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A striking relationship between dust extinction and radio detection in DESI QSOs: evidence for a dusty blow-out phase in red QSOs

Title: A striking relationship between dust extinction and radio detection in DESI QSOs: evidence for a dusty blow-out phase in red QSOs
Authors: Fawcett VA; Alexander DM; Brodzeller A; Edge AC; Rosario DJ; Myers AD; Aguilar J; Ahlen S; Alfarsy R; Brooks D; Canning R; Circosta C; Dawson K; De La Macorra A; Doel P; Fanning K; Font-Ribera A; Forero-Romero JE; Gontcho SGA; Guy J; Harrison CM; Honscheid K; Juneau S; Kehoe R; Kisner T; Kremin A; Landriau M; Manera M; Meisner AM; Miquel R; Moustakas J; Nie J; Percival WJ; Poppett C; Pucha R; Rossi G; Schlegel D; Siudek M; Tarle G; Weaver BA; Zhou Z; Zou H
Source: Monthly Notices of the Royal Astronomical Society, 1 November 2023
Publisher Information: Oxford University Press
Publication Year: 2023
Collection: Newcastle University Library ePrints Service
Description: © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.We present the first eight months of data from our secondary target programme within the ongoing Dark Energy Spectroscopic Instrument (DESI) survey. Our programme uses a mid-infrared and optical colour selection to preferentially target dust-reddened quasi-stellar objects (QSOs) that would have otherwise been missed by the nominal DESI QSO selection. So far, we have obtained optical spectra for 3038 candidates, of which ∼70 per cent of the high-quality objects (those with robust redshifts) are visually confirmed to be Type 1 QSOs, consistent with the expected fraction from the main DESI QSO survey. By fitting a dust-reddened blue QSO composite to the QSO spectra, we find they are well-fitted by a normal QSO with up to AV ∼4 mag of line-of-sight dust extinction. Utilizing radio data from the LOFAR Two-metre Sky Survey (LoTSS) DR2, we identify a striking positive relationship between the amount of line-of-sight dust extinction towards a QSO and the radio detection fraction, that is not driven by radio-loud systems, redshift and/or luminosity effects. This demonstrates an intrinsic connection between dust reddening and the production of radio emission in QSOs, whereby the radio emission is most likely due to low-powered jets or winds/outflows causing shocks in a dusty environment. On the basis of this evidence, we suggest that red QSOs may represent a transitional 'blow-out' phase in the evolution of QSOs, where winds and outflows evacuate the dust and gas to reveal an unobscured blue QSO.
Document Type: article in journal/newspaper
Language: unknown
Relation: https://eprints.ncl.ac.uk/294267
Availability: https://eprints.ncl.ac.uk/294267
Rights: https://creativecommons.org/licenses/by/4.0/
Accession Number: edsbas.10B2FD08
Database: BASE