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Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://xmm.vilspa.esa.es/sas/7.1.0/doc/eposcorr/node7.html
Дата изменения: Mon Jul 9 02:48:17 2007 Дата индексирования: Sat Dec 22 09:48:38 2007 Кодировка: Поисковые слова: crater |
| Parameter | Mand | Type | Default | Constraints |
| xrayset | yes | set | ||
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File name for the fits binary table containing X-ray source positions and their errors.
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| opticalset | yes | set | ||
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File name for the fits binary table containing optical source positions and their errors.
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| findrotation | no | boolean | no | |
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Search for a rotational offset or not? | ||||
| niter | no | integer | 3 | 1-8 |
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Once a solution is found a new iteration can be made using a smaller grid size.
This parameter determines the number of iterations.
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| maxoffset | no | real | 8.0 | 4.0-15.0 |
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Constraint on the maximum RA/DEC offset.
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| maxrotation | no | real | 1.0 | 0.5-4.0 |
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Constraint on the maximum rotational offset.
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| maxdist | no | real | 20.0 | 10.0-120.0 |
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All optical sources with distances | ||||
| maxposnerr | no | real | 20.0 | 1.0-120.0 |
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neglect xray sources with positional errors | ||||
| usemaxdist | no | boolean | yes | |
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Use maxdist to make a preselection of optical sources?
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| minbmagn | no | real | 0.0 | -2.0-30.0 |
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Preselect the optical list on basis of B Magnitude. Here the mininum is set.
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| maxbmagn | no | real | 26.0 | -2.0-30.0 |
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Preselect the optical list on basis of B Magnitude. Here the maximum is set.
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| usebmagn | no | boolean | no | |
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Use the B magnitude to make a preselection of optical sources?
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| bmag | no | string | Bmagn | |
| name of B magnitude column | ||||
| minrmagn | no | real | 0.0 | -2.0-30.0 |
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Preselect the optical list on basis of R Magnitude. Here the mininum is set.
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| maxrmagn | no | real | 26.0 | -2.0-30.0 |
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Preselect the optical list on basis of R Magnitude. Here the maximum is set.
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| usermagn | no | boolean | no | |
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Use the R magnitude to make a preselection of optical sources?
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| rmag | no | string | Rmagn | |
| name of R magnitude column | ||||
| makeimage | no | boolean | no | |
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yes: the grid containing likelihood values will be written as a fits image file
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| imagename | no | filename | likelihood_test.fits | constraints |
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the name of the image file containing the likelihood values
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| opticalra | no | string | CAT_RA | |
| column name of optical catalogue position RA | ||||
| opticaldec | no | string | CAT_DEC | |
| column name of optical catalogue position DEC | ||||
| opticalradecerr | no | string | CAT_RADEC_ERR | |
| column name of optical catalogue position error | ||||
| opticaltableext | no | string | RAWRES | |
| optical catalogue fits table extension | ||||
| xrayra | no | string | RA | |
| column name of X-ray source position RA | ||||
| xraydec | no | string | DEC | |
| column name of X-ray source position DEC | ||||
| xrayradecerr | no | string | RADEC_ERR | |
| column name of X-ray source position error | ||||
| xraytableext | no | string | SRCLIST | |
| X-ray source list fits table extension | ||||
| calculateoffsets | no | boolean | yes | |
| calculate offsets; if no: use offsets/rotation provided by input parameter | ||||
| raoffset | no | real | 0.0 | |
| RA offset (arcsec) to be used if caclulateoffsets=no | ||||
| decoffset | no | real | 0.0 | |
| DEC offset (arcsec) to be used if calculateoffsets=no | ||||
| rotation | no | real | 0.0 | |
| rotation angle (degrees) to be used if calculateoffsets=no | ||||
| withmatchtable | no | boolean | no | |
| write optional table of matched objects | ||||
| matchset | no | string | matches.fits | |
| name of matched objects file | ||||
| rawxsyserr | no | real | 1.5 | |
| systematic error of input X-ray positions | ||||
| minxsyserr | no | real | 0.2 | |
| irreducible systematic error of X-ray positions | ||||
| maxsig | no | real | 5.0 | |
| sigma cutoff for X-ray/optical matches | ||||
| usemaxsig | no | boolean | yes | |
| use sigma cutoff limit | ||||
| Parameter | Mand | Type | Default | Constraints |