Fig. 1.
60 µm emission of the Large Magellanic Cloud as constructed from
the
IRAS data.
Left: "Conventional" image produced by combining the IRAS survey
scans (angular resolution ∼5').
Right: High resolution (∼1.5') image produced by applying the maximum
entropy method
Fig. 2.
60 µm emission of the SW region of the Small Magellanic Cloud.
Above left: image produced by combining the survey scans (∼5').
Below left: image produced by applying MemSys5 to the survey data
(∼1.5').
Above right: image produced by applying MemSys5 to a combined data set
of survey and Pointed Observation data (∼1').
Below right: image produced by combining the
IRAS survey and the PO data
of only the two small 60 µm detectors (∼1.4';
the black polygons represent areas without data coverage)
[Bigger version!]
![[Fig. 1]](Pic/xmbraun_t_fig1.gif.pagespeed.ic.Q6xBv0lXrI.png)
![[Fig. 2]](Pic/mbraun_t_fig2.gif)
