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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
237.7122 -54.3111 0.0083 45.8 -34.9 0.9121 23.0 TRIG_00341114
------------------------------------------
Foreground time interval of the image:
-1.212 0.172 (delta_t = 1.384 [sec])
Background time interval of the image:
-145.907 -1.212 (delta_t = 144.695 [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 0.008000
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 0.008000
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 0.008000
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 -1.212 sec. to 0.172 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.28234 ( -0.128602 0.134682 )
Norm@50keV : 3.74042E-02 ( -0.00325171 0.00319975 )
------------------------------------------------------------
# Chi-Squared = 56.14 using 59 PHA bins.
# Reduced chi-squared = 0.9850 for 57 degrees of freedom
# Null hypothesis probability = 5.071858e-01
Photon flux (15-150 keV) in 1.384 sec: 6.47309 ( -0.456092 0.457227 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.93122e-07 ( -3.64601e-08 3.67035e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.212 sec. to 0.172 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41049 ( -0.647263 0.568622 )
Epeak [keV] : 29.5690 ( )
Norm@50keV : 0.113803 ( )
------------------------------------------------------------
# Chi-Squared = 48.88 using 59 PHA bins.
# Reduced chi-squared = 0.8728 for 56 degrees of freedom
# Null hypothesis probability = 7.389572e-01
Photon flux (15-150 keV) in 1.384 sec: 6.20525 ( -0.48424 0.48557 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65686e-07 ( -3.93803e-08 4.01775e-08 ) ergs/cm2
Band function
Time interval is from -1.212 sec. to 0.172 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.41327 ( -0.592295 0.327085 )
beta : -9.37142 ( 9.99976 19.9998 )
Epeak [keV] : 29.5610 ( -4.92004 8.53557 )
Norm@50keV : 0.113266 ( -0.0545567 0.184099 )
------------------------------------------------------------
# Chi-Squared = 48.88 using 59 PHA bins.
# Reduced chi-squared = 0.8887 for 55 degrees of freedom
# Null hypothesis probability = 7.063176e-01
Photon flux (15-150 keV) in 1.384 sec: 6.20664 ( -0.48565 0.4842 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65041e-07 ( -3.92724e-08 4.00765e-08 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from -0.828 sec. to 0.172 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.34692 ( -0.111567 0.117442 )
Norm@50keV : 4.59719E-02 ( -0.00393473 0.00387636 )
------------------------------------------------------------
# Chi-Squared = 58.69 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 57 degrees of freedom
# Null hypothesis probability = 4.132859e-01
Photon flux (15-150 keV) in 1 sec: 8.24910 ( -0.4991 0.499163 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.43337e-07 ( -3.11137e-08 3.13546e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.828 sec. to 0.172 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45954 ( -0.538599 0.484046 )
Epeak [keV] : 24.9427 ( -19.538 7.54033 )
Norm@50keV : 0.153216 ( -0.0727781 0.164428 )
------------------------------------------------------------
# Chi-Squared = 48.08 using 59 PHA bins.
# Reduced chi-squared = 0.8586 for 56 degrees of freedom
# Null hypothesis probability = 7.651323e-01
Photon flux (15-150 keV) in 1 sec: 8.10518 ( -0.505 0.50488 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.18208e-07 ( 3.4379e-08 -4.18208e-07 ) ergs/cm2
Band function
Time interval is from -0.828 sec. to 0.172 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.45787 ( -0.436543 0.454478 )
beta : -10.00000 ( 4.20081e+08 4.20081e+08 )
Epeak [keV] : 24.9728 ( -19.5702 7.50386 )
Norm@50keV : 0.153507 ( -0.0673353 0.163982 )
------------------------------------------------------------
# Chi-Squared = 48.08 using 59 PHA bins.
# Reduced chi-squared = 0.8742 for 55 degrees of freedom
# Null hypothesis probability = 7.340666e-01
Photon flux (15-150 keV) in 1 sec: 7.96525 ( -0.6194 0.30947 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17422e-07 ( -3.4231e-08 3.4396e-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: 2.28234 ( -0.128602 0.134682 )
Norm@50keV : 3.74042E-02 ( -0.00325171 0.00319975 )
------------------------------------------------------------
# Chi-Squared = 56.14 using 59 PHA bins.
# Reduced chi-squared = 0.9850 for 57 degrees of freedom
# Null hypothesis probability = 5.071858e-01
Photon flux (15-150 keV) in 1.384 sec: 6.47309 ( -0.456092 0.457227 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.93122e-07 ( -3.64601e-08 3.67035e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41049 ( -0.647263 0.568622 )
Epeak [keV] : 29.5690 ( )
Norm@50keV : 0.113803 ( )
------------------------------------------------------------
# Chi-Squared = 48.88 using 59 PHA bins.
# Reduced chi-squared = 0.8728 for 56 degrees of freedom
# Null hypothesis probability = 7.389572e-01
Photon flux (15-150 keV) in 1.384 sec: 6.20525 ( -0.48424 0.48557 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65686e-07 ( -3.93803e-08 4.01775e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.41327 ( -0.592295 0.327085 )
beta : -9.37142 ( 9.99976 19.9998 )
Epeak [keV] : 29.5610 ( -4.92004 8.53557 )
Norm@50keV : 0.113266 ( -0.0547072 0.184099 )
------------------------------------------------------------
# Chi-Squared = 48.88 using 59 PHA bins.
# Reduced chi-squared = 0.8887 for 55 degrees of freedom
# Null hypothesis probability = 7.063176e-01
Photon flux (15-150 keV) in 1.384 sec: 6.20664 ( -0.48565 0.4842 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65041e-07 ( -3.92724e-08 4.00765e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.58735e-07
S(50-100 keV) = 1.30522e-07
T90 vs. Hardness ratio plot
T90 = 1.08400002121925 sec.
Hardness ratio (energy fluence ratio) = 0.822264
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.0656
Count Ratio (50-100 keV) / (15-25 keV) = 0.500641
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 0.008000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.008000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.008000
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:
-145.907400 -1.212000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9695 -15.6440 0.2 17.6 -93.8 10.7981 61.1 0.6 Sco X-1
254.6012 35.3482 12.8 51.0 -179.3 0.4587 0.9 7.0 Her X-1
256.0274 -37.7343 4.7 38.1 -64.0 -0.9090 -2.4 6.9 4U 1700-377
256.5956 -36.4893 124.2 37.6 -66.0 -0.0367 -0.1 8.7 GX 349+2
263.0056 -24.7431 1302.9 36.6 -87.5 -0.0039 -0.0 0.2 GX 1+4
268.5009 -1.4781 2265.5 40.8 -125.5 0.0016 0.0 8.1 SW J1753.5-0127
242.5929 41.8855 2.7 52.7 166.3 3.2724 4.2 ------ UNKNOWN
249.8159 35.7810 2.4 49.3 176.0 2.0386 4.9 ------ UNKNOWN
198.1517 -60.3882 2.8 56.0 -9.8 2.6648 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.212000 0.172000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9892 -15.6055 6.3 17.6 -93.9 -0.0317 -1.8 2.2 Sco X-1
254.4373 35.3624 3.6 50.9 -179.5 -0.1121 -3.2 1.6 Her X-1
255.7609 -37.9171 9.2 38.0 -63.5 0.0434 1.3 11.6 4U 1700-377
256.3798 -36.3735 7.6 37.4 -66.0 0.0531 1.5 4.0 GX 349+2
263.2067 -24.6720 0.0 36.8 -87.7 -0.0562 -1.4 11.6 GX 1+4
268.2971 -1.5585 20.9 40.6 -125.5 -0.0222 -0.6 7.6 SW J1753.5-0127
201.3273 1.6335 2.4 28.8 83.4 0.1083 4.9 ------ UNKNOWN
237.7122 -54.3111 0.5 45.8 -34.9 0.9121 23.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
488.092600 962.461800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.5353 -60.5836 6.2 35.1 56.5 1.6710 1.9 6.9 Cen X-3
186.6622 -62.7766 0.4 27.1 55.8 18.5574 31.6 0.4 GX 301-2
244.9769 -15.6497 0.2 39.1 -164.5 30.9093 49.7 0.6 Sco X-1
255.7471 -37.7473 0.0 20.6 -131.7 0.0865 0.2 12.8 4U 1700-377
256.3432 -36.4596 3.7 22.0 -132.3 1.5019 3.1 5.0 GX 349+2
262.8839 -24.7790 4.5 34.9 -133.2 1.6512 2.6 7.1 GX 1+4
264.6925 -44.5714 21.0 19.9 -103.8 -0.2527 -0.5 7.6 4U 1735-44
270.2491 -25.0574 2.5 37.8 -123.1 3.4695 4.6 2.3 GX 5-1
270.0741 -25.6810 0.0 37.2 -122.8 -0.6883 -0.9 12.9 GRS 1758-258
276.0349 -30.2472 8.1 36.4 -111.2 1.5476 1.4 9.2 H1820-303
193.0395 -33.7924 2.3 37.2 109.3 6.0811 5.1 ------ UNKNOWN
236.7972 -29.2156 2.7 25.1 -177.6 1.6507 4.2 ------ UNKNOWN
270.2012 -42.9279 2.5 24.0 -100.5 2.2481 4.6 ------ UNKNOWN
300.7994 -49.5058 3.9 37.9 -66.1 2.6969 3.0 ------ UNKNOWN
276.0999 -20.0871 3.3 44.9 -119.9 7.2732 3.5 ------ UNKNOWN
Plot creation:
Tue Feb 16 23:25:50 EST 2010