COSMOS-Web: an overview of the JWST Cosmic Origins Survey

CM Casey, JS Kartaltepe, NE Drakos… - The Astrophysical …, 2023 - iopscience.iop.org
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr
treasury program conducted by the James Webb Space Telescope in its first cycle of …

Cosmological simulations of galaxy formation

M Vogelsberger, F Marinacci, P Torrey… - Nature Reviews …, 2020 - nature.com
Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

The JWST FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields

PA Oesch, G Brammer, RP Naidu… - Monthly Notices of …, 2023 - academic.oup.com
We present the JWST cycle 1 53.8 h medium program FRESCO, short for 'First Reionization
Epoch Spectroscopically Complete Observations'. FRESCO covers 62 arcmin2 in each of …

New Determinations of the UV Luminosity Functions from z∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency

RJ Bouwens, PA Oesch, M Stefanon… - The Astronomical …, 2021 - iopscience.iop.org
Here we provide the most comprehensive determinations of the rest-frame UV luminosity
function (LF) available to date with the Hubble Space Telescope (HST) at z∼ 2–9 …

CEERS key paper. IV. A triality in the nature of HST-dark galaxies

PG Pérez-González, G Barro… - The Astrophysical …, 2023 - iopscience.iop.org
The new capabilities that JWST offers in the near-and mid-infrared (IR) are used to
investigate in unprecedented detail the nature of optical/near-IR-faint, mid-IR-bright sources …

Full spectrum fitting with photometry in ppxf: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at …

M Cappellari - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
ABSTRACT I introduce some improvements to the ppxf method, which measures the stellar
and gas kinematics, star formation history (SFH) and chemical composition of galaxies. I …

UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10

P Behroozi, RH Wechsler, AP Hearin… - Monthly Notices of the …, 2019 - academic.oup.com
We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

De re metallica: the cosmic chemical evolution of galaxies

R Maiolino, F Mannucci - The Astronomy and Astrophysics Review, 2019 - Springer
The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …

Y Harikane, Y Ono, M Ouchi, C Liu… - The Astrophysical …, 2022 - iopscience.iop.org
We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

A Pillepich, D Nelson, L Hernquist… - Monthly Notices of …, 2018 - academic.oup.com
The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations
of galaxy formation performed with the arepo code and updated models for feedback …