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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
274.6577 -17.0691 0.0303 23.9 -11.5 0.6361 6.3 TRIG_00351323
------------------------------------------
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
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 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.33174 ( -0.616219 0.619129 )
Norm@50keV : 2.30516E-04 ( -0.000108989 0.000160619 )
------------------------------------------------------------
# Chi-Squared = 59.70 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 57 degrees of freedom
# Null hypothesis probability = 3.776505e-01
Photon flux (15-150 keV) in 64 sec: 8.21085E-02 ( -0.0174871 0.0175835 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.15441e-07 ( -5.71837e-08 6.41126e-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: 0.763229 ( -0.742007 1.2449 )
Epeak [keV] : 12.9274 ( )
Norm@50keV : 1.78617E-02 ( )
------------------------------------------------------------
# Chi-Squared = 58.04 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 56 degrees of freedom
# Null hypothesis probability = 3.999955e-01
Photon flux (15-150 keV) in 64 sec: 8.20744E-02 ( -0.0174816 0.0175775 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.91297e-07 ( -4.78438e-08 6.44813e-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 : -1.04667 ( 1.04667 5.89532 )
beta : -9.29038 ( 7.10881 17.1086 )
Epeak [keV] : 11.2069 ( -11.2556 9.34747 )
Norm@50keV : 1.10831E-02 ( -0.0110037 3.51954 )
------------------------------------------------------------
# Chi-Squared = 58.06 using 59 PHA bins.
# Reduced chi-squared = 1.056 for 55 degrees of freedom
# Null hypothesis probability = 3.631053e-01
Photon flux (15-150 keV) in 64 sec: 8.103948E-02 ( -0.0166261 0.0174958 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07744e-07 ( -4.35443e-08 4.70342e-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: 3.21913 ( -0.507397 0.640515 )
Norm@50keV : 2.53456E-04 ( -0.000121053 0.000144721 )
------------------------------------------------------------
# Chi-Squared = 60.55 using 59 PHA bins.
# Reduced chi-squared = 1.062 for 57 degrees of freedom
# Null hypothesis probability = 3.491591e-01
Photon flux (15-150 keV) in 64 sec: 8.21055E-02 ( -0.0166423 0.0167857 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.17262e-07 ( -5.66474e-08 6.39216e-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: 0.706268 ( )
Epeak [keV] : 13.2007 ( )
Norm@50keV : 1.98846E-02 ( )
------------------------------------------------------------
# Chi-Squared = 58.70 using 59 PHA bins.
# Reduced chi-squared = 1.048 for 56 degrees of freedom
# Null hypothesis probability = 3.767005e-01
Photon flux (15-150 keV) in 64 sec: 8.20734E-02 ( -0.016638 0.0167805 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.9225e-07 ( -4.64544e-08 6.24026e-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 : 4.11308 ( 1.04757 1.04757 )
beta : -3.99343 ( 7.31883 17.314 )
Epeak [keV] : 18.1651 ( -4.27672 8.7615 )
Norm@50keV : 213.374 ( -213.789 223.837 )
------------------------------------------------------------
# Chi-Squared = 58.62 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 55 degrees of freedom
# Null hypothesis probability = 3.440325e-01
Photon flux (15-150 keV) in 64 sec: 8.103948E-02 ( -0.0166261 0.0174958 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07744e-07 ( -4.35443e-08 4.70342e-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: 3.33174 ( -0.616219 0.619129 )
Norm@50keV : 2.30516E-04 ( -0.000108989 0.000160619 )
------------------------------------------------------------
# Chi-Squared = 59.70 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 57 degrees of freedom
# Null hypothesis probability = 3.776505e-01
Photon flux (15-150 keV) in 64 sec: 8.21085E-02 ( -0.0174871 0.0175835 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.15441e-07 ( -5.71837e-08 6.41126e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.763229 ( -0.742007 1.22204 )
Epeak [keV] : 12.9274 ( )
Norm@50keV : 1.78617E-02 ( )
------------------------------------------------------------
# Chi-Squared = 58.04 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 56 degrees of freedom
# Null hypothesis probability = 3.999955e-01
Photon flux (15-150 keV) in 64 sec: 8.20744E-02 ( -0.0174816 0.0175775 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.91297e-07 ( -4.78438e-08 6.44813e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.04667 ( 1.04667 5.89532 )
beta : -9.29038 ( 7.10881 17.1086 )
Epeak [keV] : 11.2069 ( -11.2556 9.34747 )
Norm@50keV : 1.10831E-02 ( -0.0110037 3.51954 )
------------------------------------------------------------
# Chi-Squared = 58.06 using 59 PHA bins.
# Reduced chi-squared = 1.056 for 55 degrees of freedom
# Null hypothesis probability = 3.631053e-01
Photon flux (15-150 keV) in 64 sec: 8.103948E-02 ( -0.0166261 0.0174958 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07744e-07 ( -4.35443e-08 4.70342e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.98054e-08
S(50-100 keV) = 2.92332e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.418781
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.420608
Count Ratio (50-100 keV) / (15-25 keV) = 0.0190352
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 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9609 -15.6370 0.9 26.0 59.8 1.8471 13.1 1.1 Sco X-1
254.5053 35.1971 7.5 32.4 -174.2 -0.1726 -1.5 9.0 Her X-1
256.1719 -37.8810 4.5 41.9 25.7 0.5297 2.6 9.1 4U 1700-377
256.4800 -36.4962 2.3 40.5 25.7 0.9180 5.0 4.9 GX 349+2
262.9301 -24.6118 3.7 28.2 17.4 0.3417 3.2 9.1 GX 1+4
264.9238 -44.4752 14.4 48.1 15.9 0.2371 0.8 7.9 4U 1735-44
268.2790 -1.5335 2.9 7.7 -29.9 0.3764 4.1 7.2 SW J1753.5-0127
270.3146 -25.2266 4.7 29.8 3.9 -0.2513 -2.4 9.0 GX 5-1
270.1411 -25.7238 4.2 30.3 4.5 0.2995 2.9 8.8 GRS 1758-258
273.9955 -13.9629 3.1 20.9 -14.4 0.3703 3.8 4.5 GX 17+2
275.8007 -30.4249 4.2 36.3 -1.3 0.3643 2.8 7.3 H1820-303
285.1762 -24.9080 4.4 36.0 -18.2 0.3090 2.6 7.7 HT1900.1-2455
288.7567 11.0224 1.9 27.0 -89.2 0.8123 6.1 5.2 GRS 1915+105
267.0766 -32.9524 3.0 36.8 11.8 0.4880 3.8 ------ UNKNOWN
274.6577 -17.0691 1.8 23.9 -11.5 0.6362 6.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
120.400600 349.170000
350.000000 963.076600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9909 -15.6500 0.5 28.5 96.2 23.2359 23.7 0.9 Sco X-1
255.9403 -37.8693 2.7 26.5 42.2 3.1324 4.3 2.7 4U 1700-377
256.5062 -36.5167 2.6 25.2 43.6 2.9547 4.5 6.6 GX 349+2
263.0307 -24.7831 3.6 13.3 60.3 1.7257 3.2 2.5 GX 1+4
264.5354 -44.3021 0.0 28.5 22.9 -0.8364 -1.3 12.6 4U 1735-44
268.3978 -1.4389 1.8 16.8 165.5 3.5229 6.5 2.0 SW J1753.5-0127
270.2375 -25.0765 2.5 9.0 34.1 2.9081 4.7 2.5 GX 5-1
270.3427 -25.6371 4.2 9.5 32.0 1.9051 3.2 6.7 GRS 1758-258
274.0247 -13.9589 3.4 3.2 176.5 2.0094 3.4 4.8 GX 17+2
275.9470 -30.2838 2.6 13.3 2.8 2.7253 4.4 5.1 H1820-303
285.2046 -24.9324 9.5 12.6 -42.0 0.6418 1.2 9.2 HT1900.1-2455
288.8004 10.9273 0.9 31.3 -144.9 8.2548 12.3 1.1 GRS 1915+105
274.6678 -17.0506 1.2 0.0 -150.4 5.2389 9.3 ------ UNKNOWN
274.9404 5.0838 3.4 22.2 -171.6 1.9066 3.4 ------ UNKNOWN
320.7992 -24.7223 5.7 43.6 -64.2 7.1400 2.1 ------ UNKNOWN
324.1140 -32.9052 4.1 47.1 -53.0 9.9281 2.8 ------ UNKNOWN
312.1707 2.9637 3.4 42.1 -107.2 10.3633 3.4 ------ UNKNOWN
Plot creation:
Tue Feb 16 17:46:36 EST 2010