The Arcetri methanol VLBI receiver

Details The Arcetri methanol VLBI receiver The Arcetri methanol VLBI receiver

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993amas.proc..187c&link_type=abstract

In: Astrophysical masers; Proceedings of the Conference, Arlington, VA, Mar. 9-11, 1992 (A93-52776 23-90), p. 187-190.

Astronomy and Astrophysics

Astronomy

Interstellar Masers, Methyl Alcohol, Spaceborne Astronomy, Spacecraft Instruments, Star Formation, Very Long Base Interferometry, Ground State, H Ii Regions, Radio Telescopes, Zeeman Effect

Scientific paper

A 12.2 GHz receiver has been designed and built to observe the 2(0) -
3(-1) methanol transition. Laboratory tests and first spectral
observation show that the rectifier's stability and sensitivity are
satisfactory. With the highest possible velocity resolution of the
spectrometer, the sensitivity is 4-6 Jy.

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