SETI public: Fw: Cornell News: New eye for Arecibo telescope

From: LARRY KLAES (ljk4_at_msn.com)
Date: Wed Apr 21 2004 - 11:54:43 PDT

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    ----- Original Message -----
    From: cunews_at_cornell.edu<mailto:cunews_at_cornell.edu>
    To: CUNEWS-PHYSICAL_SCIENCE-L_at_cornell.edu<mailto:CUNEWS-PHYSICAL_SCIENCE-L_at_cornell.edu> ; CUNEWS-SCIENCE-L_at_cornell.edu<mailto:CUNEWS-SCIENCE-L_at_cornell.edu>
    Sent: Wednesday, April 21, 2004 1:33 PM
    Subject: Cornell News: New eye for Arecibo telescope

    Arecibo Observatory gets 7-pixel eye on the sky that will make
    world's most sensitive dish radio telescope incredibly more sensitive

    FOR RELEASE: April 21, 2004

    Contact: David Brand
    Office: 607-255-3651
    E-mail: deb27_at_cornell.edu<mailto:deb27_at_cornell.edu>

    ARECIBO, P.R.. -- The Arecibo Observatory telescope, the largest and
    most sensitive single dish radio telescope in the world, is about to
    get a good deal more sensitive.

    Today (Wednesday, April 21) the telescope got a new "eye on the sky"
    that will turn the huge dish, operated by Cornell University for the
    National Science Foundation, into the equivalent of a seven-pixel
    radio camera.

       The complex new addition to the Arecibo telescope was hauled 150
    meters (492 feet) above the telescope's 1,000-foot-diameter (305
    meters) reflector dish starting in the early morning hours. The
    device, the size of a washing machine, took 30 minutes to reach a
    platform inside the suspended Gregorian dome, where ultimately it
    will be cooled and then connected to a fiber optic transmission
    system leading to ultra-high speed digital signal processors. The new
    instrument is called ALFA (for Arecibo L-Band Feed Array) and is
    essentially a camera for making radio pictures of the sky. ALFA will
    conduct large-scale sky surveys with unprecedented sensitivity,
    enabling astronomers to collect data about seven times faster than at
    present, giving the telescope an even broader appeal to astronomers.

    The ALFA receiver was built by the Australian research group,
    Commonwealth Scientific &amp; Industrial Research Organisation, under
    contract to the National Astronomy and Ionosphere Center (NAIC) at
    Cornell, in Ithaca, N.Y. Development of ALFA was overseen by the
    observatory's technical staff. The rest of the ALFA system, including
    ultra-fast data processing machines, are under development at NAIC.

    Radio telescopes traditionally have been limited to seeing just one
    spot -- a single pixel -- on the sky at once. Pictures of the sky
    have been built up by painstakingly imaging one spot after another.
    But ALFA lets the telescope see seven spots -- seven pixels -- on the
    sky at once, slashing the time needed to make all-sky surveys. Steve
    Torchinsky, ALFA project manager at Arecibo Observatory, says the new
    device will make it possible to find many new fast-spinning, highly
    dense stars called pulsars and will improve the chances of picking up
    very rare kinds of systems -- for instance, a pulsar orbiting a black
    hole.

    It also will map the neutral hydrogen gas in our galaxy, the Milky
    Way, as well as in other galaxies. Hydrogen is the most abundant
    element in the universe. "A whole range of science is planned for
    ALFA, " says Torchinsky. "Arecibo's large collecting area is
    particularly well-suited to pulsar studies."

    NAIC commissioned CSIRO to build ALFA following the success of a
    ground-breaking "multibeam" instrument it had designed and built for
    the Parkes radio telescope in eastern Australia. That instrument
    increased the Parkes telescope's view 13-fold, making it practical
    for the first time to search the whole sky for faint and hidden
    galaxies.

    Related World Wide Web sites: The following sites provide
    additional information on this news release. Some might not be part
    of the Cornell University community, and Cornell has no control over
    their content or availability.

    o Arecibo Observatory: <http://www.naic.edu>>

    o ALFA: <http://alfa.naic.edu/>>

    o CSIRO: <http://www.atnf.csiro.au/>>

    -30-

    The web version of this release may be found at
    http://www.news.cornell.edu/releases/April04/Arecibo.Eye.deb.html>

    -- 
    Cornell University News Service
    Surge 3
    Cornell University
    Ithaca, NY 14853
    607-255-4206
    cunews_at_cornell.edu<mailto:cunews_at_cornell.edu>
    http://www.news.cornell.edu>
    

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