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From the 1 of 7 linked papers with an AI index.

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7 papers

hep-ph2026

Defect-Mediated Conversion: Dark Matter from Cosmological Domain-Wall Scattering

João Paulo Pinheiro, Mohamed Younes Sassi

We propose a new mechanism for dark matter genesis, \emph{Defect-Mediated Conversion} (DMC). Cosmological domain walls can host a scalar condensate in their core acting as a mixing…

astro-ph.GA2026

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models

Jack C. Turner, Stephen M. Wilkins, Aswin P. Vijayan

JWST observations have been used in conjunction with SED fitting to infer the physical properties of galaxies throughout cosmic time, revealing tensions with the predictions of the…

astro-ph.GA2026

Stellar photoionisation modelling in SYNTHESIZER

Aswin P. Vijayan, Stephen M. Wilkins, Sophie L. Newman +5

The paper introduces photoionised gas emission modeling into the SYNTHESIZER code, allowing realistic stellar and nebular spectra to be generated for galaxy formation studies.

astro-ph.GA2026

First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe

Connor Sant Fournier, Stephen M. Wilkins, Joseph Caruana +5

UV absorption line indices trace chemical enrichment and star formation histories in high-redshift galaxies, yet their reliability as quantitative stellar metallicity, Z*, diagnost…

astro-ph.IM2026

An innovative alternative to traditional funding streams for extragalactic astronomy

Stephen M. Wilkins, Jack Turner, Connor Sant Fournier +2

With traditional sources of funding for astronomical research under increasing pressure, it is timely to explore innovative alternative mechanisms. We therefore introduce GalaxyCoi…

astro-ph.GA2026

The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES

Jack C. Turner, Will J. Roper, Aswin P. Vijayan +5

RUBIES-UDS-QG-z7 (RQG) is the earliest massive quiescent galaxy identified to date, inferred to have formed its abundant stellar mass in a single burst that ceases rapidly before $…