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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
250.1056 -47.3038 0.0361 43.3 -173.5 0.0675 5.3 TRIG_00360435
------------------------------------------
Foreground time interval of the image:
0.000 0.512 (delta_t = 0.512 [sec])
Background time interval of the image:
-60.864 -4.864 (delta_t = 56.000 [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)
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 0.512 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.72221 ( -0.702107 0.934004 )
Norm@50keV : 4.36947E-03 ( -0.00257432 0.00276431 )
------------------------------------------------------------
# Chi-Squared = 56.50 using 59 PHA bins.
# Reduced chi-squared = 0.9913 for 57 degrees of freedom
# Null hypothesis probability = 4.936821e-01
Photon flux (15-150 keV) in 0.512 sec: 0.989732 ( -0.363818 0.363819 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.39876e-08 ( -9.91805e-09 1.0948e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.512 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.325324 ( 0.378808 2.39667 )
Epeak [keV] : 23.9668 ( )
Norm@50keV : 0.501786 ( )
------------------------------------------------------------
# Chi-Squared = 54.76 using 59 PHA bins.
# Reduced chi-squared = 0.9779 for 56 degrees of freedom
# Null hypothesis probability = 5.218957e-01
Photon flux (15-150 keV) in 0.512 sec: 0.941084 ( -0.345203 0.359216 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03576e-08 ( -7.68404e-09 1.03746e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.512 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.48929 ( 0.813639 0.813639 )
beta : -9.99997 ( 126112 126122 )
Epeak [keV] : 25.5513 ( -20.5102 12.9331 )
Norm@50keV : 3.17406 ( -2.9345 421.45 )
------------------------------------------------------------
# Chi-Squared = 54.72 using 59 PHA bins.
# Reduced chi-squared = 0.9949 for 55 degrees of freedom
# Null hypothesis probability = 4.852906e-01
Photon flux (15-150 keV) in 0.512 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 0.512 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.74523 ( -0.688198 0.918609 )
Norm@50keV : 4.39466E-03 ( -0.00256516 0.00276716 )
------------------------------------------------------------
# Chi-Squared = 57.30 using 59 PHA bins.
# Reduced chi-squared = 1.005 for 57 degrees of freedom
# Null hypothesis probability = 4.637774e-01
Photon flux (15-150 keV) in 0.512 sec: 1.01088 ( -0.359233 0.359273 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43269e-08 ( -9.82129e-09 1.08721e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.512 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.160783 ( 0.210871 2.22097 )
Epeak [keV] : 23.1296 ( )
Norm@50keV : 0.416533 ( )
------------------------------------------------------------
# Chi-Squared = 55.61 using 59 PHA bins.
# Reduced chi-squared = 0.9930 for 56 degrees of freedom
# Null hypothesis probability = 4.896857e-01
Photon flux (15-150 keV) in 0.512 sec: 0.967075 ( -0.346461 0.353275 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07478e-08 ( -7.66628e-09 9.44855e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.512 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.54028 ( 0.050251 0.050251 )
beta : -6.95011 ( 5.94236 15.9421 )
Epeak [keV] : 25.8068 ( -22.2915 13.3026 )
Norm@50keV : 3.40653 ( -3.40674 368.159 )
------------------------------------------------------------
# Chi-Squared = 55.58 using 59 PHA bins.
# Reduced chi-squared = 1.011 for 55 degrees of freedom
# Null hypothesis probability = 4.527794e-01
Photon flux (15-150 keV) in 0.512 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: 2.72221 ( -0.702107 0.934004 )
Norm@50keV : 4.36947E-03 ( -0.00257432 0.00276431 )
------------------------------------------------------------
# Chi-Squared = 56.50 using 59 PHA bins.
# Reduced chi-squared = 0.9913 for 57 degrees of freedom
# Null hypothesis probability = 4.936821e-01
Photon flux (15-150 keV) in 0.512 sec: 0.989732 ( -0.363818 0.363819 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.39876e-08 ( -9.91805e-09 1.0948e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.325324 ( 0.378808 2.39667 )
Epeak [keV] : 23.9668 ( )
Norm@50keV : 0.501786 ( )
------------------------------------------------------------
# Chi-Squared = 54.76 using 59 PHA bins.
# Reduced chi-squared = 0.9779 for 56 degrees of freedom
# Null hypothesis probability = 5.218957e-01
Photon flux (15-150 keV) in 0.512 sec: 0.941084 ( -0.345203 0.359216 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03576e-08 ( -7.68404e-09 1.03746e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.48929 ( 0.813639 0.813639 )
beta : -9.99997 ( 126112 126122 )
Epeak [keV] : 25.5513 ( -20.5224 12.9333 )
Norm@50keV : 3.17406 ( -2.9345 421.45 )
------------------------------------------------------------
# Chi-Squared = 54.72 using 59 PHA bins.
# Reduced chi-squared = 0.9949 for 55 degrees of freedom
# Null hypothesis probability = 4.852906e-01
Photon flux (15-150 keV) in 0.512 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) = 8.06067e-09
S(50-100 keV) = 4.88612e-09
T90 vs. Hardness ratio plot
T90 = 0.51199996471405 sec.
Hardness ratio (energy fluence ratio) = 0.606168
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.750923
Count Ratio (50-100 keV) / (15-25 keV) = 0.0783368
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:
-60.864000 -4.864000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9744 -15.6368 0.5 23.9 -124.7 2.6089 25.4 0.4 Sco X-1
254.5224 35.4067 11.5 43.8 -26.1 0.1615 1.0 5.0 Her X-1
255.8998 -37.8254 2.9 32.9 -173.7 0.4692 4.0 4.3 4U 1700-377
256.2924 -36.5167 5.6 31.6 -173.3 0.2185 2.1 8.9 GX 349+2
262.9929 -24.7310 2.4 18.6 -177.7 0.4219 4.8 1.2 GX 1+4
264.7437 -44.5002 8.2 37.9 172.5 -0.1726 -1.4 3.0 4U 1735-44
268.4476 -1.3677 6.3 5.4 -1.1 0.1493 1.8 7.0 SW J1753.5-0127
270.2905 -25.0219 2.0 18.5 161.4 0.5042 5.8 3.5 GX 5-1
270.2817 -25.7679 5.4 19.3 161.8 0.1874 2.1 1.9 GRS 1758-258
273.9511 -13.9410 4.9 9.6 128.8 0.2125 2.4 6.5 GX 17+2
275.7681 -30.4586 5.9 25.0 152.3 0.1955 1.9 9.8 H1820-303
285.1747 -25.0583 6.2 24.9 128.7 0.2239 1.9 11.2 HT1900.1-2455
288.8058 10.9201 0.9 27.5 39.6 1.3809 12.9 1.6 GRS 1915+105
299.5941 35.2348 2.6 51.7 22.8 1.8156 4.5 2.0 Cyg X-1
263.2290 -15.9967 2.6 10.2 -166.7 0.3771 4.4 ------ UNKNOWN
230.6511 -23.4479 2.4 39.2 -130.1 0.8041 4.7 ------ UNKNOWN
225.8242 -9.6826 3.5 41.4 -107.8 1.3240 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9321 -15.7742 5.1 23.9 -125.0 0.0208 2.3 8.5 Sco X-1
254.3654 35.2005 4.5 43.7 -26.4 -0.0354 -2.6 9.6 Her X-1
256.1058 -37.9325 13.3 32.9 -174.0 -0.0083 -0.9 7.7 4U 1700-377
256.2978 -36.3595 19.1 31.4 -173.2 -0.0056 -0.6 7.7 GX 349+2
263.1573 -24.7964 13.8 18.6 -178.2 -0.0061 -0.8 8.6 GX 1+4
264.7068 -44.5974 8.1 38.0 172.5 0.0169 1.4 9.0 4U 1735-44
268.2035 -1.5183 7.4 5.2 -3.5 0.0117 1.6 10.6 SW J1753.5-0127
270.1441 -24.9822 11.9 18.5 161.8 0.0070 1.0 9.6 GX 5-1
270.3832 -25.7502 7.1 19.3 161.5 0.0125 1.6 4.4 GRS 1758-258
273.8312 -14.1554 46.3 9.7 130.1 0.0019 0.2 12.4 GX 17+2
275.7345 -30.4907 67.9 25.0 152.4 -0.0015 -0.2 12.3 H1820-303
284.9135 -24.9829 3.3 24.7 128.9 0.0341 3.5 7.6 HT1900.1-2455
288.6661 11.0271 7.3 27.5 39.3 0.0161 1.6 9.2 GRS 1915+105
299.7357 35.3007 0.0 51.8 22.9 -0.0600 -1.7 9.3 Cyg X-1
302.2081 -39.6852 2.8 45.3 131.3 0.1430 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.736590 302.186000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.5659 -60.6973 13.0 45.5 -138.0 -0.4881 -0.9 8.6 Cen X-3
186.7875 -62.7148 2.7 37.5 -138.2 1.5625 4.3 4.9 GX 301-2
244.9866 -15.6337 0.2 32.0 -9.8 10.9132 47.9 0.6 Sco X-1
255.9552 -37.7984 1.5 10.4 25.9 1.5023 7.6 3.1 4U 1700-377
256.3149 -36.3772 5.8 11.9 24.6 0.4148 2.0 6.4 GX 349+2
263.0379 -24.7187 1.6 24.8 28.5 1.5931 7.2 2.3 GX 1+4
264.6240 -44.4818 2.6 10.5 79.2 0.9021 4.5 5.4 4U 1735-44
268.3784 -1.4730 5.0 48.5 24.3 1.3759 2.3 1.4 SW J1753.5-0127
270.2351 -25.0889 3.7 27.4 42.3 0.7370 3.1 2.7 GX 5-1
270.2432 -25.7348 4.2 26.8 43.0 0.6497 2.7 3.2 GRS 1758-258
274.0303 -14.0386 3.8 38.8 38.5 1.2348 3.0 1.4 GX 17+2
276.0811 -30.3138 18.3 26.2 58.4 0.1750 0.6 8.7 H1820-303
284.8887 -24.9750 15.6 35.4 62.8 0.3475 0.7 8.7 HT1900.1-2455
276.1848 -19.6079 2.6 34.9 46.0 1.5115 4.4 ------ UNKNOWN
315.9124 -73.3068 2.8 38.4 154.6 1.5509 4.2 ------ UNKNOWN
234.1309 -56.4365 2.7 13.4 -139.3 0.8048 4.2 ------ UNKNOWN
203.8204 -36.2075 3.7 35.7 -89.5 1.9229 3.2 ------ UNKNOWN
Plot creation:
Mon Feb 15 19:21:50 EST 2010