The ages, metallicities and element abundance ratios of massive quenched galaxies at z~1.6

Abstract

We investigate the stellar population properties of a sample of 24 massive quenched galaxies at $1.25<z_{\mathrm{spec}}<2.09$ identified in the COSMOS field with our Subaru/MOIRCS near-IR spectroscopic observations. Tracing the stellar population properties as close to their major formation epoch as possible, we try to put constraints on the star formation history, post-quenching evolution, and possible progenitor star-forming populations for such massive quenched galaxies. By using a set of Lick absorption line indices on a rest-frame optical composite spectrum, the average age, metallicity [Z/H], and $\alpha$-to-iron element abundance ratio [$\alpha$/Fe] are derived as $\log (\mathrm{age}/\mathrm{Gyr})=0.04_{-0.08}^{+0.10}$, $[Z/H]=0.24_{-0.14}^{+0.20}$, and $[\alpha /\mathrm{Fe}]=0.31_{-0.12}^{+0.12}$, respectively. If our sample of quenched galaxies at $⟨z⟩=1.6$ is evolved passively to $z=0$, their stellar population properties will align in excellent agreement with local counterparts at similar stellar velocity dispersions, which qualifies them as progenitors of local massive early-type galaxies. Redshift evolution of stellar population ages in quenched galaxies combined with low redshift measurements from the literature suggests a formation redshift of $z_{\mathrm{f}}\sim 2.3$ around which the bulk of stars in these galaxies have been formed. The measured [$\alpha$/Fe] value indicates a star formation timescale of $\lesssim 1$ Gyr, which can be translated into a specific star formation rate of $\simeq 1{\mathrm{Gyr}}^{-1}$ prior to quenching. Based on these findings, we discuss identifying possible progenitor star-forming galaxies at $z\simeq 2.3$. We identify normal star-forming galaxies, i.e, those on the star-forming main sequence, followed by a rapid quenching event, as likely precursors of the quenched galaxies at $⟨z⟩=1.6$ presented here.

11 pages, 5 figures, 2 tables; accepted for ApJ

References in corpus (3)

• Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
• Stellar populations from spectroscopy of a large sample of quiescent galaxies at z > 1: Measuring the contribution of progenitor bias to early size growth
• Decoding the Star-Forming Main Sequence or: How I Learned to Stop Worrying and Love the Central Limit Theorem

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