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Professor Becklin's primary
focus is in the area of infrared imaging and spectroscopy. The current
major efforts are the search for Brown Dwarfs (objects, which do not have
sufficient mass to sustain nuclear burning, are the missing link between
stars and planets), the detection of dust rings around stars that are
related to planet formation, the dynamics and composition of the center
of our Galaxy, and the nature of luminous infrared galaxies. The research
uses UCLA instrumentation developed in collaboration with Prof. McLean,
as well as facility instrumentation at the University of California's
Lick and Keck (10 meter) observatories.
Becklin is chief scientist and director designate of the Stratospheric
Observatory for Infrared Astronomy ( SOFIA
), which will place a 2.5m infrared telescope in a modified Boeing 747-SP.
This major infrared observatory will begin operations in 2004. As part
of this development, Becklin is working with Professor McLean to build
an infrared test camera, which will be used to test the optical and infrared
properties of SOFIA. The camera, which will be finished in 2002, will
first be commissioned and used at the Lick 3-meter telescope.
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