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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
274.6969 -17.0635 0.0393 12.7 60.5 1.4653 4.9 TRIG_00361958
------------------------------------------
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)
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: 2.97617 ( -0.44832 0.546534 )
Norm@50keV : 1.64750E-04 ( -6.50377e-05 7.01697e-05 )
------------------------------------------------------------
# Chi-Squared = 58.66 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 57 degrees of freedom
# Null hypothesis probability = 4.144659e-01
Photon flux (15-150 keV) in 320 sec: 4.45305E-02 ( -0.00798321 0.00799298 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.26608e-07 ( -1.42001e-07 1.54363e-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: 1.61077 ( )
Epeak [keV] : 8.80622 ( )
Norm@50keV : 1.40829E-03 ( )
------------------------------------------------------------
# Chi-Squared = 58.52 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 56 degrees of freedom
# Null hypothesis probability = 3.832275e-01
Photon flux (15-150 keV) in 320 sec: 4.45124E-02 ( -0.0079801 0.0079899 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.91581e-07 ( -1.37677e-07 1.73802e-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 : -3.79557 ( 0.822496 3.18045 )
beta : -2.97607 ( -0.546334 0.447876 )
Epeak [keV] : 41.6389 ( -41.6389 -41.6389 )
Norm@50keV : 2.23935E-02 ( -0.00883337 0.00953611 )
------------------------------------------------------------
# Chi-Squared = 58.66 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 55 degrees of freedom
# Null hypothesis probability = 3.429108e-01
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: 2.97206 ( -0.41492 0.507618 )
Norm@50keV : 1.65886E-04 ( -6.37421e-05 6.91077e-05 )
------------------------------------------------------------
# Chi-Squared = 59.33 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 57 degrees of freedom
# Null hypothesis probability = 3.905108e-01
Photon flux (15-150 keV) in 320 sec: 4.47051E-02 ( -0.00752131 0.00754442 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.2977e-07 ( -1.40595e-07 1.53455e-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: 1.62051 ( )
Epeak [keV] : 8.35881 ( )
Norm@50keV : 1.46322E-03 ( )
------------------------------------------------------------
# Chi-Squared = 59.26 using 59 PHA bins.
# Reduced chi-squared = 1.058 for 56 degrees of freedom
# Null hypothesis probability = 3.574170e-01
Photon flux (15-150 keV) in 320 sec: 4.46883E-02 ( -0.007519 0.0075419 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.29744e-07 ( -1.40579e-07 1.53424e-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 : -2.96680 ( 0.822496 2.9668 )
beta : -2.97196 ( -0.507453 0.414436 )
Epeak [keV] : 40.4324 ( -40.4324 -40.4324 )
Norm@50keV : 2.25483E-02 ( -0.0086603 0.0093927 )
------------------------------------------------------------
# Chi-Squared = 59.33 using 59 PHA bins.
# Reduced chi-squared = 1.079 for 55 degrees of freedom
# Null hypothesis probability = 3.205776e-01
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: 2.97617 ( -0.44832 0.546534 )
Norm@50keV : 1.64750E-04 ( -6.50377e-05 7.01697e-05 )
------------------------------------------------------------
# Chi-Squared = 58.66 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 57 degrees of freedom
# Null hypothesis probability = 4.144659e-01
Photon flux (15-150 keV) in 320 sec: 4.45305E-02 ( -0.00798321 0.00799298 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.26608e-07 ( -1.42001e-07 1.54363e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61077 ( )
Epeak [keV] : 8.80622 ( )
Norm@50keV : 1.40829E-03 ( )
------------------------------------------------------------
# Chi-Squared = 58.52 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 56 degrees of freedom
# Null hypothesis probability = 3.832275e-01
Photon flux (15-150 keV) in 320 sec: 4.45124E-02 ( -0.0079801 0.0079899 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.91581e-07 ( -1.37677e-07 1.73802e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -3.79557 ( 0.822496 3.18045 )
beta : -2.97607 ( -0.546334 0.447876 )
Epeak [keV] : 41.6389 ( -41.6389 -41.6389 )
Norm@50keV : 2.23935E-02 ( -0.00883337 0.00953611 )
------------------------------------------------------------
# Chi-Squared = 58.66 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 55 degrees of freedom
# Null hypothesis probability = 3.429108e-01
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) = 2.09216e-07
S(50-100 keV) = 1.06356e-07
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 0.508355
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.539939
Count Ratio (50-100 keV) / (15-25 keV) = 0.123711
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] [']
244.9765 -15.6389 0.2 20.3 -57.4 14.3098 49.7 0.2 Sco X-1
255.9940 -37.8030 1.7 14.4 -144.8 1.8972 6.9 2.5 4U 1700-377
256.2505 -36.4155 3.1 13.1 -142.4 1.0833 3.7 8.9 GX 349+2
262.9324 -24.6827 2.9 1.2 -56.9 1.2012 4.0 5.6 GX 1+4
264.6986 -44.6060 3.4 19.4 -172.9 0.9649 3.4 9.5 4U 1735-44
268.4366 -1.4975 2.8 24.1 18.7 1.3532 4.1 4.9 SW J1753.5-0127
270.2390 -25.1100 1.9 5.5 98.5 1.7291 6.3 3.1 GX 5-1
270.2401 -25.6018 2.3 5.5 103.6 1.3535 5.0 9.1 GRS 1758-258
273.9417 -13.9687 2.6 14.5 49.3 1.3091 4.5 5.5 GX 17+2
276.0447 -30.2811 5.6 11.7 126.7 0.5692 2.1 8.1 H1820-303
284.9703 -24.9029 3.8 18.8 101.7 1.0435 3.0 3.7 HT1900.1-2455
288.8660 10.8622 3.7 43.4 44.9 2.3485 3.1 6.4 GRS 1915+105
254.2188 -15.8220 2.3 13.2 -38.4 1.3693 5.0 ------ UNKNOWN
215.4943 -38.4098 3.4 42.9 -111.9 4.5875 3.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
377.100600 963.045100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9905 -15.6384 0.3 28.5 -91.9 25.7116 38.0 0.6 Sco X-1
254.5599 35.3677 11.8 55.8 -20.2 1.5968 1.0 5.2 Her X-1
255.8926 -37.9007 4.6 26.6 -145.8 1.2666 2.5 5.6 4U 1700-377
256.3612 -36.3245 4.1 25.2 -143.9 1.3855 2.8 6.9 GX 349+2
263.0188 -24.7061 2.3 13.3 -127.4 2.4196 5.1 2.4 GX 1+4
264.9219 -44.5347 7.4 28.7 -165.8 0.7009 1.6 9.2 4U 1735-44
268.3114 -1.4770 2.0 16.8 -22.9 2.5195 5.7 3.7 SW J1753.5-0127
270.3172 -25.0413 1.5 8.9 -154.2 3.0130 7.7 2.9 GX 5-1
270.4124 -25.6886 2.3 9.5 -156.5 2.1037 5.2 6.8 GRS 1758-258
274.0679 -14.0437 2.4 3.1 -11.3 2.1798 4.9 3.6 GX 17+2
275.7557 -30.4039 5.1 13.4 175.6 0.9769 2.3 9.0 H1820-303
285.0748 -24.9473 4.7 12.5 130.4 1.0219 2.5 2.7 HT1900.1-2455
288.7736 10.9369 1.9 31.3 27.0 3.8990 6.2 1.5 GRS 1915+105
293.5804 23.1313 4.1 44.2 24.9 2.8653 2.8 ------ UNKNOWN
283.9406 24.3224 2.7 42.4 12.2 2.9523 4.2 ------ UNKNOWN
280.3443 37.9867 3.6 55.3 5.0 6.6656 3.2 ------ UNKNOWN
279.2431 33.8975 2.3 51.1 4.5 5.8703 4.9 ------ UNKNOWN
280.7966 -71.0468 3.1 54.1 177.2 6.8717 3.8 ------ UNKNOWN
238.0925 13.0113 3.2 47.0 -52.9 8.0803 3.6 ------ UNKNOWN
Plot creation:
Mon Feb 15 17:50:38 EST 2010