Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/reduc_demo/6a_dirty.html
Äàòà èçìåíåíèÿ: Tue Apr 12 03:45:28 2016
Äàòà èíäåêñèðîâàíèÿ: Tue Apr 12 03:45:28 2016
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: ï ï ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ï ï
Australia Telescope National Facility

Imaging with a large configuration -
"dirty" image from the ATCA 6-km array

á 

The uv-coverage displayed in Fig. 4 leads to a high-resolution dirty image as shown in Fig. 5. Substructure becomes visible not only in the primary target, NGC 1511, but also in several background sources (e.g. the one to the right).


á 

á 
Fig. 5: ATCA 6A configuration dirty image of NGC 1511 and its surroundings. Note: The field of view displayed here is smaller than for the 375-m configuration (otherwise one would not see the details).
ASKAP
Public