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Molecular Line Observations at Parkes with a 3 GHz Maser

Published online by Cambridge University Press:  25 April 2016

B. Höglund
Affiliation:
Division of Radiophysics, CSIRO, Sydney
J. B. Whiteoak
Affiliation:
Division of Radiophysics, CSIRO, Sydney
F. F. Gardner
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

A 3 GHz maser from the Onsala Space Observatory, Sweden, is currently at Parkes on a long-term loan basis. So far, it has been used on the 64-m radio telescope for a two-week period of spectral-line observations in February 1979, providing a system sensitivity far superior to that previously available at the same frequency. The observed lines were the ground-state transitions of CH at 3264, 3335 and 3349 MHz, the 211 – 212 transition of H2CS at 3139 MHz, and the 211-212 transition of CH3CHO at 3195 MHz.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1979

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References

Fourikis, N., Sinclair, M.W., Robinson, B.J., Godfrey, P.D., and Brown, R.D., Aust. J. Phys., 27, 425 (1974).Google Scholar
Kollberg, E.L., Proc. IEEE, 61, 1323 (1973).Google Scholar
Liszt, H.S., Astrophys. J., 219, 454 (1978).Google Scholar
Whiteoak, J.B., Gardner, F.F., and Sinclair, M.W., Mon. Not. R. Astron. Soc, 184, 235 (1978).Google Scholar
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