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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
240.3309 -46.9302 0.0464 17.7 -14.0 0.2134 4.2 TRIG_00349441
------------------------------------------
Foreground time interval of the image:
0.000 16.384 (delta_t = 16.384 [sec])
Background time interval of the image:
-60.136 -35.136 (delta_t = 25.000 [sec])
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 16.384 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.61259 ( -1.0044 1.6169 )
Norm@50keV : 1.50433E-04 ( -0.00014775 0.000199401 )
------------------------------------------------------------
# Chi-Squared = 78.11 using 59 PHA bins.
# Reduced chi-squared = 1.370 for 57 degrees of freedom
# Null hypothesis probability = 3.321209e-02
Photon flux (15-150 keV) in 16.38 sec: 6.63299E-02 ( -0.0331102 0.0335084 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07446e-08 ( -2.1884e-08 2.55566e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 16.384 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.98526 ( )
Epeak [keV] : 18.5030 ( -3.88814 4.95301 )
Norm@50keV : 1133.09 ( -1133.25 528.211 )
------------------------------------------------------------
# Chi-Squared = 73.51 using 59 PHA bins.
# Reduced chi-squared = 1.313 for 56 degrees of freedom
# Null hypothesis probability = 5.828454e-02
Photon flux (15-150 keV) in 16.38 sec: 6.63035E-02 ( -0.0331125 0.033509 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07459e-08 ( -2.18873e-08 2.55536e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 16.384 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38534 ( 1.76739 1.76739 )
beta : -9.37167 ( 6.38463 16.3836 )
Epeak [keV] : 17.3534 ( -3.12915 4.98011 )
Norm@50keV : 540.078 ( -534.839 13862.8 )
------------------------------------------------------------
# Chi-Squared = 73.81 using 59 PHA bins.
# Reduced chi-squared = 1.342 for 55 degrees of freedom
# Null hypothesis probability = 4.605866e-02
Photon flux (15-150 keV) in 16.38 sec: 7.117975E-02 ( -0.0325691 0.0325803 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17095e-08 ( -1.77897e-08 1.92223e-08 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 16.384 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.61172 ( -0.974201 1.54709 )
Norm@50keV : 1.54849E-04 ( -0.000152294 0.000198905 )
------------------------------------------------------------
# Chi-Squared = 79.14 using 59 PHA bins.
# Reduced chi-squared = 1.388 for 57 degrees of freedom
# Null hypothesis probability = 2.779964e-02
Photon flux (15-150 keV) in 16.38 sec: 6.82377E-02 ( -0.0327021 0.0330931 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19567e-08 ( -2.17304e-08 2.538e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 16.384 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.98519 ( )
Epeak [keV] : 18.5148 ( -3.79338 4.76535 )
Norm@50keV : 1150.67 ( -1150.83 523.239 )
------------------------------------------------------------
# Chi-Squared = 74.30 using 59 PHA bins.
# Reduced chi-squared = 1.327 for 56 degrees of freedom
# Null hypothesis probability = 5.138905e-02
Photon flux (15-150 keV) in 16.38 sec: 6.82099E-02 ( -0.0327002 0.0330931 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19606e-08 ( -2.17345e-08 2.53744e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 16.384 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.36445 ( 1.80339 1.98548 )
beta : -9.37167 ( 6.50913 16.5086 )
Epeak [keV] : 17.4691 ( -2.69211 5.18738 )
Norm@50keV : 502.115 ( -497.527 12023.5 )
------------------------------------------------------------
# Chi-Squared = 74.60 using 59 PHA bins.
# Reduced chi-squared = 1.356 for 55 degrees of freedom
# Null hypothesis probability = 4.043095e-02
Photon flux (15-150 keV) in 16.38 sec: 7.117975E-02 ( -0.0325691 0.0325803 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17095e-08 ( -1.77897e-08 1.92223e-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: 3.61259 ( -1.0044 1.6169 )
Norm@50keV : 1.50433E-04 ( -0.00014775 0.000199401 )
------------------------------------------------------------
# Chi-Squared = 78.11 using 59 PHA bins.
# Reduced chi-squared = 1.370 for 57 degrees of freedom
# Null hypothesis probability = 3.321209e-02
Photon flux (15-150 keV) in 16.38 sec: 6.63299E-02 ( -0.0331102 0.0335084 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07446e-08 ( -2.1884e-08 2.55566e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.98526 ( )
Epeak [keV] : 18.5030 ( -3.88814 4.95301 )
Norm@50keV : 1133.09 ( -1133.25 528.211 )
------------------------------------------------------------
# Chi-Squared = 73.51 using 59 PHA bins.
# Reduced chi-squared = 1.313 for 56 degrees of freedom
# Null hypothesis probability = 5.828454e-02
Photon flux (15-150 keV) in 16.38 sec: 6.63035E-02 ( -0.0331125 0.033509 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07459e-08 ( -2.18873e-08 2.55536e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38534 ( 1.76739 1.76739 )
beta : -9.37167 ( 6.38463 16.3836 )
Epeak [keV] : 17.3534 ( -3.12915 4.98011 )
Norm@50keV : 540.078 ( -534.839 13862.8 )
------------------------------------------------------------
# Chi-Squared = 73.81 using 59 PHA bins.
# Reduced chi-squared = 1.342 for 55 degrees of freedom
# Null hypothesis probability = 4.605866e-02
Photon flux (15-150 keV) in 16.38 sec: 7.117975E-02 ( -0.0325691 0.0325803 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17095e-08 ( -1.77897e-08 1.92223e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.20915e-08
S(50-100 keV) = 3.73271e-09
T90 vs. Hardness ratio plot
T90 = 16.3840000033379 sec.
Hardness ratio (energy fluence ratio) = 0.308705
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0483781
Count Ratio (50-100 keV) / (15-25 keV) = -0.131617
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:
-60.136000 -35.136000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.3924 -62.9068 0.0 50.2 3.0 0.2037 1.2 10.9 GX 301-2
244.9798 -15.6457 0.2 14.3 146.0 2.7487 46.4 0.3 Sco X-1
256.0212 -37.8066 2.2 11.2 -70.2 0.3134 5.4 2.8 4U 1700-377
256.3173 -36.4303 7.3 10.5 -76.7 0.0948 1.6 5.7 GX 349+2
262.9978 -24.7650 237.3 15.5 -133.2 -0.0030 -0.0 1.3 GX 1+4
264.5885 -44.3094 12.9 20.3 -67.7 -0.0561 -0.9 10.7 4U 1735-44
268.4324 -1.4140 9.8 35.2 -167.7 0.0889 1.2 4.5 SW J1753.5-0127
270.2347 -25.0652 5.3 21.5 -125.1 0.1401 2.2 2.8 GX 5-1
270.2678 -25.8023 55.9 21.3 -123.1 -0.0136 -0.2 4.0 GRS 1758-258
273.9729 -13.8799 19.9 29.9 -144.2 0.0390 0.6 9.6 GX 17+2
276.0660 -30.5177 6.2 25.5 -109.0 -0.1380 -1.9 11.6 H1820-303
285.1792 -25.0872 0.0 34.5 -116.4 -0.1583 -1.6 12.7 HT1900.1-2455
288.8179 10.9023 4.8 57.6 -156.5 0.7373 2.4 2.8 GRS 1915+105
239.4737 19.4524 3.1 49.8 143.3 1.1092 3.7 ------ UNKNOWN
250.6986 14.0811 2.5 44.1 157.9 0.6078 4.7 ------ UNKNOWN
260.3540 23.6306 2.3 55.1 167.5 1.5916 5.1 ------ UNKNOWN
250.7433 0.4517 2.5 30.6 160.4 0.3430 4.6 ------ UNKNOWN
295.0006 -33.2787 2.6 41.1 -100.3 1.0791 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 16.384000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6107 -62.7301 7.7 50.1 3.2 -0.2308 -1.5 2.7 GX 301-2
244.9057 -15.5864 3.9 14.3 145.7 0.1655 3.0 5.3 Sco X-1
255.7379 -37.9228 0.0 11.1 -69.0 0.0817 1.6 12.7 4U 1700-377
256.6784 -36.3437 0.0 10.7 -78.0 -0.0162 -0.3 12.7 GX 349+2
263.1345 -24.8554 10.4 15.6 -132.7 0.0585 1.1 9.5 GX 1+4
264.5929 -44.2997 3.8 20.3 -67.7 0.1846 3.0 11.1 4U 1735-44
268.2122 -1.5223 5.6 35.0 -167.9 0.1370 2.0 10.2 SW J1753.5-0127
270.1725 -24.8932 5.8 21.5 -125.6 -0.1209 -2.0 12.7 GX 5-1
270.2809 -25.8088 3.7 21.4 -123.1 0.1869 3.1 4.1 GRS 1758-258
273.9491 -13.9794 6.0 29.9 -144.1 0.1186 1.9 4.8 GX 17+2
275.8342 -30.4882 18.7 25.3 -109.1 0.0413 0.6 8.7 H1820-303
285.1982 -24.9067 136.5 34.5 -116.7 0.0083 0.1 8.9 HT1900.1-2455
288.8446 10.8677 8.5 57.6 -156.4 -0.3746 -1.4 5.4 GRS 1915+105
262.5317 19.3525 2.6 51.6 171.4 0.7411 4.4 ------ UNKNOWN
221.1199 -71.4750 2.2 43.9 -16.6 0.4667 5.1 ------ UNKNOWN
227.9756 -73.9205 2.3 45.1 -20.8 0.4551 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
103.664600 231.884000
232.864000 302.933000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2309 -60.5497 3.9 41.4 4.8 0.8938 3.0 5.1 Cen X-3
186.6742 -62.7958 3.2 33.4 2.4 0.9658 3.6 1.6 GX 301-2
244.9731 -15.6417 0.3 31.5 149.2 11.3821 42.5 0.4 Sco X-1
256.0240 -37.8351 1.1 14.7 -161.8 2.0524 10.2 1.9 4U 1700-377
256.2692 -36.3665 15.6 15.9 -165.2 0.1491 0.7 8.7 GX 349+2
262.9223 -24.6107 7.0 28.7 -172.6 0.3317 1.6 9.4 GX 1+4
264.7544 -44.6058 94.0 17.2 -128.2 -0.0237 -0.1 9.4 4U 1735-44
268.4630 -1.4721 9.1 51.6 177.6 0.6773 1.3 5.8 SW J1753.5-0127
270.2575 -25.1193 3.0 32.2 -161.5 0.8249 3.8 2.8 GX 5-1
270.1997 -25.8637 4.1 31.6 -160.6 0.5954 2.8 9.1 GRS 1758-258
273.9808 -14.0991 5.2 43.2 -167.6 0.7077 2.2 4.0 GX 17+2
275.9511 -30.5195 5.6 31.9 -147.5 0.4852 2.1 9.2 H1820-303
285.0381 -24.9100 391.5 41.6 -145.4 0.0095 0.0 0.6 HT1900.1-2455
Plot creation:
Tue Feb 16 19:35:33 EST 2010