Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/reduc_demo/allclean.html
Äàòà èçìåíåíèÿ: Tue Apr 12 03:45:35 2016
Äàòà èíäåêñèðîâàíèÿ: Tue Apr 12 03:45:35 2016
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ð ï ð ï ð ï ï ð ï ï ð ï ï ð ï ï ð ï ï ð ï ï ð ï
Australia Telescope National Facility

Imaging with a multi-configuration array -
"clean" image from a 7-configuration array

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Now the full source flux, both extended plus compact sources, is recovered by the observations. A residual error is visible in the form of concentric ellipses around the phase centre, which was placed 1 arcmin south of the galaxy centre.


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Fig. 9: ATCA multi-configuration cleaned image of NGC 1511 and its surroundings.
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