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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
264.8442 -30.3031 0.0288 11.6 47.4 1.9840 6.7 TRIG_00319963
------------------------------------------
Foreground time interval of the image:
-4.699 338.001 (delta_t = 342.700 [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 320.000000
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 320.000000
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 320.000000
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 -61.752 sec. to 648.896 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.73418 ( -0.244221 0.266399 )
Norm@50keV : 2.25582E-04 ( -4.46126e-05 4.55304e-05 )
------------------------------------------------------------
# Chi-Squared = 65.49 using 59 PHA bins.
# Reduced chi-squared = 1.149 for 57 degrees of freedom
# Null hypothesis probability = 2.059175e-01
Photon flux (15-150 keV) in 710.6 sec: 5.15072E-02 ( -0.00549347 0.00549349 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72618e-06 ( -2.22926e-07 2.32446e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -61.752 sec. to 648.896 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.347811 ( -2.00221 1.14336 )
Epeak [keV] : 21.9086 ( )
Norm@50keV : 8.96557E-03 ( )
------------------------------------------------------------
# Chi-Squared = 57.86 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 56 degrees of freedom
# Null hypothesis probability = 4.065145e-01
Photon flux (15-150 keV) in 710.6 sec: 4.86140E-02 ( -0.0055631 0.0055987 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47459e-06 ( -1.90171e-07 2.18865e-07 ) ergs/cm2
Band function
Time interval is from -61.752 sec. to 648.896 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.102447 ( -1.11985 1.97321 )
beta : -9.99902 ( 3251.42 3261.42 )
Epeak [keV] : 22.6619 ( -18.9397 4.74961 )
Norm@50keV : 1.32149E-02 ( -0.0115302 0.190386 )
------------------------------------------------------------
# Chi-Squared = 57.91 using 59 PHA bins.
# Reduced chi-squared = 1.053 for 55 degrees of freedom
# Null hypothesis probability = 3.683935e-01
Photon flux (15-150 keV) in 710.6 sec: 5.165069E-02 ( -0.00553651 0.00550787 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50178e-06 ( -2.59561e-07 2.43707e-07 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from -59.828 sec. to -58.828 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.94548 ( -1.05788 1.39836 )
Norm@50keV : 2.98503E-03 ( -0.00298058 0.00213191 )
------------------------------------------------------------
# Chi-Squared = 51.27 using 59 PHA bins.
# Reduced chi-squared = 0.8995 for 57 degrees of freedom
# Null hypothesis probability = 6.888461e-01
Photon flux (15-150 keV) in 1 sec: 0.436419 ( -0.266376 0.266901 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.74192e-08 ( -1.80663e-08 2.04894e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -59.828 sec. to -58.828 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.390286 ( 0.441435 2.5745 )
Epeak [keV] : 41.4953 ( )
Norm@50keV : 6.82455E-02 ( )
------------------------------------------------------------
# Chi-Squared = 50.50 using 59 PHA bins.
# Reduced chi-squared = 0.9018 for 56 degrees of freedom
# Null hypothesis probability = 6.823286e-01
Photon flux (15-150 keV) in 1 sec: 0.407752 ( -0.247743 0.268696 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.30996e-08 ( 2.15544e-08 -2.30996e-08 ) ergs/cm2
Band function
Time interval is from -59.828 sec. to -58.828 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.391988 ( 1.0782 1.0782 )
beta : -10.00000 ( 8.49485e+08 8.49485e+08 )
Epeak [keV] : 41.3832 ( -36.0471 -41.1282 )
Norm@50keV : 6.87449E-02 ( -0.0930015 23.2 )
------------------------------------------------------------
# Chi-Squared = 50.50 using 59 PHA bins.
# Reduced chi-squared = 0.9182 for 55 degrees of freedom
# Null hypothesis probability = 6.469744e-01
Photon flux (15-150 keV) in 1 sec: 0.411271 ( -0.238009 0.2691 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35603e-08 ( -1.41998e-08 2.19284e-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: 2.92823 ( -0.349478 0.40324 )
Norm@50keV : 1.79129E-04 ( -5.54243e-05 5.90531e-05 )
------------------------------------------------------------
# Chi-Squared = 73.69 using 59 PHA bins.
# Reduced chi-squared = 1.293 for 57 degrees of freedom
# Null hypothesis probability = 6.771460e-02
Photon flux (15-150 keV) in 342.7 sec: 4.67790E-02 ( -0.00726102 0.00727101 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.14248e-07 ( -1.35593e-07 1.4466e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.00625E-02 ( 0.0320372 1.94167 )
Epeak [keV] : 20.3503 ( -18.0395 5.93734 )
Norm@50keV : 1.99460E-02 ( )
------------------------------------------------------------
# Chi-Squared = 66.55 using 59 PHA bins.
# Reduced chi-squared = 1.188 for 56 degrees of freedom
# Null hypothesis probability = 1.579854e-01
Photon flux (15-150 keV) in 342.7 sec: 4.51856E-02 ( -0.0071196 0.0071257 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.19427e-07 ( -5.75839e-08 1.23362e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.384601 ( -2.01763 3.72339 )
beta : -9.99972 ( 11367.5 11377.5 )
Epeak [keV] : 21.0922 ( -18.0348 5.06103 )
Norm@50keV : 3.76291E-02 ( -0.0438589 36.3289 )
------------------------------------------------------------
# Chi-Squared = 66.48 using 59 PHA bins.
# Reduced chi-squared = 1.209 for 55 degrees of freedom
# Null hypothesis probability = 1.380081e-01
Photon flux (15-150 keV) in 342.7 sec: 4.533446E-02 ( -0.00706877 0.00673317 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.19519e-07 ( -1.12416e-07 7.43488e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.80154e-07
S(50-100 keV) = 3.48765e-07
T90 vs. Hardness ratio plot
T90 = 198.368000000715 sec.
Hardness ratio (energy fluence ratio) = 0.601159
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.718217
Count Ratio (50-100 keV) / (15-25 keV) = 0.0892883
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 320.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 320.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 320.000000
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:
-4.699400 338.000600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.5992 -62.8006 3.9 46.4 -130.8 3.4009 3.0 2.4 GX 301-2
244.9814 -15.6402 0.3 26.7 -14.3 11.3160 38.8 0.1 Sco X-1
255.9806 -37.9509 3.5 2.4 -11.0 0.9906 3.4 6.4 4U 1700-377
256.3789 -36.3355 2.5 3.9 2.9 1.2473 4.7 5.9 GX 349+2
263.1866 -24.7749 6.2 16.2 32.6 0.5341 1.9 9.8 GX 1+4
264.8587 -44.4470 14.8 7.1 142.5 0.2069 0.8 5.0 4U 1735-44
268.3558 -1.4460 2.6 40.0 30.2 2.3396 4.4 0.8 SW J1753.5-0127
270.3970 -25.0868 2.9 18.7 52.9 1.2733 4.0 6.1 GX 5-1
270.1308 -25.7519 4.0 18.0 53.5 0.8941 2.9 9.3 GRS 1758-258
274.0020 -14.0495 2.5 30.0 46.9 1.8738 4.5 0.8 GX 17+2
276.0322 -30.3221 3.6 18.2 75.9 1.0723 3.2 6.2 H1820-303
285.0168 -24.8751 2.4 27.8 77.9 1.9970 4.7 2.9 HT1900.1-2455
277.3438 -23.7991 1.8 23.5 64.8 2.2309 6.4 ------ UNKNOWN
257.7270 12.0633 2.9 52.2 13.3 4.1138 4.0 ------ UNKNOWN
312.7129 -70.7004 3.2 41.3 168.3 1.9172 3.7 ------ UNKNOWN
264.8442 -30.3031 1.7 11.6 47.4 1.9836 6.7 ------ UNKNOWN
274.2198 -55.3965 2.5 19.0 161.9 1.3712 4.7 ------ UNKNOWN
250.2133 10.8611 2.1 51.4 3.9 4.0727 5.4 ------ UNKNOWN
1.3068 -77.0349 3.6 54.1 177.1 3.4912 3.2 ------ UNKNOWN
255.2363 -41.6878 2.4 2.1 -124.3 1.4312 4.8 ------ UNKNOWN
242.1414 -11.8691 2.5 31.2 -16.7 1.4299 4.6 ------ UNKNOWN
UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
378.300600 758.200000
759.000000 963.074500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9846 -15.6350 0.3 23.4 -52.7 19.2117 36.2 0.4 Sco X-1
256.0052 -37.8280 1.6 10.5 -135.4 3.1003 7.1 1.3 4U 1700-377
256.4630 -36.3126 2.8 9.2 -130.1 1.6904 4.2 6.8 GX 349+2
263.1122 -24.7487 9.7 5.8 -12.9 0.5332 1.2 5.6 GX 1+4
264.7334 -44.4580 3.9 14.1 -176.9 1.2806 3.0 0.6 4U 1735-44
268.4209 -1.3670 3.4 29.2 10.2 1.5617 3.3 6.0 SW J1753.5-0127
270.2706 -25.1218 2.4 7.1 46.9 2.1151 4.8 2.7 GX 5-1
270.2783 -25.7384 3.7 6.6 50.5 1.4746 3.4 1.3 GRS 1758-258
274.0156 -14.0148 1.1 18.4 32.2 4.5784 10.2 1.4 GX 17+2
275.9098 -30.3526 2.1 9.6 95.8 2.2550 5.4 1.2 H1820-303
285.0485 -24.9191 3.8 18.7 80.9 1.6481 3.0 0.7 HT1900.1-2455
288.7701 10.9579 3.3 47.3 35.6 6.2631 3.5 1.8 GRS 1915+105
315.7725 -48.8398 2.7 42.4 133.5 6.2085 4.2 ------ UNKNOWN
305.5006 -43.6719 2.8 34.7 126.9 3.5901 4.1 ------ UNKNOWN
277.3296 -23.7986 2.1 12.9 65.4 2.2610 5.5 ------ UNKNOWN
264.8051 -30.3524 1.2 0.0 -143.6 4.7404 9.4 ------ UNKNOWN
261.9930 -51.3691 2.7 21.2 -172.3 1.7573 4.2 ------ UNKNOWN
199.9383 -83.8916 2.6 57.3 -170.6 9.2305 4.4 ------ UNKNOWN
244.9683 -16.9691 2.4 22.5 -55.3 2.4720 4.8 ------ UNKNOWN
233.5609 15.9306 3.6 55.2 -34.7 8.2440 3.2 ------ UNKNOWN
229.7220 7.4969 4.2 50.6 -44.7 7.0668 2.8 ------ UNKNOWN
UNKNOWN
Plot creation:
Wed Feb 17 13:15:13 EST 2010