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Date and Time of the Query: 2019-06-26 T09:55:43 PDT
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For refcode 1994A&A...286..654G:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
1994A&A...286..654G Research Note Disk brightness temperature of the planets at 43 GHz (and 43 GHz flux densities of some continuum sources) A. Greve, H. Steppe, D. Graham, and C. J. Schalinski IRAM, Nucleo Central, Avda. Divina Pastora 7, E-18012 Granada, Spain MPIfR, Auf dem Hugel 69, D-53121 Bonn, Germany IRAM, 300, rue de la Piscine, Domaine Universitaire, F-38406 St. Martin d'Heres, France Received 10 April 1993/Accepted 23 October 1993 Abstract. We have used the MPIfR 43 GHz (7 mm) Schottky receiver, installed in 1991 on the IRAM 30-m telescope for VLBI observations, for flux density measurements of several planets in comparison with several Galactic and extra-galactic continuum sources, using as calibration standards the sources W3OH and NGC 7027. The disk brightness temperatures of the planets are derived from these flux densities. Key words: Planets - radio continuum: general - radio continuum: solar system
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