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Compact Symmetric Objects -- I Towards a Comprehensive Bona Fide Catalog

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arxiv 2303.11357 v2 pith:TU5MDFYC submitted 2023-03-20 astro-ph.HE astro-ph.GA

classification astro-ph.HEastro-ph.GA
keywords csosobjectsbonafideclassificationcompactsymmetrictowards
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Compact Symmetric Objects (CSOs) are jetted Active Galactic Nuclei (AGN) with overall projected size <1 kpc. The classification was introduced to distinguish these objects from the majority of compact jetted-AGN in centimeter wavelength very long baseline interferometry observations, where the observed emission is relativistically boosted towards the observer. The original classification criteria for CSOs were: (i) evidence of emission on both sides of the center of activity, and (ii) overall size <1 kpc. However some relativistically boosted objects with jet axes close to the line of sight appear symmetric and have been mis-classified as CSOs, thereby undermining the CSO classification. This is because two essential CSO properties, pointed out in the original papers, have been neglected: (iii) low variability, and (iv) low apparent speeds along the jets. As a first step towards creating a comprehensive catalog of ``bona fide'' CSOs, we identify 79 bona fide CSOs, including 15 objects claimed as confirmed CSOs here for the first time, that match the CSO selection criteria. This sample of bona fide CSOs can be used for astrophysical studies of CSOs without contamination by mis-classified CSOs. We show that the fraction of CSOs in complete flux density limited AGN samples with S$_{\rm 5\,GHz}$ >700 mJy is between $(6.8\pm1.6)$% and $(8.5\pm1.8)$%.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Searching for $\gamma$-ray emission from a bona fide Compact Symmetric Object sample: a $\gamma$-ray signal near GB6 J0906+4124

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    No bona fide CSO in a 73-source sample is firmly detected in 16 years of Fermi-LAT data; a ~4σ signal near GB6 J0906+4124 is a plausible but unconfirmed counterpart.

  2. Spectroscopic redshifts of selected flat-spectrum radio sources I

    astro-ph.CO 2026-07 accept novelty 3.5 of 10

    New spectroscopic redshifts are reported for six of fifteen bright SMILE flat-spectrum radio sources observed with the Skinakas 1.3 m telescope.

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