Uncovering the MIR emission of quiescent galaxies with \(JWST\)

Uncovering the MIR emission of quiescent galaxies with \(JWST\)

We present a study of the mid-IR (MIR) emission of quiescent galaxies (QGs) beyond the local universe. Using deep \(JWST\) imaging in the SMACS-0723 cluster field we identify a mass limited (\(M_{*} >10^{9}\)M\(_{\odot}\)) sample of intermediate redshift QGs (\(0.20\) QGs with ALMA and \(JWST\).

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Veröffentlicht in:arXiv.org 2023-10
Hauptverfasser: Blánquez-Sesé, David, Magdis, G E, Gómez-Guijarro, C, Shuntov, M, Kokorev, V, Brammer, G, Valentino, F, Díaz-Santos, T, E -D Paspaliaris, Rigopoulou, D, Hjorth, J, Langeroodi, D, Gobat, R, Jin, S, Sillassen, N B, Gillman, S, Greve, T R, Lee, M
Format: Artikel
Sprache:eng
Schlagworte:
Dust
Emission analysis
Emissions
Galaxies
Interstellar matter
Local group (astronomy)
Polycyclic aromatic hydrocarbons
Red shift
Spectra
Star formation
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Zusammenfassung:We present a study of the mid-IR (MIR) emission of quiescent galaxies (QGs) beyond the local universe. Using deep \(JWST\) imaging in the SMACS-0723 cluster field we identify a mass limited (\(M_{*} >10^{9}\)M\(_{\odot}\)) sample of intermediate redshift QGs (\(0.20\) QGs with ALMA and \(JWST\).
ISSN:2331-8422
DOI:10.48550/arxiv.2310.01601