Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges
RA Crain, F van de Voort - Annual Review of Astronomy and …, 2023 - annualreviews.org
We review the progress in modeling the galaxy population in hydrodynamical simulations of
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …
The cold interstellar medium of galaxies in the local universe
A Saintonge, B Catinella - Annual Review of Astronomy and …, 2022 - annualreviews.org
The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …
A comprehensive measurement of the local value of the Hubble constant with 1 km s− 1 Mpc− 1 uncertainty from the Hubble Space Telescope and the SH0ES team
We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the
host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0) …
host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0) …
The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8
We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster
SMACS J0723. 3-7327, observed as part of the Early Release Observations programme of …
SMACS J0723. 3-7327, observed as part of the Early Release Observations programme of …
PHANGS–ALMA: Arcsecond CO (2–1) Imaging of Nearby Star-forming Galaxies
AK Leroy, E Schinnerer, A Hughes… - The Astrophysical …, 2021 - iopscience.iop.org
We present PHANGS–ALMA, the first survey to map CO J= 2→ 1 line emission at∼ 1''∼ 100
pc spatial resolution from a representative sample of 90 nearby (d≲ 20 Mpc) galaxies that lie …
pc spatial resolution from a representative sample of 90 nearby (d≲ 20 Mpc) galaxies that lie …
The DESI bright galaxy survey: final target selection, design, and validation
Over the next 5 yr, the Dark Energy Spectroscopic Instrument (DESI) will use 10
spectrographs with 5000 fibers on the 4 m Mayall Telescope at Kitt Peak National …
spectrographs with 5000 fibers on the 4 m Mayall Telescope at Kitt Peak National …
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 …
simba: Cosmological simulations with black hole growth and feedback
We introduce the simba simulations, the next generation of the mufasa cosmological galaxy
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …
Robust data-driven metallicities for 175 million stars from Gaia XP spectra
We derive and publish data-driven estimates of stellar metallicity [M/H] for∼ 175 million stars
with low-resolution XP spectra published in Gaia DR3. The [M/H] values, along with T eff and …
with low-resolution XP spectra published in Gaia DR3. The [M/H] values, along with T eff and …
Nitrogen enhancements 440 Myr after the big bang: supersolar N/O, a tidal disruption event, or a dense stellar cluster in GN-z11?
Recent observations of GN-z11 with JWST/NIRSpec revealed numerous oxygen, carbon,
nitrogen, and helium emission lines at z= 10.6. Using the measured line fluxes, we derive …
nitrogen, and helium emission lines at z= 10.6. Using the measured line fluxes, we derive …