The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release 3: 3000 High-Quality Spectra of $K_s$-selected galaxies at $z>0.6$ [PDF]
We present the third and final data release of the Large Early Galaxy Astrophysics Census (LEGA-C), an ESO/Very Large Telescope public spectroscopic survey targeting 0.6 < z < 1.0, Ks -selected galaxies.
Arjen van der Wel +21 more
semanticscholar +5 more sources
Local and large-scale effects on the astrophysics of void-galaxies [PDF]
Galaxies in cosmic voids have been reported with properties related to a delayed evolution compared to the rest of the Universe. These characteristics reflect the interaction of galaxies with the environment.
Agustín M. Rodríguez-Medrano +5 more
openalex +3 more sources
Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations [PDF]
With the growing number of gravitational wave (GW) detections and the advent of large galaxy redshift surveys, a new era in cosmology is emerging. This study explores the synergies between GWs and galaxy surveys to jointly constrain cosmological and GW ...
Nicola Borghi +6 more
openalex +3 more sources
The Binary–Host Connection: Astrophysics of Gravitational-Wave Binaries from Host Galaxy Properties [PDF]
Gravitational waves from the merger of binary neutron stars (BNSs) are accompanied by electromagnetic counterparts, making it possible to identify the associated host galaxy.
Susmita Adhikari +9 more
openalex +3 more sources
Atomic Hydrogen in the Milky Way: A Stepping Stone in the Evolution of Galaxies [PDF]
Atomic hydrogen (Hi) is a critical stepping stone in the gas evolution cycle of the interstellar medium (ISM) of the Milky Way. Hi traces both the cold, premolecular state before star formation and the warm, diffuse ISM before and after star formation ...
N. McClure-Griffiths +2 more
semanticscholar +1 more source
The Cold Interstellar Medium of Galaxies in the Local Universe [PDF]
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 these stars, and a sensitive tracer of internal and external ...
A. Saintonge, B. Catinella
semanticscholar +1 more source
Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies [PDF]
Magnetohydrodynamic (MHD) turbulence is a crucial component of the current paradigms of star formation, dynamo theory, particle transport, magnetic reconnection, and evolution of structure in the interstellar medium (ISM) of galaxies.
B. Burkhart
semanticscholar +1 more source
Cosmic ray feedback in galaxies and galaxy clusters [PDF]
Understanding the physical mechanisms that control galaxy formation is a fundamental challenge in contemporary astrophysics. Recent advances in the field of astrophysical feedback strongly suggest that cosmic rays (CRs) may be crucially important for our
M. Ruszkowski, C. Pfrommer
semanticscholar +1 more source
EVOLUTION OF THE STARS AND GAS IN GALAXIES. [PDF]
Essentially everything of astronomical interest is either part of a galaxy, or from a galaxy, or otherwise relevant to the origin or evolution of galaxies. Diverse examples are that the isotropic composition of meteorites provides clues to the history of
B. Tinsley
semanticscholar +1 more source
Robust Field-level Likelihood-free Inference with Galaxies [PDF]
We train graph neural networks to perform field-level likelihood-free inference using galaxy catalogs from state-of-the-art hydrodynamic simulations of the CAMELS project.
Natal'i S. M. de Santi +14 more
semanticscholar +1 more source

