Near-infrared emission line diagnostics for AGN from the local Universe to <i>z</i> ∼ 3

Calabrò, Antonello; Pentericci, L.; Feltre, A.; Arrabal Haro, Pablo; Radovich, M.; Seillé, Lise-Marie; Oliva, E.; Daddi, E.; Amorín, R.; B. Bagley, Micaela; Bisigello, Laura; Buat, V.; Castellano, M.; J. Cleri, Nikko; Dickinson, Mark; Fernández, Vital; L. Finkelstein, Steven; Giavalisco, Mauro; Grazian, A.; P. Hathi, Nimish; Hirschmann, Michaela; Juneau, S.; S. Kartaltepe, Jeyhan; M. Koekemoer, Anton; A. Lucas, Ray; Papovich, Casey; G. Pérez‐González, Pablo; Pirzkal, Nor; Santini, P.; R. Trump, Jonathan; de la Vega, Alexander; M. Wilkins, Stephen; Y. Aaron Yung, L.; Cassata, P.; Gobat, R.; Mascia, Sara; Napolitano, Lorenzo; Vulcani, Benedetta

doi:10.1051/0004-6361/202347190

Public

Near-infrared emission line diagnostics for AGN from the local Universe to z ∼ 3

Shared by NobleBlocks on Sep 21, 2023 • 12:00 AM UTC

Authors:

Antonello Calabrò

L. Pentericci

A. Feltre

Abstract

Optical rest-frame spectroscopic diagnostics are usually employed to distinguish between star formation and active galactic nucleus (AGN) powered emission. However, this method is biased against dusty sources, hampering a complete census of the AGN population across cosmic epochs. To mitigate this e...

Subject

Physics

Astrophysics

Active galactic nucleus

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