesis probability = 3.275643e-01
Photon flux (15-150 keV) in 64 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: 2.04734 ( -0.12365 0.127225 )
Norm@50keV : 2.31263E-03 ( -0.000173804 0.000170923 )
------------------------------------------------------------
# Chi-Squared = 57.88 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 57 degrees of freedom
# Null hypothesis probability = 4.425262e-01
Photon flux (15-150 keV) in 64 sec: 0.354665 ( -0.0212138 0.0212608 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.369e-06 ( -9.40269e-08 9.52896e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99842 ( )
Epeak [keV] : 2.26361 ( )
Norm@50keV : 2.42037E-03 ( )
------------------------------------------------------------
# Chi-Squared = 58.13 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 56 degrees of freedom
# Null hypothesis probability = 3.968744e-01
Photon flux (15-150 keV) in 64 sec: 0.352875 ( -0.021291 0.021339 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36655e-06 ( -9.4784e-08 9.60704e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.52188 ( 1.52102 1.52102 )
beta : -2.05079 ( 2.05229 0.128064 )
Epeak [keV] : 17.0924 ( -17.8875 82.6889 )
Norm@50keV : 6.55580E-03 ( -0.00648055 8.82611 )
------------------------------------------------------------
# Chi-Squared = 57.86 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 55 degrees of freedom
# Null hypothesis probability = 3.700963e-01
Photon flux (15-150 keV) in 64 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) = 4.17695e-07
S(50-100 keV) = 4.0421e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.967716
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.896215
Count Ratio (50-100 keV) / (15-25 keV) = 0.468185
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] [']
83.8211 22.0793 4.7 21.4 121.9 -0.2418 -2.4 11.2 Crab
71.3094 36.5246 2.1 39.4 126.0 1.2376 5.4 ------ UNKNOWN
82.9783 20.6243 0.4 21.0 117.5 2.6913 27.1 ------ UNKNOWN
105.6856 53.5095 2.7 48.1 167.0 0.9796 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
120.700590 303.089400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5486 21.8817 4.2 1.3 -156.9 0.4778 2.8 9.3 Crab
50.3650 -13.6687 2.7 47.0 46.7 3.3083 4.2 ------ UNKNOWN
44.0499 62.2593 2.4 49.4 158.3 2.4876 4.7 ------ UNKNOWN
69.6274 29.7760 3.0 15.1 130.7 0.6430 3.9 ------ UNKNOWN
82.9320 20.6077 0.2 0.1 69.2 7.8766 46.6 ------ UNKNOWN
86.6667 10.3255 3.2 10.9 -18.5 0.5865 3.6 ------ UNKNOWN
120.9571 76.0184 2.5 58.7 -169.0 4.6659 4.7 ------ UNKNOWN
117.0085 12.9691 2.1 33.4 -81.3 1.7446 5.5 ------ UNKNOWN
Plot creation:
Mon Feb 15 16:28:14 EST 2010