The 6-GHz Multibeam Maser Survey I. Techniques
J. A. Green, J. L. Caswell, G. A. Fuller, A. Avison, S. L. Breen, K., Brooks, M. G. Burton, A. Chrysostomou, J. Cox, P. J. Diamond, S. P., Ellingsen, M. D. Gray, M. G. Hoare, M. R. W. Masheder, N. M., McClure-Griffiths, M. Pestalozzi, C. Phillips, L. Quinn, M. A. Thompson, M.

TL;DR
This paper details the development and implementation of a new multibeam receiver system for the Parkes telescope, enabling a comprehensive and efficient survey of the Galaxy for methanol and hydroxyl masers associated with high-mass star formation.
Contribution
It introduces a novel 7-beam receiver system and survey methodology that significantly accelerates the detection of galactic masers, providing the first extensive Galaxy-wide maser catalog.
Findings
Over 800 methanol masers detected, with about 350 new sources.
Survey is two orders of magnitude faster than previous efforts.
First systematic, large-scale survey of Galactic plane for these masers.
Abstract
A new 7-beam 6-7 GHz receiver has been built to survey the Galaxy and the Magellanic Clouds for newly forming high-mass stars that are pinpointed by strong methanol maser emission at 6668 MHz. The receiver was jointly constructed by Jodrell Bank Observatory (JBO) and the Australia Telescope National Facility (ATNF) and allows simultaneous coverage at 6668 and 6035 MHz. It was successfully commissioned at Parkes in January 2006 and is now being used to conduct the Parkes-Jodrell multibeam maser survey of the Milky Way. This will be the first systematic survey of the entire Galactic plane for masers of not only 6668-MHz methanol, but also 6035-MHz excited-state hydroxyl. The survey is two orders of magnitude faster than most previous systematic surveys and has an rms noise level of ~0.17 Jy.This paper describes the observational strategy, techniques and reduction procedures of the…
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