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.

Under a temporary opening in the Arecibo reflector, workers prepare the ALFA unit for hoisting. Tony Acevedo/Arecibo ObservatoryCopyright © Cornell University Click on the image for a high-resolution version (750 x 1000 pixels, 667K)

The ALFA receiver was built by the Australian research group, Commonwealth Scientific & 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/