activity
20242026
collaborators

5 papers

astro-ph.GA2026

Inflow-driven galaxy evolution - I. Revealing the physics of the fundamental metallicity relation

Kai Wang, Carlton Baugh, N. F. Boardman +11

We present a unified physical framework for the fundamental metallicity relation (FMR), based on the mass-continuity equations. The FMR is not merely the anti-correlation between s…

astro-ph.CO2025

Dynamical analysis of stacked samples of asymmetric, non-static, self-gravitating systems

Yan-Chuan Cai, Nick Kaiser, Shaun Cole +1

We use numerical simulations to explore biases that arise in dynamical estimates of the mean mass profile for a collection of galaxy clusters that have been stacked to make a compo…

astro-ph.CO2025

Galaxy Mass Modelling from Multi-Wavelength JWST Strong Lens Analysis: Dark Matter Substructure, Angular Mass Complexity, or Both?

Samuel C. Lange, Aristeidis Amvrosiadis, James W. Nightingale +8

We analyze two galaxy-scale strong gravitational lenses, SPT0418-47 and SPT2147-50, using JWST NIRCam imaging across multiple filters. To account for angular complexity in the lens…

astro-ph.GA2024

A comparison of pre-existing CDM predictions with the abundance of {\it JWST} galaxies at high redshift

Shengdong Lu, Carlos S. Frenk, Sownak Bose +4

Observations with the {\it James Webb Space Telescope} have revealed a high abundance of bright galaxies at redshift, , which has been widely interpreted as conflictin…

astro-ph.CO2024

The Early Data Release of the Dark Energy Spectroscopic Instrument

DESI Collaboration, A. G. Adame, J. Aguilar +266

The Dark Energy Spectroscopic Instrument (DESI) completed its five-month Survey Validation in May 2021. Spectra of stellar and extragalactic targets from Survey Validation constitu…