Wed Jan 19 16:20:43 2000 : obs_anal.pro started
Filename = FITS/acisf1103_000N001_g02346Elt10s4G110_evt1.fits Output_prefix = obsid_1103 Output dir. = Obs_out Grating = HETG cd_width = 0.400000 mm cd_offset = 0.00000 mm Detector = ACIS-S Spatial coord = Sky * FLIPY IS set! * ROLLAXAY = -98.3243 OVERRIDE_ZERO keyword set LINE_ANALYSIS keyword set
Source of data: FITS/acisf1103_000N001_g02346Elt10s4G110_evt1.fits Reading FITS file: FITS/acisf1103_000N001_g02346Elt10s4G110_evt1.fits Tag names are: TIME CCD_ID NODE_ID EXPNO CHIPX CHIPY TDETX TDETY DETX DETY X Y PHAS PHA ENERGY PI FLTGRADE GRADE STATUS * Looks like ENERGY is in eV, converting to keV Creating ftime from TIME Total Events = 345772 Start time = 54542960. seconds Interval duration = 41037.708 seconds Ave Event Rate = 8.4257142 events/second
(Not CC mode data) * Changing the sign of SkyY Spatial coordinates are : SkyX, -SkyY pixel size = 23.9949 microns Processing method = Sky
Keeping TIME-in-range events, 100.000 %
(from 0.0000000 to 41037.708)
Start time = 54542960. seconds
Interval duration = 41037.708 seconds
Keeping STATUS=0 events, 96.0535 %
No QUALCODE selection
GRADE distribution:
0 : 137107, 41.28 %
1 : 0, 0.00 %
2 : 86013, 25.90 %
3 : 23525, 7.08 %
4 : 22157, 6.67 %
5 : 0, 0.00 %
6 : 63324, 19.07 %
Keeping GRADE = 0,2,3,4,6 events, 100.000 %
Keeping ENERGY selected events, 94.7246 %
(from 0.200000 to 10.0000 keV)
Linear binning from 0.200000 to 10.0000 keV
dE of one bin width = 0.0146000 keV
Min, Max, Unique EXPNOs: 3, 12665, 12663.0
Exposures and Events per Chip (w/selections)
MIN(EXPNO) MAX(EXPNO) TotalEvents TotalExps PoissExps * Ratio
CCD 0 :
CCD 1 :
CCD 2 :
CCD 3 :
CCD 4 : 3 12665 19227 9608 9888.46 0.971638
CCD 5 : 3 12665 110432 12662 12659.9 1.00016
CCD 6 : 3 12665 42628 12208 12225.1 0.998603
CCD 7 : 3 12665 60246 12527 12553.3 0.997903
CCD 8 : 3 12665 47824 12411 12372.1 1.00314
CCD 9 : 3 12665 34248 12554 11815.1 1.06254
* Expected number of exposures with one or more
detected events, assuming no telemetry-limit-dropped
exposures for this CCD.
Selected Events = 314605 Start time = 54542960. seconds Interval duration = 41037.708 seconds Ave Event Rate = 7.6662419 events/second Found no big ( > 15.0000 s) gaps in event data.
Zero-order search uses energies: 0.70 to 6.00 keV. Average SkyX,-SkyY gives x,y = 4273.36, -4462.33 Mouse clicked at x,y = 4244.38, -4226.99 Average SkyX,-SkyY gives x,y = 4234.91, -4197.07 Mouse clicked at x,y = 4253.99, -4206.36 Average SkyX,-SkyY gives x,y = 4251.52, -4204.37 Mouse clicked at x,y = 4247.13, -4206.32
==> MTA Monitor Task 5.2 <==
Zero-order Location SkyX,-SkyY ave-median = 4247.13, -4206.32
Events in Zero-order Region = 11302 Ave. Event Rate in Zero-order Region = 0.27540524 events/seconds SkyX,-SkyY RMS Radius = 55.5243 pixels Number of SkyX LRF pixels GT 10% of peak = 15 Number of SkyX LRF pixels GT 50% of peak = 4
* Rolling the AX,AY coordinates by -98.324 degrees.
Total Events = 314605
Start time = 54542960. seconds
Interval duration = 41037.708 seconds
Ave Event Rate = 7.6662419 events/second
The spatial coordinates to be used for grating spectra are:
AX, AY = SkyX,-98.324deg., -SkyY,-98.324deg.
AX,AY RMS Radius = 55.5243 pixels
Width of AX LRF at 10% of peak = 292.7 microns
Width of AX LRF at 50% of peak = 48.0 microns
Gaussian center = -0.877510 pixels
Gaussian fit FWHM = 172.2 microns
FWHM error = 2.0 microns
* Zero-order FWHM manually set to: 200.000 microns.
Width of Streak LRF at 10% of peak = 120.0 microns
Width of Streak LRF at 50% of peak = 38.4 microns
Gaussian center = -0.798679 pixels
Gaussian fit FWHM = 37.0 microns
FWHM error = 1.0 microns
Creating ISIS format: obsid_1103_Sky_strk_1d_isis.dat ... Creating ISIS format: obsid_1103_Sky_zo_1d_isis.dat ... * Streak fit used to offset aveAX
Creating ISIS format: obsid_1103_Sky_Zero_isis.dat ...
==> MTA Monitor Task 5.5 <==
Selecting events in the grating parts... cd_width = 0.400000 mm cd_offset = 0.00000 mm HEG_minus number of events = 13269 HEG_minus slope is -0.0914202, --> -5.22347 degrees on detector MEG_plus number of events = 35923 MEG_plus slope is 0.0827097, --> 4.72816 degrees on detector MEG_minus number of events = 50200 MEG_minus slope is 0.0831901, --> 4.75549 degrees on detector HEG_plus number of events = 10025 HEG_plus slope is -0.0920238, --> -5.25777 degrees on detector HEG_all number of events = 23294 HEG_all slope is -0.0915684, --> -5.23189 degrees on detector MEG_all number of events = 86123 MEG_all slope is 0.0827666, --> 4.73139 degrees on detector
Rowland spacing used is 8632.65 mm MEG Zero-order offset: 0.00000 pixels HEG Zero-order offset: 0.00000 pixels Use ACIS ENERGY for Order selection... MEG minus order selection keeps 88.4681 %, 44411 events MEG plus order selection keeps 90.9167 %, 32660 events HEG minus order selection keeps 84.9499 %, 11272 events HEG plus order selection keeps 88.6384 %, 8886 events
Estimating pileup level in dispersed spectra... MEG-minus Max rate: 0.202164 per frame MEG-plus Max rate: 0.108426 per frame HEG-minus Max rate: 0.0284293 per frame HEG-plus Max rate: 0.0262971 per frame
Constant d-Lambda binning from 0.400000 to 10.0000 keV E/dE of one bin width at 1 keV = 3332.78
==> MTA Monitor Task 5.7 <==
Smoothing the spectra by E/dE ~ 40.5623
==> MTA Monitor Task 5.4 <==
Creating obsid_1103_Sky_MEGm1_hist.rdb ... Creating ISIS format: obsid_1103_Sky_MEGm1_isis.dat ...
| Spectrum | Line Fits | E/dE vs E | Line list .txt or .rdb |
Creating obsid_1103_Sky_MEGp1_hist.rdb ... Creating ISIS format: obsid_1103_Sky_MEGp1_isis.dat ...
| Spectrum | Line Fits | E/dE vs E | Line list .txt or .rdb |
Creating obsid_1103_Sky_HEGm1_hist.rdb ... Creating ISIS format: obsid_1103_Sky_HEGm1_isis.dat ...
| Spectrum | Line Fits | E/dE vs E | Line list .txt or .rdb |
Creating obsid_1103_Sky_HEGp1_hist.rdb ... Creating ISIS format: obsid_1103_Sky_HEGp1_isis.dat ...
| Spectrum | Line Fits | E/dE vs E | Line list .txt or .rdb |
No Level 1.5 columns found in the file.
No Level 1.5 columns - cannot create L1.5 histograms.
Wed Jan 19 16:24:37 2000 : obs_anal.pro finished
