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 …
[HTML][HTML] From clusters to proto-clusters: the infrared perspective on environmental galaxy evolution
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …
can control the critical process of transforming galaxies from star forming to quiescent …
An atlas of color-selected quiescent galaxies at z> 3 in public JWST fields
F Valentino, G Brammer, KML Gould… - The Astrophysical …, 2023 - iopscience.iop.org
We present the results of a systematic search for candidate quiescent galaxies in the distant
universe in 11 JWST fields with publicly available observations collected during the first 3 …
universe in 11 JWST fields with publicly available observations collected during the first 3 …
An extremely compact, low-mass galaxy on its way to quiescence at z= 5.2
We report the discovery of a low-mass z= 5.200±0.002 galaxy that is in the process of
ceasing its star formation. The galaxy, MACS0417-z5BBG, is multiply imaged with …
ceasing its star formation. The galaxy, MACS0417-z5BBG, is multiply imaged with …
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 …
Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
M Donnari, A Pillepich, GD Joshi… - Monthly Notices of …, 2021 - academic.oup.com
We use the IllustrisTNG hydrodynamical simulations to show how the fractions of quenched
galaxies vary across different environments and cosmic time, and to quantify the role AGN …
galaxies vary across different environments and cosmic time, and to quantify the role AGN …
Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
M Donnari, A Pillepich, D Nelson… - Monthly Notices of …, 2021 - academic.oup.com
We make an in-depth comparison of the IllustrisTNG cosmological simulations with
observed quenched fractions of central and satellite galaxies, for M stars= 109–12 M⊙ at …
observed quenched fractions of central and satellite galaxies, for M stars= 109–12 M⊙ at …
Very high redshift quasars and the rapid emergence of supermassive black holes
P Kroupa, L Subr, T Jerabkova… - Monthly Notices of the …, 2020 - academic.oup.com
The observation of quasars at very high redshift such as Pōniuā'ena is a challenge for
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …
The massive ancient galaxies at z> 3 NEar-infrared (MAGAZ3NE) survey: Confirmation of extremely rapid star formation and quenching timescales for massive …
The Massive Ancient Galaxies at z > 3 NEar-infrared (MAGAZ3NE) Survey: Confirmation of
Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early …
Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early …
A massive galaxy that formed its stars at z ≈ 11
The formation of galaxies by gradual hierarchical co-assembly of baryons and cold dark
matter halos is a fundamental paradigm underpinning modern astrophysics, and predicts a …
matter halos is a fundamental paradigm underpinning modern astrophysics, and predicts a …