Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.eso.org/~chummel/oyster/manual/node239.html
Дата изменения: Tue Apr 28 19:12:50 2015
Дата индексирования: Sun Apr 10 20:40:29 2016
Кодировка:

Поисковые слова: enceladus
Visibilities next up previous contents
Next: Fringe delays Up: Introduction Previous: Frames   Contents

Visibilities

fringevis(bincounts),[k]

Function. Return complex visibility for bincounts. The parameter k selects a particular baseline, i.e. fringe frequency. Examples: v=fringevis(bincounts(*,0,*),7), which returns the (complex) visibility of channel 1, and the baseline with the frequency number 7. If no sub-array of bincounts is selected, then the returned visibility array has the same dimensions as the input, minus the bin index.
fringevissq(bincounts$<$_real$>$),[k,n]
Function. Return the (averaged) squared visibility amplitude for bincounts. The parameter n selects how many samples will be averaged.
visrotate(v, l, d)
Function. Return rotated complex visibility for input visibility $v$, wavelength scale $l$, and group delay $d$.



Christian Hummel 2015-04-28