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Table · dataset · 2026

Recognizing blazars from VLASS radio morphology

Listed in IVOA Registry (Virtual Observatory)

Blazars are radio-loud active galactic nuclei whose jets have a very small angle to our line of sight.

Description

Observationally, the radio emissions are mostly compact or compact-core with a one-sided jet. With 2.5" resolution at 3GHz, the Very Large Array Sky Survey (VLASS) enables us to resolve the structure of some blazar candidates in the sky north of decl. -40{deg}.

We introduce an algorithm to classify radio sources as either blazar-like or non-blazar-like based on their morphology in the VLASS images. We apply our algorithm to three existing catalogs, including one of the known blazars (Roma-BzCAT) and two blazar candidates identified by Wide-field Infrared Survey Explorer colors and radio emission (WIBRaLS, KDEBLLACS). We show that in all three catalogs, there are objects with morphologies inconsistent with being blazars.

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Considering all the catalogs, more than 12% of the candidates are unlikely to be blazars, based on this analysis. Notably, we show that 3% of the Roma-BzCAT confirmed blazars could be a misclassification based on their VLASS morphology. The resulting table with all sources and their radio morphological classification is available online.

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Documentation and papers

Catalogue records · 2

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Stated by source
Optical · Radio
Inferred from text
Astronomical sciences 69% · Image 65% · Tabular 65%
Provenance · 1 source records, 12 field assertions
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