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[en] A spectral line receiver system developed at the Max-Planck-Institut fuer Radioastronomie in Bonn was installed on the ESO 3.6-m and 1-m telescopes in July 1981. The cooled mixer front end gave DSB receiver temperatures of 260-600 K at 230 GHz. The spectrometer was a 256 x 1 MHz filterbank. The authors have observed the CO 2-1 transition towards 42 positions corresponding to the brightest southern HII regions. (Auth.)
Source
Burton, W.B.; Israel, F.P. (eds.); Astrophysics and Space Science Library; v. 105; 309 p; ISBN 90-277-1651-X; 
; 1983; p. 217-222; D. Reidel; Dordrecht (Netherlands); Workshop on surveys of the Southern Galaxy; Leyden (Netherlands); 4-6 Aug 1982; 4 figs.; 2 tables.
; 1983; p. 217-222; D. Reidel; Dordrecht (Netherlands); Workshop on surveys of the Southern Galaxy; Leyden (Netherlands); 4-6 Aug 1982; 4 figs.; 2 tables.