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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
170.2774 -61.9691 0.0351 20.9 176.9 2.0119 5.5 TRIG_00339131
------------------------------------------
Foreground time interval of the image:
0.000 512.000 (delta_t = 512.000 [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
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)
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 512.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.82807 ( -0.329072 0.440525 )
Norm@50keV : 1.50502E-04 ( -5.03352e-05 4.8832e-05 )
------------------------------------------------------------
# Chi-Squared = 63.24 using 59 PHA bins.
# Reduced chi-squared = 1.110 for 57 degrees of freedom
# Null hypothesis probability = 2.654487e-01
Photon flux (15-150 keV) in 512 sec: 3.65255E-02 ( -0.00586395 0.00589268 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.49725e-07 ( -1.74388e-07 1.89866e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 512.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.98349 ( 0.940121 2.30757 )
Epeak [keV] : 22.8063 ( -2.86806 4.41597 )
Norm@50keV : 0.452574 ( )
------------------------------------------------------------
# Chi-Squared = 54.48 using 59 PHA bins.
# Reduced chi-squared = 0.9729 for 56 degrees of freedom
# Null hypothesis probability = 5.325868e-01
Photon flux (15-150 keV) in 512 sec: 3.54438E-02 ( -0.0055124 0.0056035 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.11875e-07 ( -1.23996e-07 1.45725e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 512.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98765 ( -166.677 -156.677 )
beta : -4.67735 ( 4.67269 1.48774 )
Epeak [keV] : 22.9656 ( -3.46412 2.89016 )
Norm@50keV : 99.3562 ( -21.7398 27.7588 )
------------------------------------------------------------
# Chi-Squared = 55.02 using 59 PHA bins.
# Reduced chi-squared = 1.000 for 55 degrees of freedom
# Null hypothesis probability = 4.740186e-01
Photon flux (15-150 keV) in 512 sec: 3.637007E-02 ( -0.00552649 0.00553455 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.13037e-07 ( -1.23546e-07 1.11514e-07 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 512.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.82293 ( -0.328511 0.384159 )
Norm@50keV : 1.49924E-04 ( -4.70759e-05 5.06997e-05 )
------------------------------------------------------------
# Chi-Squared = 64.74 using 59 PHA bins.
# Reduced chi-squared = 1.136 for 57 degrees of freedom
# Null hypothesis probability = 2.248226e-01
Photon flux (15-150 keV) in 512 sec: 3.63636E-02 ( -0.00551434 0.00556039 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.54917e-07 ( -1.73033e-07 1.89297e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 512.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.48908 ( 0.545478 2.02677 )
Epeak [keV] : 22.0852 ( -10.1996 4.41765 )
Norm@50keV : 0.209348 ( )
------------------------------------------------------------
# Chi-Squared = 56.01 using 59 PHA bins.
# Reduced chi-squared = 1.000 for 56 degrees of freedom
# Null hypothesis probability = 4.743957e-01
Photon flux (15-150 keV) in 512 sec: 3.61785E-02 ( -0.005138 0.0051843 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.26339e-07 ( -1.24216e-07 1.42618e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 512.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.471936 ( -1.19403 1.19403 )
beta : -9.37167 ( 10 20 )
Epeak [keV] : 21.0101 ( -6.21554 3.84761 )
Norm@50keV : 3.53510E-02 ( -0.083723 11.4183 )
------------------------------------------------------------
# Chi-Squared = 56.24 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 55 degrees of freedom
# Null hypothesis probability = 4.281474e-01
Photon flux (15-150 keV) in 512 sec: 3.637007E-02 ( -0.00552649 0.00553455 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.13037e-07 ( -1.23546e-07 1.11514e-07 ) 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: 2.82807 ( -0.329072 0.440525 )
Norm@50keV : 1.50502E-04 ( -5.03352e-05 4.8832e-05 )
------------------------------------------------------------
# Chi-Squared = 63.24 using 59 PHA bins.
# Reduced chi-squared = 1.110 for 57 degrees of freedom
# Null hypothesis probability = 2.654487e-01
Photon flux (15-150 keV) in 512 sec: 3.65255E-02 ( -0.00586395 0.00589268 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.49725e-07 ( -1.74388e-07 1.89866e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.98349 ( 0.940121 2.30757 )
Epeak [keV] : 22.8063 ( -2.86806 4.41597 )
Norm@50keV : 0.452574 ( )
------------------------------------------------------------
# Chi-Squared = 54.48 using 59 PHA bins.
# Reduced chi-squared = 0.9729 for 56 degrees of freedom
# Null hypothesis probability = 5.325868e-01
Photon flux (15-150 keV) in 512 sec: 3.54438E-02 ( -0.0055124 0.0056035 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.11875e-07 ( -1.23996e-07 1.45725e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.03535 ( -2.16696 -0.779206 )
beta : -9.37167 ( 10 19.9985 )
Epeak [keV] : 23.1434 ( -5.3911 4.55522 )
Norm@50keV : 0.468153 ( -0.46814 28.8848 )
------------------------------------------------------------
# Chi-Squared = 54.52 using 59 PHA bins.
# Reduced chi-squared = 0.9912 for 55 degrees of freedom
# Null hypothesis probability = 4.930878e-01
Photon flux (15-150 keV) in 512 sec: 3.637007E-02 ( -0.00552649 0.00553455 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.13037e-07 ( -1.23546e-07 1.11514e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.85287e-07
S(50-100 keV) = 1.57293e-07
T90 vs. Hardness ratio plot
T90 = 512 sec.
Hardness ratio (energy fluence ratio) = 0.55135
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.700982
Count Ratio (50-100 keV) / (15-25 keV) = -0.00270866
Mask shadow pattern
IMX = 0, IMY = 0
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 512.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5392 -40.5465 2.0 35.5 117.8 4.8545 5.7 0.7 Vela X-1
170.4022 -60.7927 3.9 22.0 175.4 1.0531 3.0 10.5 Cen X-3
186.6147 -62.7829 4.2 24.3 -165.3 1.0564 2.8 1.4 GX 301-2
46.5499 -33.6897 3.3 54.1 14.8 7.1703 3.5 ------ UNKNOWN
170.2767 -61.9692 2.1 20.9 176.9 2.0134 5.5 ------ UNKNOWN
40.6822 -59.3662 3.6 31.7 -5.3 1.5281 3.2 ------ UNKNOWN
28.4940 -48.4105 2.7 44.6 -8.5 2.7730 4.3 ------ UNKNOWN
283.4029 -62.9344 3.4 41.0 -92.3 7.0768 3.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
634.500600 646.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1631 -60.7317 44.2 35.2 65.8 -0.0231 -0.3 7.9 Cen X-3
186.8841 -62.8483 3.2 27.0 65.3 0.1931 3.6 7.8 GX 301-2
245.0087 -15.6318 4.7 39.1 -154.8 0.1303 2.5 1.8 Sco X-1
256.1071 -37.8370 2.5 20.7 -121.2 0.1910 4.5 5.7 4U 1700-377
256.6882 -36.4829 0.0 22.1 -122.0 -0.0972 -2.3 12.7 GX 349+2
262.9083 -24.8109 4.4 34.9 -123.5 -0.1578 -2.6 6.7 GX 1+4
264.7427 -44.3915 168.0 20.0 -94.5 0.0028 0.1 3.5 4U 1735-44
270.4604 -25.1285 6.4 37.9 -113.1 0.1474 1.8 10.0 GX 5-1
270.4628 -25.6876 9.3 37.4 -112.6 0.0979 1.2 9.3 GRS 1758-258
275.8350 -30.2725 11.4 36.3 -101.7 0.0874 1.0 7.3 H1820-303
198.4518 -36.8355 3.3 32.0 121.0 0.2081 3.5 ------ UNKNOWN
220.9166 -19.8557 3.3 36.8 167.1 0.1931 3.5 ------ UNKNOWN
228.8882 -47.8997 2.6 8.5 149.6 0.1547 4.5 ------ UNKNOWN
Plot creation:
Wed Feb 17 01:07:24 EST 2010