14 citations · 16 across the 8 of their papers we have counts for
11 papers · 1 filter
The Connection between Halo Assembly History and the Stellar Distribution I: The Central Stellar Mass - Richness Plane
Shuo Xu, Song Huang, Alexie Leauthaud +4
Recent observations suggest intrinsic links between the stellar components of massive halos and their assembly histories. Using massive halos with $\log[M_{\rm halo}/M_\odot] \geq…
Feedback driven interactions between dark and luminous matter to explain tight galaxy scaling relations
Leen Alrawas, Andrea V. Macciò, Carlo Cannarozzo
The tight empirical correlation linking the stellar disk scale length to the dark matter scale radius has been proposed as possible evidence for a fundamental coupling…
Empirical estimates of how massive galaxies can be in ΛCDM
Miguel Enríquez-Vargas, Aldo Rodríguez-Puebla, Aditya Manuwal +3
Using Extreme Value Statistics applied to the observed galaxy stellar mass and the UV luminosity functions, we empirically estimate masses and luminosities of the most extreme gala…
On matching galaxy number densities to reconstruct galaxy evolutionary tracks
Aldo Rodriguez-Puebla, Vladimir Avila-Reese, Joel R. Primack +1
The cumulative number density matching approach equates number densities between adjacent redshifts to derive empirical galaxy evolution tracks from the observed galaxy stellar mas…
Gas accretion at high redshift: cold flows all the way
Stefan Waterval, Carlo Cannarozzo, Andrea V. Macciò
We study in detail how massive galaxies accrete gas through cosmic time using cosmological hydrodynamical simulations from the High-z Evolution of Large and Luminous Objects (HELLO…
The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
Shuo Xu, Song Huang, Alexie Leauthaud +4
Recent observations suggest that the extended stellar halos of low-redshift massive galaxies are tightly connected to the assembly of their dark matter halos. In this paper, we use…