Early type galaxies have been the predominant morphological class for massive galaxies since only z~1
Fernando Buitrago, Ignacio Trujillo, Christopher J. Conselice, Boris, Haeussler

TL;DR
This study investigates the evolution of massive galaxy morphologies from high redshift to the present, revealing a significant increase in early-type galaxies since z~1, consistent with hierarchical formation models.
Contribution
It provides a large, multi-survey analysis of massive galaxy morphologies over a broad redshift range, confirming the dominance of early types since z~1.
Findings
Early-type galaxy fraction increased from ~20-30% at z~3 to ~70% at z=0.
Early types have been predominant for massive galaxies since only z~1.
Morphological change aligns with hierarchical galaxy formation scenarios.
Abstract
Present-day massive galaxies are composed mostly of early-type objects. It is unknown whether this was also the case at higher redshifts. In a hierarchical assembling scenario the morphological content of the massive population is expected to change with time from disk-like objects in the early Universe to spheroid-like galaxies at present. In this paper we have probed this theoretical expectation by compiling a large sample of massive (M_{stellar}>10^{11} h_{70}^{-2} M_{Sun}$) galaxies in the redshift interval 0 < z < 3. Our sample of 1082 objects comprises 207 local galaxies selected from SDSS plus 875 objects observed with the HST belonging to the POWIR/DEEP2 and GNS surveys. 639 of our objects have spectroscopic redshifts. Our morphological classification is performed as close as possible to the optical restframe according to the photometric bands available in our observations both…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
