Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...275..679t&link_type=abstract
Astronomy and Astrophysics, Vol. 275, p. 679 (1993)
Astronomy and Astrophysics
Astrophysics
2
Telescopes, Methods: Numerical
Scientific paper
The surface profile of the 32-m parabolic radiotelescope located in Medicina has been measured with the Misell phase-recovery technique using commercial geostationary satellites at 11 GHz and checked on H2O astronomical masers at 22 GHz as reference sources. The telescope is a parabolic reflector antenna operating in Cassegrain configuration and designed for observations up to the frequency of 23 GHz. The accuracy obtained with this technique is about 0.2 mm and the spatial resolution is 0.7 m.
Comoretto Gianni
Tarchi D.
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