The role of mergers and rejuvenation in the buildup of the quiescent population at cosmic noon

TL;DR

This study uses a semi-analytic galaxy evolution model to analyze how mergers and rejuvenation contribute to the formation of quiescent galaxies during cosmic noon, revealing different quenching pathways for low- and high-mass galaxies.

Contribution

It provides new estimates of the role of post-starburst phases, mergers, and rejuvenation in galaxy quenching, highlighting mass-dependent differences in quenching mechanisms.

Findings

18-28% of massive passive galaxies at 1<z<2 pass through a PSB phase.

Rejuvenation and mergers significantly influence the build-up of quiescent galaxies.

Low-mass galaxies have a higher fraction of PSB phases, around 60-80%.

Abstract

We investigate the quenching of galaxies using a mock observational lightcone generated from the Semi-Analytic Model (SAM) L-Galaxies, closely matched to observations from the UKIDSS Ultra Deep Survey (UDS). The sample is used to study merging, rejuvenation, and visibility times for star-forming, quiescent, and post-starburst (PSB) galaxies, to assess the impact on the build-up of the passive galaxy mass functions. We find, for example, that a typical PSB ($M_\ast\sim10^{10}$\,M$_\odot$) at $z\approx1$ has a 15 per cent likelihood of merging and around a 25 per cent likelihood of rejuvenating within 1 Gyr of being identified. Applying these rates and timescales to the observational data, we estimate the fraction of quiescent galaxies that passed through a PSB phase. We find that $18 - 28$ per cent of the build-up in the massive end ($M_\ast>10^{10}$\,M$\,_\odot$) of the passive mass function at $1<z<2$ can be explained by PSBs, with the contribution declining to $\sim5$ per cent by $z \simeq 0.5$. Accounting for mergers and rejuvenation reduces the inferred PSB contribution by approximately a factor of two. At lower stellar masses ($M_\ast < 10^{10}$\,M$_\odot$), rapid quenching through a PSB phase explains a significantly larger fraction of the growth in the passive mass function. With a visibility time of $\sim$ 0.75 Gyr, we find that around $60-80$ per cent of low-mass passive galaxies underwent a PSB phase. Our findings provide further evidence that low- and high-mass galaxies follow different quenching pathways.