University of Hertfordshire

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From the same journal

By the same authors

Documents

  • Frits Sweijen
  • Leah K. Morabito
  • Jeremy Harwood
  • Reinout J. van Weeren
  • Huub J. A. Röttgering
  • Joseph R. Callingham
  • Neal Jackson
  • George Miley
  • Javier Moldon
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Original languageEnglish
Article numberA3
Number of pages13
JournalAstronomy & Astrophysics
Volume658
Early online date25 Jan 2022
DOIs
Publication statusPublished - 1 Feb 2022

Abstract

It has long been known that radio sources with the steepest spectra are preferentially associated with the most distant galaxies, the α - 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 and 166 MHz. We measure the spatial distribution of spectra, and discuss the implications for models of the α-z relation. We targeted 4C 43.15 with the High Band Antennas of the International LOFAR Telescope with a range of baselines up to 1300 km. At the central frequency of 143 MHz we achieve an angular resolution of ∼0.3″. By complementing our data with archival Very Large Array data we study the spectral index distribution across 4C 43.15 between 55 MHz and 8.4 GHz at resolutions of 0.4″ and 0.9″. With a magnetic field strength of B = 5.2 nT and fitted injection indices of αinjnorth = -0.8 and αinjsouth = -0.6, fitting a Tribble spectral ageing model results in a spectral age of τspec = 1.1 ± 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 α-z relation. Statistical studies of these objects will become possible in the future when wide-area subarcsecond surveys start.

Notes

© ESO 2021. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1051/0004-6361/202039871

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