AM. 01 UV Spectro-Interferometry from the Shuttle Bay

Details AM. 01 UV Spectro-Interferometry from the Shuttle Bay AM. 01 UV Spectro-Interferometry from the Shuttle Bay

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baas...16..747w&link_type=abstract

Bulletin of the American Astronomical Society, Vol. 16, p.747

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Scientific paper

The 18m-long shuttle bay offers potential for sub-milliarc second resolution at near-UV wavelengths. The authors explore its potential for spectro-interferometric comparison of the continuum source and the broad emission line regions of the quasar 3C273 and Seyfert galaxy NGC 4151. In their concept, two moderate-size telescopes are linked to each other and a beam combiner by a laser. The direction of the baseline is set by a photoelectric guider on the telescopes. Diffraction and light collection combine to make the coherence time and thus sensitivity a rapid function of telescope diameters.

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