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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
264.8735 -30.3004 0.0393 11.7 -157.3 1.2382 4.8 TRIG_00308797
------------------------------------------
Foreground time interval of the image:
0.000 178.230 (delta_t = 178.230 [sec])
179.000 320.000 (delta_t = 141.000 [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 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
Multiple GTIs in the spectrum
tstart tstop
0.000000 178.230000
179.000000 320.000000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.44248 ( -0.373859 0.420978 )
Norm@50keV : 1.81625E-04 ( -5.4975e-05 5.5303e-05 )
------------------------------------------------------------
# Chi-Squared = 44.08 using 59 PHA bins.
# Reduced chi-squared = 0.7733 for 57 degrees of freedom
# Null hypothesis probability = 8.948132e-01
Photon flux (15-150 keV) in 319.2 sec: 3.44611E-02 ( -0.00654063 0.00654141 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71244e-07 ( -1.31612e-07 1.39957e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 178.230000
179.000000 320.000000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.590152 ( )
Epeak [keV] : 25.0136 ( )
Norm@50keV : 2.45300E-02 ( )
------------------------------------------------------------
# Chi-Squared = 42.04 using 59 PHA bins.
# Reduced chi-squared = 0.7507 for 56 degrees of freedom
# Null hypothesis probability = 9.167397e-01
Photon flux (15-150 keV) in 319.2 sec: 3.308998E-02 ( 0.00660459 -0.03309 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.6893e-07 ( 1.72049e-07 -4.6893e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 178.230000
179.000000 320.000000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97056 ( -76.8729 -66.8732 )
beta : -3.31473 ( -2.50229 0.763369 )
Epeak [keV] : 24.0579 ( -6.43278 3.62536 )
Norm@50keV : 59.5708 ( -37.8112 47.4791 )
------------------------------------------------------------
# Chi-Squared = 39.35 using 59 PHA bins.
# Reduced chi-squared = 0.7155 for 55 degrees of freedom
# Null hypothesis probability = 9.449593e-01
Photon flux (15-150 keV) in 319.2 sec: 3.433717E-02 ( -0.00640991 0.0065359 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.97891e-07 ( -1.20364e-07 9.4879e-08 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 179.000 sec. to 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.45345 ( -0.359723 0.408841 )
Norm@50keV : 1.82930E-04 ( -5.47184e-05 5.51858e-05 )
------------------------------------------------------------
# Chi-Squared = 45.08 using 59 PHA bins.
# Reduced chi-squared = 0.7908 for 57 degrees of freedom
# Null hypothesis probability = 8.733260e-01
Photon flux (15-150 keV) in 319.2 sec: 3.49339E-02 ( -0.00631204 0.00631548 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.76865e-07 ( -1.30074e-07 1.38821e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 179.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.450971 ( -0.450679 1.85641 )
Epeak [keV] : 23.4221 ( )
Norm@50keV : 4.49666E-03 ( )
------------------------------------------------------------
# Chi-Squared = 42.84 using 59 PHA bins.
# Reduced chi-squared = 0.7651 for 56 degrees of freedom
# Null hypothesis probability = 9.018543e-01
Photon flux (15-150 keV) in 319.2 sec: 3.36193E-02 ( -0.0063607 0.0063648 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.73179e-07 ( -1.24928e-07 1.70973e-07 ) ergs/cm2
Band function
Time interval is from 179.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.81633 ( -22.3538 -12.366 )
beta : -3.16508 ( -2.37173 0.770332 )
Epeak [keV] : 22.6044 ( -5.18184 4.58394 )
Norm@50keV : 70.0561 ( -70.0561 17.6391 )
------------------------------------------------------------
# Chi-Squared = 40.32 using 59 PHA bins.
# Reduced chi-squared = 0.7332 for 55 degrees of freedom
# Null hypothesis probability = 9.308938e-01
Photon flux (15-150 keV) in 319.2 sec: 3.433717E-02 ( -0.00640991 0.0065359 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.97891e-07 ( -1.20364e-07 9.4879e-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: 2.44248 ( -0.373859 0.420978 )
Norm@50keV : 1.81625E-04 ( -5.4975e-05 5.5303e-05 )
------------------------------------------------------------
# Chi-Squared = 44.08 using 59 PHA bins.
# Reduced chi-squared = 0.7733 for 57 degrees of freedom
# Null hypothesis probability = 8.948132e-01
Photon flux (15-150 keV) in 319.2 sec: 3.44611E-02 ( -0.00654063 0.00654141 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71244e-07 ( -1.31612e-07 1.39957e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.590152 ( )
Epeak [keV] : 25.0136 ( )
Norm@50keV : 2.45300E-02 ( )
------------------------------------------------------------
# Chi-Squared = 42.04 using 59 PHA bins.
# Reduced chi-squared = 0.7507 for 56 degrees of freedom
# Null hypothesis probability = 9.167397e-01
Photon flux (15-150 keV) in 319.2 sec: 3.308998E-02 ( 0.00660459 -0.03309 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.6893e-07 ( 1.72049e-07 -4.6893e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97056 ( -76.873 -66.8732 )
beta : -3.31473 ( -2.50229 0.763369 )
Epeak [keV] : 24.0579 ( -6.46974 3.632 )
Norm@50keV : 59.5708 ( -37.8112 47.4791 )
------------------------------------------------------------
# Chi-Squared = 39.35 using 59 PHA bins.
# Reduced chi-squared = 0.7155 for 55 degrees of freedom
# Null hypothesis probability = 9.449593e-01
Photon flux (15-150 keV) in 319.2 sec: 3.433717E-02 ( -0.00640991 0.0065359 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.97891e-07 ( -1.20364e-07 9.4879e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.88358e-07
S(50-100 keV) = 1.38605e-07
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 0.735859
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.704701
Count Ratio (50-100 keV) / (15-25 keV) = 0.252749
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:
0.000000 178.230000
179.000000 320.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6472 -62.7530 1.6 46.4 24.4 4.1453 7.3 1.1 GX 301-2
244.9795 -15.6530 0.3 26.7 140.9 9.9768 33.9 0.8 Sco X-1
256.0027 -37.8486 3.1 2.5 146.0 0.8052 3.7 0.8 4U 1700-377
256.5398 -36.4067 2.3 3.8 160.1 1.0670 4.9 5.1 GX 349+2
263.1809 -24.6191 6.0 16.3 -172.4 0.4414 1.9 12.1 GX 1+4
264.6500 -44.3898 3.4 7.0 -62.3 0.7124 3.3 5.4 4U 1735-44
268.4205 -1.4872 3.7 40.0 -174.5 1.0663 3.2 3.8 SW J1753.5-0127
270.2223 -25.1027 2.6 18.6 -152.3 1.0229 4.4 3.6 GX 5-1
270.3008 -25.6916 4.5 18.1 -151.1 0.6203 2.7 3.1 GRS 1758-258
274.0250 -13.9999 4.1 30.0 -158.0 0.7393 2.8 2.5 GX 17+2
275.9106 -30.2752 2.6 18.2 -129.3 1.0857 4.4 5.6 H1820-303
285.0321 -24.9201 48.1 27.8 -126.9 0.0718 0.2 0.2 HT1900.1-2455
288.7625 10.9109 45.3 58.9 -155.2 0.4857 0.3 3.0 GRS 1915+105
244.1406 0.6370 2.4 42.5 148.3 2.3586 4.8 ------ UNKNOWN
266.8159 -27.3385 1.2 15.1 -157.3 2.3642 9.6 ------ UNKNOWN
267.1851 -26.6523 1.7 15.9 -157.5 1.6958 7.0 ------ UNKNOWN
261.7324 -74.2305 2.3 34.1 -14.4 1.2585 4.9 ------ UNKNOWN
277.3510 -23.7967 2.2 23.6 -140.0 1.2076 5.3 ------ UNKNOWN
61.0413 -83.4128 3.3 56.2 -14.4 3.2454 3.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
372.900590 885.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9865 -15.6373 0.3 23.4 119.6 15.9535 41.6 0.4 Sco X-1
255.9722 -37.8475 1.2 10.5 37.1 2.9908 9.4 0.7 4U 1700-377
256.4454 -36.3613 2.9 9.2 42.3 1.2208 4.1 3.7 GX 349+2
262.9725 -24.5916 9.2 6.0 158.6 0.3771 1.2 9.4 GX 1+4
264.5394 -44.4409 6.3 14.1 -4.1 0.5739 1.8 8.7 4U 1735-44
268.3746 -1.4870 3.9 29.1 -177.7 0.9772 3.0 2.1 SW J1753.5-0127
270.2718 -25.1164 2.5 7.1 -141.3 1.5292 4.9 2.3 GX 5-1
270.3832 -25.6503 22.7 6.8 -137.7 0.1990 0.6 7.1 GRS 1758-258
273.9931 -14.0233 2.2 18.4 -155.7 1.6282 5.3 1.1 GX 17+2
275.9571 -30.4113 2.1 9.6 -92.0 1.8146 5.5 3.1 H1820-303
284.8837 -25.0498 5.8 18.5 -106.8 0.6609 2.0 11.3 HT1900.1-2455
288.7023 10.8175 0.0 47.2 -152.2 -0.9755 -1.3 9.5 GRS 1915+105
249.1637 -15.5295 2.2 20.7 127.5 1.8750 5.2 ------ UNKNOWN
244.3831 -70.3491 2.7 41.6 5.2 2.1131 4.3 ------ UNKNOWN
259.8006 -29.7768 2.5 4.4 91.6 1.3385 4.6 ------ UNKNOWN
268.4860 25.1309 2.9 55.6 179.0 5.3852 4.0 ------ UNKNOWN
266.8577 -27.3406 1.8 3.5 -154.3 2.1896 6.5 ------ UNKNOWN
267.3230 -26.6115 2.0 4.4 -154.3 1.9694 5.9 ------ UNKNOWN
Plot creation:
Wed Feb 17 16:10:02 EST 2010