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An obscured quasar census with the 4MOST IR AGN survey: design, predicted properties, and scientific goals

Andonie, Carolina; Alexander, David M; Greenwell, Claire; Fotopoulou, Sotiria; Hickox, Ryan; Rosario, David J; Villforth, Carolin; Buchner, Johannes; Krogager, Jens-Kristian; Laloux, Brivael; Merloni, Andrea; Salvato, Mara; Streicher, Ole; Yan, Wei

An obscured quasar census with the 4MOST IR AGN survey: design, predicted properties, and scientific goals Thumbnail


Authors

Carolina Andonie

Sotiria Fotopoulou

David J Rosario

Carolin Villforth

Johannes Buchner

Jens-Kristian Krogager

Brivael Laloux brivael.laloux@durham.ac.uk
PGR Student Doctor of Philosophy

Andrea Merloni

Mara Salvato

Ole Streicher

Wei Yan



Abstract

We present the 4MOST (4-metre Multi-Object Spectroscopic Telescope) infrared (IR) AGN survey, the first large-scale optical spectroscopic survey characterizing mid-infrared (MIR) selected obscured active galactic nuclei (AGNs). The survey targets obscured IR AGN candidates over down to a magnitude limit of and will be larger than any existing obscured IR AGN spectroscopic sample. We select the targets using an MIR colour criterion applied to the unWISE catalogue from the WISE (Wide-field Infrared Survey Explorer) all-sky survey, and then apply a cut; we demonstrate that this selection will mostly identify sources obscured by . The survey complements the 4MOST X-ray survey, which will follow up eROSITA (extended ROentgen Survey with an Imaging Telescope Array)-selected (typically unobscured) AGN. We perform simulations to predict the quality of the spectra that we will obtain and validate our MIR–optical colour-selection method using X-ray spectral constraints and UV-to-far-IR spectral energy distribution (SED) modelling in four well-observed deep-sky fields. We find that: (1) of the WISE-selected targets are AGN down to of which are obscured by , and (2) of the 4MOST IR AGN sample will remain undetected by the deepest eROSITA observations due to extreme absorption. Our SED-fitting results show that the 4MOST IR AGN survey will primarily identify obscured AGN and quasars ( of the sample is expected to have ) residing in massive galaxies () at with expected to be hosted by starburst galaxies.

Citation

Andonie, C., Alexander, D. M., Greenwell, C., Fotopoulou, S., Hickox, R., Rosario, D. J., Villforth, C., Buchner, J., Krogager, J.-K., Laloux, B., Merloni, A., Salvato, M., Streicher, O., & Yan, W. (2025). An obscured quasar census with the 4MOST IR AGN survey: design, predicted properties, and scientific goals. Monthly Notices of the Royal Astronomical Society, 539(3), 2202-2229. https://doi.org/10.1093/mnras/staf624

Journal Article Type Article
Acceptance Date Apr 10, 2025
Online Publication Date Apr 17, 2025
Publication Date 2025-05
Deposit Date May 20, 2025
Publicly Available Date May 20, 2025
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 539
Issue 3
Pages 2202-2229
DOI https://doi.org/10.1093/mnras/staf624
Keywords infrared: galaxies, surveys, quasars: general
Public URL https://durham-repository.worktribe.com/output/3942094

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