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The MOST Galactic Plane Survey

Published online by Cambridge University Press:  05 March 2013

A. J. Green*
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; [email protected]
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Abstract

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The Molonglo Observatory Synthesis Telescope (MOST) has been upgraded to increase the diameter of the field of view from 70′ to 2·7°. A survey of the Galactic Plane is proposed to completely cover the region 240° ≤ l ≤ 365°, ∣ b ∣ ≤ 10° with a (1σ) sensitivity of 1–2 mJy. The results will provide a major resource for the investigation of supernova remnants, HII regions and transient radio sources. They will also be correlated with the galaxy search from the HI multibeam survey to be conducted at the Parkes telescope.

Type
Research Article
Copyright
Copyright © Astronomical Society of Australia 1997

References

Condon, J. J., Cotton, W. D., Greisen, E. W., Perley, R. A., Yin, Q. F., & Broderick, J. J. 1993, Bull. AAS, 183, @ 64·02Google Scholar
Henning, P. A. 1997, PASA, 14, 21 Google Scholar
Juraszek, S. 1995, Physics Honours Report, University of SydneyGoogle Scholar
Large, M. I., Campbell-Wilson, D., Cram, L. E., Davison, R. G., & Robertson, J. G. 1994, PASA, 11, 44 Google Scholar
Robertson, J. G. 1991, Aust. J. Phys., 44, 729 Google Scholar
Sadler, E. M. 1996, private communicationGoogle Scholar
Staveley-Smith, L. 1997, PASA, 14, 111 CrossRefGoogle Scholar
Subrahmanya, C. R., & Mills, B. Y. 1987, IAU Symposium 124, Observatonal Cosmology, ed. A. Hewitt et al. (Dordrecht: Kluwer), 569 CrossRefGoogle Scholar
Whiteoak, J. B. Z. 1993, PhD Thesis, University of Sydney Google Scholar
Whiteoak, J. B. Z., & Green, A. J. 1996, A&AS, 118, 329 Google Scholar