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    The science case for simultaneous mm-wavelength receivers in radio astronomy

    256481.pdf (8.217Mb)
    Access Status
    Open access
    Authors
    Dodson, R.
    Rioja, M.
    Jung, T.
    Goméz, J.
    Bujarrabal, V.
    Moscadelli, L.
    Miller-Jones, James
    Tetarenko, A.
    Sivakoff, G.
    Date
    2017
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Dodson, R. and Rioja, M. and Jung, T. and Goméz, J. and Bujarrabal, V. and Moscadelli, L. and Miller-Jones, J. et al. 2017. The science case for simultaneous mm-wavelength receivers in radio astronomy. New Astronomy Reviews. 79: 85-102
    Source Title
    New Astronomy Reviews
    DOI
    10.1016/j.newar.2017.09.003
    ISSN
    1387-6473
    School
    Curtin Institute of Radio Astronomy (Physics)
    Funding and Sponsorship
    http://purl.org/au-research/grants/arc/FT140101082
    URI
    http://hdl.handle.net/20.500.11937/57963
    Collection
    • Curtin Research Publications
    Abstract

    This review arose from the European Radio Astronomy Technical Forum (ERATec) meeting held in Firenze, October 2015, and aims to highlight the breadth and depth of the high-impact science that will be aided and assisted by the use of simultaneous mm-wavelength receivers.Recent results and opportunities are presented and discussed from the fields of: continuum VLBI (observations of weak sources, astrometry, observations of AGN cores in spectral index and Faraday rotation), spectral line VLBI (observations of evolved stars and massive star-forming regions) and time domain observations of the flux variations arising in the compact jets of X-ray binaries.Our survey brings together a large range of important science applications, which will greatly benefit from simultaneous observing at mm-wavelengths. Such facilities are essential to allow these applications to become more efficient, more sensitive and more scientifically robust. In some cases without simultaneous receivers the science goals are simply unachievable. Similar benefits would exist in many other high frequency astronomical fields of research.

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