CSIRO logo
Australia Telescope Compact Array
Green End Bar
Spacer image

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:

  1. Fixed centimetre projects: These are projects which are scheduled into specific time slots and cannot be swapped.
  2. 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).
  3. 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:

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

  1. Scheduled mm projects should only be abandoned in poor weather (e.g. rain) or in case of mm equipment failure.
  2. The decision to switch to the swap project will be that of the mm observer.
  3. 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.
  4. If a swap is made to a service observing project, an operator will conduct the swap observation.
  5. 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.
  6. 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).
  7. 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)
© Copyright CSIRO Australia, 1994-2012.
Legal Notice and Disclaimer, Privacy Statement.