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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
248.1898 -47.4392 0.0259 9.5 112.8 1.7407 7.5 TRIG_00354542
------------------------------------------
Foreground time interval of the image:
0.000 320.000 (delta_t = 320.000 [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 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91569 ( -0.310704 0.333512 )
Norm@50keV : 2.90373E-04 ( -6.10662e-05 5.84141e-05 )
------------------------------------------------------------
# Chi-Squared = 76.59 using 59 PHA bins.
# Reduced chi-squared = 1.344 for 57 degrees of freedom
# Null hypothesis probability = 4.276959e-02
Photon flux (15-150 keV) in 320 sec: 4.19519E-02 ( -0.00665633 0.00665683 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.54429e-07 ( -1.691e-07 1.75999e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.53790 ( )
Epeak [keV] : 185.111 ( )
Norm@50keV : 1.44614E-04 ( )
------------------------------------------------------------
# Chi-Squared = 76.38 using 59 PHA bins.
# Reduced chi-squared = 1.364 for 56 degrees of freedom
# Null hypothesis probability = 3.647983e-02
Photon flux (15-150 keV) in 320 sec: 4.19358E-02 ( -0.0066538 0.0066546 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.5423e-07 ( -1.69085e-07 1.75997e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99856 ( -1324.29 -1324.29 )
beta : -2.12540 ( -0.666477 0.355588 )
Epeak [keV] : 23.7785 ( -23.7298 4.27681 )
Norm@50keV : 62.8934 ( -42.7217 184826 )
------------------------------------------------------------
# Chi-Squared = 75.56 using 59 PHA bins.
# Reduced chi-squared = 1.374 for 55 degrees of freedom
# Null hypothesis probability = 3.434037e-02
Photon flux (15-150 keV) in 320 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 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.92056 ( -0.297791 0.32105 )
Norm@50keV : 2.91659E-04 ( -6.08742e-05 5.8298e-05 )
------------------------------------------------------------
# Chi-Squared = 77.38 using 59 PHA bins.
# Reduced chi-squared = 1.358 for 57 degrees of freedom
# Null hypothesis probability = 3.751362e-02
Photon flux (15-150 keV) in 320 sec: 4.22263E-02 ( -0.00649023 0.00649026 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.58275e-07 ( -1.6834e-07 1.75304e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.31073 ( )
Epeak [keV] : 116.906 ( )
Norm@50keV : 1.82770E-04 ( )
------------------------------------------------------------
# Chi-Squared = 76.93 using 59 PHA bins.
# Reduced chi-squared = 1.374 for 56 degrees of freedom
# Null hypothesis probability = 3.319750e-02
Photon flux (15-150 keV) in 320 sec: 4.22109E-02 ( -0.0064882 0.0064882 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.58077e-07 ( -1.68326e-07 1.75293e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.78118 ( -10.6896 -10.6896 )
beta : -2.11251 ( -0.678963 0.360535 )
Epeak [keV] : 22.6952 ( -22.6952 4.94805 )
Norm@50keV : 58.6041 ( -10.2235 70.9441 )
------------------------------------------------------------
# Chi-Squared = 76.48 using 59 PHA bins.
# Reduced chi-squared = 1.391 for 55 degrees of freedom
# Null hypothesis probability = 2.929382e-02
Photon flux (15-150 keV) in 320 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: 1.91569 ( -0.310704 0.333512 )
Norm@50keV : 2.90373E-04 ( -6.10662e-05 5.84141e-05 )
------------------------------------------------------------
# Chi-Squared = 76.59 using 59 PHA bins.
# Reduced chi-squared = 1.344 for 57 degrees of freedom
# Null hypothesis probability = 4.276959e-02
Photon flux (15-150 keV) in 320 sec: 4.19519E-02 ( -0.00665633 0.00665683 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.54429e-07 ( -1.691e-07 1.75999e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.53790 ( )
Epeak [keV] : 185.111 ( )
Norm@50keV : 1.44614E-04 ( )
------------------------------------------------------------
# Chi-Squared = 76.38 using 59 PHA bins.
# Reduced chi-squared = 1.364 for 56 degrees of freedom
# Null hypothesis probability = 3.647983e-02
Photon flux (15-150 keV) in 320 sec: 4.19358E-02 ( -0.0066538 0.0066546 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.5423e-07 ( -1.69085e-07 1.75997e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99856 ( -1324.29 -1324.29 )
beta : -2.12540 ( -0.666477 0.355588 )
Epeak [keV] : 23.7785 ( -23.7298 4.27681 )
Norm@50keV : 62.8934 ( -42.7217 184826 )
------------------------------------------------------------
# Chi-Squared = 75.56 using 59 PHA bins.
# Reduced chi-squared = 1.374 for 55 degrees of freedom
# Null hypothesis probability = 3.434037e-02
Photon flux (15-150 keV) in 320 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) = 2.50557e-07
S(50-100 keV) = 2.65636e-07
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 1.06018
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.813078
Count Ratio (50-100 keV) / (15-25 keV) = 0.421355
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 320.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2587 -60.6551 3.3 35.1 -63.8 1.5449 3.5 2.6 Cen X-3
186.7173 -62.6103 48.7 27.1 -64.0 -0.0764 -0.2 9.7 GX 301-2
244.9906 -15.6529 1.1 39.0 75.7 10.5526 10.1 1.0 Sco X-1
255.9999 -37.8378 0.8 20.7 109.2 3.9343 13.6 0.7 4U 1700-377
256.4161 -36.3759 2.4 22.1 107.9 1.4098 4.8 3.0 GX 349+2
262.9537 -24.6346 3.3 35.1 106.9 1.9239 3.5 7.3 GX 1+4
264.7625 -44.5821 5.8 20.0 136.5 0.5572 2.0 8.0 4U 1735-44
270.1938 -25.0200 4.6 37.9 116.9 1.7750 2.5 6.1 GX 5-1
270.3306 -25.8561 4.9 37.2 117.8 1.5287 2.3 7.0 GRS 1758-258
275.8738 -30.3439 3.3 36.3 128.8 1.9598 3.5 3.0 H1820-303
285.0245 -24.9311 199.6 45.5 133.7 -0.0652 -0.1 0.9 HT1900.1-2455
248.1891 -47.4392 1.6 9.5 112.8 1.7391 7.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
369.400590 963.040900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.3080 -62.7203 14.7 36.8 -70.1 0.9976 0.8 10.0 GX 301-2
244.9768 -15.6341 0.4 31.9 61.7 23.7705 31.0 0.4 Sco X-1
255.9730 -37.8374 0.4 11.1 101.3 10.6162 27.4 0.8 4U 1700-377
256.3330 -36.4327 2.1 12.5 99.4 2.1873 5.6 5.0 GX 349+2
263.0266 -24.8061 2.6 25.5 100.3 2.6864 4.5 3.8 GX 1+4
264.6407 -44.3588 7.8 11.9 148.7 0.6362 1.5 7.0 4U 1735-44
270.3510 -25.1327 3.0 28.4 113.6 2.6248 3.9 4.8 GX 5-1
270.3933 -25.6407 6.5 28.0 114.2 1.2745 1.9 7.9 GRS 1758-258
274.1365 -13.9146 0.0 39.9 109.1 -1.2480 -0.8 10.5 GX 17+2
275.9640 -30.4013 2.4 27.3 129.0 2.8243 4.8 2.9 H1820-303
284.9174 -25.0469 4.6 36.6 133.0 -2.4403 -2.5 10.0 HT1900.1-2455
263.0481 -33.8317 2.0 17.6 112.5 2.6511 5.8 ------ UNKNOWN
265.8389 -38.3573 2.7 15.7 128.9 1.8709 4.3 ------ UNKNOWN
270.9736 -39.9528 3.4 18.0 141.5 1.5295 3.4 ------ UNKNOWN
203.5430 -31.9317 2.8 37.0 -14.2 2.3767 4.2 ------ UNKNOWN
353.3994 -78.5533 3.2 46.7 -127.7 8.4672 3.6 ------ UNKNOWN
Plot creation:
Tue Feb 16 13:09:21 EST 2010