The CERGA infrared interferometer

Details The CERGA infrared interferometer The CERGA infrared interferometer

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jopt...10..345a&link_type=abstract

Journal of Optics, vol. 10, Nov.-Dec. 1979, p. 345-350. In French.

Astronomy and Astrophysics

Astronomy

5

Astronomical Observatories, Infrared Astronomy, Infrared Interferometers, Carbon Dioxide Lasers, Heterodyning, Infrared Telescopes, Signal To Noise Ratios

Scientific paper

The CERGA stellar IR interferometer operates at a wavelength of 11 microns via a heterodyne system. The local oscillator is a CO2 laser tuned to the P56 line. The attained performance is short of theoretical predictions but present modifications promise a flux limit sufficient to permit the observation of more than 100 sources with a spatial resolution of 0.07 arc sec.

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