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dc.contributor.authorGiroletti, M.
dc.contributor.authorParagi, Z.
dc.contributor.authorBignall, Hayley
dc.contributor.authorDoi, A.
dc.contributor.authorFoschini, L.
dc.contributor.authorGabanyi, K.
dc.contributor.authorReynolds, Cormac
dc.contributor.editorLuigi Foschini
dc.contributor.editorMonica Colpi
dc.contributor.editorLuigi Gallo
dc.contributor.editorDirk Grupe
dc.contributor.editorStefanie Komossa
dc.contributor.editorKaren Leighly
dc.contributor.editorSmita Mathur
dc.identifier.citationGiroletti, 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).

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.

dc.publisherThe International School for Advanced Studies (SISSA)
dc.titleGlobal eVLBI observations of the radio loud NLS1 PMN J0948+0022
dc.typeConference Paper
dcterms.source.titlePublications of Science
dcterms.source.seriesPublications of Science
dcterms.source.conferenceNarrow-Line Seyfert 1 Galaxies and their place in the Universe
dcterms.source.conference-start-dateApr 4 2011
dcterms.source.conferencelocationMilano, Italy
dcterms.source.placeTrieste, Italy

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

curtin.departmentCurtin Institute of Radio Astronomy
curtin.accessStatusOpen access

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