The University of Tokyo-Norbeyama Radio Observatory submillimeter survey telescope

Details The University of Tokyo-Norbeyama Radio Observatory submillimeter survey telescope The University of Tokyo-Norbeyama Radio Observatory submillimeter survey telescope

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..391s&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 391-395 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astronomy

Astronomical Observatories, Galactic Structure, Radio Astronomy, Submillimeter Waves, Telescopes, Temperature Distribution, Thermal Analysis, Galactic Radiation, Japanese Space Program, Milky Way Galaxy

Scientific paper

A 60 cm submillimeter telescope optimized for survey operations is described. The main task of this telescope is to survey the Galactic plane in CO (J = 2-1) emission with the same angular resolution as the CfA CO (J = 1-0) survey. Direct comparison of each set of data allows information on the large scale temperature structure of the Galaxy to be derived. Copies of the telescope planned for operation at higher frequencies, CI (490 GHz) or CO (J = 3-2) (345 GHz) are described.

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