In our modern understanding of galaxy formation, every galaxy forms within a dark matter
halo. The formation and growth of galaxies over time is connected to the growth of the halos …

We present a new-generation tool to model and interpret spectral energy distributions
(SEDs) of galaxies, which incorporates in a consistent way the production of radiation and its …

Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …

We extend the halo-based group finder developed by Yang et al.(2005c) to use data
simultaneously with either photometric or spectroscopic redshifts. A mock galaxy redshift …

The connection between galaxies and dark matter haloes is often inferred from data using
probabilistic models, such as the halo occupation distribution (HOD). Conventional HOD …

The variation of galaxy stellar masses and colour types with the distance to projected cosmic
filaments are quantified using the precise photometric redshifts of the COSMOS2015 …

We present a new rest-frame color–color selection method using synthetic us− gs and gs−
is,(ugi) s colors to identify star-forming and quiescent galaxies. Our method is similar to the …

We study galactic star formation activity as a function of environment and stellar mass over
0.5< z< 2.0 using the FourStar Galaxy Evolution (ZFOURGE) survey. We estimate the galaxy …

We use a mass complete (log ($ M/{M} _ {\odot} $) $\geqslant\, 9.6$) sample of galaxies with
accurate photometric redshifts in the COSMOS field to construct the density field and the …

We develop a new Multitracer Halo Occupation Distribution (MTHOD) framework for the
galaxy distribution and apply it to the extended Baryon Oscillation Spectroscopic Survey …