Johannes Zabl

TL;DR: In this paper, the authors examined the Fundamental Plane (FP) and mass-to-light ratio (M/L$) scaling relations using the largest sample of massive quiescent galaxies at $1.5 11.26, and showed that they cannot passively evolve to the local Coma cluster relation alone and must undergo significant structural evolution to mimic the sizes of local massive galaxies.

TL;DR: In this paper, the authors examined the Fundamental Plane (FP) and mass-to-light ratio (M/L$) scaling relations using the largest sample of massive quiescent galaxies at $1.5 11.26, and showed that they cannot passively evolve to the local Coma cluster relation alone and must undergo significant structural evolution to mimic the sizes of local massive galaxies.

TL;DR: In this article , the authors show that quiescent galaxies in the REQUIEM-2D survey have diverse formation histories with age gradients at the 1σ-3σ level, including examples of a younger central region supporting outside-in formation, and flat age gradient that show evidence for both spatially uniform early formation and inside-out quenching.

TL;DR: In this paper, the diffuse gas and metals in the circumgalactic medium of 96 z = 2.9-3.8 Ly$\alpha$ emitters (LAEs) detected with the Multi-Unit Spectroscopic Explorer (MUSE) in fields centered on 8 bright background quasars as part of our MUSEQuBES survey.

TL;DR: In this paper, the authors presented ALMA observations of a sub-millimeter selected galaxy group at the MS 0451.6-0305 foreground cluster at the level of 10^9-10^{10} \; M_\odot.