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Australia Telescope Compact Array
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Flexible Scheduling at ATCA
Swap scheduling
At the Compact Array we are using a system which allows
some degree of flexible scheduling. During periods where
millimetre observations are scheduled, most millimetre projects will
be assigned partnering centimetre `swap' projects. These swap partners
can be either regular observations, or observations that are observed
in a service mode.
The rationale for swap schedule can be found in a memo by Bob Sault.
There are basically three different types of scheduled observations:
- Fixed centimetre projects: These are projects
which are scheduled into specific time slots and cannot be swapped.
- Millimetre projects: Each 3mm (and in some cases
12mm) project is matched with one or more "swap" projects that are
scheduled a few days later in the same configuration. If the
millimetre project meets with poor weather, the swap project(s) will
be observed instead, and the mm project moved into the slot vacated by
the swap project(s).
- Swap centimetre projects: These are centimetre
projects (involving regular or service observing) which can be
substituted for millimetre projects in poor weather. The
partnering between millimetre and centimetre projects is done as part
of the scheduling process by the Head of Science Operations.
Service Observing
The ATCA offers a limited form of service observing. A service observing
proposal will only be accepted where it can be used as a swap partner for
an unrelated 3-mm proposal. The authors of service proposals will be
expected to provide schedule files and instructions so that the observations
can be taken by an operator. Data taken in service mode will be sent
to the proposers by CD.
Proposals for service observing must be for a wavelength of 3cm or longer,
and be relatively straightforward. To request service observing the proposal
must state either:
- that service observing is desirable but not essential; or
- that the proposal is contingent on service observing time being
granted.
In the later case, time will not be allocated unless a 3-mm partner proposal
can be found. This is regardless of the scientific merit of the proposal.
Because of the nature of 3-mm astronomy, there is more potential for
service observing in compact
array configurations at Galactic time.
Swap rules
- Scheduled mm projects should only be abandoned in poor weather
(e.g. rain) or in case of mm equipment failure.
- The decision to switch to the swap project will be that of the mm
observer.
- If a swap is made to a regular observing project, the mm observer is
(by default) responsible for conducting the swap observation.
If a swap is not made, the proposers of the cm project are responsible for
observing their project at the originally scheduled time.
- If a swap is made to a service observing project, an operator will
conduct the swap observation.
- Proposers of swap cm projects may request (in advance)
to be contacted in the event of a swap, so as to be involved in the
observation.
- If a swap is made, the mm observer (or his/her collaborators) is
responsible for conducting the makeup mm observation at
the time originally designated for the swap project (generally about 2
days later).
- The decision to swap must be made at the start of the assigned
mm time, and cannot be changed once observing starts (except at the
discretion of the Head of Science Operations).
The table of swap assignments can be accessed via the
ATCA
schedule page.
Original: Jessica Chapman
Modified: Bob Sault (9-Jan-2004), Phil Edwards (22-oct-2008)