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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
301.1588 +21.6843 0.0344 2.5 72.0 0.0267 5.6 TRIG_00332287
------------------------------------------
Foreground time interval of the image:
0.000 0.256 (delta_t = 0.256 [sec])
Background time interval of the image:
-114.779 -6.080 (delta_t = 108.699 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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 0.256000
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 0.256000
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 0.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84078 ( -0.593831 0.637506 )
Norm@50keV : 4.37453E-03 ( -0.00193919 0.00189958 )
------------------------------------------------------------
# Chi-Squared = 57.43 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 57 degrees of freedom
# Null hypothesis probability = 4.592758e-01
Photon flux (15-150 keV) in 0.256 sec: 0.612971 ( -0.228232 0.228232 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0309e-08 ( -4.37824e-09 4.72407e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.89271 ( )
Epeak [keV] : 31.0999 ( -5.03917 5.88414 )
Norm@50keV : 207.159 ( -207.161 87.9402 )
------------------------------------------------------------
# Chi-Squared = 49.37 using 59 PHA bins.
# Reduced chi-squared = 0.8817 for 56 degrees of freedom
# Null hypothesis probability = 7.220442e-01
Photon flux (15-150 keV) in 0.256 sec: 0.634926 ( -0.205506 0.20565 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.62414e-09 ( -2.59036e-09 2.68628e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98763 ( -166.337 -156.338 )
beta : -8.10127 ( 6.47272 4.09698 )
Epeak [keV] : 30.9391 ( -4.85665 6.01174 )
Norm@50keV : 247.740 ( -88.9256 213.513 )
------------------------------------------------------------
# Chi-Squared = 49.31 using 59 PHA bins.
# Reduced chi-squared = 0.8966 for 55 degrees of freedom
# Null hypothesis probability = 6.906773e-01
Photon flux (15-150 keV) in 0.256 sec: 0.640033 ( -0.221817 0.221852 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.57933e-09 ( -3.20566e-09 1.71366e-09 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84958 ( -0.581886 0.628537 )
Norm@50keV : 4.41157E-03 ( -0.00193582 0.0018974 )
------------------------------------------------------------
# Chi-Squared = 58.08 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.352227e-01
Photon flux (15-150 keV) in 0.256 sec: 0.620389 ( -0.226981 0.226987 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03955e-08 ( -4.36001e-09 4.70812e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.88858 ( )
Epeak [keV] : 30.9895 ( -4.97327 5.78188 )
Norm@50keV : 212.829 ( -212.831 87.0231 )
------------------------------------------------------------
# Chi-Squared = 49.86 using 59 PHA bins.
# Reduced chi-squared = 0.8903 for 56 degrees of freedom
# Null hypothesis probability = 7.051451e-01
Photon flux (15-150 keV) in 0.256 sec: 0.641616 ( -0.204277 0.204378 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.62665e-09 ( 2.7019e-09 -7.62665e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98908 ( -186.82 -176.82 )
beta : -8.16771 ( 6.5428 4.13161 )
Epeak [keV] : 30.8220 ( -4.78454 5.91311 )
Norm@50keV : 257.176 ( -257.213 301.083 )
------------------------------------------------------------
# Chi-Squared = 49.80 using 59 PHA bins.
# Reduced chi-squared = 0.9054 for 55 degrees of freedom
# Null hypothesis probability = 6.730613e-01
Photon flux (15-150 keV) in 0.256 sec: 0.640033 ( -0.221817 0.221852 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.57933e-09 ( -3.20566e-09 1.71366e-09 ) 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: 1.84078 ( -0.593831 0.637506 )
Norm@50keV : 4.37453E-03 ( -0.00193919 0.00189958 )
------------------------------------------------------------
# Chi-Squared = 57.43 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 57 degrees of freedom
# Null hypothesis probability = 4.592758e-01
Photon flux (15-150 keV) in 0.256 sec: 0.612971 ( -0.228232 0.228232 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0309e-08 ( -4.37824e-09 4.72407e-09 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.89271 ( )
Epeak [keV] : 31.0999 ( -5.03917 5.88414 )
Norm@50keV : 207.159 ( -207.161 87.9402 )
------------------------------------------------------------
# Chi-Squared = 49.37 using 59 PHA bins.
# Reduced chi-squared = 0.8817 for 56 degrees of freedom
# Null hypothesis probability = 7.220442e-01
Photon flux (15-150 keV) in 0.256 sec: 0.634926 ( -0.205506 0.20565 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.62414e-09 ( -2.59036e-09 2.68628e-09 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98763 ( -166.337 -156.338 )
beta : -8.10127 ( 6.47272 4.09698 )
Epeak [keV] : 30.9391 ( -4.85639 6.01097 )
Norm@50keV : 247.740 ( -88.9256 213.513 )
------------------------------------------------------------
# Chi-Squared = 49.31 using 59 PHA bins.
# Reduced chi-squared = 0.8966 for 55 degrees of freedom
# Null hypothesis probability = 6.906773e-01
Photon flux (15-150 keV) in 0.256 sec: 0.640033 ( -0.221817 0.221852 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.57933e-09 ( -3.20566e-09 1.71366e-09 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.94541e-09
S(50-100 keV) = 3.29124e-09
T90 vs. Hardness ratio plot
T90 = 0.255999982357025 sec.
Hardness ratio (energy fluence ratio) = 1.11741
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36872
Count Ratio (50-100 keV) / (15-25 keV) = -0.0129983
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 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-114.779400 -6.080000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5810 35.4618 5.0 41.0 -58.3 0.6620 2.3 9.4 Her X-1
268.3490 -1.4173 2.8 37.0 -122.1 0.8139 4.1 2.4 SW J1753.5-0127
270.3603 -25.1598 9.1 53.6 -146.6 -0.5924 -1.3 6.4 GX 5-1
270.4630 -25.9123 6.4 54.2 -147.2 0.9351 1.8 13.4 GRS 1758-258
273.8769 -14.0487 2700.0 42.5 -141.9 0.0005 0.0 7.5 GX 17+2
276.0615 -30.4336 5.0 55.7 -155.2 1.0852 2.3 8.1 H1820-303
284.9312 -24.8092 6.1 47.6 -161.9 0.4313 1.9 8.8 HT1900.1-2455
288.8374 10.9391 1.9 13.6 -134.0 0.6383 5.9 2.3 GRS 1915+105
299.5910 35.2058 0.3 14.4 4.6 4.6545 45.7 0.3 Cyg X-1
308.0965 40.8043 5.5 21.5 21.2 0.2428 2.1 8.9 Cyg X-3
326.1946 38.4118 6.2 29.5 48.7 0.2871 1.9 5.5 Cyg X-2
286.0598 -32.7340 2.5 54.9 -165.9 1.6010 4.7 ------ UNKNOWN
258.1368 6.5059 2.8 41.7 -103.0 1.9673 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.256000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5669 35.5398 0.0 41.1 -58.1 0.0197 1.6 13.0 Her X-1
268.2384 -1.5262 7.2 37.2 -122.1 -0.0145 -1.6 8.9 SW J1753.5-0127
270.2325 -25.1049 5.7 53.6 -146.5 -0.0451 -2.0 3.2 GX 5-1
270.3183 -25.8332 13.2 54.2 -147.0 -0.0202 -0.9 5.5 GRS 1758-258
274.1082 -14.0569 3.9 42.4 -142.2 -0.0278 -2.9 6.1 GX 17+2
275.7733 -30.2500 10.2 55.6 -154.8 -0.0233 -1.1 10.5 H1820-303
285.0727 -24.9513 18.1 47.7 -162.1 -0.0064 -0.6 2.7 HT1900.1-2455
288.9056 11.0993 9.8 13.5 -133.7 -0.0060 -1.2 11.2 GRS 1915+105
299.5433 35.2069 2.8 14.4 4.4 0.0193 4.1 2.3 Cyg X-1
307.9167 40.8163 0.0 21.5 20.8 -0.0035 -0.7 12.0 Cyg X-3
326.0805 38.2110 9.2 29.4 49.0 0.0088 1.3 7.9 Cyg X-2
301.1591 21.6845 2.1 2.5 72.0 0.0267 5.6 ------ UNKNOWN
290.3990 54.9763 2.1 34.7 -7.0 0.0320 5.5 ------ UNKNOWN
251.1115 61.5810 1.8 52.1 -25.1 0.0866 6.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
44.620590 963.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3758 35.3615 25.9 42.7 -52.1 0.7095 0.4 4.2 Her X-1
268.3472 -1.5792 3.7 39.5 -113.2 4.4914 3.1 7.7 SW J1753.5-0127
274.0276 -14.0341 4.3 44.5 -132.4 3.4222 2.7 1.3 GX 17+2
285.0683 -24.9632 4.7 49.2 -152.1 3.0508 2.4 3.1 HT1900.1-2455
288.7904 10.9727 1.2 15.9 -121.9 5.1129 9.9 1.7 GRS 1915+105
299.5938 35.2018 0.1 13.6 3.8 37.3058 81.8 0.2 Cyg X-1
308.0937 40.9630 1.8 20.2 24.4 3.4048 6.4 1.0 Cyg X-3
326.3558 38.3026 7.0 27.4 55.7 1.1819 1.7 8.7 Cyg X-2
336.5044 10.9429 3.1 35.6 110.5 4.5274 3.7 ------ UNKNOWN
327.9474 22.5630 2.6 24.9 91.6 3.1121 4.4 ------ UNKNOWN
313.2206 -20.1721 2.4 43.5 172.0 4.4068 4.8 ------ UNKNOWN
312.2196 -31.3956 3.8 54.2 176.9 6.0409 3.0 ------ UNKNOWN
Plot creation:
Wed Feb 17 01:49:28 EST 2010