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Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://xmm.vilspa.esa.es/sas/7.0.0/doc/dpssflag/node4.html
Дата изменения: Thu Jun 29 00:04:28 2006 Дата индексирования: Sat Dec 22 09:29:33 2007 Кодировка: Поисковые слова: asteroid |
| Parameter | Mand | Type | Default | Constraints |
| srclisttable | yes | table | srclist.ds:SRCLIST | |
|
Name of the EPIC (combined) ML source list table
| ||||
| mfraclimit | no | real | 0.75 | |
|
Threshold value for MASKFRAC column. All sources with MASKFRAC | ||||
| brcolumn | no | string | RATE | |
|
Name of column to be used to define a circle of influence of a bright source (used to set flags 2 and 4)
| ||||
| op1 | no | string | sqrt | sqrt|none |
|
Operation to apply to 'brcolumn' to build the total expression to calculate the radius of the circle of influence to set flag 2 (and 4).
| ||||
| op2 | no | string | mul | add|mul|none |
|
Operation to apply to 'brfactor' to build the total expression to calculate the radius of the circle of influence to set flag 2 (and 4).
| ||||
| brfactor | no | real | 100. | |
|
Number by which the 'brcolumn' is multiplied to obtain the 'circle of influence' radius in arcs (for flag 2)
| ||||
| minrad | no | real | 10. | |
|
Minimum value (in arcs) of the 'circle of influence' of a source (for flag 2)
| ||||
| maxrad | no | real | 400. | |
|
Maximum value (in arcs) of the 'circle of influence' of a source (for flag 2)
| ||||
| extfactor | no | real | 1. | |
|
Number by which the column EXT is multiplied to obtain the 'circle of extended emission' radius in pixels (internally converted to arcs) (for flag 3 and 5)
| ||||
| extlimit | no | real | 1. | |
|
Threshold value in pixels for a source to be considered extended.
| ||||
| maxextrad | no | real | 200. | |
|
Maximum value (in arcs) of the 'circle of extended emission' of an extended source (for flag 3)
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| brlimit | no | real | 10000. | |
|
Number of counts from SCTS for a point source to be considered causing spurious extended sources around it as set by flag 4
| ||||
| brexfraction | no | real | 0.20 | |
|
Likely spurious extended sources flagged with flag 5 should have less than this fraction of the brighter extended source brightness.
| ||||
| fixext | no | real | 200. | |
|
Likely spurious extended sources flagged with flag 5 should be closer than this fixed distance to a brighter extended source.
| ||||
| detmlfraction | no | real | 0.9 | |
|
Likely spurious extended sources flagged with flag 6 should have (for just
one of the 15 images) more than this fraction of the summed detection
likelihood
| ||||
| badcolumn | no | string | CUTRAD | |
|
Name of column to be used to define the critical distance to a bad column in PN band 1 images (used to set flag 8)
| ||||
| badfactor | no | real | 1. | |
|
Number by which the 'badcolumn' is multiplied to obtain the critical distance in image pixels (for flag 8)
| ||||
| pnclosetobadon | no | bool | no | yes|no |
|
It switches flag 9 (close to bad column) on or off for PN
| ||||
| Parameter | Mand | Type | Default | Constraints |