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    Global eVLBI observations of the radio loud NLS1 PMN J0948+0022

    182960_51209_NLS1_051.pdf (648.4Kb)
    Access Status
    Open access
    Authors
    Giroletti, M.
    Paragi, Z.
    Bignall, Hayley
    Doi, A.
    Foschini, L.
    Gabanyi, K.
    Reynolds, Cormac
    Date
    2011
    Type
    Conference Paper
    
    Metadata
    Show full item record
    Citation
    Giroletti, M. and Paragi, Z. and Bignall, H.E. and Doi, A. and Foschini, L. and Gabányi, K. and Reynolds, C. 2011. Global eVLBI observations of the radio loud NLS1 PMN J0948+0022, in M. Colpi and others (ed), Narrow-Line Seyfert 1 Galaxies and their place in the Universe (NLS1), Apr 4-6 2011. Milano, Italy: International School for Advanced Studies (SISSA).
    Source Title
    Publications of Science
    Source Conference
    Narrow-Line Seyfert 1 Galaxies and their place in the Universe
    Additional URLs
    http://pos.sissa.it/archive/conferences/126/051/NLS1_051.pdf
    ISSN
    1824-8039
    School
    Curtin Institute of Radio Astronomy
    Remarks

    This article is published under the Open Access publishing model and distributed under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/3.0/ Please refer to the licence to obtain terms for any further reuse or distribution of this work.

    URI
    http://hdl.handle.net/20.500.11937/4890
    Collection
    • Curtin Research Publications
    Abstract

    We have performed three real-time e-VLBI observations of the radio loud NLS1 PMN J0948+0022 at 22 GHz, using a global array including telescopes in Europe, East Asia, and Australia, reaching a maximum baseline length of ~12500 km. The observations were part of a large multi-wavelength campaign carried out in 2009. We report on the results, including flux density variability, brightness temperature, jet structure, and polarization. Overall, these provide strong support for the presence of a relativistic jet in this source. We also present a new VLBI project aimed at improving our understanding of this jet, by studying proper motion and Faraday rotation.

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