2k citations · 8.3k across the 58 of their papers we have counts for
9 papers · 1 filter
Critical Stellar Central Densities Drive Galaxy Quenching in the Nearby Universe
Bingxiao Xu, Yingjie Peng
We study the structural and environmental dependence of the star formation on the plane of stellar mass versus central core density () in the nearby universe. We st…
On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
Joanna M. Piotrowska, Asa F. L. Bluck, Roberto Maiolino +1
In this paper we investigate how massive central galaxies cease their star formation by comparing theoretical predictions from cosmological simulations: EAGLE, Illustris and Illust…
A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
Rui Shi, Wenting Wang, Zhaozhou Li +5
We propose a random forest (RF) machine learning approach to determine the accreted stellar mass fractions () of central galaxies, based on various dark matter halo…
The KLEVER survey: Nitrogen abundances at 2 and probing the existence of a fundamental nitrogen relation
Connor Hayden-Pawson, Mirko Curti, Roberto Maiolino +14
We present a comparison of the nitrogen-to-oxygen ratio (N/O) in 37 high-redshift galaxies at 2 taken from the KMOS Lensed Emission Lines and VElocity Review (KLEVER) Survey…
The HASHTAG project: The First Submillimeter Images of the Andromeda Galaxy from the Ground
Matthew W. L. Smith, Stephen A. Eales, Thomas G. Williams +46
Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths com…
The stellar mass versus stellar metallicity relation of star-forming galaxies at and implications for the evolution of the -enhancement
Daichi Kashino, Simon J. Lilly, Alvio Renzini +10
We measure the relationship between stellar mass and stellar metallicity, the stellar mass--metallicity relation (MZR), for 1336 star-forming galaxies at (<z>=2.2)…