• DocumentCode
    126620
  • Title

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

  • Author

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

  • Author_Institution
    Univ. of Arizona, Tucson, AZ, USA
  • fYear
    2014
  • fDate
    16-23 Aug. 2014
  • Firstpage
    1
  • Lastpage
    4
  • 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.
  • Keywords
    antennas; astronomical observatories; radio receivers; radiotelescopes; submillimetre astronomy; ALMA prototype antennas; Arizona Radio Observatory; Band 2 receiever; HEMT amplifier technology; Kitt Peak; Mount Graham SubMillimeter Telescope; NRAO telescope; SIS mixer; dual polarization sideband; frequency 385 GHz to 500 GHz; radio telescopes; size 12 m; subarcsecond pointing; submillimeter wavelength region; Amplitude modulation; Antennas; Mixers; Observatories; Receivers; Scattering; Telescopes;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    General Assembly and Scientific Symposium (URSI GASS), 2014 XXXIth URSI
  • Conference_Location
    Beijing
  • Type

    conf

  • DOI
    10.1109/URSIGASS.2014.6929986
  • Filename
    6929986