[HTML][HTML] 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 …

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 …

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 …

The Horizon-AGN simulation: morphological diversity of galaxies promoted by AGN feedback

Y Dubois, S Peirani, C Pichon… - Monthly Notices of …, 2016 - academic.oup.com
The interplay between cosmic gas accretion on to galaxies and galaxy mergers drives the
observed morphological diversity of galaxies. By comparing the state-of-the-art …

The illustris simulation: Public data release

D Nelson, A Pillepich, S Genel, M Vogelsberger… - Astronomy and …, 2015 - Elsevier
We present the full public release of all data from the Illustris simulation project. Illustris is a
suite of large volume, cosmological hydrodynamical simulations run with the moving-mesh …

Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors

F Valentino, M Tanaka, I Davidzon, S Toft… - The Astrophysical …, 2020 - iopscience.iop.org
We report two secure (= z 3.775, 4.012) and one tentative (z≈ 3.767) spectroscopic
confirmations of massive and quiescent galaxies through K-band observations with …

Compaction and quenching of high-z galaxies in cosmological simulations: blue and red nuggets

A Zolotov, A Dekel, N Mandelker… - Monthly Notices of …, 2015 - academic.oup.com
We use cosmological simulations to study a characteristic evolution pattern of high-redshift
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …

Shark: introducing an open source, free, and flexible semi-analytic model of galaxy formation

CP Lagos, RJ Tobar, ASG Robotham… - Monthly Notices of …, 2018 - academic.oup.com
We present a new, open source, free, semi-analytic model (SAM) of galaxy formation, Shark,
designed to be highly flexible and modular, allowing easy exploration of different physical …

Near infrared spectroscopy and star-formation histories of 3≤ z≤ 4 quiescent galaxies

C Schreiber, K Glazebrook, T Nanayakkara… - Astronomy & …, 2018 - aanda.org
We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …

The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation

S Genel, D Nelson, A Pillepich… - Monthly Notices of …, 2018 - academic.oup.com
We analyse scaling relations and evolution histories of galaxy sizes in TNG100, part of the
IllustrisTNG simulation suite. Observational qualitative trends of size with stellar mass, star …