High-resolution international LOFAR observations of 4C~43.15 -- Spectral ages and injection indices in a high-z radio galaxy

Abstract

Radio sources with steep spectra are preferentially associated with the most distant galaxies, the $\alpha -z$ relation, but the reason for this relation is an open question. The spatial distribution of spectra in high-z radio sources can be used to study this relation, and low-frequency observations are particularly important in understanding the particle acceleration and injection mechanisms. However, the small angular sizes of high-z sources together with the inherently low resolution of low-frequency radio telescopes until now has prevented high angular resolution low-frequency observations of distant objects. Here we present subarcsecond observations of a $z=2.4$ radio galaxy at frequencies between $121$ MHz and $166$ MHz. We measure the spatial distribution of spectra, and discuss the implications for models of the $\alpha -z$ relation. We targeted 4C 43.15 with the High Band Antennas (HBAs) of the \textit{International LOFAR Telescope} (ILT) with a range of baselines up to $1300\mathrm{km}$. At the central frequency of $143$ MHz we achieve an angular resolution of $\sim 0.3^{\prime \prime }$. By complementing our data with archival \textit{Very Large Array} (VLA) data we study the spectral index distribution across 4C 43.15 between $55\mathrm{MHz}$ and $8.4\mathrm{GHz}$ at resolutions of $0.4^{\prime \prime }$ and $0.9^{\prime \prime }$. With a magnetic field strength of $B=5.2$ nT and fitted injection indices of ${\alpha }_{\mathrm{inj}}^{\mathrm{north}}=-0.8$ and ${\alpha }_{\mathrm{inj}}^{\mathrm{south}}=-0.6$, fitting a Tribble spectral ageing model results in a spectral age of ${\tau }_{\mathrm{spec}}=1.1\pm 0.1$ Myr. We conclude that our data on 4C 43.15 indicates that inverse Compton losses could become comparable to or exceed synchrotron losses at higher redshifts and that inverse Compton losses could be a viable explanation for the $\alpha -z$ relation.

arXiv commentAccepted to a special issue of A&A on sub-arcsecond imaging with LOFAR. 13 pages, 9 figures

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