Early galaxy formation and its large-scale effects
Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a
consensus that galaxies emerged from the expanding matter background by gravitational …
consensus that galaxies emerged from the expanding matter background by gravitational …
The dust attenuation law in galaxies
S Salim, D Narayanan - Annual Review of Astronomy and …, 2020 - annualreviews.org
Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …
mechanisms that shape them are among the fundamental questions of extragalactic …
A Comprehensive Study of Galaxies at z∼ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre …
We conduct a comprehensive study on dropout galaxy candidates at z∼ 9–16 using the first
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …
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< …
The brightest galaxies at cosmic dawn
Recent JWST observations suggest an excess of z≳ 10 galaxy candidates above most
theoretical models. Here, we explore how the interplay between halo formation time-scales …
theoretical models. Here, we explore how the interplay between halo formation time-scales …
On the Stellar Populations of Galaxies at z= 9–11: The Growth of Metals and Stellar Mass at Early Times
S Tacchella, SL Finkelstein, M Bagley… - The Astrophysical …, 2022 - iopscience.iop.org
We present a detailed stellar population analysis of 11 bright (H< 26.6) galaxies at z= 9–11
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …
The MOSDEF Survey: The Evolution of the Mass–Metallicity Relation from z= 0 to z∼ 3.3
RL Sanders, AE Shapley, T Jones… - The Astrophysical …, 2021 - iopscience.iop.org
We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z= 0–3.3
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …
GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …
We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7
L Sommovigo, A Ferrara, A Pallottini… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …
of galaxies in the Universe. However, the dust temperature T d remains mostly …
The impact of UV variability on the abundance of bright galaxies at z ≥ 9
X Shen, M Vogelsberger… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT JWST observations have revealed a population of galaxies bright enough that
potentially challenge standard galaxy formation models in the Λ cold dark matter (ΛCDM) …
potentially challenge standard galaxy formation models in the Λ cold dark matter (ΛCDM) …