Recognizing Blazars Using Radio Morphology from the VLA Sky Survey

• DOI: 10.3847/1538-4357/ad20d3
• Publication Date: 2024-03-20T09:45:57Z
• Authors: Zhang-Liang 彰亮 Xie 谢; Eduardo Bañados; Silvia Belladitta; Chiara Mazzucchelli; Jan-Torge Schindler; Frederick Davies; Bram P. Venemans
• Keywords: QB460-466; Active galactic nuclei; Radio jets; Astrophysics; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Astrophysics of Galaxies; Blazars

Abstract Blazars are radio-loud active galactic nuclei whose jets have a very small angle to our line of sight. Observationally, the radio emissions are mostly compact or compact-core with a one-sided jet. With 2.″5 resolution at 3 GHz, the Very Large Array Sky Survey (VLASS) enables us to resolve the structure of some blazar candidates in the sky north of decl. −40°. 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. 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.