UNCOVER: Significant Reddening in Cosmic Noon Quiescent Galaxies | CU Experts

Abstract; We explore the physical properties of five massive quiescent galaxies at z ∼ 2.5, revealing the presence of nonnegligible dust reservoirs. JWST NIRSpec observations were obtained for each target, finding no significant line emission; multiple star formation tracers independently place upper limits between 0.1 and 10 M; ⊙ yr−1. Spectral energy distribution modeling with Prospector infers stellar masses of ; ; ; ; ; ; ; log; ; ; 10; ; ; [; M; /; ; ; M; ; ; ⊙; ; ; ]; ∼; 10; −; 11; ; and stellar-mass-weighted ages between 1 and 2 Gyr. The inferred mass-weighted effective radii (r; eff ∼ 0.4–1.4 kpc) and inner 1 kpc stellar surface densities (; ; ; ; ; ; log; 10; ; [; ; Σ; ; <; 1; ; kpc; ; ; /; ; M; ⊙; ; ; ; kpc; 2; ; ]; ≳; 9; ; ) are typical of quiescent galaxies at z ≳ 2. The galaxies predominately display negative color gradients (redder core and bluer outskirts); for one galaxy, this effect results from a dusty core. Unlike local quiescent galaxies, we identify significant reddening in these typical cosmic noon passive galaxies; all but one require A; ; V; ≳ 0.4. This finding is in qualitative agreement with previous studies, but our deep 20-band NIRCam imaging is able to significantly suppress the dust–age degeneracy and confidently determine that these galaxies are reddened. We speculate about the physical effects that may drive the decline in dust content in quiescent galaxies over cosmic time.

Siegel JC; Setton DJ; Greene JE; Suess KA; Whitaker KE; Bezanson R; Leja J; Furtak LJ; Cutler SE; de Graaff A

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