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 Dark Energy Survey: more than dark energy–an overview
Dark Energy Survey Collaboration:… - Monthly Notices of …, 2016 - academic.oup.com
This overview paper describes the legacy prospect and discovery potential of the Dark
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …
Toward a better understanding of cosmic chronometers: a new measurement of H (z) at z∼ 0.7
We analyze the stellar ages obtained from a combination of Lick indices in Borghi et al. for
140 massive and passive galaxies selected in the LEGA-C survey at 0.6< z< 0.9. From their …
140 massive and passive galaxies selected in the LEGA-C survey at 0.6< z< 0.9. From their …
Eppur è piatto? The cosmic chronometers take on spatial curvature and cosmic concordance
The question of whether cosmic microwave background (CMB) temperature and polarization
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …
A 6% measurement of the Hubble parameter at z∼ 0.45: direct evidence of the epoch of cosmic re-acceleration
Deriving the expansion history of the Universe is a major goal of modern cosmology. To
date, the most accurate measurements have been obtained with Type Ia Supernovae (SNe) …
date, the most accurate measurements have been obtained with Type Ia Supernovae (SNe) …
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 …
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 …
[引用][C] First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger …
M Soares-Santos - Default journal, 2019 - andrews.elsevierpure.com
First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy
Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814 — Andrews …
Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814 — Andrews …
emerge – an empirical model for the formation of galaxies since z ∼ 10
We present emerge, an E mpirical M od E l for the fo R mation of G alaxi E s, describing the
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …
The COSMOS2015 galaxy stellar mass function-Thirteen billion years of stellar mass assembly in ten snapshots
I Davidzon, O Ilbert, C Laigle, J Coupon… - Astronomy & …, 2017 - aanda.org
We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …