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 …
treasury program conducted by the James Webb Space Telescope in its first cycle of …
Cosmological simulations of galaxy formation
Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …
in advancing our understanding of structure and galaxy formation in the Universe. These …
The main sequence of star-forming galaxies across cosmic times
P Popesso, A Concas, G Cresci, S Belli… - Monthly Notices of …, 2023 - academic.oup.com
By compiling a comprehensive census of literature studies, we investigate the evolution of
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …
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 …
function (LF) available to date with the Hubble Space Telescope (HST) at z∼ 2–9 …
UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
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 …
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …
A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
AC Carnall, DJ McLeod, RJ McLure… - Monthly Notices of …, 2023 - academic.oup.com
We report a robust sample of 10 massive quiescent galaxies at redshift, z> 3, selected using
the first data from the JWST Cosmic Evolution Early Release Science programme. Three of …
the first data from the JWST Cosmic Evolution Early Release Science programme. Three of …
Star-forming galaxies at cosmic noon
NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …
star-formation history, which culminated around; this period is often nicknamed “cosmic …
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 …
of galaxy formation performed with the arepo code and updated models for feedback …
Galaxy Stellar Mass Functions from z∼ 10 to z∼ 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of …
M Stefanon, RJ Bouwens, I Labbé… - The Astrophysical …, 2021 - iopscience.iop.org
We present new stellar mass functions at z∼ 6, z∼ 7, z∼ 8, z∼ 9 and, for the first time, z∼
10, constructed from∼ 800 Lyman-break galaxies previously identified over the eXtreme …
10, constructed from∼ 800 Lyman-break galaxies previously identified over the eXtreme …
The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z= 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History
R Bouwens, J González-López… - The Astrophysical …, 2020 - iopscience.iop.org
We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …