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Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://xmm.vilspa.esa.es/sas/8.0.0/doc/emldetect/node5.html
Дата изменения: Wed Jul 2 04:42:18 2008 Дата индексирования: Fri Sep 5 20:45:24 2008 Кодировка: Поисковые слова: http www.astronomy.ru forum index.php topic 4644.0.html |
| Parameter | Mand | Type | Default | Constraints |
| imagesets | yes | filename list | image.fits | |
| Names of input EPIC fits images | ||||
| expimagesets | no | filename list | expimage.fits | |
| Names of exposure images | ||||
| detmasksets | no | filename list | detmask.fits | |
| Names of detection masks | ||||
| bkgimagesets | yes | filename list | bkgimage.fits | |
| Names of background maps | ||||
| boxlistset | yes | filename | eboxlist.fits | |
| Name of eboxdetect source list | ||||
| mllistset | yes | filename | emllist.fits | |
| Name of output emldetect source list | ||||
| mergedlistset | no | filename | mergedlist.fits | |
| Name of merged source list | ||||
| mlmin | no | float | 10.0 | [1.0 |
| Minimum detection likelihood for inclusion of source in output list | ||||
| dmlextmin | no | float | 10.0 | [1.0 |
| Required likelihood improvement for source extent | ||||
| scut | no | float | 0.9 | [0.4 |
| Source selection radius for multi-source fitting (expressed as fraction of the normalized PSF integrated
to the desired radius) | ||||
| ecut | no | float | 0.68 | [0.4 |
| Event cut-out radius for multi-source fitting (expressed as fraction of the normalized PSF integrated to
the desired cut-out radius) | ||||
| ecf | no | float | 1.0 | [0.001 |
| Energy conversion factors,
given in units of | ||||
| xidecf | no | float | 1.0 | [0.001 |
| XID band energy conversion factors,
given in units of | ||||
| useevents | no | binary | false | |
| Photon mode flag | ||||
| fitposition | no | binary | true | |
| Fit source positions | ||||
| fitextent | no | binary | false | |
| Fit source extent | ||||
| fitcounts | no | binary | true | |
| Fit source counts | ||||
| fitnegative | no | binary | false | |
| Allow fitted count rates to become negative | ||||
| determineerrors | no | binary | true | |
| Determine statisitical errors | ||||
| withexpimage | no | binary | true | |
| Use exposure maps | ||||
| withdetmask | no | binary | false | |
| Only sky pixels inside the detection mask will be used in the PSF fits if set to true | ||||
| withoffsets | no | boolean | false | |
| Controls whether the merged source list will be read | ||||
| withxidband | no | boolean | false | |
| Controls whether XID band output will be written | ||||
| withsourcemap | no | boolean | false | |
| Controls whether source maps (one per input image) will be written | ||||
| sourceimagesets | no | filename list | srcmap.fits | |
| Names of source maps (one per input image) | ||||
| usecalpsf | no | boolean | true | |
| True: read PSF from the calibration db; false: use hardcoded PSF | ||||
| extentmodel | no | string | gaussian | gaussian|beta |
| Model function for source extent | ||||
| minextent | no | float | 1.5 | [0.0 |
| Minimum allowed value for the extent parameter of an extent model in image pixels | ||||
| maxextent | no | float | 20.0 | [0.1 |
| Maximum allowed value for the extent parameter of an extent model in image pixels | ||||
| withhotpixelfilter | no | boolean | false | |
| if true, the likelihood contribution of the brightest pixel will be ignored (i.e., detections relying
on a single pixel will be disregarded) | ||||
| nmaxfit | no | integer | 1 | 1,6 |
| Max. number of sources to be fit simultaneously | ||||
| nmulsou | no | integer | 1 | 1,3 |
| Allow fit to split up one input source in maximum nmulsou sources | ||||
| pimin | no | integer | 2000 | [0 |
| Lower energy boundaries of exposure images; units: eV | ||||
| pimax | no | integer | 4500 | [0 |
| Higher energy boundaries of exposure images; units: eV | ||||
| hrpndef | no | integer | 1 2 2 3 3 4 | 0,10 |
| Array of six integer numbers
specifiying the upper and lower energy band for each of three hardness
ratios (PN) | ||||
| hrm1def | no | integer | 1 2 2 3 3 4 | 0,10 |
| Array of six integer numbers
specifiying the upper and lower energy band for each of three hardness
ratios (MOS1) | ||||
| hrm2def | no | integer | 1 2 2 3 3 4 | 0,10 |
| Array of six integer numbers
specifiying the upper and lower energy band for each of three hardness
ratios (MOS2) | ||||
| xidpndef | no | integer | 2 3 | 0,10 |
| energy bands used as xid band (PN) | ||||
| xidm1def | no | integer | 2 3 | 0,10 |
| energy bands used as xid band (MOS1) | ||||
| xidm2def | no | integer | 2 3 | 0,10 |
| energy bands used as xid band (MOS 2) | ||||
| xidfixed | no | boolean | false | |
| Run emldetect on XID band image with positions and source extent fixed to input values | ||||
| withthreshold | no | boolean | false | |
| Allow splitting up into multi-PSF fitting only for sources above threshold | ||||
| threshold | no | float | 20 | [1.0 |
| Value of threshold for multi-PSF fitting | ||||
| threshcolumn | no | string | LIKE | LIKE|SCTS|RATE |
| Column in input list, on which threshold will be applied | ||||
| withtwostage | no | boolean | false | |
| use two stage process for multi PSF (nmulsou > 1) fitting | ||||
| Parameter | Mand | Type | Default | Constraints |
Space separated list, sorted by instrument and energy band. I.e.,energy band 1 to energy band
of instrument one is followed by energy band one to
of instrument two.
One per instrument per energy band
One per instrument
A parameter value of 1.0 would thus correspond to an infinite radius.
Photon mode is not yet implemented in the current task version.