• DocumentCode
    474009
  • Title

    Facility heterodyne receiver for the Atacama Pathfinder Experiment Telescope

  • Author

    Belitsky, V. ; Lapkin, Igor ; Vassilev, Vessen ; Monje, Raquel ; Pavolotsky, Alexey ; Meledin, Denis ; Henke, D. ; Nyström, Olle ; Desmaris, Vincent ; Risacher, Christophe ; Svensson, Magnus ; Olberg, Michael ; Sundin, Erik ; Fredrixon, Matthias ; Dochev,

  • Author_Institution
    Dept. of Radio & Space Sci., Chalmers Univ. of Technol., Goteborg
  • fYear
    2007
  • fDate
    2-9 Sept. 2007
  • Firstpage
    326
  • Lastpage
    328
  • Abstract
    APEX, the Atacama PAthflnder Experiment (APEX) Telescope, is a partnership between Max Planck Institut fur Radioastronomie (in collaboration with Astronomisches Institut Ruhr Universitat Bochum (AIRUB)), Onsala Space Observatory and the European Southern Observatory. The telescope antenna, supplied by VERTEX Antennentechnik, is a 12 m antenna with a 17 mum rms surface accuracy operating at the Atacama Desert in the Chilean Andes at a 5100 m altitude. The APEX heterodyne facility receiver is placed in the telescope Nasmyth Cabin A. The receivers are coupled to the antenna via relay optics allowing the operation of two different Pi-type instruments and a 6-channel facility heterodyne receiver to cover approximately 210 - 1500 GHz frequency range while providing frequency independent illumination of the secondary. In this report, we present details on the optics for the APEX facility heterodyne receiver and details of its design. The report includes a very brief review of the APEX Band 1, 211 - 270 GHz, Band 2, 270 - 370 GHz, Band 3, 385 - 500 GHz, all based on sideband separation SIS mixer technology and Band T2, 1250 - 1390 GHz, a balanced waveguide HEB mixer, all developed by GARD.
  • Keywords
    astronomical instruments; optical receivers; radiotelescopes; submillimetre wave antennas; APEX; Atacama pathfinder experiment telescope; Pi-type instruments; VERTEX Antennentechnik; altitude 5100 m; balanced waveguide HEB mixer; facility heterodyne receiver; frequency 210 GHz to 1500 GHz; relay optics; sideband separation SIS mixer technology; size 12 m; telescope antenna; Collaboration; Frequency; Observatories; Optical coupling; Optical mixing; Optical receivers; Optical surface waves; Receiving antennas; Relays; Telescopes; APEX facility receiver; Nasmyth Cabin A optics; SIS and HEB mixers; cryogenics;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Infrared and Millimeter Waves, 2007 and the 2007 15th International Conference on Terahertz Electronics. IRMMW-THz. Joint 32nd International Conference on
  • Conference_Location
    Cardiff
  • Print_ISBN
    978-1-4244-1438-3
  • Type

    conf

  • DOI
    10.1109/ICIMW.2007.4516518
  • Filename
    4516518