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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
345.7138 -39.6894 0.0375 18.2 37.6 0.3960 5.1 TRIG_00534017
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
The mask-weighted light curves based on cleaned DPHs
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 124.708 sec. to 124.724 sec.
Usage: bat_spec_fit_sys_xspec12.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Cutoff power-law model
Time interval is from 124.708 sec. to 124.724 sec.
Usage: bat_spec_fit_cutoff_sys_xspec12.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Band function
Time interval is from 124.708 sec. to 124.724 sec.
Usage: bat_spec_fit_band_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Single BB
Usage: bat_spec_fit_bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Thermal bremsstrahlung (OTTB)
Usage: bat_spec_fit_brems_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Double BB
Usage: bat_spec_fit_2bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Peak spectrum fit
Power-law model
Time interval is from 124.218 sec. to 125.218 sec.
Usage: bat_spec_fit_sys_xspec12.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Cutoff power-law model
Time interval is from 124.218 sec. to 125.218 sec.
Usage: bat_spec_fit_cutoff_sys_xspec12.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Band function
Time interval is from 124.218 sec. to 125.218 sec.
Usage: bat_spec_fit_band_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Single BB
Usage: bat_spec_fit_bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Thermal bremsstrahlung (OTTB)
Usage: bat_spec_fit_brems_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Double BB
Usage: bat_spec_fit_2bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Cutoff power-law model
Band function
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.89992e-08
S(50-100 keV) = 6.11523e-08
T90 vs. Hardness ratio plot
T90 = 0.0119999647140503 sec.
Hardness ratio (energy fluence ratio) = 1.03649
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.19697
Count Ratio (50-100 keV) / (15-25 keV) = 0.625631
Mask shadow pattern
IMX = 2.598000899107398E-01, IMY = -2.003472186013460E-01
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:
-239.000000 71.000600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
82.5913 -50.5509 3.6 46.1 -145.1 1.5284 3.2 ------ UNKNOWN
274.3657 -42.3047 2.9 58.7 -25.9 6.1984 4.0 ------ UNKNOWN
89.7388 -45.8140 2.7 52.7 -146.4 3.6883 4.3 ------ UNKNOWN
268.4599 -59.0441 4.2 50.7 -44.5 3.4566 2.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
335.9152 -35.7936 2.2 26.3 29.7 0.4713 5.3 ------ UNKNOWN
351.4259 -52.0558 2.4 8.7 -4.0 0.3299 4.8 ------ UNKNOWN
70.9962 -27.8589 2.4 53.6 -175.6 1.1626 4.9 ------ UNKNOWN
342.9972 -64.2455 2.4 17.2 -51.5 0.3715 4.8 ------ UNKNOWN
99.5113 -74.9732 2.6 41.7 -108.7 1.4935 4.4 ------ UNKNOWN
96.3886 -58.3954 2.5 48.5 -130.2 1.6571 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
112.900600 340.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
275.9653 -30.4393 11.6 56.4 -30.5 1.3710 1.0 4.8 H1820-303
285.0399 -24.7128 11.9 52.4 -19.4 -0.4731 -1.0 12.5 HT1900.1-2455
310.3551 -3.8919 2.4 48.0 22.4 2.3831 4.9 ------ UNKNOWN
340.5197 -19.1595 2.5 21.0 59.6 0.8578 4.7 ------ UNKNOWN
323.0811 -21.5058 2.1 26.5 20.0 1.0178 5.5 ------ UNKNOWN
348.2155 -58.5317 3.9 18.9 -110.7 0.5395 3.0 ------ UNKNOWN
276.3128 -43.1621 3.2 50.6 -44.6 4.0149 3.7 ------ UNKNOWN
Plot creation:
Wed Sep 19 05:56:25 EDT 2012