Discovery of a radio galaxy at z = 5.72
|dc.identifier.citation||Saxena, A. and Marinello, M. and Overzier, R. and Best, P. and Röttgering, H. and Duncan, K. and Prandoni, I. et al. 2018. Discovery of a radio galaxy at z = 5.72. Monthly Notices of the Royal Astronomical Society. 480 (2): pp. 2733-2742.|
We report the discovery of the most distant radio galaxy to date, TGSS J1530+1049 at a redshift of z = 5.72, close to the presumed end of the Epoch of Reionization. The radio galaxy was selected from the TGSS ADR1 survey at 150 MHz for having an ultra-steep spectral index, a1.4 GHz150 MHz = -1.4 and a compact morphology obtained using VLA imaging at 1.4 GHz. No optical or infrared counterparts for the radio source were found in publicly available sky surveys. Follow-up optical spectroscopy at the radio position using GMOS on Gemini North revealed the presence of a single emission line. We identify this line as Lyman alpha at z = 5.72, because of its asymmetric line profile, the absence of other optical/UV lines in the spectrum, and a high equivalent width. With an Lya luminosity of 5.7 × 1042 erg s-1 and an FWHM of 370 km s-1, TGSS J1530+1049 is comparable to 'non-radio' Lyman alpha emitters (LAEs) at a similar redshift. However, with a radio luminosity of log L150MHz = 29.1 W Hz-1 and a deconvolved physical size 3.5 kpc, its radio properties are similar to other known radio galaxies at z > 4. Subsequent J and K band imaging using LUCI on the Large Binocular Telescope resulted in non-detection of the host galaxy down to 3s limits of J > 24.4 and K > 22.4 (Vega). The K band limit is consistent withz > 5 from the K-z relation for radio galaxies and helps rule out low redshifts. The stellar mass limit derived using simple stellar population models is Mstars < 1010.5 M?. Its relatively low stellar mass and small radio and Lya sizes suggest that TGSS J1530+1049 may be a radio galaxy in an early phase of its evolution.
|dc.publisher||Oxford University Press|
|dc.title||Discovery of a radio galaxy at z = 5.72|
|dcterms.source.title||Monthly Notices of the Royal Astronomical Society|
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.