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Proceedings Article

The Allen Telescope Array

[+] Author Affiliations
David R. DeBoer, John Dreher, Jill Tarter, Michael Davis, G. Girmay-Keleta, Larry R. D'Addario, Gerry R. Harp, Rob Ackermann

SETI Institute (USA)

William J. Welch, Leo Blitz, Matt Fleming, Douglas Bock, Geoffrey Bower, John Lugten, Greg Engargiola, Doug Thornton

Univ. of California/Berkeley (USA)

Sander Weinreb, Niklas Wadefalk

Jet Propulsion Lab. (USA)

Proc. SPIE 5489, Ground-based Telescopes, 1021 (September 28, 2004); doi:10.1117/12.551737
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From Conference Volume 5489

  • Ground-based Telescopes
  • Jacobus M. Oschmann, Jr.
  • USA | June 21, 2004


The Allen Telescope Array, originally called the One Hectare Telescope (1hT) [1] will be a large array radio telescope whose novel characteristics will be a wide field of view (3.5 deg-GHz HPBW), continuous frequency coverage of 0.5 - 11 GHz, four dual-linear polarization output bands of 100 MHz each, four beams in each band, two 100 MHz spectral correlators for two of the bands, and hardware for RFI mitigation built in. Its scientific motivation is for deep SETI searches and, at the same time, a variety of other radio astronomy projects, including transient (e.g. pulsar) studies, HI mapping of the Milky Way and nearby galaxies, Zeeman studies of the galactic magnetic field in a number of transitions, mapping of long chain molecules in molecular clouds, mapping of the decrement in the cosmic background radiation toward galaxy clusters, and observation of HI absorption toward quasars at redshifts up to z=2. The array is planned for 350 6.1-meter dishes giving a physical collecting area of about 10,000 square meters. The large number of components reduces the price with economies of scale. The front end receiver is a single cryogenically cooled MIMIC Low Noise Amplifier covering the whole band. The feed is a wide-band log periodic feed of novel design, and the reflector system is an offset Gregorian for minimum sidelobes and spillover. All preliminary and critical design reviews have been completed. Three complete antennas with feeds and receivers are under test, and an array of 33 antennas is under construction at the Hat Creek Radio Observatory for the end of 2004. The present plan is to have a total of about 200 antennas completed by the summer of 2006 and the balance of the array finished before the end of the decade.

© (2004) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.

David R. DeBoer ; William J. Welch ; John Dreher ; Jill Tarter ; Leo Blitz, et al.
"The Allen Telescope Array", Proc. SPIE 5489, Ground-based Telescopes, 1021 (September 28, 2004); doi:10.1117/12.551737; http://dx.doi.org/10.1117/12.551737

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