UV_TRACKS
[CLEAN\]UV_TRACKS Declination [Frequency [Astro_Station]] [/FRAME
[size]] [/HORIZON Elmin] [/HOUR_ANGLE Hmin [Hmax]] [/INTEGRATION t] [/STA-
TIONS ALL|list] [/TABLE [Name]] [/WEIGHT Mode] [/SIZE [Size1] [NantSize1]
[Size2] [NantSize2] ...] [/OFFSET offset]
Plot interferometer UV coverage as observed with the interferometer. The
default is for NOEMA, but the command is more general and can be used with
any array, especially ALMA or SMA.
Station coordinates are searched for in the file defined by the ASTRO_STA-
TIONS logical variable. Stations should be referred to by a mnemonic (e.g.
E003, W000 ...) given as arguments of UV_TRACKS. Note that with the con-
truction of the NOEMA track extension the mnemonic names changed from
[E,N,W]+2digits for the station number to [E,N,W]+3digits for the station
number. Old names are still accepted during a transition period.
The size of the antennas can be specified with the /SIZE option.
The /STATIONS option allows to use the ranks of the stations in the file
rather than the mnemonic names.
Some configuration files for NOEMA, ALMA, and SMA are distributed with
gildas and can be used as ASTRO_STATIONS files combined with UV_TRACKS ALL
to avoid typing a lot of station names (see HELP UV_TRACKS NOEMA|ALMA|SMA)
The coordinates of the most recently selected SOURCE or PLANET are consid-
ered. The frequency of the simulated observation is read from the Sic FRE-
QUENCY variable (which is also set by LET FREQUENCY command).
UV_TRACKS can be used iteratively, to simulate the observations of several
configurations. Option /FRAME indicate the start of a new observations: if
not present, configurations are being stacked on the current UV coverage.
The user may select another color pen to distringuish between the various
coverages. A sketch of the interferometer described by ASTRO_STATIONS is
also drawn, and the selected stations/antennas are highlighted.
Subsections