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COSMOS2020: The galaxy stellar mass function-The assembly and star formation cessation of galaxies at 0.2< z≤ 7.5
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 …
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
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 …
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 …
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
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 …
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
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 …
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 …
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 …
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 …
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 …
(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
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 …
of the key properties of galaxies, and their measurement is a core aim of observational …