The Arizona radio observatory: A new 12-M telescope and other developments

Robert W. Freund, Lucy M. Ziurys, Eugene F. Lauria, George P. Reiland

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The Arizona Radio Observatory (ARO) operates two radio telescopes in the millimeter and sub-millimeter wavelength region. Recently, one of these instruemnts, the aging, former NRAO 12 meter telescope on Kitt Peak, was replaced with one of the 12 m ALMA prototype antennas. The high performance design of this new instrument, including its 20 microns surface and sub-arcsecond pointing, will expand observational capabilites at the ARO. New receivers and backends are also in development at ARO. A dual polarization sideband separating SIS mixer covering the 0.7 mm atmospheric windw, ranging from 385 GHz to 500 GHz, has been installed as a facility instrument on the Sub-Millimeter Telescope (SMT) on Mount Graham. A prototype Band 2 receiever, based on HEMT amplifier technology, has been built and tested on the sky. These new additions and other developments will be presented.

Original languageEnglish (US)
Title of host publication2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014
PublisherInstitute of Electrical and Electronics Engineers Inc.
ISBN (Electronic)9781467352253
DOIs
StatePublished - Oct 17 2014
Event31st General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2014 - Beijing, China
Duration: Aug 16 2014Aug 23 2014

Publication series

Name2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014

Other

Other31st General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2014
Country/TerritoryChina
CityBeijing
Period8/16/148/23/14

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Computer Networks and Communications

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