- ...
- Present address:
Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19,
Chile.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1992)
- The Australia Telescope is
funded by the Commonwealth of Australia for operation as a
National Facility managed by CSIRO.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
cube
- Note that the "standard'' procedure for the
production of "moment maps'' is to smooth the original
data cube and use a user-defined flux-density threshold in
that smoothed version as a "mask'' to circumscribe features
that are considered to be real emission, while data points
below the threshold are blanked. In this process, the
signal-to-background ratio of the moment maps is increased
significantly. However, since features below a certain
threshold are removed systematically, there is no measure
any more of the inherent thermal noise of the data. Such
blanked moment maps will be shown below. Here, in the
display of the total FOV, we want to present an image
including the true noise of the data, especially in the
region of particular interest, between NGC1792 and
NGC1808.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.