Focal Plane Arrays are arrays of receivers placed at the focus of a radio-telescope. Traditional radio-telescopes have only one receiver at the focus of the telescope, but radio-telescopes are now starting to be equipped with focal plane arrays, which are of three different types: multi-beam feed arrays, bolometer arrays, and the experimental phased-array feeds.
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Multi-beam feed arrays
Multi-beam feed arrays consist of a small array of feed horns at the focus of a radio-telescope. Each feed horn is connected to a receiver to measure the received power and each horn and receiver pair is sensitive to radio waves from a slightly different direction in the sky. A feed array with n receivers will increase the survey speed of the telescope by a factor of n, making them very powerful survey instruments. Because radio wavelengths are large, the resulting feed arrays are amongst the largest radio-astronomy receivers ever built. Examples include the multi-beam arrays on the Parkes Observatory, and the ALFA array at Arecibo Observatory, both of which have been used for major pulsar and Hydrogen line studies, such as HIPASS.
Bolometer Arrays
Bolometer arrays are arrays of bolometer receivers which measure the energy of incoming radio photons. They are typically used for astronomy at millimeter wavelengths. Examples include the SCUBA receiver on the James Clerk Maxwell Telescope and the LABOCA instrument on the APEX telescope.
Phased Array Feeds
Phased Array Feeds are an experimental type of focal plane array using phased array technology in which antenna elements are closely spaced so that they do not act independently, but instead act as sensors of the electromagnetic field across the focal plane of the telescope. The outputs of the receivers are then coherently combined in a beamformer with appropriate weights to synthesise several discrete beams. They are currently being developed for the Apertif upgrade to the Westerbork Synthesis Radio Telescope, and for the Australian Square Kilometre Array Pathfinder radio telescope.