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 …
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
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 …
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 …
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
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 …
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 …
application areas. In this review, we examine the science behind the quantum hype and …
Influence of local structure on relic neutrino abundances and anisotropies
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 …
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
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 …
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 …
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 …
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?
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 …
formation in comparison to the cold, collisionless dark matter paradigm (CDM), resulting in …