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DRS Technologies' Infrared Technology Supports NASA's Launch of Infrared Telescope.


Business Editors/Technology Writers

PARSIPPANY, N.J.--(BUSINESS WIRE)--Sept. 3, 2003

DRS Technologies, Inc. (NYSE NYSE

See: New York Stock Exchange
:DRS DRS Drives (street suffix)
DRS Dispute Resolution Service
DRS Doctorandus
DRS Department of Rehabilitative Services
DRS Direct Registration System (securities)
DRS Department of Rehabilitation Services
) today announced that its infrared sensors were used on two of the three astronomical instruments supporting the NASA NASA: see National Aeronautics and Space Administration.
NASA
 in full National Aeronautics and Space Administration

Independent U.S.
 Space Infrared Telescope Facility Space Infrared Telescope Facility: see observatory, orbiting.  (SIRTF SIRTF Space Infrared Telescope Facility (now Spitzer Space Telescope; NASA) ), which was launched last week. SIRTF is the largest infrared telescope ever launched into space.

The DRS-produced infrared sensors, known as focal plane arrays (FPAs), were integrated into the Infrared Spectrograph and the Multi-band Imaging Photometer Photometer

An instrument used for making measurements of light, or electromagnetic radiation, in the visible range. In general, photometers may be divided into two classifications: laboratory photometers, which are usually fixed in position and yield results
, two of the SIRTF's three science instruments, to provide advanced imaging capabilities in the long wavelength region up to 40 micrometers. DRS's FPAs provide high reliability and spectral sensitivity while recording the position, intensity and wavelength of radiation of spatial objects. The company's DRS Sensors & Targeting Systems unit, based in Anaheim, California, developed the focal plane arrays.

The SIRTF observatory is expected to be approximately one thousand times more sensitive than Earth-based infrared telescopes. This is because nearly all of the infrared radiation emitted by objects in space is absorbed by the Earth's atmosphere, creating the need for a space-based infrared observatory with high sensitivity. Advanced sensor arrays and infrared detectors will give SIRTF the ability to map large complex areas and measure spectra at least one million times faster than any other space-borne infrared telescope.

"We have produced some of the world's most accurate and sensitive infrared cooled sensor systems, which have been recognized as crucial to the space industry," said Fred L. Marion, president of DRS's Electro-Optical Systems Group. "Our sensors have a strong record of performance operating on the U.S. Government's most advanced satellite and space telescope programs, including Defense Support Program satellites and NASA's Hubble Space Telescope Hubble Space Telescope (HST), the first large optical orbiting observatory. Built from 1978 to 1990 at a cost of $1.5 billion, the HST (named for astronomer E. P. Hubble) was expected to provide the clearest view yet obtained of the universe. ."

The Space Infrared Telescope Facility is a space-borne, cryogenically cooled infrared observatory capable of studying objects ranging from our solar system to the distant reaches of the universe. The observatory carries an 85-centimeter cryogenic telescope and three cryogenically cooled science instruments capable of performing imaging and spectroscopy in the 3.6 to 160 micron range. SIRTF is the final element in NASA's Great Observatories Program NASA's series of Great Observatories satellites are four large, powerful space-based telescopes. Each of the Great Observatories has had a similar size and cost at program outset, and each has made a substantial contribution to astronomy.  -- a family of four orbiting observatories and an important scientific and technical link to the new Astronomical Search for Origins Program. This program is designed to provide information associated with how galaxies, stars and planets form and develop. Other missions included the Hubble Space Telescope, Compton Gamma-Ray Observatory Compton Gamma-Ray Observatory: see gamma-ray astronomy.  and the Chandra X-Ray Observatory Chandra X-ray Observatory

U.S. X-ray space telescope. It was named after astrophysicist Subrahmanyan Chandrasekhar and was launched into orbit in 1999. Its mirror, with an aperture of 1.2 m (4 ft) and a focal length of 10 m (33 ft), produces unprecedented resolution.
. Each mission observed the universe in a different kind of light, including visible, gamma rays Gamma rays

Electromagnetic radiation emitted from excited atomic nuclei as an integral part of the process whereby the nucleus rearranges itself into a state of lower excitation (that is, energy content).
, X-rays and infrared.

The SIRTF's highly sensitive instruments will provide a unique view of the universe and allow visualization into regions of space that are hidden from optical telescopes. Many areas of space are filled with vast, dense clouds of gas and dust that block the view from Earth. Infrared penetrates these clouds, allowing visibility into regions of star formation, the centers of galaxies and newly forming planetary systems. Infrared space also provides information about much colder objects, such as smaller stars too dim to be detected by their visible light, extra solar planets and giant molecular clouds.

DRS Technologies provides leading-edge products and services to government and commercial customers worldwide. Focused on defense electronics, the company develops and manufactures a broad range of mission critical systems and components in the areas of communications, combat systems, battlefield digitization, electro-optics, power conversion, data storage, digital imaging, flight safety and space.

For more information about DRS Technologies, please visit the company's Web site at www.drs.com.
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Publication:Business Wire
Geographic Code:1USA
Date:Sep 3, 2003
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