Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang

B Robertson, BD Johnson, S Tacchella… - The Astrophysical …, 2024 - iopscience.iop.org
We characterize the earliest galaxy population in the JADES Origins Field, the deepest
imaging field observed with JWST. We make use of ancillary Hubble Space Telescope …

AbacusHOD: a highly efficient extended multitracer HOD framework and its application to BOSS and eBOSS data

S Yuan, LH Garrison, B Hadzhiyska… - Monthly Notices of …, 2022 - academic.oup.com
We introduce the AbacusHOD model and present two applications of AbacusHOD and the
AbacusSummit simulations to observations. AbacusHOD is a Halo Occupation Distribution …

The MillenniumTNG Project: refining the one-halo model of red and blue galaxies at different redshifts

B Hadzhiyska, L Hernquist, D Eisenstein… - Monthly Notices of …, 2023 - academic.oup.com
Luminous red galaxies (LRGs) and blue star-forming emission-line galaxies (ELGs) are key
tracers of large-scale structure used by cosmological surveys. Theoretical predictions for …

The desi one-percent survey: exploring the halo occupation distribution of emission line galaxies with abacussummit simulations

A Rocher, V Ruhlmann-Kleider, E Burtin… - … of Cosmology and …, 2023 - iopscience.iop.org
Abstract The One-Percent survey of the Dark Energy Spectroscopic Instrument collected∼
270k emission line galaxies (ELGs) at 0.8< z< 1.6. The high completeness of the sample …

The MillenniumTNG Project: an improved two-halo model for the galaxy–halo connection of red and blue galaxies

B Hadzhiyska, D Eisenstein, L Hernquist… - Monthly Notices of …, 2023 - academic.oup.com
Approximate methods to populate dark-matter haloes with galaxies are of great utility to
galaxy surveys. However, the limitations of simple halo occupation models (HODs) preclude …

Illustrating galaxy–halo connection in the DESI era with illustrisTNG

S Yuan, B Hadzhiyska, S Bose… - Monthly Notices of the …, 2022 - academic.oup.com
We employ the hydrodynamical simulation illustrisTNG to inform the galaxy–halo connection
of the Luminous Red Galaxy (LRG) and Emission Line Galaxy (ELG) samples of the Dark …

Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model

B Hadzhiyska, S Liu, RS Somerville… - Monthly Notices of …, 2021 - academic.oup.com
In this work, we compare large scale structure observables for stellar mass selected samples
at z= 0, as predicted by two galaxy models, the hydrodynamical simulation IllustrisTNG and …

The MillenniumTNG Project: the large-scale clustering of galaxies

S Bose, B Hadzhiyska, M Barrera… - Monthly Notices of …, 2023 - academic.oup.com
Modern redshift surveys are tasked with mapping out the galaxy distribution over enormous
distance scales. Existing hydrodynamical simulations, however, do not reach the volumes …

Modeling galaxies in redshift space at the field level

M Schmittfull, M Simonović, MM Ivanov… - … of Cosmology and …, 2021 - iopscience.iop.org
We develop an analytical forward model based on perturbation theory to predict the redshift-
space galaxy overdensity at the field level given a realization of the initial conditions. We find …

Taming assembly bias for primordial non-Gaussianity

E Fondi, L Verde, F Villaescusa-Navarro… - … of Cosmology and …, 2024 - iopscience.iop.org
Primordial non-Gaussianity of the local type induces a strong scale-dependent bias on the
clustering of halos in the late-time Universe. This signature is particularly promising to …