The Parsec-Scale Morphology of Southern GPS Sources

Multi-frequency, multi-epoch ATCA observations of a sample of AGN resulted in the identification of nine new candidate Giga-hertz Peaked Spectrum sources. Here, we present Long Baseline Array observations at 4.8 GHz of the four candidates with no previously published VLBI image, and consider these t...

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Main Authors: Edwards, P., Tingay, Steven
Format: Journal Article
Published: Cambridge University Press 2016
Online Access:http://hdl.handle.net/20.500.11937/16021
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author Edwards, P.
Tingay, Steven
author_facet Edwards, P.
Tingay, Steven
author_sort Edwards, P.
building Curtin Institutional Repository
collection Online Access
description Multi-frequency, multi-epoch ATCA observations of a sample of AGN resulted in the identification of nine new candidate Giga-hertz Peaked Spectrum sources. Here, we present Long Baseline Array observations at 4.8 GHz of the four candidates with no previously published VLBI image, and consider these together with previously published VLBI images of the other five sources. We find core-jet or compact double morphologies dominate, with further observations required to distinguish between these two possibilities for some sources. One of the nine candidates, PKS 1831–711, displays appreciable variability, suggesting its GPS spectrum is more ephemeral in nature. We focus in particular on the apparent relationship between a narrow spectral width and ‘compact double’ parsec-scale morphology, finding further examples, but also exceptions to this trend. An examination of the VLBI morphologies high-redshift (z > 3) sub-class of GPS sources suggests that core-jet morphologies predominate in this class.
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spelling curtin-20.500.11937-160212018-03-29T09:07:32Z The Parsec-Scale Morphology of Southern GPS Sources Edwards, P. Tingay, Steven Multi-frequency, multi-epoch ATCA observations of a sample of AGN resulted in the identification of nine new candidate Giga-hertz Peaked Spectrum sources. Here, we present Long Baseline Array observations at 4.8 GHz of the four candidates with no previously published VLBI image, and consider these together with previously published VLBI images of the other five sources. We find core-jet or compact double morphologies dominate, with further observations required to distinguish between these two possibilities for some sources. One of the nine candidates, PKS 1831–711, displays appreciable variability, suggesting its GPS spectrum is more ephemeral in nature. We focus in particular on the apparent relationship between a narrow spectral width and ‘compact double’ parsec-scale morphology, finding further examples, but also exceptions to this trend. An examination of the VLBI morphologies high-redshift (z > 3) sub-class of GPS sources suggests that core-jet morphologies predominate in this class. 2016 Journal Article http://hdl.handle.net/20.500.11937/16021 10.1017/pasa.2016.57 Cambridge University Press restricted
spellingShingle Edwards, P.
Tingay, Steven
The Parsec-Scale Morphology of Southern GPS Sources
title The Parsec-Scale Morphology of Southern GPS Sources
title_full The Parsec-Scale Morphology of Southern GPS Sources
title_fullStr The Parsec-Scale Morphology of Southern GPS Sources
title_full_unstemmed The Parsec-Scale Morphology of Southern GPS Sources
title_short The Parsec-Scale Morphology of Southern GPS Sources
title_sort parsec-scale morphology of southern gps sources
url http://hdl.handle.net/20.500.11937/16021