Multifrequency study of GHz-peaked spectrum sources

TL;DR

This study presents a comprehensive multifrequency analysis of GHz-peaked spectrum sources, revealing their spectral properties, distribution, and evolution, based on data from 2006-2017 and multiple radio surveys.

Contribution

It provides a new catalog of 164 GPS sources, including 17 new discoveries, and analyzes their spectral and physical properties across a broad frequency range.

Findings

Identified 164 GPS sources, 17 of which are new discoveries.

Confirmed the deficit of distant GPS with low peak frequencies.

Found that radio spectra become steeper with increasing redshift.

Abstract

Gigahertz-Peaked spectrum (GPS) sources are compact active galactic nuclei, presumably young precursors of bright radio sources. The study of GPS radio properties provides information about the features of synchrotron radiation in extragalactic sources. Also in applied research GPS sources are useful as compact stationary radio sources in the sky for astrometric purposes. This paper presents the results of a multifrequency GPS study based on quasi-simultaneous measurements with the RATAN-600 radio telescope during the 2006-2017. The catalog containing spectral flux densities measured at six frequencies (1.1, 2.3, 4.8, 7.7/8.2, 11.2, and 21.7 GHz) have been obtained. In addition, for the analysis of radio spectra, data from the following low-frequency surveys have been used: GLEAM (GaLactic and Extragalactic All-sky Murchison widefield array survey) and TGSS (Tata institute for fundamental research GMRT Sky Survey) and high-frequency measurements from Planck survey. A total number of 164 GPS and candidates to GPS have been identified (17 of them are new discoveries), which makes up a small fraction of GPS in the initial sample of bright AGNs, about 2%. The physical properties and formation conditions of synchrotron radiation is found to be quite different in GPS of different AGN types. The deficit of distant GPS ($z > 2$) with low maximum frequencies (less than 1 GHz) is confirmed. The existing 'size - peak frequency' anticorrelation is continuous. The continuum radio spectra are found to become statistically steeper with increasing redshift.