Undermassive Host Galaxies of Five z∼ 6 Luminous Quasars Detected with JWST

MA Stone, J Lyu, GH Rieke, S Alberts… - The Astrophysical …, 2024 - iopscience.iop.org
We measure host galaxy stellar masses for a sample of five luminous quasars at z∼ 5–7.
Using JWST/NIRCam medium-band images of nearby point-spread function reference stars …

Galaxy Formation in ΛCDM Cosmology

JR Primack - Annual Review of Nuclear and Particle Science, 2024 - annualreviews.org
This is a golden age for galaxy formation: Existing and especially new telescopes are
providing observations that challenge and illuminate rapidly improving theory and …

Evolution of the Size–Mass Relation of Star-forming Galaxies Since z= 5.5 Revealed by CEERS

E Ward, A de la Vega, B Mobasher… - The Astrophysical …, 2024 - iopscience.iop.org
We combine deep imaging data from the CEERS early release JWST survey and Hubble
Space Telescope imaging from CANDELS to examine the size–mass relation of star-forming …

GA-NIFS: the interplay between merger, star formation, and chemical enrichment in MACS1149-JD1 at z= 9.11 with JWST/NIRSpec

C Marconcini, F D'Eugenio, R Maiolino… - Monthly Notices of …, 2024 - academic.oup.com
We present JWST/NIRSpec integral-field spectroscopy observations of the z 9.11 lensed
galaxy MACS1149-JD1, as part of the GA-NIFS programme. The data were obtained with …

[HTML][HTML] Testing CCC+ TL Cosmology with Observed Baryon Acoustic Oscillation Features

RP Gupta - The Astrophysical Journal, 2024 - iopscience.iop.org
The primary purpose of this paper is to see how well a recently proposed new model fits (a)
the position of the baryon acoustic oscillation (BAO) features observed in the large-scale …

The Size–Mass Relation at Rest-frame 1.5 μm from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS Fields

M Martorano, A van der Wel, M Baes… - The Astrophysical …, 2024 - iopscience.iop.org
We present the galaxy stellar mass–size relation in the rest-frame near-IR (1.5 μm) and its
evolution with redshift up to z= 2.5. Sérsic profiles are measured for∼ 26,000 galaxies with …

UVCANDELS: The Role of Dust on the Stellar Mass–Size Relation of Disk Galaxies at 0.5≤ z≤ 3.0

KV Nedkova, M Rafelski, HI Teplitz… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep
Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest …

Star formation and AGN activity 500 Myr after the Big Bang: Insights from JWST

JCJ D'Silva, SP Driver, CDP Lagos… - The Astrophysical …, 2023 - iopscience.iop.org
We consider the effect of including an active galactic nuclei (AGN) component when fitting
spectral energy distributions of 109 spectroscopically confirmed z≈ 3.5–12.5 galaxies with …

Multivariate Predictors of Lyman Continuum Escape. II. Predicting Lyman Continuum Escape Fractions for High-redshift Galaxies

AE Jaskot, AC Silveyra, A Plantinga… - The Astrophysical …, 2024 - iopscience.iop.org
JWST is uncovering the properties of ever-increasing numbers of galaxies at z> 6, during the
epoch of reionization. Connecting these observed populations to the process of reionization …

The sizes of bright Lyman-break galaxies at z ≃ 3–5 with JWST PRIMER

RG Varadaraj, RAA Bowler, MJ Jarvis… - Monthly Notices of …, 2024 - academic.oup.com
We use data from the JWST Public Release IMaging for Extragalactic Research survey to
measure the size scaling relations of 1668 rest-frame UV-bright Lyman-break galaxies …