Search and characterization of remnant radio galaxies in the XMM$-$LSS deep field

TL;DR

This study searches for and characterizes remnant radio galaxies in the XMM-LSS field using multi-frequency radio observations, identifying 21 candidates and estimating a remnant fraction of about 5%, consistent with evolutionary models.

Contribution

The paper presents the first large-scale search for remnant radio galaxies in the XMM-LSS field using multi-frequency data, and provides estimates of the remnant fraction and properties.

Findings

Identified 21 remnant candidates with diverse properties.

Estimated remnant fraction to be around 5%.

Remnants mostly found in non-cluster environments.

Abstract

The remnant phase of a radio galaxy is characterized by the cessation of AGN activity resulting in the stoppage of jets supplying plasma to radio lobes. In this paper, we present the search and characterization of remnant candidates in 12.5 deg$^{2}$ of the {\em XMM$-$Newton} Large$-$Scale Structure (XMM$-$LSS) field by using deep radio observations at 325 MHz from the Giant Metrewave Radio Telescope (GMRT), at 150 MHz from the LOw Frequency ARray (LOFAR), at 1.4 GHz from the Jansky Very Large Array (JVLA), and at 3 GHz from the VLA Sky Survey (VLASS). By using both morphological criteria {\viz}undetected radio core as well as spectral criteria {\viz}high spectral curvature, and ultra$-$steep spectrum, we identify 21 remnant candidates that are found to reside mostly in non$-$cluster environments, and exhibit diverse properties in terms of morphology, spectral index ($\alpha_{\rm 150}^{\rm 1400}$ in the range of $-1.71$ to $-0.75$ with a median of $-1.10$), and linear radio size (ranging from 242 kpc to 1.3 Mpc with a median of 469 kpc). Our study attempts to identify remnant candidates down to the flux density limit of 6.0 mJy at 325 MHz, and yields an upper limit on the remnant fraction ($f_{\rm rem}$) to be around 5$\%$. The observed $f_{\rm rem}$ seems consistent with the predictions of an evolutionary model assuming power law distributions of the duration of active phase and jet kinetic power with index $-0.8$ to $-1.2$.