COSMOS2020: The galaxy stellar mass function-The assembly and star formation cessation of galaxies at 0.2< z≤ 7.5

JR Weaver, I Davidzon, S Toft, O Ilbert… - Astronomy & …, 2023 - aanda.org
Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

EPOCHS. II. The ultraviolet luminosity function from 7.5< z< 13.5 using 180 arcmin2 of deep, blank fields from the PEARLS survey and public JWST data

NJ Adams, CJ Conselice, D Austin… - The Astrophysical …, 2024 - iopscience.iop.org
We present an analysis of the ultraviolet luminosity function (UV LF) and star formation rate
density of distant galaxies (7.5< z< 13.5) in the" blank" fields of the Prime Extragalactic Areas …

Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at z ~ 4–9 from JWST NIRCam observations

A Weibel, PA Oesch, L Barrufet… - Monthly Notices of …, 2024 - academic.oup.com
Combining the public JWST/NIRCam imaging programs CEERS, PRIMER, and JADES,
spanning a total area of, we obtain a sample of 30 000 galaxies at that allows us to perform …

The assembly of dusty galaxies at z ≥ 4: the build-up of stellar mass and its scaling relations with hints from early JWST data

C Di Cesare, L Graziani, R Schneider… - Monthly Notices of …, 2023 - academic.oup.com
The increasing number of distant galaxies observed with ALMA by the ALPINE and REBELS
surveys and the early release observations of the JWST promise to revolutionize our …

Constraints on the Faint End of the Galaxy Stellar Mass Function at z≃ 4–8 from Deep JWST Data

R Navarro-Carrera, P Rinaldi, KI Caputi… - The Astrophysical …, 2024 - iopscience.iop.org
We analyze a sample of 3300 galaxies between redshifts z≃ 3.5 and z≃ 8.5 selected from
James Webb Space Telescope (JWST) images in the Hubble Ultra Deep Field and UKIDSS …

Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z= 4–8 from CEERS

K Chworowsky, SL Finkelstein… - The Astronomical …, 2024 - iopscience.iop.org
We analyze the evolution of massive (log 10 [M⋆/M⊙]> 10) galaxies at z∼ 4–8 selected
from JWST Cosmic Evolution Early Release Survey (CEERS). We infer the physical …

MIGHTEE: the nature of the radio-loud AGN population

IH Whittam, MJ Jarvis, CL Hale… - Monthly Notices of …, 2022 - academic.oup.com
We study the nature of the faint radio source population detected in the MeerKAT
International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the …

MIGHTEE: deep 1.4 GHz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei

CL Hale, IH Whittam, MJ Jarvis, PN Best… - Monthly Notices of …, 2023 - academic.oup.com
We present deep 1.4 GHz source counts from∼ 5 deg2 of the continuum Early Science data
release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration survey …

MIGHTEE polarization early science fields: the deep polarized sky

AR Taylor, S Sekhar, L Heino… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT The MeerKAT International GigaHertz Tiered Extragalactic Exploration
(MIGHTEE) is one of the MeerKAT large survey projects, designed to pathfind SKA key …

First Light And Reionization Epoch Simulations (FLARES) VII: The star formation and metal enrichment histories of galaxies in the early Universe

SM Wilkins, AP Vijayan, CC Lovell… - Monthly Notices of …, 2023 - academic.oup.com
The star formation and metal enrichment histories of galaxies–at any epoch–constitute one
of the key properties of galaxies, and their measurement is a core aim of observational …