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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
Foreground time interval of the image:
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
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 186.632 sec. to 416.204 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 186.632 sec. to 416.204 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 186.632 sec. to 416.204 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 303.628 sec. to 304.628 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 303.628 sec. to 304.628 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 303.628 sec. to 304.628 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) =
S(50-100 keV) =
T90 vs. Hardness ratio plot
T90 = 229.571999996901 sec.
Hardness ratio (energy fluence ratio) =
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.132529
Count Ratio (50-100 keV) / (15-25 keV) = 0.0987019
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:
-199.499410 75.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9928 -15.6297 0.2 25.6 43.6 16.5792 56.4 1.0 Sco X-1
255.9107 -37.8448 1.1 10.4 -27.5 2.3593 10.4 3.6 4U 1700-377
256.5480 -36.5596 4.3 9.3 -22.2 0.6153 2.7 9.8 GX 349+2
262.9189 -24.7758 4.1 8.1 74.3 0.6778 2.9 5.2 GX 1+4
264.5663 -44.6161 0.0 12.5 -75.1 0.2411 1.0 12.5 4U 1735-44
268.3835 -1.5321 2.9 30.7 102.0 1.6521 4.0 4.9 SW J1753.5-0127
270.1007 -24.9989 11.4 7.8 122.8 -0.2516 -1.0 11.1 GX 5-1
270.3424 -25.7002 2.9 7.3 126.5 0.9961 4.1 3.4 GRS 1758-258
274.0261 -14.0520 1.5 19.4 120.8 2.0588 7.6 1.5 GX 17+2
275.9433 -30.3612 2.0 8.2 178.0 1.4174 5.8 1.0 H1820-303
285.0341 -25.0706 370.0 17.7 169.4 0.0083 0.0 9.0 HT1900.1-2455
226.3254 -1.4172 2.7 48.8 39.3 4.6926 4.3 ------ UNKNOWN
268.5508 -26.3222 1.6 6.1 115.5 1.7196 7.3 ------ UNKNOWN
329.7192 -27.4087 2.8 54.2 -159.0 3.3861 4.1 ------ UNKNOWN
274.6519 -60.0321 3.2 28.4 -90.1 1.3458 3.6 ------ UNKNOWN
324.7351 -37.5222 3.1 47.3 -148.1 2.3108 3.7 ------ UNKNOWN
196.5786 -48.7484 3.0 53.7 -31.4 4.1713 3.9 ------ UNKNOWN
200.4992 -52.2197 3.4 50.8 -35.3 2.9991 3.4 ------ UNKNOWN
325.8071 -52.3513 2.5 46.7 -127.8 5.2814 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
Post-slew image of 15-350 keV band
Time interval of the image:
146.500590 539.900580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9743 -15.6411 0.2 24.4 98.6 22.7090 52.7 0.3 Sco X-1
255.9894 -37.8771 0.8 15.7 26.8 4.3332 14.5 2.0 4U 1700-377
256.5638 -36.3808 5.6 14.3 29.9 0.6583 2.1 6.7 GX 349+2
262.9873 -24.7271 4.8 5.3 94.1 0.6993 2.4 1.6 GX 1+4
264.8340 -44.3121 4.2 18.2 -4.1 -0.7790 -2.8 9.2 4U 1735-44
268.3386 -1.5073 4.0 24.9 166.8 0.9434 2.9 3.7 SW J1753.5-0127
270.4491 -25.0976 5.9 2.1 -138.7 0.6495 2.0 9.0 GX 5-1
270.3942 -25.6073 4.9 1.8 -126.6 0.7752 2.4 9.5 GRS 1758-258
273.9737 -13.9815 2.5 13.4 -169.3 1.4655 4.6 3.8 GX 17+2
275.9563 -30.3612 1.7 7.6 -69.4 2.1760 6.7 1.7 H1820-303
285.2140 -24.7914 0.0 15.1 -105.0 -0.5463 -1.5 12.4 HT1900.1-2455
288.8269 10.9520 2.1 42.2 -162.3 3.1193 5.5 1.7 GRS 1915+105
233.0174 -4.5543 3.0 40.4 103.8 4.6208 3.9 ------ UNKNOWN
260.9429 -69.7684 2.2 43.6 -8.9 2.5174 5.2 ------ UNKNOWN
296.4870 -14.2463 3.9 28.8 -122.1 1.1601 2.9 ------ UNKNOWN
Plot creation:
Wed Jun 1 16:15:08 EDT 2011