High-resolution international LOFAR observations of 4C~43.15 -- Spectral ages and injection indices in a high-z radio galaxy
arXiv:2108.07290 · doi:10.1051/0004-6361/202039871
Abstract
Radio sources with steep spectra are preferentially associated with the most distant galaxies, the 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 radio galaxy at frequencies between MHz and MHz. We measure the spatial distribution of spectra, and discuss the implications for models of the 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 . At the central frequency of MHz we achieve an angular resolution of . By complementing our data with archival \textit{Very Large Array} (VLA) data we study the spectral index distribution across 4C 43.15 between and at resolutions of and . With a magnetic field strength of nT and fitted injection indices of and , fitting a Tribble spectral ageing model results in a spectral age of 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 relation.
Accepted to a special issue of A&A on sub-arcsecond imaging with LOFAR. 13 pages, 9 figures