activity
20172020
most citedThe Roles of Mass and Environment in the Quenching of Galaxies. II

50 citations · 81 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202025 cited

On the Mass Distribution of the Intra-Cluster Light in Galaxy Groups and Clusters

Emanuele Contini, Qiu Sheng Gu

We take advantage of a semi-analytic model with a state-of-art implementation of the formation of the intra-cluster light (ICL) to study the mass distribution of the ICL in galaxy…

astro-ph.GA2020

YZiCS: Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis

Jinsu Rhee, Rory Smith, Hoseung Choi +4

We used the time since infall (TSI) of galaxies, obtained from the Yonsei Zoom-in Cluster Simulation, and the star formation rate (SFR) from the Sloan Digital Sky Survey (SDSS) Dat…

astro-ph.GA202050 cited

The Roles of Mass and Environment in the Quenching of Galaxies. II

E. Contini, Q. Gu, X. Ge +3

We take advantage of an analytic model of galaxy formation coupled to the merger tree of an N-body simulation to study the roles of environment and stellar mass in the quenching of…

astro-ph.GA2019

The Roles of Mass and Environment in the Quenching of Galaxies

E. Contini, Q. Gu, X. Kang +2

We study the roles of stellar mass and environment in quenching the star formation activity of a large set of simulated galaxies by taking advantage of an analytic model coupled to…

astro-ph.GA2018

Theoretical Predictions of Colors and Metallicity of the Intra-Cluster Light

E. Contini, S. K. Yi, X. Kang

We study colors and metallicities of the Brightest Cluster Galaxies (BCGs) and Intra-Cluster Light (ICL) in galaxy groups and clusters, as predicted by a semi-analytic model of gal…

astro-ph.GA20176 cited

Constraints on the Evolution of the Galaxy Stellar Mass Function II: Quenching Timescale of Galaxies and its Implication for their Star Formation Rate

E. Contini, X. Kang, A. D. Romeo +2

We study the connection between the observed star formation rate-stellar mass (SFR-) relation and the evolution of the stellar mass function (SMF) by means of a subhalo abunda…