Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/sensitivity/ext.html
Дата изменения: Tue Apr 12 03:13:07 2016
Дата индексирования: Tue Apr 12 03:13:07 2016
Кодировка:

Поисковые слова: п п п п п п п п п п п п п
Australia Telescope National Facility

Extended sources


б 

All formulae derived above are valid for point sources at the phase centre of the interferometer. The behaviour of extended sources is slightly different.


б 

For a point source, the quantity , which can be expressed in units Jansky per beamsize, is independent of the beam size. This means that also the signal-to-noise ratio will be independent of the beam size.


б 

The same is not true for extended sources! For an extended source (with constant surface brightness) that is larger than the synthesised beam, the flux density per beam varies as a function of beam size as


б 

б 

where is the flux density per beam area and is the imaging sensitivity of the interferometer.


б 

RESOLUTION KILLS!

ASKAP
Public