The nature of compact radio sources: the case of FR 0 radio galaxies

RD Baldi - The Astronomy and Astrophysics Review, 2023 - Springer
Radio-loud compact radio sources (CRSs) are characterised by morphological compactness
of the jet structure centred on the active nucleus of the galaxy. Most of the local elliptical …

Moon-forming impactor as a source of Earth's basal mantle anomalies

Q Yuan, M Li, SJ Desch, B Ko, H Deng, EJ Garnero… - Nature, 2023 - nature.com
Seismic images of Earth's interior have revealed two continent-sized anomalies with low
seismic velocities, known as the large low-velocity provinces (LLVPs), in the lowermost …

EIGER. VI. The Correlation Function, Host Halo Mass, and Duty Cycle of Luminous Quasars at z≳ 6

AC Eilers, R Mackenzie, E Pizzati… - The Astrophysical …, 2024 - iopscience.iop.org
We expect luminous (M 1450≲− 26.5) high-redshift quasars to trace the highest-density
peaks in the early Universe. Here, we present observations of four z≳ 6 quasar fields using …

The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST

S Lim, S Tacchella, J Schaye, M Schaller… - Monthly Notices of …, 2024 - academic.oup.com
Motivated by the recent JWST discovery of galaxy overdensities during the Epoch of
Reionzation, we examine the physical properties of high-z protoclusters and their evolution …

Quantum algorithms for scientific applications

R Au-Yeung, B Camino, O Rathore… - arXiv preprint arXiv …, 2023 - arxiv.org
Quantum computing promises to provide the next step up in computational power for diverse
application areas. In this review, we examine the science behind the quantum hype and …

Influence of local structure on relic neutrino abundances and anisotropies

F Zimmer, CA Correa, S Ando - Journal of Cosmology and …, 2023 - iopscience.iop.org
Gravitational potentials of the Milky Way and extragalactic structures can influence the
propagation of the cosmic neutrino background (CNB). Of particular interest to future CNB …

A unified model for the clustering of quasars and galaxies at z≈ 6

E Pizzati, JF Hennawi, J Schaye… - Monthly Notices of …, 2024 - academic.oup.com
Recent observations from the EIGER JWST program have measured for the first time the
quasar–galaxy cross-correlation function at. The autocorrelation function of faint quasars …

Tetrahedral grids in Monte Carlo radiative transfer

A Lauwers, M Baes, P Camps… - Astronomy & …, 2024 - aanda.org
Context. To understand the structures of complex astrophysical objects, 3D numerical
simulations of radiative transfer processes are invaluable. For Monte Carlo radiative transfer …

Relativistic SZ temperatures and hydrostatic mass bias for massive clusters in the FLAMINGO simulations

ST Kay, J Braspenning, J Chluba… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT The relativistic Sunyaev-Zel'dovich (SZ) effect can be used to measure
intracluster gas temperatures independently of X-ray spectroscopy. Here, we use the large …

TangoSIDM Project: is the stellar mass Tully–Fisher relation consistent with SIDM?

CA Correa, M Schaller, J Schaye… - Monthly Notices of …, 2025 - academic.oup.com
Self-interacting dark matter (SIDM) has the potential to significantly influence galaxy
formation in comparison to the cold, collisionless dark matter paradigm (CDM), resulting in …