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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
299.1669 +34.2190 0.0128 41.7 -22.5 2.1920 15.1 TRIG_00343319
------------------------------------------
Foreground time interval of the image:
-5.799 71.201 (delta_t = 77.000 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 64.000000
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 64.000000
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
Multiple GTIs in the spectrum
tstart tstop
-91.556000 -83.450000
-73.000000 660.600000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88915 ( -0.0650942 0.0657759 )
Norm@50keV : 1.50178E-03 ( -5.28752e-05 5.25756e-05 )
------------------------------------------------------------
# Chi-Squared = 52.74 using 59 PHA bins.
# Reduced chi-squared = 0.9252 for 57 degrees of freedom
# Null hypothesis probability = 6.355779e-01
Photon flux (15-150 keV) in 741.7 sec: 0.214535 ( -0.00793792 0.00797351 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02399e-05 ( -3.58233e-07 3.58985e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-91.556000 -83.450000
-73.000000 660.600000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49504 ( -0.2535 0.302208 )
Epeak [keV] : 64.9949 ( -10.0611 47.5115 )
Norm@50keV : 2.33697E-03 ( -0.000645231 0.000764175 )
------------------------------------------------------------
# Chi-Squared = 47.45 using 59 PHA bins.
# Reduced chi-squared = 0.8473 for 56 degrees of freedom
# Null hypothesis probability = 7.850286e-01
Photon flux (15-150 keV) in 741.7 sec: 0.208378 ( -0.009016 0.00905 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.95977e-06 ( -4.14981e-07 4.12904e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-91.556000 -83.450000
-73.000000 660.600000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.53227 ( -0.259553 0.310521 )
beta : -2.47250 ( 2.45426 0.491127 )
Epeak [keV] : 66.4494 ( -14.4082 38.9251 )
Norm@50keV : 2.24394E-03 ( -0.00052533 0.000992008 )
------------------------------------------------------------
# Chi-Squared = 47.40 using 59 PHA bins.
# Reduced chi-squared = 0.8618 for 55 degrees of freedom
# Null hypothesis probability = 7.569570e-01
Photon flux (15-150 keV) in 741.7 sec: 0.208350 ( -0.008136 0.008395 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.94471e-06 ( -4.00444e-07 4.16168e-07 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from -61.376 sec. to -60.376 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93668 ( -0.500439 0.561795 )
Norm@50keV : 4.94932E-03 ( -0.00174666 0.0016481 )
------------------------------------------------------------
# Chi-Squared = 61.38 using 59 PHA bins.
# Reduced chi-squared = 1.077 for 57 degrees of freedom
# Null hypothesis probability = 3.218730e-01
Photon flux (15-150 keV) in 1 sec: 0.721599 ( -0.202706 0.202835 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.55302e-08 ( -1.47876e-08 1.54822e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -61.376 sec. to -60.376 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72543 ( -4.38998 0.426764 )
Epeak [keV] : 51.6679 ( )
Norm@50keV : 6.58190E-03 ( )
------------------------------------------------------------
# Chi-Squared = 61.38 using 59 PHA bins.
# Reduced chi-squared = 1.096 for 56 degrees of freedom
# Null hypothesis probability = 2.891333e-01
Photon flux (15-150 keV) in 1 sec: 0.719641 ( -0.201347 0.204363 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.50359e-08 ( -1.8984e-08 1.56969e-08 ) ergs/cm2
Band function
Time interval is from -61.376 sec. to -60.376 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99744 ( -748.999 -748.999 )
beta : -2.23085 ( -1.66873 0.665536 )
Epeak [keV] : 24.7080 ( -24.3827 10.4326 )
Norm@50keV : 878.115 ( -878.115 5.66804e+06 )
------------------------------------------------------------
# Chi-Squared = 60.21 using 59 PHA bins.
# Reduced chi-squared = 1.095 for 55 degrees of freedom
# Null hypothesis probability = 2.927254e-01
Photon flux (15-150 keV) in 1 sec: 0.713385 ( -0.205505 0.204145 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27529e-08 ( -1.35798e-08 1.48601e-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: 1.87714 ( -0.179243 0.186756 )
Norm@50keV : 1.74159E-03 ( -0.000207297 0.000203732 )
------------------------------------------------------------
# Chi-Squared = 52.75 using 59 PHA bins.
# Reduced chi-squared = 0.9255 for 57 degrees of freedom
# Null hypothesis probability = 6.350353e-01
Photon flux (15-150 keV) in 77 sec: 0.247550 ( -0.0256832 0.025709 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23282e-06 ( -1.44453e-07 1.46442e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02397 ( -0.803914 0.802453 )
Epeak [keV] : 50.7419 ( -12.4336 222.734 )
Norm@50keV : 5.14263E-03 ( -0.00503411 0.00919239 )
------------------------------------------------------------
# Chi-Squared = 49.84 using 59 PHA bins.
# Reduced chi-squared = 0.8899 for 56 degrees of freedom
# Null hypothesis probability = 7.059871e-01
Photon flux (15-150 keV) in 77 sec: 0.240555 ( -0.026597 0.026611 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.159e-06 ( -1.58797e-07 1.63155e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.23693 ( -0.440354 0.878496 )
beta : -10.00000 ( 2.98226e+11 2.98226e+11 )
Epeak [keV] : 52.9402 ( -14.216 206.786 )
Norm@50keV : 3.95160E-03 ( -0.00411493 0.0100538 )
------------------------------------------------------------
# Chi-Squared = 49.83 using 59 PHA bins.
# Reduced chi-squared = 0.9060 for 55 degrees of freedom
# Null hypothesis probability = 6.719183e-01
Photon flux (15-150 keV) in 77 sec: 0.240535 ( -0.026584 0.026631 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16955e-06 ( -1.65088e-07 1.64657e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.97635e-06
S(50-100 keV) = 3.21406e-06
T90 vs. Hardness ratio plot
T90 = 645.116000026464 sec.
Hardness ratio (energy fluence ratio) = 1.07987
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1228
Count Ratio (50-100 keV) / (15-25 keV) = 0.748277
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 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-5.799400 71.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5175 35.3060 5.4 40.6 -21.9 -0.3039 -2.1 7.2 Cyg X-1
307.9745 41.0549 8.0 32.0 -24.2 -0.1485 -1.4 8.7 Cyg X-3
326.3897 38.1950 0.0 25.9 -51.6 0.0631 0.6 12.8 Cyg X-2
74.6796 69.3493 2.7 34.9 118.1 0.8851 4.3 ------ UNKNOWN
73.7852 66.1129 2.7 36.1 123.3 0.9401 4.3 ------ UNKNOWN
350.6807 69.0770 3.1 10.3 80.1 0.3438 3.8 ------ UNKNOWN
307.3880 40.1455 2.2 32.9 -24.7 0.5621 5.3 ------ UNKNOWN
299.1669 34.2190 0.8 41.7 -22.5 2.1920 14.9 ------ UNKNOWN
285.8875 24.2861 2.7 56.5 -17.8 1.5781 4.3 ------ UNKNOWN
300.6266 26.8603 2.7 46.9 -30.1 0.8096 4.2 ------ UNKNOWN
37.7336 11.0624 3.1 59.3 -156.3 2.8157 3.7 ------ UNKNOWN
27.5466 10.9593 3.6 55.2 -145.4 1.9488 3.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
133.400600 903.050000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6269 35.3093 12.6 36.3 56.7 -0.9971 -0.9 8.5 Her X-1
268.4859 -1.4643 6.5 45.8 -2.8 1.7739 1.8 7.1 SW J1753.5-0127
274.0082 -14.0376 84.3 53.8 -17.4 0.1970 0.1 0.2 GX 17+2
288.8838 10.8346 5.8 25.2 -23.8 0.9574 2.0 8.3 GRS 1915+105
299.4591 35.1808 5.6 1.0 146.5 -1.0541 -2.1 6.6 Cyg X-1
308.1144 40.7712 25.3 9.7 176.6 -0.2114 -0.5 10.9 Cyg X-3
326.1080 38.4544 15.5 22.0 -157.0 0.3687 0.7 8.5 Cyg X-2
13.2302 53.3655 3.6 54.1 177.1 6.5251 3.2 ------ UNKNOWN
307.3580 40.2853 0.9 8.9 176.6 6.3658 13.6 ------ UNKNOWN
299.1517 34.3544 0.3 0.1 132.4 21.0189 41.1 ------ UNKNOWN
307.4305 36.9369 2.0 7.3 -162.5 2.7012 5.9 ------ UNKNOWN
275.7522 6.6601 2.0 35.0 -4.6 3.7206 5.8 ------ UNKNOWN
264.6789 -10.5341 2.8 55.4 -5.5 7.0470 4.2 ------ UNKNOWN
288.9149 9.9196 0.9 26.0 -24.6 5.9426 12.1 ------ UNKNOWN
Plot creation:
Tue Feb 16 22:39:21 EST 2010